Monday, March 11, 2024

NATURE NEWS FEATURE

Superconductivity scandal: the inside story of deception in a rising star's physics lab

Ranga Dias claimed to have discovered the first room-temperature superconductors, but the work was later retracted. An investigation by Nature’s news team reveals new details about what happened — and how institutions missed red flags.

LONG READ

By Dan Garisto
08 March 2024
NATURE

Ranga Dias and his team at the University of Rochester compressed materials in a device called a diamond anvil cell to explore superconductivity. 
Credit: Lauren Petracca/New York Times/Redux/eyevine

In 2020, Ranga Dias was an up-and-coming star of the physics world. A researcher at the University of Rochester in New York, Dias achieved widespread recognition for his claim to have discovered the first room-temperature superconductor, a material that conducts electricity without resistance at ambient temperatures. Dias published that finding in a landmark Nature paper1.

Nearly two years later, that paper was retracted. But not long after, Dias announced an even bigger result, also published in Nature: another room-temperature superconductor2. Unlike the previous material, the latest one supposedly worked at relatively modest pressures, raising the enticing possibility of applications such as superconducting magnets for medical imaging and powerful computer chips.

Most superconductors operate at extremely low temperatures, below 77 kelvin (−196 °C). So achieving superconductivity at room temperature (about 293 K, or 20 °C) would be a “remarkable phenomenon”, says Peter Armitage, a condensed-matter researcher at Johns Hopkins University in Baltimore, Maryland.

But Dias is now infamous for the scandal that surrounds his work. Nature has since retracted his second paper2 and many other research groups have tried and failed to replicate Dias’s superconductivity results. Some researchers say the debacle has caused serious harm. The scandal “has damaged careers of young scientists — either in the field, or thinking to go into the field”, says Paul Canfield, a physicist at Iowa State University in Ames.



Why a blockbuster superconductivity claim met a wall of scepticism


Previous reporting by The Wall Street Journal, Science and Nature’s news team has documented allegations that Dias manipulated data, plagiarized substantial portions of his thesis and attempted to obstruct the investigation of another paper by fabricating data.

Three previous investigations into Dias’s superconductivity work by the University of Rochester did not find evidence of misconduct. But last summer, the university launched a fourth investigation, led by experts external to the university. In August 2023, Dias was stripped of his students and laboratories. That fourth investigation is now complete and, according to a university spokesperson, the external experts confirmed that there were “data reliability concerns” in Dias’s papers.

Now, Nature’s news team reveals new details about how the scandal unfolded.

The news team interviewed several of Dias’s former graduate students, who were co-authors of his superconductivity research. The individuals requested anonymity because they were concerned about the negative impact on their careers. Nature’s news team verified student claims with corroborating documents; where it could not do so, the news team relied on the fact that multiple, independent student accounts were in agreement.

The news team also obtained documents relevant to the acceptance of the two Nature papers and their subsequent retractions. (Nature’s news and journal teams are editorially independent.)

The investigation unearths fresh details about how Dias distorted the evidence for room-temperature superconductivity — and indicates that he concealed information from his students, manipulated them and shut them out of key steps in the research process. The investigation also reveals, for the first time, what happened during the peer-review process for Dias’s second Nature paper on superconductivity. Dias did not respond to multiple requests for comment.

Together, the evidence raises questions about why the problems in Dias’s lab did not prompt stronger action, and sooner, by his collaborators, by Nature’s journal team and by his university.
Zero resistance

Dias came to the University of Rochester in 2017, fresh from a postdoctoral fellowship at Harvard University in Cambridge, Massachusetts, where he worked under physicist Isaac Silvera. “He’s not only a very talented scientist, but he’s an honest person,” Silvera told Nature’s news team.

Once Dias settled at Rochester, he pursued high-temperature superconductivity. Three years earlier, the field had been electrified when researchers in Germany discovered superconductivity in a form of hydrogen sulfide with the formula H3S at 203 K (−70 °C) and at extremely high pressures3. This was a much higher temperature than any superconductor had achieved before, which gave researchers hope that room-temperature superconductivity could be around the corner.

Dias proposed that adding carbon to H3S might lead to superconductivity at even higher temperatures.

Ranga Dias at the University of Rochester, New York.Credit: Lauren Petracca/New York Times/Redux/eyevine

His former graduate students say they synthesized samples of carbon, sulfur and hydrogen (CSH), but did not take measurements of electrical resistance or magnetic susceptibility that showed superconductivity. When a superconducting material is cooled past a critical temperature, its electrical resistance drops sharply to zero, and the material displays a similarly sharp change in its magnetic properties, called the Meissner effect. Students say they did not observe these key signs of superconductivity in CSH.

Because of this, students say they were shocked when Dias sent them a manuscript on 21 July 2020 announcing the discovery of room-temperature superconductivity in CSH. E-mails seen by the news team show that the students had little time to review the manuscript: Dias sent out a draft at 5.13 p.m. and submitted the paper to Nature at 8.26 p.m. the same evening.

When the students asked Dias about the stunning new data, they say, he told them he had taken all the resistance and magnetic-susceptibility data before coming to Rochester. The news team obtained e-mails that show Dias had been making similar claims since 2014. In the e-mails, Dias says he has observed a sulfur-based superconductor with a temperature above 120 K — which is relatively high, but far from room temperature. The students recall that they felt odd about Dias’s explanation but did not suspect misconduct at the time. As relatively inexperienced graduate students, they say, they trusted their adviser.

During peer review, however, Dias’s claims about CSH met more resistance. Nature’s news team obtained the reports of all three referees who reviewed the manuscript. Two of the referees were concerned over a lack of information about the chemical structure of CSH. After three rounds of review, only one referee supported publication.

The news team showed five superconductivity specialists these reports. They shared some of the referees’ concerns but say it was not unreasonable for the Nature editors to have accepted the paper, given the strongly positive report from one referee and what was known at the time.

The paper was published on 14 October 2020 to fanfare. Dias and a co-author, Ashkan Salamat, a physicist at the University of Nevada, Las Vegas (UNLV), also announced their new venture: Unearthly Materials, a Rochester-based company established to develop superconductors that operate at ambient temperatures and pressures.

At the time, students say, they trusted Dias’s explanations of where the resistance and magnetic-susceptibility data came from. Now, however, they no longer believe the result, or Dias’s explanation for the data. “I don’t think any of the other data was collected,” one student says.
Matters arise

Soon after the CSH paper was published, Jorge Hirsch, a condensed-matter theorist at the University of California, San Diego, began pressing Dias to release the raw magnetic-susceptibility data, which were not included in the paper. More than a year later, Dias and Salamat finally made the raw data public.

In January 2022, Hirsch and Dirk van der Marel, a retired professor at the University of Geneva in Switzerland, posted an analysis of the raw data on the preprint server arXiv4. They reported that the data points were separated by suspiciously regular intervals — each exactly a multiple of 0.16555 nanovolts. Hirsch and van der Marel stated that this feature was evidence of data manipulation.
Dias’s team used laser spectroscopy to measure the pressure of samples in diamond anvil cells.
Credit: Lauren Petracca/New York Times/Redux/eyevine

Dias and Salamat responded in an arXiv preprint, arguing that the voltage intervals were simply a result of a background subtraction5 (the preprint was subsequently withdrawn by arXiv administrators). In high-pressure experiments, the signal of a sample’s superconductivity — a drop in voltage — can be drowned out by background noise. Researchers sometimes subtract this background, but the CSH paper did not mention the technique.

Questions about the data prompted Nature’s journal team to look further. In response to the concerns from Hirsch and van der Marel, editors at Nature asked four new referees to participate in a post-publication review of the CSH paper, which, like most peer review, was confidential.

Now, Nature’s news team has obtained the reports, which show that two of the anonymous referees found no evidence of misconduct. But two other reviewers, whom the news team can identify as physicists Brad Ramshaw at Cornell University in Ithaca, New York, and James Hamlin at the University of Florida in Gainesville, found serious problems with the paper.

In particular, Hamlin found evidence that led him to conclude the raw data had been altered. Nature applied an editor’s note to the CSH paper on 15 February 2022, alerting readers to concerns about the data.

On 4 March 2022, Dias and Salamat sent a rebuttal to the referees, denying data manipulation. But the rebuttal, seen by the news team, does not provide an explanation for the issues that Hamlin and Ramshaw found in the raw magnetic-susceptibility data. “I don’t know of any reasonable way this could come about,” Ramshaw wrote in a 13 March e-mail to Nature’s manuscript team in response to the rebuttal. “The simplest conclusion would be that these data sets are all generated by hand and not actually measured.”

On 27 March 2022, Hamlin sent Nature’s journal team his response to the rebuttal, which proposed an explanation for the odd data: rather than deriving the published data from raw data, Dias had added noise to the published data to generate a set of ‘raw’ data.

To assess the evidence for data fabrication, Nature’s news team last month asked two superconductivity specialists to review the post-publication reports. They said that Hamlin’s analysis gives credence to claims of misconduct.

In July 2022, using a different analysis, van der Marel and Hirsch independently came to the same conclusion and posted their findings on arXiv as an update to their original preprint. In it, they state that the raw data must have been constructed from the published data6.



Why superconductor research is in a ‘golden age’ — despite controversy


In light of these concerns, Nature started the process of retracting the CSH paper. On 11 August, Nature editors sent an e-mail to all the co-authors asking them whether they agreed to the retraction. Students who spoke to the news team say that they were surprised by this, because Dias had kept them out of the loop about the post-publication review process. They remained unaware of any of the referees’ findings, including that there was evidence for data fabrication.

Nature retracted the CSH paper on 26 September 2022, with a notice that states “issues undermine confidence in the published magnetic susceptibility data as a whole, and we are accordingly retracting the paper”. Karl Ziemelis, Nature’s chief applied and physical sciences editor, says the journal’s investigation ceased as soon as the editors lost confidence in the paper, which “did leave other technical concerns unresolved”.

The retraction does not state what Hamlin and Ramshaw found in the post-publication review process instigated by Nature: that the raw data were probably fabricated. Felicitas Heβelmann, a specialist in retractions at the Humboldt University of Berlin, says misconduct is difficult to prove, so journals often avoid laying blame on authors in retractions. “A lot of retractions use very vague language,” she says.

Publicly, Dias continued to insist that CSH was legitimate and that the retraction was simply down to an obscure technical disagreement.

As Nature journal editors were investigating the CSH paper, the University of Rochester conducted two investigations into Dias’s work; a separate one followed the retraction. One of the university’s inquiries was in response to an anonymous report, which included some of the evidence indicating possible data fabrication that surfaced during Nature’s post-publication review.

The university told Nature’s news team that the three investigations regarding the CSH study did not find evidence of misconduct.

A spokesperson for Nature says that the journal took the university’s conclusions into account during its deliberations, but still decided to retract the paper.

The lack of industry-wide standards for investigating misconduct leaves it unclear whether the responsibility to investigate lands more on journals or on institutions. Ziemelis says: “Allegations of possible misconduct are outside the remit of peer review and more appropriately investigated by the host institution.”

Heβelmann says the responsibility to investigate can “vary from case to case”, but that there is a trend of more journals investigating misconduct, regardless of institutional action.

Funding agencies can also investigate alleged misconduct. In this case, Dias has received funding from both the US National Science Foundation (NSF) and the Department of Energy (DoE). The DoE did not respond to questions from Nature’s news team about Dias’s grant. The NSF declined to say whether it is investigating Dias, but it noted that awards can be terminated and suspended in response to an investigation.

The students who spoke to Nature’s news team say that none of them were interviewed in the three investigations of the CSH work by the university, which they were not aware of at the time. “We were hoping someone would come talk to us,” one student says. “It never happened.”
A new claim

By the time the CSH paper came under scrutiny by Nature journal editors in early 2022, Dias’s graduate students were starting to grow concerned. In summer 2021, Dias had tasked them with investigating a compound of lutetium and hydrogen (LuH), which he thought might be a high-temperature superconductor.

They began testing commercially purchased samples of LuH and, before long, a student measured the resistance dropping to zero at a temperature of around 300 K (27 °C). Dias concluded the material was a room-temperature superconductor, even though there was extremely little evidence, several students told Nature. “Ranga was convinced,” one student says.


Physicist James Hamlin raised concerns about data reported by the Rochester group.
Credit: Zach Stovall for Nature

But the measurements were plagued by systematic errors, which students say they shared with Dias. “I was very, very concerned that one of the probes touching the sample was broken,” one student says. “We could be measuring something that looks like a superconducting drop, but be fooling ourselves.” Although students did see resistance drops in a few other samples, there was no consistency across samples, or even for repeated measurements of a single sample, they told Nature’s news team.

Students were also worried about the accuracy of other measurements. During elemental analysis of a sample, they detected trace amounts of nitrogen. Dias concluded that the samples included the element — and the resulting paper refers to nitrogen-doped lutetium hydride. But further analysis, performed after the paper was submitted, indicated that nitrogen was not incorporated into the LuH. “Ranga ignored what I was saying,” one student says.

Because they were not consulted on the CSH paper, the students say they wanted to make sure they were included in the process of writing the LuH paper. According to the students, Dias initially agreed to involve them. “Then, one day, he sends us an e-mail and says, ‘Here’s the paper. I’m gonna submit it,’” one student says.

E-mails seen by Nature’s news team corroborate the timeline. Dias sent out the first draft of the LuH paper in an e-mail at 2.09 a.m. on 25 April 2022. “Please send me your comments by 10.30 AM,” Dias wrote. “I am submitting it today.” The manuscript they received did not contain any figures, making it difficult to assess. The students convinced Dias to hold off on submitting until the next day, when they could discuss it in person.

One student was upset enough by the meeting that they wrote a memorandum of the events four days afterwards. The memo gives details of how students raised concerns and Dias dismissed them. Students worried that the draft was misleading, because it included a description of how to synthesize LuH; in reality, all the measurements were taken on commercially bought samples of LuH. “Ranga responded by pointing out that it was never explicitly mentioned that we synthesized the sample so technically he was not lying,” the student wrote.

The students say they also raised concerns about the pressure data reported in the draft. “None of those pressure points correspond to anything that we actually measured,” one student says. According to the memo, Dias dismissed their concerns by saying: “Pressure is a joke.”

Students say that Dias gave them an ultimatum: remove their names, or let him send the draft. Despite their worries, the students say they had no choice but to acquiesce. “I just remember being very intimidated,” one student says. The student says they regret not speaking up more to Dias. “But it’s scary at the time. What if I do and he makes the rest of my life miserable?”

Dias made some changes that the students requested, but ignored others; the submitted manuscript contained a description of a synthesis procedure that had not been used. He sent the LuH manuscript to Nature that evening.
Paper problems

After Nature published the LuH paper in March 2023, many scientists were critical of the journal’s decision, given the rumours of misconduct surrounding the retracted CSH paper. They wanted to know on what basis Nature had decided to accept it. (In the case of both papers, neither the peer-review reports nor the referees’ identities were revealed.) Nature’s news team obtained those reviews and can, for the first time, reveal what happened during the review process for the LuH paper. Nature editors received the manuscript in April 2022 (about a month after Nature received the CSH post-publication review reports) and sent it out to four referees.


Physicist Brad Ramshaw, together with James Hamlin, investigated data questions surrounding Dias’s superconductivity research.
Credit: Kim Modic

All four referees agreed that the findings, if true, were highly significant. But they emphasized caution in accepting the manuscript, because of the extraordinary nature of the claims. Referee 4 wrote that the journal should be careful with such extraordinary claims to avoid another “Schön affair”, referring to the extensive data fabrication by German physicist Jan Hendrik Schön, which has become a cautionary tale in physics and led to dozens of papers being retracted, seven of them in Nature. Referees 2 and 3 also expressed concern about the results because of the CSH paper, which at the time bore an editor’s note of concern but had not yet been retracted. Referees raised a plethora of issues, from a lack of details about the synthesis procedure to unexplainable features in the data.

Although Dias and Salamat managed to assuage some of those concerns, referees said the authors’ responses were “not satisfactory” and the manuscript went through five stages of review. In the end, only one referee said there was solid proof of superconductivity, and another gave qualified support for publication. The other two referees did not voice support for publication, and one of them remained unsatisfied with the authors’ responses and wanted more measurements taken.

The news team asked five superconductivity specialists to review key information available to Nature journal editors when they were considering the LuH manuscript: the referee reports for the LuH paper and the reports indicating data fabrication in the CSH paper. All five said the documents raised serious questions about the validity of the LuH results and the integrity of the data.

“The second paper — from my understanding of timelines — was being considered after the Nature editors and a lot of the condensed-matter community were aware there were profound problems” with the CSH paper, Canfield says. The specialists also pointed to negative comments from some of the LuH referees, such as the observation by Referee 1 that “raw data does not look like a feature corresponding to superconducting transition”.

When asked why Nature considered Dias’s LuH paper after being warned of potential misconduct on the previous paper, Magdalena Skipper, Nature’s editor-in-chief, said: “Our editorial policy considers every submission in its own right.” The rationale, Skipper explains, is that decisions should be made on the basis of the scientific quality, not who the authors are.

Many other journals have similar policies, and guidelines from the Committee on Publication Ethics state that peer reviewers should “not allow their reviews to be influenced by the origins of a manuscript”. But not all journals say they treat submissions independently. Van der Marel, who is the editor-in-chief of Physica C, says that he would consider past allegations of misconduct if he were assessing a new paper by the same author. “If you have good reasons to doubt the credibility of authors, you are not obliged to publish,” he says.
Under review

Soon after the LuH paper was published in March 2023, it came under further scrutiny. Several teams of researchers independently attempted to replicate the results. One group, using samples from Dias’s lab, reported electrical resistance measurements that it said indicated high-temperature superconductivity7. But numerous other replication attempts found no evidence of room-temperature superconductivity in the compound.

As previously reported in Science, Hamlin and Ramshaw sent Nature a formal letter of concern in May. Dias and Salamat responded to the issues later that month, but the students say they were not included in the response, and learnt about the concerns much later.

A recording of a 6 July 2023 meeting between Dias and his students, obtained by Nature’s news team, shows that Dias continued to manipulate the students. Throughout the hour-long meeting, Dias said he wanted to involve the students in deciding how the team would respond to concerns about the LuH paper. But he didn’t tell them that he and Salamat had already responded to the technical issues raised by Hamlin and Ramshaw
.
One of Dias’s students adjusts a diamond anvil cell, which the team used in its experiments.
Credit: Lauren Petracca/New York Times/Redux/eyevine

The recording also reveals how Dias tried to manipulate the Nature review, because he believed the process would turn against him once more. “We can pretend we’re going to cooperate and buy time for a month or so, and then gather some senior scientists from the community,” Dias says in the recording. Dias explains how he wants to use the credibility of senior scientists — or the University of Rochester — to pressure Nature and avert a retraction.

But Dias’s plans were thwarted. Later that month, the students received an e-mail from Nature’s editors that showed Dias and Salamat had, in fact, already responded to the concerns. The students realized that Dias had sent them a document with the dates removed, apparently to perpetuate the falsehood.

On 25 July 2023, the journal initiated a post-publication review and asked four new referees to assess the dispute. All of the referees agreed that there were serious problems with the data, and that Dias and Salamat did not “convincingly address” the issues raised by Hamlin and Ramshaw. A spokesperson for Nature says the journal communicated with University of Rochester representatives during the post-publication review.

Separately, Dias’s students were beginning to mobilize, re-examining the LuH data they were able to access. The students hadn’t done this before, because, they say, Dias produced almost all of the figures and plots in both of the Nature papers.

Several other researchers told the news team that the principal investigator does not typically produce all the plots. “That’s weird,” Canfield says.

The students say they were especially concerned about the magnetic susceptibility measurements — again, the raw data seemed to have been altered. Looking at the real raw data, one student says, the material does not look like a superconductor. But when Dias subtracted the background, the student says, that “basically flips that curve upside down and makes it look superconducting instead”.

They continued finding problems. For the resistance measurements, too, the alleged raw data didn’t match data actually taken in the lab. Instead, it had been tweaked to look neater. “Science can be really messy … some of these plots just look too good,” a student says.
Back to school

By this point, some students were deeply concerned about their careers. “My thesis is going to be full of fabricated data. How am I supposed to graduate in this lab?” one student says. “At that point, I was thinking of either taking a leave of absence, or of dropping out.”

During the summer, Dias began facing other issues. One of his papers in Physical Review Letters8 — unrelated to room-temperature superconductivity — was being retracted after the journal found convincing evidence of data fabrication. Around the same time, Dias was stripped of his students and the University of Rochester launched a fourth investigation — this time, the students say they were interviewed.



‘A very disturbing picture’: another retraction imminent for controversial physicist


In late August, the students decided to request a retraction of the LuH paper and compiled their concerns about the data and Dias’s behaviour. Before they sent a letter to Nature, Dias apparently caught wind of it and sent the students a cease-and-desist notice, which the news team has seen. But, after consulting a university official who gave them the green light, the students sent their letter to Nature editors, precipitating the retraction process. Eight out of 11 authors, including Salamat, signed the letter and the LuH paper was retracted two months later, on 7 November.

According to multiple sources familiar with the company, Salamat left Unearthly Materials in 2023 and is under investigation at UNLV. He did not respond to multiple requests for comment, and a spokesperson for UNLV declined to comment publicly on personnel issues.

The scandal has also had an impact on Nature’s journal team. “This has been a deeply frustrating situation, and we understand the strength of feelings this has stirred within the community,” Ziemelis says. “We are looking at this case carefully to see what lessons can be learnt for the future.”

With the university’s investigation now complete, Dias remains at Rochester while a separate process for addressing “personnel actions” proceeds. He has no students, is not teaching any classes and has lost access to his lab, according to multiple sources. Dias’s prestigious NSF grant — which has US$333,283 left to pay out until 2026 — could also be in jeopardy if the NSF finds reason to terminate it.

Dias has not published any more papers about LuH, but on X (formerly Twitter), he occasionally posts updates about the material. In a 19 January tweet, Dias shared an image of data, which he said showed the Meissner effect — “definitive proof of superconductivity!”

doi: https://doi.org/10.1038/d41586-024-00716-2


References


Snider, E. et al. Nature 586, 373–377 (2020); retraction 610, 804 (2022).

Article PubMed Google Scholar


Dasenbrock-Gammon, N. et al. Nature 615, 244–250 (2023); retraction 624, 460 (2023).

Article PubMed Google Scholar


Drozdov, A. P., Eremets, M. I., Troyan, I. A., Ksenofontov, V. & Shylin, S. I. Nature 525, 73–76 (2015).

Article PubMed Google Scholar


van der Marel, D. & Hirsch, J. E. Preprint at https://arxiv.org/abs/2201.07686v1 (2022).


Dias, R. P. & Salamat, A. Preprint at https://arxiv.org/abs/2201.11883 (2022).


van der Marel, D. & Hirsch, J. E. Preprint at https://arxiv.org/abs/2201.07686v6 (2022).


Salke, N. P., Mark, A. C., Ahart, M. & Hemley, R. J. Preprint at https://arxiv.org/abs/2306.06301 (2023).


Durkee, D. et al. Phys. Rev. Lett. 127, 016401 (2021); erratum 130, 129901 (2023); retraction 131, 079902 (2023).
Pentagon UFO office developing 'Gremlin' sensors to help identify anomalies in orbit

"We're really starting to understand what's in orbit around our planet and how we can eliminate those as anomalous objects."


By Brett Tingley published 2 days ago
AARO's seal in front of the Pentagon. (Image credit: AARO/Wikimedia Commons)

The Pentagon's UFO office is developing sensor kits to help it collect data in real time on unidentified objects in the sky or in space.

That's according to Tim Phillips, the acting head of the All-Domain Anomaly Resolution Office, or AARO, a U.S. Department of Defense office aimed at studying unidentified anomalous phenomena (UAP), a new term for UFOs that encompasses mysterious objects not only in the sky but also underwater or in space.

Phillips said that his office is working with government laboratories and academia to develop a highly portable sensor kit known as the "Gremlin System" that can capture data across multiple spectra, according to a report in DefenseScoop.

Related: Pentagon has 'no credible evidence' of aliens or UFOs that defy physics

Phillips added that the Gremlin System has already proven capable of detecting a wide range of phenomena, including in space. "It's picking up a lot of bats and birds. We're learning a lot about solar flaring," Phillips told a select group of reporters on Thursday (March 7).

"We're really starting to understand what's in orbit around our planet and how we can eliminate those as anomalous objects," he added.

RELATED STORIES:


 —  Previous Chinese spy balloons over US were classified as UFOs: report

 —  Pentagon UFO office unveils official website for US government personnel to report sightings

 —  Pentagon releases its long-awaited 2022 UFO report

The AARO director said that these Gremlin System sensors could be used to surveil sensitive sites for airspace intrusions, or even keep an eye on U.S. satellites in orbit.

"If we have a national security site and there are objects being reported that trend within restricted airspace, or within a maritime range, or in the proximity of one of our spaceships, we need to understand what that is. And so that's why we're developing a sensor capability that we can deploy in reaction to reports," Phillips said.

AARO plans to present the Gremlin System to Pentagon leaders so that the sensor kits could be deployed in the event of "UAP encounters at militarily significant locations or near U.S. critical infrastructure," DefenseScoop reported.
Scientists make shocking claim dark matter may really be an alternate shadow universe

Dark matter has proved an elusive concept to scientists, with some claiming it does not even exist. Now, researchers think the phenomenon could actually be part of an alternate universe.


By JOHN MAC GHLIONN
 Sun, Mar 10, 2024

The behaviour of galaxies would be inexplicable without the existence of dark matter 
(Image: Getty)

Scientists believe that dark matter could be viewed as an alternative universe following a breakthrough study.

The new paper by Dr. Arushi Bodas, a postdoctoral fellow at the University of Chicago’s Enrico Fermi Institute, and his colleagues, states that dark matter could and possibly should be viewed as a distorted alternate universe that never fully developed.

But before discussing the paper, it’s important to understand just how mysterious dark matter really is.

That's easier said than done, however.

Despite it constituting more than 80 percent of all matter in the universe, scientists have yet to observe dark matter, Its existence is inferred because the behavior of stars, planets, and galaxies would be wholly inexplicable without its presence.

Dark matter is difficult to observe; in fact, it’s completely imperceptible. It emits zero light or energy, making it undetectable by conventional sensors and detectors.

Scientists believe its composition is the key to understanding its mysterious nature. Visible matter, also known as baryonic matter, is composed of subatomic particles called baryons, which consist of protons, neutrons, and electrons. The composition of dark matter, on the other hand, remains speculative.

Potentially, it could consist of baryons, but it could also be composed of non-baryonic matter, which refers to different types of particles. The prevailing belief among scientists is that dark matter is primarily composed of non-baryonic matter. Another potential candidate is neutralinos, hypothetical particles that are heavier and slower than neutrinos, although they have yet to be observed.

Sterile neutrinos are also considered as a candidate for dark matter. Neutrinos are particles that do not contribute to regular matter. While a stream of neutrinos emanates from the sun, they rarely interact with normal matter and pass through the Earth and billions of inhabitants. Among the three known types of neutrinos, the sterile neutrino is proposed as a potential dark matter candidate. It would only interact with regular matter through gravity.

The most recent hypothesis proposes that dark matter exists in a distorted parallel universe within our own, where atoms are unable to come together. In the realm of ordinary matter, protons and neutrons possess almost identical masses, creating the necessary conditions for the formation of stable atoms.

The recent study proposes the existence of a potential shadow universe where protons and neutrons have asymmetrical masses, resulting in a chaotic mix of subatomic particles that rarely interact. In other words, the polar opposite of how conventional matter operates. This phenomenon could also clarify why dark matter does not aggregate.

Ever since astronomers initially suspected the presence of dark matter in the 1930s, debates surrounding what it is (and isn’t) have raged. Observations indicate that it surpasses ordinary matter by a ratio of 6 to 1. Galaxies and galaxy clusters are surrounded by massive spheres, known as "halos," of dark matter.

To remain undetected, astronomers theorize that this substantial amount of material must be composed of particles that have minimal interaction with ordinary matter or even with each other. Their primary function is to provide the gravitational framework for luminous matter. Astronomers believe that these halos were created in the early stages of cosmic history and subsequently attracted ordinary matter, which, due to its diverse range of behaviors, evolved into complex structures, while dark matter, being inert, remained unchanged.

Dark energy, on the other hand, seems to only serve the purpose of accelerating cosmic expansion, and the existing evidence suggests that it has remained constant throughout the existence of the universe.

Although a minority of scientists reject the idea of dark matter, there is now a plethora of evidence supporting its existence, with one of the most straightforward explanations involving the rotation of galaxies.

As Dr. Don Lincoln, a senior scientist at Fermilab, America’s leading particle physics laboratory, has noted, despite the gravitational pull towards the Sun, the planets' velocities result in nearly circular orbits.

The balance between velocity and gravity dictates that planets farther from the Sun move at a slower pace compared to those in closer proximity. Similarly, in galaxies, stars follow a similar pattern, with the laws of physics making analogous predictions.

Specifically, stars located further from the galactic center should move at a slower pace than those nearer to it.

However, observations by astronomers reveal that stars in the outer regions of galaxies move faster than anticipated. If the laws of gravity and motion hold true, the only plausible explanation is the presence of additional, unseen matter intensifying the gravitational force experienced by these rapidly moving stars.

The new paper by Dr. Bodas and his colleagues is just the latest to solidify the "dark matter really does exist' thesis.


Controversial new theory of gravity rules out need for dark matter


Exclusive: Paper by UCL professor says ‘wobbly’ space-time could instead explain expansion of universe and galactic rotation




Hannah Devlin 
THE GUARDIAN
Science correspondent
Sat 9 Mar 2024 

Dark matter is supposed to account for 85% of the mass in the universe, according to conventional scientific wisdom. But proponents of a radical new theory of gravity, in which space-time is “wobbly”, say their approach could render the elusive substance obsolete.

The proposition, outlined in a new paper, raises the controversial possibility that dark matter, which has never been directly observed, is a mirage that a substantial portion of the physics community has been chasing for several decades. The theory is viewed as quite left-field and is yet to be thoroughly tested, but the latest claims are creating a stir in the world of physics.

Announcing the paper on X, Prof Jonathan Oppenheim, of University College London, said: “Folks, something seems to be happening. We show that our theory of gravity … can explain the expansion of the universe and galactic rotation without dark matter or dark energy.”

There are multiple lines of evidence for dark matter, but its nature has remained mysterious and searches by the Large Hadron Collider have come up empty-handed. Last year, the European Space Agency launched a mission, Euclid, aiming to produce a cosmic map of dark matter.

The latest paper, published on the Arxiv website and yet to be peer-reviewed, raises the question of whether it even exists, drawing parallels between dark matter and flawed concepts of the past, such as “the ether”, an invisible substance that was thought to permeate all of space.

“In the absence of any direct evidence for dark energy or dark matter it is natural to wonder whether they may be unnecessary scientific constructs like celestial spheres, ether, or the planet Vulcan, all of which were superseded by simpler explanations,” it states. “Gravity has a long history of being a trickster.”

In this case, the simpler explanation being proposed is Oppenheim’s “postquantum theory of classical gravity”. The UCL professor has spent the past five years developing the approach, which aims to unite the two pillars of modern physics: quantum theory and Einstein’s general relativity, which are fundamentally incompatible.

Oppenheim’s theory envisages the fabric of space-time as smooth and continuous (classical), but inherently wobbly. The rate at which time flows would randomly fluctuate, like a burbling stream, space would be haphazardly warped and time would diverge in different patches of the universe. The theory also envisions an intrinsic breakdown in predictability.


The paper, by Oppenheim and Andrea Russo, a PhD candidate at UCL, claims this take on the universe could explain landmark observations of rotating galaxies that led to the “discovery” of dark matter. Stars at the edges of galaxies, where gravity is expected to be weakest based on visible matter, ought to be rotating more slowly than stars at the centre. But in reality, the orbital motion of stars does not drop off. From this, astronomers inferred the presence of a halo of unseen (dark) matter exerting a gravitational pull.

In Oppenheim’s approach the additional energy required to keep the stars locked in orbit is provided by the random fluctuations in spacetime, which in effect add in a background hum of gravitation. This would be negligible in a high gravity interaction, such as the Earth orbiting the Sun. But in low gravity situations, such as the fringes of a galaxy, the phenomenon would dominate – and cumulatively could account for the majority of the energy in the universe.

“We show that it can explain the expansion of the universe and galactic rotation curves without the need for dark matter or dark energy,” Oppenheim said on X. “We do urge caution, however, since there is other indirect evidence for dark matter, so further calculations and comparison with data are needed. But if it holds, it would appear that 95% of the energy in the universe is due to the erratic nature of spacetime, signalling either a fundamental breakdown in predictability of physics, or we are immersed in an environment which does not obey the laws of classical or quantum theory.”

Not everyone is convinced, including the well-known theorists Prof Carlo Rovelli and Prof Geoff Penington, who have signed a 5,000:1 odds bet with Oppenheim against his theory being proven correct.

“I think it’s good that physicists explore a wide variety of approaches to very difficult problems like combining quantum mechanics with gravity,” said Penington.

“Personally, I don’t think this particular approach is likely to be the correct one. I’ve obviously put my money where my mouth is on that front and there is nothing new in the recent papers that would make me change that assessment.”

Others are more enthusiastic. “I think the authors are on to something really interesting here, exploring some beautiful and novel ideas,” said Prof Andrew Pontzen, a cosmologist at University College London. “However, the challenge for replacing dark matter is that there are so many different lines of evidence that suggest its presence. So far they have only addressed one of these lines. Only time will tell whether the new ideas can truly explain the huge variety of phenomena that point towards dark matter.”








Roger Penrose on quantum mechanics and consciousness | Full interview

The Institute of Art and Ideas
Mar 9, 2024 

Roger Penrose full interview on quantum physics, consciousness, his career, and his idols.

Could quantum consciousness be the answer?

 

Watch Roger Penrose debate String Theory with Brian Greene and Eric Weisntein at https://iai.tv/video/the-trouble-with... Watch Roger Penrose debate The Multiverse with Sabine Hossenfelder and Michio Kaku at https://iai.tv/video/the-mystery-of-t... Join Nobel laureate Sir Roger Penrose as he outlines his views on quantum mechanics, Gödel's incompleteness theorem and consciousness. He also provides a glimpse into his visual thought process and scientific idol Galileo Galilei. #RogerPenrose #QuantumConsciousness #QuantumMechanics Sir Roger Penrose is a world-renowned physicist, best known for his work on general relativity and sharing the Wolf Prize for Physics with Stephen Hawking for their work on black holes. The Institute of Art and Ideas features videos and articles from cutting edge thinkers discussing the ideas that are shaping the world, from metaphysics to string theory, technology to democracy, aesthetics to genetics. Subscribe today! https://iai.tv/subscribe?utm_source=Y...
Why scientists think the Multiverse isn’t just fiction

The Multiverse fuels some of the 21st century's best fiction stories. But its supporting pillars are on extremely stable scientific footing.


How likely or unlikely was our Universe to produce a world like Earth? And how plausible would those odds be if the fundamental constants or laws governing our Universe were different? These questions may be scientifically answerable within the theory of the Multiverse, which predicts a large number of disconnected regions where a Big Bang occurs, separated by continuously inflating space.
Credit: Stu Gray / Alamy

KEY TAKEAWAYS

One of the most successful theories of 20th century science is cosmic inflation, which preceded and set up the hot Big Bang, pushing back the origin of our Universe earlier than ever.

We also know how quantum fields generally work, and if we assume inflation is an inherently quantum field, then there will always be more "still-inflating" space out there beyond the edge of our Universe.


Whenever and wherever inflation ends, you get a hot Big Bang: an infinite number of them as time goes on. If inflation and quantum field theory are both correct, a Multiverse is absolutely necessary.

Ethan Siegel

STARTS WITH A BANG — MARCH 6, 2024


Everywhere we look in the Universe, we see many examples of objects that are similar, but each one is unique. Of all the galaxies, stars, and planets we know of, no two are identical, but rather each one has its own unique history, properties, and composition. Yet it’s a compelling idea that, given enough Universe to work with, eventually the particles within it would have organized themselves in such a way that the same possibility — no matter how unlikely — occurs multiple different times. Perhaps, given the idea of an infinite Universe, there may even be an infinite number of copies of every single system we can imagine, including planet Earth, complete with each and every one of us living on it.

It’s this idea, that there might be an infinite number of copies of each one of us out there, somewhere, that gave rise to our modern notion of the Multiverse. Perhaps there are different versions of us out there, where one tiny decision, outcome, or even a quantum measurement led to a vastly different result down the road. While many have derided the Multiverse as a fundamentally unscientific idea — as, after all, there’s no way to see, test, or access information about any portion of the cosmos beyond our limited observable Universe — the fact is that the Multiverse’s very existence is rooted in science itself. In fact, if just two things are true: that cosmic inflation, which preceded and set up the Big Bang, occurred as we think it did, and that inflation, like all other fields in the Universe, is inherently a quantum field in nature, obeying all the quantum rules that other quantum theories obey,

then a Multiverse comes along as an inevitable consequence of those ideas. Here’s why physicists, despite the objections of a few, overwhelmingly claim that a multiverse must exist
.
The ‘raisin bread’ model of the expanding Universe, where relative distances increase as the space (dough) expands. The farther away any two raisins are from one another, the greater the observed redshift will be by the time the light is received. The redshift-distance relation predicted by the expanding Universe is borne out in observations and has been consistent with what’s been known since the 1920s.
Credit: NASA/WMAP Science Team

The story begins back with the discovery of the expanding Universe. Back in the 1920s, the evidence became overwhelming that not only were the copious spirals and ellipticals in the sky actually entire galaxies unto themselves, but that the farther away such a galaxy was determined to be, the greater the amount its light was shifted to systematically longer wavelengths. While a variety of interpretations were initially suggested, they all fell away with more abundant evidence until only one remained: the Universe itself was undergoing cosmological expansion, like a loaf of leavening raisin bread, where bound objects like galaxies (e.g., raisins) were embedded in an expanding Universe (e.g., the dough).


If the Universe was expanding today, and the radiation within it was being shifted toward longer wavelengths and lower energies, then that means that in the past, the Universe must have been smaller, denser, more uniform, and hotter. As long as any amount of matter and radiation are a part of this expanding Universe, the idea of the Big Bang yields three explicit and generic predictions:a large-scale cosmic web whose galaxies grow, evolve, and cluster more richly over time,
a low-energy background of blackbody radiation, left over from when neutral atoms first formed in the hot, early Universe,
and a specific set of ratios for the lightest elements — hydrogen, helium, lithium, and their various isotopes — that exist even in regions that have never yet formed stars at all.


This snippet from a structure-formation simulation, with the expansion of the Universe scaled out, represents billions of years of gravitational growth in a dark matter-rich Universe. Over time, overdense clumps of matter grow richer and more massive, growing into galaxies, groups, and clusters of galaxies, while the less dense regions than average preferentially give up their matter to the denser surrounding areas.
Credit: Ralf Kaehler and Tom Abel (KIPAC)/Oliver Hahn

All three of these predictions have been observationally borne out, and that’s why the Big Bang reigns supreme as our leading theory of the origin of our Universe, while all of its other competitors have fallen by the wayside. However, the Big Bang only describes what our Universe was like in its very early stages; it doesn’t explain why the Universe possessed the specific properties we’ve observed. In physics, if you know the initial conditions of your system and what the rules that it obeys are, you can predict extremely accurately — to the limits of your computational power and the uncertainty inherent in your system — how it will evolve arbitrarily far into the future.

Therefore, we can ask the important question: what initial conditions did the Big Bang need to have at its beginning in order to give us the Universe we observe now? The answers are a bit surprising, but what we find is that:there had to be a maximum temperature that’s significantly (about a factor of ~1000, at least) lower than the Planck scale, which is where the known laws of physics break down,
the Universe had to have been born with density fluctuations of approximately the same magnitude on all scales (with slightly, by a few percent, smaller magnitude fluctuations on small cosmic scales than large ones),
the expansion rate and the total matter-and-energy density must have balanced almost perfectly: to at least ~30 significant digits at the moment the hot Big Bang began,
the same initial conditions — same temperature, density, and spectrum of fluctuations — must have existed at all locations, even between two locations where a signal at the speed of light could not have traversed the distance between them in the time elapsed since the Big Bang,and the total entropy of the Universe must have been much, much lower than it is today, by a factor of many trillions.


If these three different regions of space never had time to thermalize, share information, or transmit signals to one another, then why are they all the same temperature? This is one of the problems with the initial conditions of the Big Bang; how could these regions all obtain the same temperature unless they started off that way, somehow?
Credit: E. Siegel/Beyond the Galaxy

Whenever we come up against a question of initial conditions — basically, why did our system start off the way it must have begun — we only have two options available to us. We can appeal to the unknowable, saying that it is this way because it’s the only way it could’ve been (i.e., the Lady Gaga explanation, saying it was simply “born this way”), and we can’t know anything further. However, there’s a scientific approach we can try as well: we can attempt to find a mechanism for setting up and creating the conditions that we know we needed to have. That second pathway is what physicists call “appealing to dynamics,” where the mechanism we devise must do three important things.It has to reproduce every success that the model it’s trying to supersede — the hot Big Bang in this instance — produces. Those earlier cornerstones must all arise from any mechanism we propose.
It has to explain the key observational fact that the Big Bang cannot: the initial conditions the Universe started off with. These problems, the ones that come unexplained within the Big Bang alone, must be explained by whatever novel idea comes along.
And it has to make new predictions that differ from the original (Big Bang) theory’s predictions, where those predictions must lead to a consequence that is in some way observable, testable, and/or measurable.

The only idea we’ve had that met all three of these criteria was the theory of cosmic inflation, which has now achieved unprecedented successes on all three fronts.


Exponential expansion, which takes place during inflation, is so powerful because it is relentless. With every ~10^-35 seconds (or so) that passes, the volume of any particular region of space doubles in each direction, causing any particles or radiation to dilute and causing any curvature to quickly become indistinguishable from flat. After only a few hundred doubling times, or ~10^-32 seconds, a fluctuation that was initially smaller than the Planck scale would now be stretched to be larger than the presently observable Universe.
Credit: E. Siegel (L); Ned Wright’s Cosmology Tutorial (R)

What inflation basically says is that the Universe, before it was hot, dense, and filled with matter-and-radiation everywhere, was in a state where it was dominated by a very large amount of energy that was inherent to space itself: some sort of field or vacuum energy. Only, unlike today’s dark energy, which has a very small energy density (the equivalent of about one proton per cubic meter of space), the energy density during inflation was tremendous: some ~1025 times greater than the dark energy density is today. Since it’s the energy density, according to Einstein’s general relativity, that determines the expansion rate, that means that during inflation, not only was the expansion rate incredibly large, but it was relentless: as space continues to expand, the expansion rate remains enormous.

This is profoundly different behavior than the Universe we’re familiar with today. In an expanding Universe with matter and radiation, the volume increases while the number of particles stays the same, and hence the density drops. Since the energy density is related to the expansion rate, the expansion rate of the Universe slows down over time.

But if the energy density is in a form that’s intrinsic to space itself, then the energy density remains constant with time, and so too will the expansion rate. The result is what we know as exponential expansion, where after a very small period of time, the Universe doubles in size, and after that time passes again, it doubles again, and so on. In very short order — a tiny fraction of a second — a region that was initially smaller than the smallest subatomic particle can get stretched to be larger than the entire visible Universe is today.



In the top panel, our modern Universe has the same properties (including temperature) everywhere because they originated from a region possessing the same properties. In the middle panel, the space that could have had any arbitrary curvature is inflated to the point where we cannot observe any curvature today, solving the flatness problem. And in the bottom panel, pre-existing high-energy relics are inflated away, providing a solution to the high-energy relic problem. This is how inflation solves the three great puzzles that the Big Bang cannot account for on its own.
Credit: E. Siegel/Beyond the Galaxy

During inflation, the Universe — irrespective of what properties it had at the start of inflation — gets stretched to enormous scales. This accomplishes a tremendous number of things in the process, among them:stretching the observable Universe, irrespective of what its initial curvature was, to be indistinguishable from flat,
taking whatever initial conditions existed in the region that began inflating, and stretching them so that they’re now uniform across the entire visible Universe,
taking whatever quanta were present within that region, prior to inflation, and rapidly driving them away from one another to arbitrarily low densities,
creating minuscule quantum fluctuations and stretching them across the Universe as well, so that they’re almost the same on all distance scales, but with slightly smaller-magnitudes on smaller scales (when inflation is about to end),
converting all that “inflationary” field energy into matter-and-radiation, but only allowing that matter-and-radiation to reach a maximum temperature that’s still well below the Planck scale (but comparable to the inflationary energy scale),
and creating a spectrum of density and temperature fluctuations that exist on scales larger than the cosmic horizon, and that are adiabatic (of constant entropy) and not isothermal (of constant temperature) everywhere.

This, at last, does all three of the things we require for a new theory to be considered for superseding an older one. Inflation reproduces the successes of the non-inflationary hot Big Bang, provides a mechanism for explaining the Big Bang’s initial conditions, and makes a slew of novel predictions that differ from those with a non-inflationary beginning. Beginning in the 1990s and through the present day, the inflationary scenario’s predictions agree with observations, distinct from the non-inflationary hot Big Bang

.
The quantum fluctuations inherent to space, stretched across the Universe during cosmic inflation, gave rise to the density fluctuations imprinted in the cosmic microwave background, which in turn gave rise to the stars, galaxies, and other large-scale structures in the Universe today. This is the best picture we have of how the entire Universe behaves, where inflation precedes and sets up the Big Bang. Unfortunately, we can only access the information contained inside our cosmic horizon, which is all part of the same fraction of one region where inflation ended some 13.8 billion years ago.
Credit: E. Siegel; ESA/Planck and the DOE/NASA/NSF Interagency Task Force on CMB research

Based on the properties that we observe our Universe to possess today, there’s a minimum amount of inflation that had to have occurred in the past in order to reproduce what we see. That further implies that there are certain conditions that inflation has to satisfy in order to be successful: the conditions that give rise to those predictions and post-dictions we just mentioned. Perhaps the simplest, most easy-to-understand way to model inflation is to treat it as a hill, where as long as you stay on top of the hill, you inflate, but as soon as you roll down into the valley below, inflation comes to an end and transfers its energy into matter and radiation.


If you do this, you’ll find that there are certain shapes your hill can have, or what physicists call “potentials,” that succeed on these fronts, while others simply don’t. The key to getting the amount of inflation that you need has everything to do with the top of the hill: it needs to be flat enough in shape over a large enough region. In simple terms, if you think of the inflationary field as a ball atop that hill, it needs to roll slowly for the majority of inflation’s duration, only picking up speed and rolling rapidly when it enters the valley, which is what brings inflation to an end. We, as scientists, have quantified how slowly inflation needs to roll, which allows us to learn something about the required shape of this potential. As long as the top is sufficiently flat, inflation can work as a viable solution to the beginning of our Universe.



When cosmic inflation occurs, the energy inherent in space is large, as it is at the top of this hill. As the ball rolls down into the valley, that energy converts into particles. This provides a mechanism for not only setting up the hot Big Bang, but for both solving the problems associated with it and making new predictions as well.
Credit: E. Siegel/Beyond the Galaxy

So, where does the idea of a Multiverse come into play? It has to do with the one way we can’t treat the ball-and-hill analogy too seriously: the fact that this is a purely classical view of things. The Universe, at least as we understand it, isn’t purely classical, but rather is quantum in nature. And that implies that inflation, like all of the fields we know of, ought to be a quantum field, too, as far as its very nature is concerned. The quantum nature of a field teaches us that many of its properties cannot be exactly determined, but rather will possess a probability distribution to them. And, just as with all time-dependent quantum systems, the greater the amount of time that passes, the greater the amount that the probability distribution will spread out.

In other words, inflation isn’t about rolling a point-like ball down a hill. Instead, what’s actually rolling down the hill is a quantum probability wavefunction, which is able to take on a variety of allowed values.

But as the ball rolls along the hill, the Universe is undergoing cosmic inflation, which means it’s expanding exponentially in all three dimensions. If we were to take a 1-by-1-by-1 cube and call that “our Universe,” then we could watch that cube expand during inflation. If it takes some tiny amount of time for the size of that cube to double, then it becomes a 2-by-2-by-2 cube, which requires 8 of the original cubes to fill. Allow that same amount of time to elapse, and it becomes a 4-by-4-by-4 cube, needing 64 original cubes to fill. Let that time elapse again, and it’s an 8-by-8-by-8 cube, with a volume of 512. After only about ~100 “doubling times,” we’ll have a Universe with approximately ~1090 original cubes in it, or a Universe that’s expanded in volume by that same factor: ~1090
.
If inflation is a quantum field, then the field value spreads out over time, with different regions of space taking different realizations of the field value. In many regions, the field value will wind up in the bottom of the valley, ending inflation, but in many more, inflation will continue so long as the ball remains on the flat part of the hill, where it can remain arbitrarily far into the future.
Credit: E. Siegel/Beyond the Galaxy

Here’s where the problem arises. If inflation is a quantum field, and quantum fields spread out over time, then what happens when the “quantum ball” atop the hill is rolling slowly, along the flat part of the hill?

The answer is that the part of the wavefunction that spreads closer to the valley-end of the hill is more likely to roll into the valley itself. In those regions, inflation is very likely to swiftly come to an end, where that field energy will then get converted to matter-and-radiation, and something that we know as a hot Big Bang will ensue. This region might be irregularly shaped at the boundaries, but some region that was just like it seems to describe the portion of the observable Universe that we can see and access. So long as enough inflation occurred to reproduce the observational successes we see in our Universe, this appears to be a good description of our own cosmic history.

But what about the portions of the wavefunction that spread out closer to the top, flatter part of the hill? Inflation continues for longer there, and these are the regions that we can consider to be “outside” of the regions where inflation swiftly comes to an end. What does that imply, as far as regions where:inflation comes to an end and a hot Big Bang ensues, versus those where inflation continues on, unabated, even while it ends elsewhere?


Wherever inflation occurs (blue cubes), it gives rise to exponentially more regions of space with each step forward in time. Even if there are many cubes where inflation ends (red Xs), there are far more regions where inflation will continue on into the future. The fact that inflation never comes to an end absolutely everywhere is what makes inflation ‘eternal’ once it begins, and where our modern notion of a Multiverse (where the regions with a red X describe separated, disconnected universes) comes from.
Credit: E. Siegel/Beyond the Galaxy

When you work out the mathematics for getting enough inflation before a hot Big Bang ensues, this is where science tells us that the Multiverse is all but inevitable. We have to mandate that the Universe experiences enough inflation so that our Universe can exist with the properties we observe it to have. We also know that, outside of the region where inflation ended, inflation must have continued onward for longer.

Now we ask the big question, “What is the relative size of those regions?” If we compare the regions where:inflation ends at a certain time,
with the regions where inflation hasn’t ended after that time has elapsed,

we find that the latter regions, where inflation continues, are exponentially larger (and still growing with time) compared to the regions where it ends and a hot Big Bang ensues. Moreover, that size disparity continues to get worse as time goes on. Even if there are an infinite number of regions where inflation ends, there will be a larger infinity of regions where it persists. Moreover, the various regions where it ends — where hot Big Bangs occur — will all be causally disconnected, separated further by more regions of inflating space.

Put simply, if each hot Big Bang occurs in a “bubble” Universe, then the bubbles simply can never collide. What we wind up with is a larger and larger number of disconnected bubbles as time goes on, all separated by an eternally inflating space.


While many independent Universes are predicted to be created in an inflating spacetime, inflation never ends everywhere at once, but rather only in distinct, independent areas separated by space that continues to inflate. This is where the scientific motivation for a Multiverse comes from, and why no two Universes will ever collide. The Universe doesn’t expand into anything; it itself is expanding.
Credit: Ozytive/Public Domain

That’s what the Multiverse is, and why scientists accept its existence as the default position. We have overwhelming evidence for the hot Big Bang, and also that the Big Bang began with a set of conditions that don’t come with a de facto explanation. If we add in an explanation for it — cosmic inflation — then that inflating spacetime that set up and gave rise to the Big Bang makes its own set of novel predictions. Many of those predictions are borne out by observation, but other non-observable predictions also still arise as consequences of inflation.

One of them is the existence of myriads of universes, of disconnected regions each with their own hot Big Bang, that comprise what we know as a Multiverse when you take them all together. This doesn’t necessarily imply that different Universes have different rules or laws or fundamental constants, or that all the possible quantum outcomes you can imagine occur in some other pocket of the Multiverse. It doesn’t even necessarily mean that the Multiverse is physically real, as this is a prediction we cannot verify, validate, or falsify. But if:the theory of inflation is a good one, and the data says it is,
and our Universe is quantum in nature, and all evidence suggests that it is,

then a multiverse is all but inevitable. You may not like it, and you really may not like how some physicists abuse the idea, but until a better, viable alternative to inflation comes around — and until that alternative can clear those same three theoretical hurdles that inflation has already cleared — the Multiverse is very much here to stay.

 

Quantum Gravity Unveiled – Scientists Crack the Cosmic Code That Baffled Einstein

Gravity Quantum Physics Concept Art

Researchers have developed a method to measure gravity at a microscopic level, marking a significant advancement in understanding quantum gravity. Credit: SciTechDaily.com

Physicists successfully measure gravity in the quantum world, detecting weak gravitational pull on a tiny particle with a new technique that uses levitating magnets, putting scientists closer to solving mysteries of the universe.

Scientists are a step closer to unraveling the mysterious forces of the universe after working out how to measure gravity on a microscopic level.

Experts have never fully understood how the force discovered by Isaac Newton works in the tiny quantum world.

Even Einstein was baffled by quantum gravity and, in his theory of general relativity, said there is no realistic experiment that could show a quantum version of gravity.

A Breakthrough in Quantum Gravity

However, physicists at the University of Southampton, working with scientists in Europe, have now successfully detected a weak gravitational pull on a tiny particle using a new technique.

They claim it could pave the way to finding the elusive quantum gravity theory.

The experiment, published in the Science Advances journal, used levitating magnets to detect gravity on microscopic particles – small enough to border on the quantum realm.

Quantum Experiment Artist Impression

Artist impression of the quantum experiment. Credit: University of Southampton

Pioneering Gravity Research

Lead author Tim Fuchs, from the University of Southampton, said the results could help experts find the missing puzzle piece in our picture of reality.

He added: “For a century, scientists have tried and failed to understand how gravity and quantum mechanics work together.

“Now we have successfully measured gravitational signals at the smallest mass ever recorded, it means we are one step closer to finally realizing how it works in tandem.

“From here we will start scaling the source down using this technique until we reach the quantum world on both side

“By understanding quantum gravity, we could solve some of the mysteries of our universe – like how it began, what happens inside black holes, or uniting all forces into one big theory.”

The rules of the quantum realm are still not fully understood by science – but it is believed that particles and forces at a microscopic scale interact differently than regular-sized objects.

Academics from Southampton conducted the experiment with scientists at Leiden University in the Netherlands and the Institute for Photonics and Nanotechnologies in Italy, with funding from the EU Horizon Europe EIC Pathfinder grant (QuCoM).

Their study used a sophisticated setup involving superconducting devices, known as traps, with magnetic fields, sensitive detectors, and advanced vibration isolation.

It measured a weak pull, just 30aN, on a tiny particle 0.43mg in size by levitating it in freezing temperatures a hundredth of a degree above absolute zero – about minus-273 degrees Celsius.

Expanding the Horizons of Quantum Research

The results open the door for future experiments between even smaller objects and forces, said Professor of Physics Hendrik Ulbricht also at the University of Southampton.

He added: “We are pushing the boundaries of science that could lead to new discoveries about gravity and the quantum world.

“Our new technique that uses extremely cold temperatures and devices to isolate the vibration of the particle will likely prove the way forward for measuring quantum gravity.

“Unravelling these mysteries will help us unlock more secrets about the universe’s very fabric, from the tiniest particles to the grandest cosmic structures.”

Reference: “Measuring gravity with milligram levitated masses” by Tim M. Fuchs, Dennis G. Uitenbroek, Jaimy Plugge, Noud van Halteren, Jean-Paul van Soest, Andrea Vinante, Hendrik Ulbricht and Tjerk H. Oosterkamp, 23 February 2024, Science Advances.
DOI: 10.1126/sciadv.adk2949

Where Do Humans Fit in the Universe? This Physicist Wants to Change Your Perspective

In Waves in an Impossible Sea, Matt Strassler explains how human life is intimately connected to the larger cosmos.

By Isaac Schultz
Published Yesterday

An artist’s concept of a particle collision.
Illustration: Jurik Peter (Shutterstock)

Pondering the scale of the cosmos can feel as if you’re peering over the edge of the brink; it can be daunting enough to make you want to flee to the comforts of working, commuting, and other quotidian endeavors. But in Waves in an Impossible Sea: How Everyday Life Emerges From the Cosmic Ocean, theoretical physicist and science communicator Matt Strassler doesn’t flinch in the face of the universe.

Published this week, Strassler’s book expands on the ideas he’s explored for years on his blog, Of Particular Significance. Readers are given a window into how the fundamental laws that govern the universe shape our daily experiences, and how even the most exotic phenomena are not as alien to our day-to-day as they may seem.

‘Huh, That’s Funny’: Physicists Delighted by New Measurement for the W Boson

What Should Fans Take Away From Imaginary?

Strassler recently spoke with Gizmodo about the book’s origins and goals. Below is our conversation, lightly edited for clarity.

Isaac Schultz, Gizmodo: There’s this interesting dichotomy between the physics that’s happening here on Earth, what I call “looking down,” and the physics that’s astronomical observation—“looking up,” so to speak. And I was wondering if you have thought about the same thing, and how you see that relationship.

Matt Strassler: One of the first things I try to do in the book is to break that dichotomy down. Because we do have this tendency to think about the universe writ large, this big place that we live in. And then there’s kind of this tiny stuff going on inside of us or inside of the materials around us, and we don’t really connect them. But of course, they are profoundly connected. And, you know, the universe—we used to call it outer space, and we think of it as mostly a vacuum. It’s emptiness. But the stuff that’s inside of us is also mostly empty. It’s the same emptiness. And so there is no distinction between the outer-ness and the inner-ness. It’s the same stuff doing many of the same things. We’re not disconnected from that larger universe. We’re actually, in some sense, made from it. And so, that is a message which I wanted to be able to convey that I hope will change people’s perspective on how they think about what it is to be alive in this universe. That we don’t just live in it, but we grow from it in a very meaningful sense: not just in a spiritual one, but in a very explicit physics sense.


Gizmodo: Yeah. Whenever I’m slightly stressed out, I remind myself that I am just dying particles.

Strassler: We are much more than that. But even when we say we are particles, we are missing something. In English, by a particle we mean a little localized thing, like a dust particle, that’s not connected to everything else. But when we understand that what we call particles are actually little ripples, little waves in the fields of the universe, and the fields of the universe extend everywhere. Across the entire universe. That’s a very different way of understanding what we’re made from. We’re not made from these little localized things that move around in a universe. We’re made from ripples of a universe, and that is a very different picture.

Gizmodo: The crux of the book is this relationship between our modern understanding of physics and human life, human existence as we experience it. When you were writing the book, did you have a specific reader in mind? Who do you hope will, you know, stumble across this title and pick it up?

Strassler: There are certainly some readers who read a lot of particle physics books already, and I hope that for them, what I’m providing is a way of looking at something they already know. And in particular a way of understanding what the Higgs field is all about. For those readers, it’s something they will not have seen before. But I also had in mind that there are a lot of friends of mine, family members, who don’t read the books about particle physics precisely because they’re rather difficult to understand and often seem irrelevant to their lives. The goal of this book was to strip away, as much as possible, the things that don’t matter to our ordinary daily existence and focus on the things that do. And try to tell a story, which certainly doesn’t explain all of particle physics by any means, but walks a path that takes the reader through all of the things that they would need to know to start from scratch and come out the end with a sense for how the universe works and how we fit in it.


I hope that I’ve provided a path for a reader who is curious but willing to take the time that it requires to understand subjects that are that aren’t hard just because “physics is hard.” They’re hard because the universe is hard. It’s hard for me. I can’t make it any easier than it is for me.

Gizmodo: That’s going to be the headline. “Physicist Confesses: ‘It’s Hard For Me, Too.’”


Strassler: Okay. I’m happy with that.

Gizmodo: How did this book emerge from the work that you’ve been doing for years?


Strassler: I was a full-time academic scientist for a good two decades. I had always been interested in doing public outreach. But I had never had really that much time being a full-time scientist. There was a certain moment in my career where it wasn’t clear what I wanted to do next. And I started a blog at that point. That was just before the expected and then actual discovery of what is known as the particle called the Higgs boson.



Image: Basic Books

The story of the Higgs particle is really a story of a field known as the Higgs field, which is much more important to us than the Higgs particle is. The Higgs field affects our lives in all sorts of ways. But to understand what the Higgs field is and how it does what it does, which is typically what people ask me, requires some understanding of both Einstein’s relativity and quantum physics. There wasn’t any way to write the book without starting with those things. Even though explaining the Higgs field was the original motivation, I discovered that really this is a book about what we know today based on the last 125 years of scientific research in physics: what is the big picture? How does it all fit together? And once you see that—once you understand what particles actually are and how they emerge from relativity on the one hand and quantum physics on the other—then it’s not so hard to explain what the Higgs field is. But you have to spend two-thirds of the book to get to that point.


Gizmodo: When you say to someone that you’re going to open with relativity and quantum physics, it’s a great way to end the conversation.

Strassler: There is that risk, right? But that’s part of why I really opened with the questions about those subjects that are not even obviously about them. They are questions about daily life. And the fact is that these subjects, which seem remote and very esoteric... they’re not. They’re deeply ingrained in ordinary human experience. And that was really what I wanted to convey in this book, that these rather strange-sounding subjects that originate with Einstein and are made often in the media and by scientists to seem, “gee whiz”—and they are—they’re more than that. They are the foundations of our daily experiences. And so I wanted to bring that sense of how important these things are to us, to all of us.


Gizmodo: I think that, scientists on the one hand and science communicators on the other, struggle with this issue of, well, it’s not going to be possible to convey all the nuance in, say, a 400-word article. It’s just not going to happen. It’s more about writing the least-wrong thing than the most-right thing. You wrote a book that grapples with complex science. How were you checking to make sure that this would actually grok to the average reader?

Strassler: It helps that I have had the blog for 10 years. I also have some humility about how well I have achieved this goal. That’s partly because I know these are difficult subjects. They’re not difficult in the sense of that you have to know mathematics to grapple with them, but they’re difficult in the sense that they are just strange and difficult for scientists to wrap their heads around. I know that whatever methods I have used in the book, they’re going to work for some people on some pages and for other people on other pages. And so one of the things that I’m doing with my website is, I’m creating a whole wing of the website whose goal is to add additional information. For example, the figures, some will be animated on the website to give greater clarity. The goal is to really explain the science, and I’m not done with that part.

Gizmodo: It’s been over ten years since the Higgs discovery. How do you go about writing this book, thinking about a post-Higgs world and trying to address the next big question?

Strassler: In a sense, the discovery of the Higgs boson and the lack of any immediate discoveries thereafter over the ensuing 10 years—leaving aside gravitational waves, which were discovered in 2015—has put our understanding of the universe into a very interesting place. It’s like having a short story which is complete but has all sorts of loose ends, which fits into a larger narrative which we don’t understand. And so it’s kind of a perfect moment to describe what we know and what we don’t. And really break it into those two parts.

There was a way in which, 10 years after the Higgs discovery, and also with the discovery of gravitational waves, things came out more or less the way we thought they would. There were no huge surprises that completely changed the way we think about things. So it’s a good moment to take stock and to look at what we have learned from Einstein’s relativity, on the one hand, and from quantum physics and all of its realization in particle physics on the other, and see how it all fits together and try to really describe that as a package.

To use a cliche, it’s really more like the end of the beginning here. We have achieved something that is really remarkable in the past 125 years. But we’re clearly also in some ways still at the beginning of our understanding of how the universe really works.


Gizmodo: One question that I was left with was basically, where is this next breakthrough going to come from? Do you have any particular preference for the variety of wonderful experiments going on right now in particle physics, in plans for gravitational wave observatories, all that jazz? What are you most excited about on the physical horizon?

Strassler: All the way up to the discovery of the Higgs boson, there has been a path. But there’s always been something where it’s clear that there are things we need to know that in some way feed into the deepest questions about how the universe works. And for the first time in 150 years, that is no longer true.

We do not now have a clear path. We have many possible paths, and we don’t really know which one is the best one. And this is part of why there is so much controversy about particle physics right now. It’s because there are definitely things that we know give us a decent chance of finding something new. But we don’t have the kind of confidence that we would have had 30 years ago or 60 years ago, that the next wave of experiments definitely will answer one or more of the questions that we have.

So when you ask me what is my preferred direction, I would prefer that the Large Hadron Collider, which has 10 more years to run, discover something. Because that would make it a lot easier to know what to do next. And the machine will run for 10 more years, producing 10 times as much data. So we do have that opportunity. But, I would like a clue from nature before answering that question.

Gizmodo: You mention that the LHC is keeps on ticking and you know, the high-luminosity LHC is on the horizon. Do you anticipate that kind of juicing the the collider will yield results?

Strassler: I’m not a person to express optimism or pessimism about what nature may deliver to us. I mean, I don’t think I have the insights into nature to guess. But what I can say is that there is an enormous amount still to do, even with the data that we have. It is certainly possible that there is something to discover in the existing LHC data, in addition to the opportunities that having 10 times that data will offer. So, I think people are sometimes too quick to imagine that, “oh well, the LHC looked. It’s not there. We’re done.” No, no, no, no. The LHC produces an enormous pile of data, and every analysis you do has to cut through that data in a particular way.



I wouldn’t say optimistic or pessimistic, but I would say I’m cognizant of the fact that there is still a tremendous amount left to do at the LHC, and we should definitely not be writing it off at all at this point. What we can probably say with some certainty is that the most popular ideas for what might be found at the Large Hadron Collider are mostly ruled out or unlikely at this point, but there are plenty of things, plenty of examples in history where the thing that was really interesting was something that no theoretical physicist had imagined. And we may just need to be really imaginative about how we analyze the data at the LHC.
Holst The Planets with Professor Brian Cox 

WAIT, WHAT?!

World's oldest star Methuselah is older than Universe — but how?


World's oldest star Methuselah is 16 billion years old, 190 light-years away from Earth


The oldest star in the universe is HD140283 — or Methuselah as it's commonly known. 
— Caltech/File

Saturday, March 09, 2024
Web Desk
Sci-tech

Methuselah or HD140283 was found to be an astonishing 16 billion years old or "oldest star of the Universe", when scientists observed it with the European Space Agency's (ESA) Hipparcos satellite in 2002.

This number was really surprising, as the age of the Universe itself was estimated to be 13.8 billion years old, so a star being older than the Universe baffled experts, according to Space.

"It was a serious discrepancy," says astronomer Howard Bond of Pennsylvania State University.

Keeping this in mind, he and his colleagues planned to explore the truth and determine the precision of this number. As a result, their conclusions were found to be mind-blowing.

Methuselah is named after a biblical patriarch, who died at the age of 969, which makes him the oldest figure in the Bible.

The wonderous star resides some 190 light-years away from the Earth and in the constellation of Libra.

It fastly travels across the sky at 800,000 mph (1.3 kilometres per hour).

The tests explained that the star was really old. It is made up of hydrogen and helium and consists of very little iron.

This also signifies that this star must have been born when the Universe was ruled helium and hydrogen before iron, as the heavier elements started appearing when gigantic stars created them in their cores.