Thursday, August 19, 2021

How Big Can the Quantum World Be? Physicists Probe the Limits.

By showing that even large objects can exhibit bizarre quantum behaviors, physicists hope to illuminate the mystery of quantum collapse, identify the quantum nature of gravity, and perhaps even make Schrödinger’s cat a reality.




How large can an object be and still act like a quantum wave? In theory, any size at all.


Hannes Hummel for Quanta Magazine
Philip Ball
Contributing Writer


August 18, 2021
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It’s a mere speck of matter — a piece of silica crystal no bigger than a virus, levitated in a light beam. But it is almost as motionless as the laws of physics permit.

Two teams of researchers, in Austria and Switzerland, have independently succeeded in freezing such minuscule nanoparticles, just 100 to 140 nanometers across, almost entirely into their lowest-energy quantum state, giving them effectively a temperature just a few millionths of a degree above absolute zero — and fixing them in place with unearthly precision.

Holding a nanoparticle this tightly in a single spot is just the start. The goal is to put these objects into a so-called quantum superposition — where it becomes impossible to say, before measuring them, just where they are. A particle in a superposition could be found in one of two or more places, and you just don’t know which of them it will be until you look. It is perhaps the most startling example of how quantum mechanics seems to insist that our familiar world of objects with definite properties and positions comes into being only through the act of looking at it.

Superpositions of subatomic particles, atoms, and the massless “particles” of light called photons are well established. But because such quantum effects tend to be very easily disturbed when the particles interact with their surroundings, setting up superpositions gets rapidly harder as the objects get bigger and experience more interactions. Those interactions tend to almost instantaneously destroy a superposition and leave the object with unique, well-defined properties.

All the same, researchers have been steadily increasing the size at which superpositions and related quantum effects can still be observed — from particles to small molecules, then bigger molecules, and now, they hope, nanoscale lumps of matter. No one knows how far in principle this expansion of quantumness can continue. Is there — as some think — a size limit at which it simply vanishes, perhaps because quantum behavior is incompatible with gravity (which is negligible for atoms and molecules)? Or is there no fundamental limit to how big quantumness can be?


A silica nanoparticle has been cooled to its quantum ground state.
Lorenzo Magrini, Yuriy Coroli/University of Vienna



These questions have been around throughout the century-long history of quantum theory. Now, for the first time, researchers are on the cusp of being able to answer them — and perhaps to point the way toward describing how gravity fits into the quantum world. “I’ve been working on macroscopic superpositions for 10 years,” said the quantum theorist Oriol Romero-Isart of the University of Innsbruck in Austria, one of the leaders in the field, “but now we’re at a very timely moment.” In the coming years, we might discover whether or not the world is quantum all the way up.





Aquantum particle in a superposition, contrary to common belief, is not really in two (or more) states at once. Rather, a superposition means that there is more than one possible outcome of a measurement. For an object at everyday scales, described by classical physics, that makes no sense — it is either here or there, red or blue. If we can’t say which it is, that’s just because of our ignorance: We haven’t looked. But for quantum superpositions, there simply is no definite answer — the property of “position” is ill-defined.

If, however, we only see one outcome or the other when we look, how can we know the particle was in a superposition before we looked? The answer is that so long as we don’t try to find out what the outcome is — so long as we don’t measure that property — the two (or more) alternatives somehow embodied in the superposition can interfere with one another, just like two waves. This wavy behavior is embodied in a mathematical entity called the wave function, which encodes everything we are able to say about the particle.

Quantum interference is most famously seen when a particle passes through two narrowly spaced slits in a screen. If we don’t look to see which slit the particle goes through, then the particle will behave much like a water wave, and its wave function will spread through both slits at once, creating an interference pattern.

But if we place a measuring device by a slit to tell us if each particle went through it or not — to observe the particle’s path — then the interference pattern goes away.

How big can objects get and still behave as interfering “matter waves”? The quantum physicist Anton Zeilinger and his co-workers at the University of Vienna studied that question in 1999 with a double-slit experiment using carbon molecules called fullerenes (C60), made from exactly 60 carbon atoms linked into hexagonal and pentagonal rings like the leather patches of a soccer ball. They found a clear interference pattern, demonstrating that even molecules like C60 — at 0.7 nanometers across, much bigger and heftier than an individual atom — could be put into a superposition.

Perhaps just as important, they went on to study how that superposition went away.

Interactions between a quantum particle and neighboring particles, such as gas molecules or photons, entangle both objects into a kind of joint quantum state. In this way, a superposition of the original particle gets spread into the environment.

Rather like an ink droplet diffusing and spreading in a glass of water, this spreading superposition makes it ever harder to see the original one unless you look at every spot it has spread to and reconstruct it from that information. As entanglement mixes the wave function of the initial superposed particle with those of its surrounding particles, the wave function seems to lose coherence and become just a mass of incoherent little waves. This process is called decoherence, and it makes the superposition undetectable in the original object: Its quantum nature seems to disappear.





The high-vacuum chamber of the interferometer in Markus Arndt’s laboratory includes a violet mirror and nanomotors to move the mechanical gratings.


Quantum Nanophysics Group

Decoherence of a quantum superposition happens extremely fast unless the interactions of the particle with its environment can be minimized — for example, by cooling it to extremely low temperatures to reduce the disruptive effect of heat, and keeping the object in a vacuum to eliminate molecular collisions. The bigger the object is, the more interactions it is likely to have, and the faster decoherence happens. For a dust grain about 10 micrometers across floating in the air, a superposition state of two positions in space separated by about the same width as the grain itself is estimated to decohere in about 10−31 seconds — less than the time it takes for a beam of light to travel the width of a proton.

Decoherence seems to be the main obstacle to making quantum superpositions of large objects that last long enough to be observed. The interference experiments with fullerenes lent support to that picture. The Vienna team predicted that the interference of the particles should gradually disappear as they let a background gas into the chamber, where its molecules would collide with the fullerenes and destroy the coherence of their quantum waves. That’s exactly what they saw.

One of the members of Zeilinger’s team was Markus Arndt, who has continued the quest to scale up quantum interference over the past two decades. In 2011, he and his team interfered beams of carbon-based organic molecules with up to 430 atoms each, measuring up to 6 nanometers across. In 2019, they did it with molecules of around 2,000 atoms. Then last year, they created interference patterns in a biological molecule — specifically, a natural peptide called gramicidin A1 — even though these are fragile molecules to submit to the arduous conditions of molecular-beam interference experiments.

Arndt says his goal is to increase the mass of the particles by a factor of 10 every year or two. That would soon take them well into the size and mass range of biological objects such as viruses. Meanwhile, in 2009 Romero-Isart, then at the Max Planck Institute for Quantum Optics in Garching, Germany, and his co-workers sketched out an idea to levitate viruses in an optical trap — where tiny objects are held fast by the forces induced by intense, focused light beams — and then coax them into a superposition of two vibration states and look for interference between them.

Why stop there? The researchers even speculated about doing the same to unambiguously living organisms, such as the phenomenally robust little animals called tardigrades, which are about a millimeter wide and have been found to survive several days of exposure to outer space. The researchers wrote that the plan would allow them to create “quantum superposition states in very much the same spirit as the original Schrödinger’s cat” — the famous thought experiment intended to highlight the apparent absurdity of quantum superpositions for large (and especially living) entities.




The prospect of making Schrödinger’s absurdities into reality is one animating principle behind the Q-Xtreme project, a collaboration between the groups of Markus Aspelmeyer of the University of Vienna, Lukas Novotny and Romain Quidant at the Swiss Federal Institute of Technology Zurich, and Romero-Isart.

In 2019 three of the groups, in two independent studies, reported that they could cool down silica nanoparticles about 100 to 150 nanometers across, containing around a hundred million atoms, almost into their lowest-energy (ground) quantum state while holding them in an optical trap produced by laser beams.

Then last year, Aspelmeyer’s team reported that they had ushered such particles even more fully into the ground state, where the vibrations of the crystalline lattice of atoms are as minimal as they can be. At absolute zero, the particle would be entirely in the ground state, and the only motion remaining would be the so-called zero-point motion of the atoms. In Aspelmeyer’s experiment, the particle was in its ground state 70% of the time on average.

Now in their latest experiments, Aspelmeyer and Novotny have managed to get rid of the optical trap — which affects the quantum behavior of the free particle — so that they can observe the particle “in the wild,” as it were, rather than in captivity. The researchers use laser light to constantly measure the particle’s position, then apply an electric field to nudge the particle so that it stays in its designated location — not by trapping, but by gentle coaxing. This “active feedback” approach suppresses the particle’s thermal jiggling and cools it to an extremely low temperature.

Aspelmeyer’s group says that the spread in their particle’s position is only 1.3 times that of the zero-point motion, equivalent to a temperature of just a few millionths of a kelvin above absolute zero. Novotny and colleagues obtained comparable cooling with a similar setup.




Inside a vacuum chamber in the lab of Lukas Novotny (left), 
two optical lenses hold a levitated silica nanoparticle (right).
ETH Zurich


The next step will be to make a superposition. In order to do so, the researchers will need to control three key environmental influences. First, they must eliminate any noisiness in the active-feedback potential. Then they need to use a very high vacuum — about 10−11 millibars of pressure — so that there’s almost nothing for the particle to collide with. Finally, they need to stop the particle from radiating any photons — as any warm object does. Though the particle is very tightly localized, as if supercold, it absorbs enough of the photons buzzing around to be at an internal temperature of 1,000 degrees Kelvin or so, which would make it radiate like a hot poker. Suppressing the decoherence induced by that radiation is going to be tough, said Romero-Isart.

The need to suppress radiation from the particle speaks to a subtle yet critical issue. A quantum superposition isn’t destroyed because a disturbance from the environment comes in and knocks it off balance. Rather, it’s destroyed when information about the object’s location leaks out into the environment where it can be measured — just as interference in a quantum double-slit experiment is destroyed by measuring particle paths.

If a gas molecule bounces off it, say, in principle you could figure out where the particle is by looking at the molecule’s trajectory. Or if it radiates photons, you can see where it is just as you can locate your front door at night from the light on your porch. Yet in the case of your front door, the light only reveals its location. For quantum objects, the radiated light creates it.





This sensitivity of a superposition to interactions with the environment makes the experiment hard, but it can also be useful. For example, a system like this could be used to study how quantum objects lose their quantumness through decoherence and become classically fixed in one place. “Large superpositions are very fragile and sensitive to decoherence,” said Romero-Isart — but “decoherence is something we don’t understand completely.” So the experiments could test theories of how it happens.

Researchers are particularly keen to examine one idea about how quantum becomes classical. This switch has long been described as “collapse of the wave function”: A superposition of two possible states, say, collapses to just one of them when measured. This collapse was first proposed by the Hungarian mathematical physicist John von Neumann in the 1930s as an ad hoc way to get from the probabilities encoded in the wave function to the definite values that actual measurements produce. It was a sleight of hand with no real justification from the theory itself: a mathematical convenience to reconcile the theory with what we actually see.

Ideas about decoherence and interaction with the measuring apparatus have now largely replaced von Neumann’s mysterious notion of an abrupt collapse. But some researchers have proposed that collapse is nonetheless a real, physical process that produces classical definiteness from quantum possibilities. “Collapse models predict breakdowns of [standard] quantum mechanics when you have large masses and large superpositions,” said Romero-Isart. “Quantum mechanics has not been tested in that space.”




Kahan Dare (left) and Manuel Reisenbauer, researchers 
in the lab of Markus Aspelmeyer, work on the experiment to cool  levitated nanoparticle to its quantum ground state.Lorenzo Magrini, Yuriy Coroli/University of Vienna

He and his colleagues in Q-Xtreme hope to test physical-collapse models, which predict that large superpositions will be shorter-lived than expected. In particular, they hope to explore what happens to quantum mechanics at size scales where gravity matters.

Right now, quantum mechanics seems incompatible with the modern theory of gravity, namely Albert Einstein’s general relativity. The quantum world is discrete and granular, whereas relativity describes space-time as smooth and continuous. Usually this discord can be ignored, because quantum mechanics describes the very small while general relativity describes large, massive objects.

But the British mathematical physicist Roger Penrose has suggested that at intermediate scales, when quantum theory collides with general relativity, the latter will win, destroying quantum effects. Under general relativity, any object that has a significant gravitational field distorts space-time. But an object in a superposition of locations would then produce two superposed space-times: a situation that general relativity doesn’t allow. So Penrose believes that gravity would force a choice between the alternatives.

Aspelmeyer thinks that Q-Xtreme should finally be able to put theories like this one to the test. “At the scale of our planned experiment, all existing collapse models would either be ruled out or constrained to parameter regimes that render them meaningless,” he said.

Superpositions of masses large enough for gravity to come into play could probe quantum aspects of gravity itself. One idea for doing that is to use gravitational interaction to entangle the masses. In 2017, the physicists Sougato Bose of University College London and Vlatko Vedral and Chiara Marletto of the University of Oxford independently proposed experiments that might do just that. Such experiments are “super exciting but very hard,” said Romero-Isart — although Vedral thinks that it could be feasible in the next 10 years or so.

No one knows quite what to expect. “Once we can study a situation where quantum theory would suggest that space-time itself should be in a superposition of two measurably different states,” said Aephraim Steinberg, a quantum physicist at the University of Toronto, “all bets are off, and we have nothing but experiment to guide us. It’s reasonable to keep an open mind to the possibility that we will discover something new.”

Vedral expects we will find that gravity (at least when it is not super strong) can indeed be described using standard quantum field theory, just like the other known forces. But he admits that “secretly I’m hoping that it would fail, because as a theoretician you would like something extraordinary to happen.”





Attempting large quantum superpositions is a win-win situation, said Bose. If we find that physical collapse prohibits them, that would be a huge discovery about the fundamental nature of quantum mechanics. But if, as many suspect, physical collapse doesn’t occur and the quantum world can just keep getting bigger, then big superpositions, with their extreme sensitivity to sources of decoherence, could act as very delicate sensors. The physicists Jess Riedel and Itay Yavin in Canada, for example, have proposed that quantum systems that are sensitive to gravitational effects might offer a way to look for dark matter particles, which seem to interact with ordinary matter only via gravity. Bose, meanwhile, is interested in using such systems as benchtop detectors of gravitational waves, which so far have only been seen with the aid of immense detectors several kilometers in size.

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In other words, expanding the quantum scale up to sizes where gravity matters might teach us new things about quantum mechanics, gravity and hidden aspects of the universe. The project will push technological capabilities to the limit, but the payoff could be enormous. And the current resurgence of interest in creating quantum phenomena such as superposition and entanglement on large scales is not a chance occurrence, said Arndt — because these are precisely what will be needed if we are going to scale up quantum computers so that they have many thousands or even millions of entangled quantum bits. “Quantum technologies will receive dozens of billions of dollars of investments in the coming years,” he said, “and we had better understand the foundations of the theory underlying all these technological hopes.”

Scientists discover crystal exhibiting exotic spiral magnetism

Scientists discover crystal exhibiting exotic spiral magnetism
This “semimetal” crystal consists of repeating unit cells such as the one to the left, which has a square top and rectangular sides. The spheres represent silicon (violet), aluminum (turquoise), and — in gold — neodymium (Nd) atoms, the last of which are magnetic. Understanding the special magnetic properties of the material requires nine of these unit cells, shown as the larger block to the right (which has a unit single cell outlined in red). This 3x3 block shows green “Weyl” electrons traveling diagonally across the top of the cells and affecting the magnetic spin orientation of the Nd atoms. A special property of the Weyl electron is the locking of its spin direction, which either points parallel or antiparallel to the direction of its motion, as represented by the small arrows in the Weyl electrons. As these electrons travel along the four gold Nd atoms, the Nd spins reorient themselves into a “spin spiral” which can be imagined as pointing successively in the 12 o’clock direction (closest to viewer with red arrow pointing upward), 4 o’clock (blue arrow), 8 o’clock (also in blue) and again 12 o’clock (farthest from viewer and again in red). Lines of Nd atoms stretch through many layers of the crystal, offering many instances of this unusual magnetic pattern. Credit: N. Hanacek/NIST

An exotic form of magnetism has been discovered and linked to an equally exotic type of electrons, according to scientists who analyzed a new crystal in which they appear at the National Institute of Standards and Technology (NIST). The magnetism is created and protected by the crystal's unique electronic structure, offering a mechanism that might be exploited for fast, robust information storage devices.

The newly invented material has an unusual structure that conducts electricity but makes the flowing electrons behave as massless particles, whose  is linked to the direction of their motion. In other materials, such Weyl electrons have elicited new behaviors related to electrical conductivity. In this case, however, the electrons promote the spontaneous formation of a magnetic spiral. 

"Our research shows a rare example of these particles driving collective magnetism," said Collin Broholm, a physicist at Johns Hopkins University who led the  at the NIST Center for Neutron Research (NCNR). "Our experiment illustrates a unique form of magnetism that can arise from Weyl electrons."

The findings, which appear in Nature Materials, reveal a complex relationship among the material, the electrons flowing through it as current and the magnetism the material exhibits. 

In a refrigerator magnet, we sometimes imagine each of its  as having a bar magnet piercing it with its "north" pole pointing in a certain direction. This image refers to the atoms' spin orientations, which line up in parallel. The material the team studied is different. It is a "semimetal" made of silicon and the metals aluminum and neodymium. Together these three elements form a crystal, which implies that its component atoms are arranged in a regular repeating pattern. However, it is a crystal that breaks inversion symmetry, meaning that the repeating pattern is different on one side of a crystal's unit cells—the smallest building block of a crystal lattice—than the other. This arrangement stabilizes the electrons flowing through the crystal, which in turn drive unusual behavior in its magnetism. 

The electrons' stability shows itself as a uniformity in the direction of their spins. In most materials that conduct electricity, such as , the electrons that flow through the wire have spins that point in random directions. Not so in the semimetal, whose broken symmetry transforms the flowing electrons into Weyl electrons whose spins are oriented either in the direction the electron travels or in the exact opposite direction. It is this locking of the Weyl electrons' spins to their direction of motion—their momentum—that causes the semimetal's rare magnetic behavior.

The material's three types of atoms all conduct electricity, providing steppingstones for electrons as they hop from atom to atom. However, only the neodymium (Nd) atoms exhibit magnetism. They are susceptible to the influence of the Weyl electrons, which push the Nd atom spins in a curious way. Look along any row of Nd atoms that stretches diagonally through the semimetal, and you will see what the research team refers to as a "spin spiral." 

"A simplified way to imagine it is the first Nd atom's spin points to 12 o'clock, then the next one to 4 o'clock, then the third to 8 o'clock," Broholm said. "Then the pattern repeats. This beautiful spin 'texture' is driven by the Weyl electrons as they visit neighboring Nd atoms."

It took a collaboration among many groups within the Institute for Quantum Matter at Johns Hopkins University to reveal the special magnetism arising in the crystal. It included groups working on crystal synthesis, sophisticated numerical calculations and neutron scattering experiments. 

"For the neutron scattering, we greatly benefited from the extensive amount of neutron diffraction beam time that was available to us at the NIST Center for Neutron Research," said Jonathan Gaudet, one of the paper's co-authors. "Without the beam time, we would have missed these beautiful new physics."

Each loop of the spin spiral is about 150 nanometers long, and the spirals only appear at  below 7 K. Broholm said that there are materials with similar physical properties that function at room temperature, and that they might be harnessed to create efficient magnetic memory devices.

"Magnetic memory technology like hard disks usually requires you to create a magnetic field for them to work," he said. "With this class of materials, you can store information without needing to apply or detect a magnetic field. Reading and writing the information electrically is faster and more robust." 

Understanding the effects that the Weyl electrons drive also might shed light on other materials that have brought consternation to physicists. 

"Fundamentally, we might be able to create a variety of materials that have different internal spin characteristics—and perhaps we already have," Broholm said. "As a community, we have created many magnetic structures we don't immediately comprehend. Having seen the special character of Weyl-mediated magnetism, we may finally be able to understand and use such exotic magnetic structures." New quantum material discovered

More information: Gaudet, J. et al. Weyl-mediated helical magnetism in NdAlSi. Nat. Mater. (2021). doi.org/10.1038/s41563-021-01062-8 , www.nature.com/articles/s41563-021-01062-8

Journal information: Nature Materials 

Provided by National Institute of Standards and Technology 

This exotic particle had an out-of-body experience; these scientists took a picture of it

This exotic particle had an out-of-body experience; these scientists took a picture of it
Schematic of the triangular spin lattice and star-of-David charge density wave pattern in a
 monolayer of tantalum diselenide. Each star consists of 13 tantalum atoms.
 Localized spins are represented by a blue arrow at the star center. The wavefunction
 of the localized electrons is represented by gray shading.
 Credit: Mike Crommie et al./Berkeley Lab

Scientists have taken the clearest picture yet of electronic particles that make up a mysterious magnetic state called quantum spin liquid (QSL).

The achievement could facilitate the development of superfast quantum computers and energy-efficient superconductors.

The scientists are the first to capture an image of how electrons in a QSL decompose into spin-like particles called spinons and charge-like particles called chargons.

"Other studies have seen various footprints of this phenomenon, but we have an actual picture of the state in which the spinon lives. This is something new," said study leader Mike Crommie, a senior faculty scientist at Lawrence Berkeley National Laboratory (Berkeley Lab) and physics professor at UC.

"Spinons are like ghost particles. They are like the Big Foot of quantum physics—people say that they've seen them, but it's hard to prove that they exist," said co-author Sung-Kwan Mo, a staff scientist at Berkeley Lab's Advanced Light Source. "With our method we've provided some of the best evidence to date."

A surprise catch from a quantum wave

In a QSL, spinons freely move about carrying heat and spin—but no electrical charge. To detect them, most researchers have relied on techniques that look for their heat signatures.

This exotic particle had an out-of-body experience; these scientists took a picture of it
Scanning tunneling microscopy image of a tantalum diselenide sample that is just 3 atoms
 thick. Credit: Mike Crommie et al./Berkeley Lab

Now, as reported in the journal Nature Physics, Crommie, Mo, and their research teams have demonstrated how to characterize spinons in QSLs by directly imaging how they are distributed in a material.

To begin the study, Mo's group at Berkeley Lab's Advanced Light Source (ALS) grew single-layer samples of tantalum diselenide (1T-TaSe2) that are only three-atoms thick. This material is part of a class of materials called transition metal dichalcogenides (TMDCs). The researchers in Mo's team are experts in , a technique for synthesizing atomically thin TMDC crystals from their constituent elements.

Mo's team then characterized the thin films through angle-resolved , a technique that uses X-rays generated at the ALS.

Using a microscopy technique called scanning tunneling microscopy (STM), researchers in the Crommie lab—including co-first authors Wei Ruan, a postdoctoral fellow at the time, and Yi Chen, then a UC Berkeley graduate student—injected electrons from a metal needle into the tantalum diselenide TMDC sample.

Images gathered by scanning tunneling spectroscopy (STS) – an imaging technique that measures how particles arrange themselves at a particular energy—revealed something quite unexpected: a layer of mysterious waves having wavelengths larger than one nanometer (1 billionth of a meter) blanketing the material's surface.

"The long wavelengths we saw didn't correspond to any known behavior of the crystal," Crommie said. "We scratched our heads for a long time. What could cause such long wavelength modulations in the crystal? We ruled out the conventional explanations one by one. Little did we know that this was the signature of spinon ghost particles."

This exotic particle had an out-of-body experience; these scientists took a picture of it
Illustration of an electron breaking apart into spinon ghost particles and chargons inside a 
quantum spin liquid. Credit: Mike Crommie et al./Berkeley Lab

How spinons take flight while chargons stand still

With help from a theoretical collaborator at MIT, the researchers realized that when an electron is injected into a QSL from the tip of an STM, it breaks apart into two different particles inside the QSL—spinons (also known as ghost particles) and chargons. This is due to the peculiar way in which spin and charge in a QSL collectively interact with each other. The spinon ghost particles end up separately carrying the spin while the chargons separately bear the electrical charge.

In the current study, STM/STS images show that the chargons freeze in place, forming what scientists call a star-of-David charge-density-wave. Meanwhile, the spinons undergo an "out-of-" as they separate from the immobilized chargons and move freely through the material, Crommie said. "This is unusual since in a conventional material, electrons carry both the spin and charge combined into one particle as they move about," he explained. "They don't usually break apart in this funny way."

Crommie added that QSLs might one day form the basis of robust quantum bits (qubits) used for quantum computing. In conventional computing a bit encodes information either as a zero or a one, but a qubit can hold both zero and one at the same time, thus potentially speeding up certain types of calculations. Understanding how spinons and chargons behave in QSLs could help advance research in this area of next-gen computing.

Another motivation for understanding the inner workings of QSLs is that they have been predicted to be a precursor to exotic superconductivity. Crommie plans to test that prediction with Mo's help at the ALS.

"Part of the beauty of this topic is that all the complex interactions within a QSL somehow combine to form a simple ghost particle that just bounces around inside the crystal," he said. "Seeing this behavior was pretty surprising, especially since we weren't even looking for it."Researchers discover a unique orbital texture in single-layer of 3-D material

More information: Ruan, W., Chen, Y., Tang, S. et al. Evidence for quantum spin liquid behaviour in single-layer 1T-TaSe2 from scanning tunnelling microscopy. Nat. Phys. (2021). doi.org/10.1038/s41567-021-01321-0 , www.nature.com/articles/s41567-021-01321-0

Journal information: Nature Physics 

Provided by Lawrence Berkeley National Laboratory 


SpaceX Starship to Take Civilians Where Civilians Never Went Before: to the dearMoon

SpaceX Starship dearMoon MissionSpaceX Starship dearMoon MissionSpaceX Starship dearMoon MissionSpaceX Starship dearMoon MissionSpaceX spacesuitSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX StarshipSpaceX Starship
 In 2024, NASA is scheduled to return humans to the surface of the Moon with the Artemis III mission. One year before that, Artemis II should circle the satellite without touching down. Both missions are to be crewed by experienced astronauts. But not the dearMoon mission, which will carry civilians to the Moon and back on SpaceX hardware.

Back in 2018, a guy named Yusaku Maezawa, owner of a Japanese online fashion retail giant called Zozotown and founder of the local Contemporary Art Foundation, paid an undisclosed fortune to earn the privilege to ride what was then known as the Big Falcon Rocket all the way to the Moon and back.

For a while, Maezawa looked left and right for people to go with him. At one point, he even tried to find a lady friend to accompany him to the stars, but he eventually gave that plan up.

You see, the man did not just pay for his own seat on the rocket (we now call that rocket Starship), but for the entire damn thing. That would be a seat for himself, eight seats for an equal number of civilians, and one or two seats for crew members.

So, a total of at least ten people, the largest number ever sent to space on a single mission, and only a fraction of the planned capacity of 100 humans the Starship should be capable of carrying in Mars-going configuration.

Maezawa himself dubbed his mission dearMoon, and if successful, it will go down in history as the longest (both in terms of distance and time) trip ever taken by civilians, and it will also probably open the doors for true space tourism, not the kind Jeff Bezos and Richard Branson are promising.

In March 2021, Maezawa announced he wants to “give as many talented individuals as possible the opportunity to go” on dearMoon, so he launched a social-media call to arms. By the end of June, the selection of the eight civilians was completed (after combing through some 1 million entries), although we don’t know many of their names yet.

We do know most of them are artists (the Japanese man owns an art foundation, remember?), who will be taken to the sky to find inspiration and create something new.

Although not much news comes out of the dearMoon headquarters, the timeline of the mission shows how throughout next year the civilian crew will be undergoing training in preparation for their trip to the space one year later.

Now, all this dearMoon experiment of course is dependent on the Starship being ready by then. To date, SpaceX has flown only prototypes inside the atmosphere, trying to make the damn thing land properly. They eventually did, and are now planning an orbital flight sometime over the next few weeks.

The ship that will be used for the orbital mission will, of course, not be the one that will go to the Moon. That one will be much larger, offering something on the lines of 35,000 cubic feet (1,000 cubic meters) of pressurized volume, divided into common areas, galley, and a solar storm shelter. For parts of the trip, the people onboard would be wearing the SpaceX spacesuits we all know by now. As per the current details of the dearMoon mission, the entire flight around the Moon should take about six days.

Before he goes to the Moon accompanied by artists, though, Maezawa is scheduled to head to the International Space Station in December this year, after he paid probably another fortune to be taken up there by a company called Space Adventures onboard a Russian Soyuz rocket.

Most detailed-ever images of galaxies revealed using LOFAR

After almost a decade of work, an international team of astronomers has published the most detailed images yet seen of galaxies beyond our own, revealing their inner workings in unprecedented detail. The images were created from data collected by the Low Frequency Array (LOFAR), a radio telescope built and maintained by ASTRON, LOFAR is a network of more than 70,000 small antennae spread across nine European counties, with its core in Exloo, the Netherlands. The results come from the team’s years of work, led by Dr Leah Morabito at Durham University. The team was supported in the UK by the Science and Technology Facilities Council (STFC).


As well as supporting science exploitation, STFC also funds the UK subscription to LOFAR including upgrade costs and operation of its LOFAR station in Hampshire.

PUBLISHED BY THE EDITORIAL TEAM, 17 AUGUST 2021


Revealing a hidden universe of light in HD

The universe is awash with electromagnetic radiation, of which visible light comprises just the tiniest slice. From short-wavelength gamma rays and X-rays, to long-wavelength microwave and radio waves, each part of the light spectrum reveals something unique about the universe.

The LOFAR network captures images at FM radio frequencies that, unlike shorter wavelength sources like visible light, are not blocked by the clouds of dust and gas that can cover astronomical objects. Regions of space that seem dark to our eyes, actually burn brightly in radio waves – allowing astronomers to peer into star-forming regions or into the heart of galaxies themselves.

The new images, made possible because of the international nature of the collaboration, push the boundaries of what we know about galaxies and super-massive black holes. A special issue of the scientific journal Astronomy & Astrophysics is dedicated to 11 research papers describing these images and the scientific results.



A compilation of the science results. Credit from left to right starting at the top: N. Ramírez-Olivencia et el. [radio]; NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), edited by R. Cumming [optical], C. Groeneveld, R. Timmerman; LOFAR & Hubble Space Telescope,. Kukreti; LOFAR & Sloan Digital Sky Survey, A. Kappes, F. Sweijen; LOFAR & DESI Legacy Imaging Survey, S. Badole; NASA, ESA & L. Calcada, Graphics: W.L. Williams.

Better resolution by working together

The images reveal the inner-workings of nearby and distant galaxies at a resolution 20 times sharper than typical LOFAR images. This was made possible by the unique way the team made use of the array.

The 70,000+ LOFAR antennae are spread across Europe, with the majority being located in the Netherlands. In standard operation, only the signals from antennae located in the Netherlands are combined, and creates a ‘virtual’ telescope with a collecting ‘lens' with a diameter of 120 km. By using the signals from all of the European antennae, the team have increased the diameter of the ‘lens’ to almost 2,000 km, which provides a twenty-fold increase in resolution.

Unlike conventional array antennae that combine multiple signals in real time to produce images, LOFAR uses a new concept where the signals collected by each antenna are digitised, transported to central processor, and then combined to create an image. Each LOFAR image is the result of combining the signals from more than 70,000 antennae, which is what makes their extraordinary resolution possible.



This shows real radio galaxies from Morabito et al. (2021). The gif fades from the standard resolution to the high resolution, showing the detail we can see by using the new techniques. Credit: L.K. Morabito; LOFAR Surveys KSP

Revealing jets and outflows from super-massive black holes


Super-massive black holes can be found lurking at the heart of many galaxies and many of these are ‘active’ black holes that devour in-falling matter and belch it back out into the cosmos as powerful jets and outflows of radiation. These jets are invisible to the naked eye, but they burn bright in radio waves and it is these that the new high-resolution images have focused upon.

Dr Neal Jackson of The University of Manchester, said: “These high resolution images allow us to zoom in to see what’s really going on when super-massive black holes launch radio jets, which wasn’t possible before at frequencies near the FM radio band,”

The team’s work forms the basis of nine scientific studies that reveal new information on the inner structure of radio jets in a variety of different galaxies.



Hercules A is powered by a supermassive black hole located at its centre, which feeds on the surrounding gas and channels some of this gas into extremely fast jets. Our new high-resolutions observations taken with LOFAR have revealed that this jet grows stronger and weaker every few hundred thousand years. This variability produces the beautiful structures seen in the giant lobes, each of which is about as large as the Milky Way galaxy. Credit: R. Timmerman; LOFAR & Hubble Space Telescope

A decade-long challenge


Even before LOFAR started operations in 2012, the European team of astronomers began working to address the colossal challenge of combining the signals from more than 70,000 antennae located as much as 2,000 km apart. The result, a publicly-available data-processing pipeline, which is described in detail in one the scientific papers, will allow astronomers from around the world to use LOFAR to make high-resolution images with relative ease.

Dr Leah Morabito of Durham University, said: “Our aim is that this allows the scientific community to use the whole European network of LOFAR telescopes for their own science, without having to spend years to become an expert.”

Super images require supercomputers


The relative ease of the experience for the end user belies the complexity of the computational challenge that makes each image possible. Because LOFAR doesn’t just ‘take pictures’ of the night sky, it must stitch together the data gathered by more than 70,000 antennae, which is a huge computational task. To produce a single image, more than 13 terabits of raw data per second – the equivalent of more than a three hundred DVDs – must be digitised, transported to a central processor and then combined.

Frits Sweijen of Leiden University, said: “To process such immense data volumes we have to use supercomputers. These allow us to transform the terabytes of information from these antennas into just a few gigabytes of science-ready data, in only a couple of days.”

Media

All images and video's belonging to this press release can be found in high resolution here.

Links to Arxiv (free) papers can be found here.


About LOFAR

The International LOFAR Telescope is a trans-European network of radio antennas, with a core located in Exloo in the Netherlands. LOFAR works by combining the signals from more than 70,000 individual antenna dipoles, located in ‘antenna stations’ across the Netherlands and in partner European countries. The stations are connected by a high-speed fibre optic network, with powerful computers used to process the radio signals in order to simulate a trans-European radio antenna that stretches over 1,300 kilometres. The International LOFAR Telescope is unique, given its sensitivity, wide field-of-view, and image resolution or clarity. The LOFAR data archive is the largest astronomical data collection in the world.

LOFAR was designed, built and is presently operated by ASTRON, the Netherlands Institute for Radio Astronomy. France, Germany, Ireland, Italy, Latvia, the Netherlands, Poland, Sweden and the UK are all partner countries in the International LOFAR Telescope.

Breathtaking New Images Reveal Several Distant Galaxies in Unprecedented Detail


Hercules A. (R. Timmerman; LOFAR & Hubble Space Telescope)

SPACE
MICHELLE STARR
19 AUGUST 2021

A telescope network that has spent years staring into deep space has finally delivered some of the most gloriously detailed images we've ever seen of other galaxies.

Not only are these images spectacularly beautiful, they reveal in unprecedented detail the inner workings of these giant cosmic objects, giving us new insight into how galaxies work in general. The findings made so far have been published in a special issue of Astronomy & Astrophysics.


The observations were made using the Low Frequency Array (LOFAR), the largest low-frequency radio telescope network currently operating on Earth. It can combine observations from around 70,000 antennas spread across Europe using a technique called radio interferometry to take some of the most sensitive radio observations possible of the night sky.

This has given us some incredible new information about the Universe, but the new observations are taking it a step further, with a resolution 20 times higher than usual. This is because standard LOFAR operations are conducted only using the antennas in the Netherlands, where the collaboration is headquartered.


Above: Radio imaging reveals a huge wind blowing from merging galaxies. (N. Ramírez-Olivencia et al.; NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans
 (UVA Charlottesville/NRAO/Stony Brook University); R. Cumming)

Since these antennas are spread across a region of 120 kilometers (75 miles), this means the telescope 'aperture' is, effectively, around 120 kilometers in size. For the new observations, an international collaboration used the entire array from across Europe - effectively, a 2,000-kilometer (1,243-mile) radio telescope.


"Our aim is that this allows the scientific community to use the whole European network of LOFAR telescopes for their own science, without having to spend years to become an expert," said astronomer Leah Morabito of Durham University in the UK.

Nine papers in the special issue of Astronomy & Astrophysics are devoted to one of the most amazing phenomena associated with galactic behavior - relativistic particle jets blasted out into intergalactic space by active supermassive black holes at the centers of galaxies.

(A. Kappes)

These are invisible in optical wavelengths, but in radio wavelengths, they gleam - which means radio images can give us some insight into how the jets form and propagate.

It's common knowledge that, once anything passes the critical threshold called the event horizon, nothing can escape the gravitational pull of a black hole. But the region around an active black hole is wildly dynamic. Material is spun into a disk that circles the black hole, spooling into it like water down a drain.

From the inner rim of this accretion disk, a small amount of the swirling material is somehow funneled around the outside of the event horizon towards the poles, where it is launched at speeds that are a significant percentage of the speed of light. Scientists believe that the magnetic field lines around the black hole act as a synchrotron, accelerating these particles to produce relativistic speeds.

This is what distant jets look like at super-low frequencies. (C. Groeneveld)

There is a lot we don't understand about this process, however, and the new LOFAR data are helping to fill in the missing pieces.

"These high-resolution images allow us to zoom in to see what's really going on when supermassive black holes launch radio jets, which wasn't possible before at frequencies near the FM radio band," explained astronomer Neal Jackson from The University of Manchester in the UK.

The galaxies analyzed include 3C 293, a galaxy with huge, peculiar radio lobes that suggest interrupted jet flow. The researchers concluded that the galaxy has undergone multiple periods of activity due to jet disruptions and intermittent fueling, suggesting its supermassive black hole has undergone at least one dormant period.

Another paper analyzed light from a galaxy that had traveled more than 11 billion light-years - usually quite challenging to observe in detail at low frequencies.

This observation allowed a probe into why such distant radio galaxies exhibit specific signatures; ultimately, no conclusive answer could be found, but the observation does pave the way for more in the future.

(R. Timmerman; LOFAR & Hubble Space Telescope)

And a probe into the spectacular radio galaxy Hercules A examined ring structures in its radio lobes. These, the researchers concluded, were the result of intermittent strengthening and weakening of the jets, producing the observed structures.

These clues can help us to understand the processes that produce and shape radio jets, but the collected work has much deeper implications. The papers also represent a significant milestone in radio astronomy, demonstrating the capabilities of a network like LOFAR for understanding the mysteries of the Universe.

The series of papers have been published in Astronomy & Astrophysics.

 

Saturn’s rings oscillate to the tune of its large and ‘messy’ core

18 Aug 2021
Saturn rings
Iconic view: Saturn as seen by Cassini in 2010. (Courtesy: NASA/JPL-Caltech/Space Science Institute)

The internal structure of Saturn has been mapped by using data from the Cassini spacecraft to observe seismic oscillations in the planet’s rings. The study reveals that the core is both larger and more diffuse than previously thought.

The research is described in a paper in Nature Astronomy and could improve our understanding of the Saturn’s formation and evolution.

“The conventional picture of Saturn’s interior is of a compact core of rocks and ices that is surrounded by an envelope of hydrogen and helium,” explains the paper’s co-author Christopher Mankovich  who is at the California Institute of Technology (Caltech). “Based on the unique information now available from Cassini ring seismology, we found that this distinction between core and envelope is not so tidy. The transition must be gradual, hence the ‘diffuse’ or ‘dilute’ core.”

Rock and ice

Along with co-author Jim Fuller at Caltech, Mankovich has found a rock and ice-dominated fluid at the centre of the planet. The hydrogen and helium content of the fluid gradually increases, moving outwards from the core as does the fraction of heavier elements.

In addition to discovering the lack of a clear boundary separating the core from the planet’s outer layers, the duo also found that the core is considerably larger than previous models had suggested.

“The diffuse core region to occupies the inner 60% of Saturn by radius, a dramatically larger number than the 10% or 20% expected from conventional models with a neatly separated core and envelope,” explains Mankovich. “At 60% of Saturn’s total radius this is a dramatic departure from previous models for Saturn’s structure, which came as a surprise to both of us. But after a long and careful investigation it does simply seem to be what the data require.”

What separates this latest work from previous studies of Saturn is the unique use of seismology data collected from the rings of Saturn — arguably the gas giant’s most famous feature.

Shaken from the core

Saturn’s rings were first observed by Galileo in 1610. They comprise a multitude of objects made of ice and traces of silicates, ranging in size from microns to metres. The closest ring to the surface of the planet is about 7000 km away, so it might come as a surprise that monitoring this stunning feature can reveal details of the interior of Saturn.

Mankovich explains that this is possible thanks to spiral patterns stirred up in Saturn’s rings by the planet’s gravitational influence and natural oscillations. “The planet itself is constantly ringing at a variety of frequencies, just like a musical instrument has its own rich spectrum of sounds at any given time,” he explains, adding “These oscillations in the planet cause small amounts of mass in the planet to essentially wobble back and forth slightly as a function of time, and this carries over into a wobbling gravitational field that can stir up waves in the rings.”

Saturn’s ring system is sub-divided into separate bands and data from Cassini has revealed dozens of waves in the C ring of Saturn driven by the gas giant’s oscillations. The frequencies of these waves allowed Fuller and Mankovich to better constrain the planet’s interior than previous methods have allowed.

Internal gravity waves

“Typically the interior structures of the outer solar system planets are constrained using their gravity fields, but this information only goes so far, since the gravity measurements are not very sensitive to the deepest parts of the interior,” Mankovich says. “Seismology is a handy and independent way to study the interior, especially at Saturn where the ring waves include those produced by Saturn’s internal gravity waves which inherently probe the deepest parts of the interior. It’s the frequencies of these internal gravity waves that turned out to eliminate many otherwise plausible interior models and let us arrive at our surprising result.”

Mankovich says that when it comes to their approach to mapping Saturn, he and Fuller took considerable inspiration from helioseismology — the use of the Sun’s regular oscillations to model its interior. Despite decades of development in this field and the growth of the related field of asteroseismology, a powerful method of charting the interiors of stars, understanding gas giants with seismology is still no mean feat.

“It’s difficult! This success story never would have happened were it not for the Cassini mission, which orbited Saturn for longer than a decade and collected a wealth of data,” concludes Mankovich. “The crucial next step will be to search for an interior model in which both of these stable regions might coexist, with the aim of explaining the ring seismology, gravity field, and magnetic field simultaneously. The best picture ever for Saturn’s structure is really starting to come into focus.”