Monday, April 20, 2026

 

The 2040 milestones that Europe must meet to achieve climate-neutrality by 2050





Potsdam Institute for Climate Impact Research (PIK)





Energy, transport, heating and industrial transition: a major modelling study now provides EU-wide guidance with high sector detail on the required pace of transition to fossil-free technologies. The conclusion is encouraging: the EU Green Deal is realistic, and it will ultimately make the continent stronger and more independent from oil and gas crises. The study was conducted at the Potsdam Institute for Climate Impact Research (PIK) and published in Nature Communications.

To understand the scope for useful policy measures, the research team focuses on how the EU can achieve its 2050 climate neutrality target at minimal cost. It draws on the accurate energy–economy–climate model REMIND, runs through a reference scenario – based on assumptions deemed to be most plausible – and then varies key assumptions: Where does the EU stand in terms of emissions reduction and energy efficiency in 2030? How will the costs of wind and solar power develop by 2050? How available will hydrogen and synthetic fuels be as fossil-free sources of energy? Additionally, how much capacity can the EU create for removing CO₂ from the atmosphere to offset hard-to-avoid residual emissions?

One finding is that the EU climate transition, at minimal cost and under the most plausible scenario assumptions, would require a reduction of 2040 net greenhouse gas emissions by 86 percent, relative to 1990. “This result is grounded in techno-economic optimisation of the EU’s transformation path, without looking at questions of fair global burden-sharing,” says PIK researcher and study co-author Robert Pietzcker. 

The EU climate advisory board had recommended a 90 to 95 percent reduction based on considerations of both what is possible and what is fair globally. In doing so, the board had been drawing, among other things, on preliminary results from scenarios developed for the current study. The recommendation was taken up by the EU Commission’s proposal for a 90 percent reduction target. In order to slightly reduce the pressure on member states, it was allowed that 5 percent reductions can come from projects outside the EU. “Our results now show that the resulting 85 percent EU-internal reductions are in line with a cost-effective transition to climate neutrality,” explains Pietzcker. 

Electricity generation from wind and solar must increase seven-fold

To achieve such a significant emissions reduction within just 14 years, the EU must double down on its achievements until now – having reduced greenhouse gas emissions by 37 percent in 2024, relative to 1990 – and further accelerate the transition. To guide future measures, the research team provides “milestones” for individual sectors by 2040 based on its model analysis. These are shown as a point value (representing the reference scenario under the most plausible assumptions) and as a “sensitivity range” (across the entire set of scenarios with the varied assumptions still deemed to be reasonable).

Two pillars of the transition are the expansion of renewable electricity, and the electrification of energy demands. In the reference pathway to climate neutrality, electricity generation from wind and solar will need to be seven times higher in 2040 than in the period from 2018 to 2022 (sensitivity range: four to eight times higher). The share of electricity in final energy consumption, which was fairly constant at 20 percent in the 2010s, will need to rise to 49 percent by 2040 (range: 45 to 59 percent). 

Although a sevenfold rise in wind and solar electricity by 2040 is ambitious, recent experience indicates that it may well be achievable: the required annual growth rate was already achieved over the period 2021–2025, driven by the policy response to the energy crisis. Similarly for electrification: the EU-wide share of battery-electric vehicles in car sales has increased from 2 percent in 2019 to 19 percent in 2025, with Norway and Denmark reaching sales shares above 80 percent.

Dependence on gas and oil imports falls by 60 percent

The study also provides milestones regarding the capture of CO₂ from the atmosphere and storing it permanently in geological formations – a capability that will be indispensable for climate neutrality, but which has so far been virtually non-existent. Carbon capture and storage capacity must rise by 26 (range: 16 to 30) percent annually between 2030 and 2040, reaching 188 (56 to 257) million tonnes of CO₂ annually

“The path to EU climate neutrality by 2050 is still feasible, as long as the EU now shapes the period up to 2040 with ambitious policies,” says Renato Rodrigues, PIK researcher and lead author of the study. “Successful decarbonisation can make the EU economically stronger and strategically more independent.”

This is because, in the reference scenario of the model analysis, demand for both natural gas and crude oil in 2040 is 60 percent lower than in the period from 2018 to 2022, Rodrigues explains. “Although the EU might still need alternative energy imports – e.g. green hydrogen, ammonia, or e-fuels – the volumes would be much lower than current fossil fuels, reducing the EU’s reliance on off-shore energy producers.” 

 

‘Dancing jets’ from black hole reveal their immense power



New Curtin University-led research has used a radio telescope that spans the Earth to snap images that measure the immense power of jets from black holes.



Curtin University

The strong stellar wind from the supergiant star pushes the jets launched by the black hole away from the star 

image: 

The strong stellar wind from the supergiant star pushes the jets launched by the black hole away from the star. This causes the jet direction to vary as the black hole and the supergiant star move around their orbit.

view more 

Credit: International Centre for Radio Astronomy Research (ICRAR)





New Curtin University-led research has used a radio telescope that spans the Earth to snap images that measure the immense power of jets from black holes, confirming scientists’ theories of how black holes help shape the structure of the Universe.

 

In a paper published in Nature Astronomy, researchers found the power of the jets in Cygnus X-1 – a system comprised of the first confirmed black hole and a supergiant star – was equivalent to the power output of 10,000 Suns.

 

To record the measurement, researchers used an array of linked up telescopes separated by large distances to observe the black hole jets being buffeted by the winds of the star as the black hole moved around its orbit – much like how strong winds on Earth can push around water in a fountain.

 

By knowing the power of the wind and measuring how much the jets were bent, the researchers could determine the instantaneous power of the jets for the first time.

 

In addition, they were able to determine the speed of the black hole’s jets – about half the speed of light, or 150,000 km per second – another measurement that has challenged scientists for decades.

 

The research was led from the Curtin Institute of Radio Astronomy (CIRA) and the Curtin node of the International Centre for Radio Astronomy Research (ICRAR), in collaboration with the University of Oxford.

 

Lead author Dr Steve Prabu, who worked at CIRA at the time of the research and who is now based at the University of Oxford, said researchers were able to make the measurement using a sequence of images of the “dancing jets” – a term he used to describe the jets’ movement pattern as they were repeatedly deflected in different directions by the supergiant star’s powerful winds as the star and black hole moved around their orbits.

 

Dr Prabu said the measurement allowed scientists to understand what fraction of the energy released around black holes could be deposited into the surrounding environment, thereby changing the environment.

 

“A key finding from this research is that about 10 per cent of the energy released as matter falls in towards the black hole is carried away by the jets,” Dr Prabu said.

 

“This is what scientists usually assume in large-scale simulated models of the Universe, but it has been hard to confirm by observation until now.”

 

Co-author Professor James Miller-Jones, from CIRA and the Curtin node of ICRAR, said previous methods could only measure the average jet power over thousands or even millions of years, preventing accurate comparisons with the X-ray energy released instantaneously from the infalling matter.

 

"And because our theories suggest that the physics around black holes is very similar, we can now use this measurement to anchor our understanding of jets, whether they are from black holes 10 or 10 million times the mass of the Sun," Professor Miller-Jones said.

 

"With radio telescope projects such as the Square Kilometre Array Observatory currently under construction in Western Australia and South Africa, we expect to detect jets from black holes in millions of distant galaxies, and the anchor point provided by this new measurement will help calibrate their overall power output.

 

“Black hole jets provide an important source of feedback to the surrounding environment and are critical to understanding the evolution of galaxies.”

 

Other collaborating institutions included the University of Barcelona, the University of Wisconsin-Madison, the University of Lethbridge and the Institute of Space Science.

 

The paper, ‘A jet bent by a stellar wind in the black hole X-ray binary Cygnus X-1’, published in journal Nature Astronomy, can be found here.


Artist’s impression of the Cygnus X-1 binary system [VIDEO] 


The direction of the radio jet changes as the black hole and the star move around their orbit 

The direction of the radio jet changes as the black hole and the star move around their orbit (shown in red).

Credit

International Centre for Radio Astronomy Research (ICRAR)

 

Ancient viruses serving as gene delivery couriers to help bacteria resist antibiotics




John Innes Centre

Caulobacter crescentus bacterial host cells producing GTA particles 

image: 

Left: fluorescence microscopy showing C. crescentus bacterial cells producing GTA particles (cells have been engineered to glow green when producing GTAs). Right: cryo-electron microscopy tomogram showing a ‘cross-section’ through a single C. crescentus cell producing GTA particles (magenta and yellow). Bacterial envelope layers are shown in blue, cyan, and green. A nutrient storage granule is visible (grey). Ribosomes (protein factories) are shown in orange.

view more 

Credit: Dr Emma Banks





Research has shed important new light on the enemies-turned-allies that allow bacteria to exchange genes, including those linked to antimicrobial resistance (AMR).   

 

The insights, which expand our understanding of the major global health threat of AMR, came as John Innes Centre researchers investigated the curious phenomena of gene transfer agents (GTAs).   

These gene-carrying particles look like bacteriophages (viruses that infect bacteria), but they have been domesticated from ancient viruses and put to beneficial use under the control of the bacterial host cell.  

Acting as couriers, they take up parcels of host bacterial DNA and deliver them to neighbouring bacteria. This “selfless” sharing, known as horizontal gene transfer, can rapidly spread useful traits including genes that confer resistance to antibiotic drugs used to treat infections. 

A crucial GTA life stage is host cell lysis: the breaking down of a host cell to release DNA-packed GTA particles. Previously, it was unclear how GTA particles escape their host bacterial cells. 

In this study, which appears in Nature Microbiology, the team used a deep sequencing-based screening method to identify genes critical for GTA function in the model bacterium Caulobacter crescentus.  

This identified a three-gene control hub, LypABC, encoding bacterial proteins. When these lypABC genes were deleted, bacteria could no longer lyse to release GTA particles. In contrast, by overexpressing the lypABC hub they obtained a very high proportion of lysing cells. Together, these experiments identified LypABC as a control mechanism for GTA-mediated cell lysis.  

Surprisingly, LypABC resembles a bacterial anti-phage immune system since it contains protein domains which are typically required for defence against viruses. However, this collaborative effort between the John Innes Centre, the University of York, and the Rowland Institute at Harvard, suggests it has been repurposed to release GTA particles for gene transfer.  

They also identified a regulatory protein which is required for strict control of both GTA activation and GTA-mediated lysis. This control is important as misregulation of LypABC is highly toxic to bacterial cells.  

In highlighting the plasticity of bacterial domains, the study advances fundamental knowledge of how gene transfer occurs between bacterial cells and offers an important clue to understanding how AMR occurs.  

First author of the study Dr Emma Banks, a Royal Commission for the Exhibition of 1851 Research Fellow, said: “What’s particularly interesting is that LypABC looks like an immune system, yet bacteria are using it to release GTA particles. It suggests that immune systems can be repurposed to help bacteria share DNA with each other - a process that can contribute to the spread of antibiotic resistance.” 

The next step for the research is to discover how the LypABC control hub is activated and how it functions to control the rupture of bacterial cells and release of GTA particles. 

“A bacterial CARD-NLR-like immune system controls the release of gene transfer agents”, appears in Nature Microbiology.  

 

 

How gut bacteria and acute stress are linked


Possible avenue for new strategies related to acute stress responses and stress-related conditions




University of Vienna





The gut microbiome influences numerous physiological processes. Researchers at the University of Vienna have now demonstrated for the first time that, in healthy adults, the diversity of gut bacteria and their capacity to produce certain metabolites are associated with the acute stress response - particularly stress reactivity. Higher microbial diversity was associated with stronger hormonal and subjectively perceived stress reactivity. The results suggest that the gut microbiome may play a role in regulating the acute stress response. The study was published in Neurobiology of Stress.

The gut microbiome comprises all microorganisms living in the gut, which, among other things, perform important functions in metabolism and the immune system and are also connected to the brain through various pathways. Research suggests they can modulate the stress response. However, it has remained unclear until now whether differences in the human gut microbiome are actually associated with acute stress reactivity.

The latest findings by researchers Thomas Karner, Isabella Wagner, David Berry, and Paul Forbes from the Faculty of Psychology and the Center for Microbiology and Environmental Systems Sciences (CeMESS) at the University of Vienna provide new evidence that the gut microbiome, and thus potentially also diet and lifestyle, is associated with how our bodies respond to stress. In the long term, targeted modulation of gut microbial composition and its metabolites, particularly short-chain fatty acids, could represent a possible avenue for new strategies to related to acute stress responses, stress-related conditions and improve well-being.

Stress tests, saliva samples, and more provide insight into the association

In the study, healthy participants either underwent a standardized stress test or performed a comparable, stress-free task. Stress hormones (cortisol) in saliva and subjective stress levels were measured. In addition, the gut microbiome was analyzed using stool samples. Both the composition of the microbiome and the estimated production capacity of short-chain fatty acids were examined. The results show that higher microbial diversity was associated with higher hormonal and subjective stress reactivity. Greater microbial diversity is often associated with a more stable and resilient microbial ecosystem and with greater functional flexibility, which may contribute to the appropriate regulation of stress responses.

"A stronger acute stress response is not necessarily detrimental. Appropriate activation of the stress system enables flexible adaptation to challenges and threats. A greater diversity of gut bacteria, as well as certain metabolic products, could play a supportive role in this process," explains study leader and psychologist Thomas Karner.

Complex relationship between microbial metabolites and stress reactivity

Furthermore, stress reactivity was associated with gut bacteria’s capacity to produce different metabolic products: a higher estimated capacity for butyrate production was associated with higher stress reactivity, whereas higher propionate production was associated with lower reactivity. Butyrate and propionate are short-chain fatty acids produced by gut bacteria that are involved in metabolic and immune processes and can also affect the brain. This suggests that the relationship between microbial metabolites and the acute stress response is more complex and cannot be reduced to a single direction.

The results provide new insights into possible biological mechanisms of stress regulation and underscore the role of the gut microbiome and its metabolites as potential factors influencing the stress system and the acute stress response in humans.

Summary:

  • Higher gut microbial diversity is associated with higher hormonal and subjective stress reactivity in healthy adults
  • Estimated capacity for short-chain fatty acid production is associated with hormonal stress reactivity. Higher butyrate production is associated with higher stress reactivity, while higher propionate production is associated with lower stress reactivity
  • The findings demonstrate an association between the gut microbiome and acute stress, as well as the possible role of the gut microbiome as a factor influencing the stress system
  • In the long term, changes in the gut microbiome and its metabolites, for example, through diet or targeted interventions, could represent a possible approach to influencing stress responses and stress-related conditions

About the University of Vienna: 

At the University of Vienna, curiosity has been the core principle of academic life for more than 650 years. For over 650 years the University of Vienna has stood for education, research and innovation. Today, it is ranked among the top 100 and thus the top four per cent of all universities worldwide and is globally connected. With degree programmes covering over 180 disciplines, and more than 10,000 employees we are one of the largest academic institutions in Europe. Here, people from a broad spectrum of disciplines come together to carry out research at the highest level and develop solutions for current and future challenges. Its students and graduates develop reflected and sustainable solutions to complex challenges using innovative spirit and curiosity.

You can find out more about stress here in the special feature Don't stress! in the University of Vienna’s science magazine Rudolphina.

 

Closing the carbon cycle: Unraveling the roles of light and heat in CO2 photocatalysis



Researchers reveal how photocatalytic and photothermal processes work together to enhance CO2-to-CH4 conversion




Chiba University

Clarifying the Differences in Reaction Pathways for Photocatalytic Carbon Dioxide (CO2) Reduction 

image: 

Photocatalytic reduction test of CO2 using Ru–Ni–ZrO2 catalyst when the reactor was cooled with liquid (left) and when the reactor was not cooled (right).

view more 

Credit: Professor Yasuo Izumi from Chiba University, Japan





Rising carbon dioxide (CO2) emissions from human activities are the largest contributor to global warming. According to the International Energy Agency (IEA), global CO₂ emissions reached an all-time high of 37.8 gigatons in 2024. While some of this CO2 is absorbed by soil, forests, and the oceans, a large fraction remains in the atmosphere, where it can persist for hundreds to thousands of years, leading to long-term impacts on the global climate.

To address this challenge, scientists are exploring ways to convert CO2 into useful fuels, creating a closed carbon cycle. One promising approach is photocatalytic reduction, in which CO2 is converted into methane using a catalyst powered by sunlight. However, the efficiency of this process is still too low for practical use. A key difficulty lies in understanding how the reaction occurs—whether it is driven by true photocatalytic processes involving light-induced electron excitation, or by heat generated from light, known as the photothermal effect.

Now, a team led by Professor Yasuo Izumi at the Graduate School of Science at Chiba University, Japan, has elucidated these pathways. Their study, available online on March 20, 2026, and published in Volume 148, Issue 13 of the Journal of the American Chemical Society on April 8, 2026, achieved one of the highest reported rates of CO2-to-methane conversion to date, reaching up to 10 millimoles per gram of catalyst per hour. By clarifying the underlying reaction mechanisms, their work provides important insights that could guide the design of more efficient catalysts for COconversion.

The team included first author Masahito Sasaki, along with Tomoki Oyumi and Dr. Keisuke Hara from the Graduate School of Science and Engineering, Chiba University, and Associate Professor Hongwei Zhang from the Biogas Institute of the Ministry of Agriculture and Rural Affairs, China (and a former Ph.D. student at Chiba University).

Prof. Izumi explains the current challenge: “The true reaction pathway and the catalytic role responsible for it remain uncertain in photocatalysis, where charge separation, hot spots, and energetic modulation of ground and excited states are involved.”

To separate photothermal and photocatalytic effects in CO2 reduction, the researchers irradiated Ru–Ni–ZrOand Ni–ZrO2 catalysts with ultraviolet (UV)–visible light at varying intensities from 90 to 900 milliwatts per centimeter square (mW cm−2) while carefully controlling the temperature of the system, either maintaining it at 295 K (22 °C) using a cooling bath or allowing it to increase under irradiation.

Without the cooling bath, the Ru–Ni–ZrO2 catalyst converted CO2 to methane more than 2.7 times faster than the Ni–ZrO2 catalyst, reaching over 7.9 millimoles per gram of catalyst per hour. Under these conditions, the photothermal effects became increasingly dominant. CO2 is directly adsorbed onto Ru–Ni active sites, where it is more easily activated and dissociated into CO and oxygen atom with a low activation energy of 0.45 eV—much lower than the 0.79 eV required on pure nickel.

In contrast, when the cooling bath was applied, the reaction was primarily driven by photocatalytic processes, with some contribution from local heating. Light generates separated electrical charges on the ZrO2 surface, forming intermediate species via OCOH intermediates at oxygen vacancy sites. These intermediates are then transferred to nickel sites, where they undergo multiple hydrogenation steps to form methane. Under these conditions, localized ‘hotspots’ can form on nickel, where temperatures can reach 126 °C under strong irradiation (654 mW cm−2). At these sites, the methane formation rate is 1.72 times higher than expected from simple thermal reactions, showing that both charge separation and local heating work together.

Together, these findings show that CO2 reduction depends on a balance between photocatalytic and photothermal processes, with their relative contributions determined by temperature and light intensity. By clearly identifying how these mechanisms interact, the study provides a deeper understanding of light-driven CO2 conversion and offers a pathway toward designing more efficient catalysts.

The researchers aim to further expand this approach to produce more complex and valuable chemicals. “Going forward, we aim to further enhance the efficiency of sustainable CO2 utilization technologies using sunlight, such as the synthesis of C2 and C3 compounds and alcohols,” says Prof. Izumi.

To see more news from Chiba University, click here.

 

***

Reference:
DOI: 10.1021/jacs.5c17533

Authors: Masahito Sasaki1, Tomoki Oyumi1, Keisuke Hara1, Hongwei Zhang2, and Yasuo Izumi1

Affiliations: 1Department of Chemistry, Graduate School of Science, Chiba University, Japan

2Key Laboratory of Development and Application of Rural Renewable Energy, Biogas Institute of Ministry of Agriculture and Rural Affairs, the People’s Republic of China

 

About Professor Yasuo Izumi from Chiba University, Japan
Professor Yasuo Izumi is a faculty member at the Graduate School of Science, Chiba University, Japan, studying catalytic processes on solid surfaces. His research focuses on complex reaction pathways using advanced analytical techniques to design efficient catalysts for a sustainable society. He earned his Doctor of Science from the University of Tokyo (1993), with work on supported metal cluster catalysts. Prof. Izumi’s recent research explores the photocatalytic conversion of CO₂ into fuels and valuable resources. He is a member of several scientific societies, including the Chemical Society of Japan and the American Chemical Society, and has authored over 100 publications.

 

Funding:
The study received financial support for Scientific Research B (grant numbers: 24K01522 and 20H02834) from the Japan Society for the Promotion of Science. X-ray absorption experiments were performed with the approval of the Photon Factory Proposal Review Committee (grant numbers: 2022G527, 2021G546, 2020G676, and 2019G141).