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HKU Science Scholars Rank Among World’s Top 10 in Their Fields in Stanford’s 2026 List

More than 40 current Faculty members of the Faculty of Science at the University of Hong Kong (HKU) have been recognised in Stanford University's 2026 Top 2% Scientists List, with several ranking among the world's top 10 in their fields.  In the 2026 rankings, Professor Bing Zhang, Global STEM Scholar and Chair of Astrophysics in the Department of Physics, ranked 4th globally in Astronomy & Astrophysics. Professor Guochun Zhao, Mok Sau-King Professor and Chair of Earth Sciences in the Department of Earth and Planetary Sciences, secured 6th place globally in Geochemistry and Geophysics. Professor Peng Gong, Vice-President and Pro-Vice-Chancellor (Academic Development) and Chair of Global Sustainability, with appointments in the Department of Geography and the Department of Earth and Planetary Sciences, ranked 9th globally in Geological and Geomatics Engineering. In the global career-long impact ranking, Professor Guochun Zhao also ranked 6th globally in Geochemistry and Geophysics, reflecting his sustained contributions to the field. Professor Hongjie Dai, Sapientia Eminence Professor and Chair of Chemistry in the Department of Chemistry, ranked 9th globally in Nanoscience and Nanotechnology. These achievements form part of HKU's outstanding performance, with 597 scholars recognised across the University. HKU recorded the highest number of scholars among local universities in both the "single-year impact" and "career-long impact" categories, with 502 and 406 scholars respectively. Stanford University's Top 2% Scientists List recognises influential researchers across scientific disciplines based on their research impact. The latest results underscore the breadth and strength of HKU Science's contributions to scientific research worldwide.

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Figure 1. Conceptual model of coastal groundwater phosphorus driving the global acceleration of algal blooms. Image credit: Cheng et al., Nature Communications (2026), CC BY 4.0.

Hidden phosphorus in coastal groundwater fuels global rise in algal blooms

Professor Jiu Jimmy JIAO and Dr Xin LUO from the HKU Department of Earth and Planetary Sciences, together with Dr Kaihao CHENG from the Chinese University of Hong Kong, have published a research paper in Nature Communications titled “Coastal groundwater phosphorus drives global acceleration of algal blooms”. The study reveals that excessive dissolved inorganic phosphorus (DIP) in coastal groundwater is a long-overlooked key driver of the global acceleration of coastal algal blooms (CABs), providing a new scientific basis for understanding the ecological paradox of worsening algal blooms despite nitrogen control measures. Coastal algal blooms pose significant threats to marine ecosystems, fisheries, and human health, causing billions of dollars in economic losses worldwide each year. Although many regions have reduced nitrogen inputs over the past decades in an effort to curb blooms, their frequency and intensity have continued to rise, creating a well-known “ecological paradox”. To investigate this paradox, the study combined a process-oriented physical-chemical framework with a global multi-decadal dataset, systematically analysing coastal chlorophyll-a concentrations, nutrients, and water column stability from 1998 to 2022. The analysis covered 237,540 coastal sites worldwide and integrated 1,533 paired groundwater-seawater DIP observations from 140 coastal groundwater sites. The study found that phosphorus, rather than nitrogen or physical water conditions, was most closely linked to the worsening of coastal algal blooms worldwide. While dissolved inorganic nitrogen (DIN) declined over the study period, dissolved inorganic phosphorus (DIP) continued to rise, driving down the N:P ratio and creating conditions that favour algal blooms. Among the factors examined, chlorophyll-a showed the strongest correlation with DIP (r=0.74). The researchers further traced this excess phosphorus to coastal groundwater. Their global analysis showed a strong link between groundwater and adjacent seawater DIP levels, revealing that groundwater can deliver phosphorus-rich, nitrogen-poor nutrients to coastal waters. In oxygen-depleted aquifers, phosphorus is released from iron oxides while denitrification removes nitrogen, producing groundwater with a particularly low N:P ratio. High-resolution observations from Hong Kong and Delaware Bay provided further evidence: pulses of groundwater phosphorus occurred shortly before algal bloom events, temporarily pushing seawater N:P ratios below 16 and creating favourable conditions for blooms. The researchers describe this combined spatial and temporal control as a “spatio-temporal gating” mechanism, which helps explain why coastal algal blooms can continue to intensify even as nitrogen pollution declines. The study establishes a new mechanistic framework linking groundwater, nutrient balance, and algal blooms, challenging the traditional focus on surface nutrient inputs alone. The findings show that even when surface nitrogen inputs are reduced, groundwater can continue to deliver dissolved inorganic phosphorus (DIP) to coastal waters and sustain algal blooms. The researchers therefore highlight the need to incorporate groundwater flow and aquifer redox conditions into future monitoring and management strategies. Aquifer redox state may also indicate regional vulnerability, particularly as climate change and human activities could drive more aquifers toward reductive conditions and increase the risk of phosphorus-driven blooms. The study further calls for incorporating groundwater DIP and its redox-driven release mechanisms into the next generation of coastal biogeochemical models, which currently tend to overlook the role of groundwater nutrient stoichiometry. The first author, Dr Kaihao Cheng, graduated from the research group of Professor Jiu Jimmy Jiao at The University of Hong Kong and is currently a Research Assistant Professor in the School of Life Sciences at the Chinese University of Hong Kong. The co-corresponding authors are Dr Kaihao Cheng (CUHK), Professor Jiu Jimmy Jiao (HKU), Professor Jin Wu (HKU), and Dr Xin Luo (HKU). Collaborative institutions include the Chinese University of Hong Kong, the University of Hong Kong, the Macau University of Science and Technology, the University of California, Santa Cruz, the Woods Hole Oceanographic Institution, the University of Delaware, and Hainan University. This study was supported by multiple research funds. Click here to read the journal paper.     

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HKU and BNU Astrophysicists Use Wave Simulations to Open a New Window on Dark Matter

Figure 1. Artist’s impression illustrating how wave-like density patterns produced by ultralight dark matter could warp space and alter the path of light from a distant source. As the light travels past the lensing object on its way to Earth, it follows a distorted path shaped by the surrounding mass distribution. The reflective sphere symbolises the still-unknown nature of dark matter. The image was created using 3D computer graphics software. (Photo courtesy: Amruth Alfred)   Astrophysicists from The University of Hong Kong (HKU), working with a research team led by Beijing Normal University (BNU), have developed a more physically realistic approach to testing how ultralight, or “fuzzy”, dark matter could influence gravitationally lensed images. The study is the first to make gravitational-lensing predictions directly from three-dimensional wave simulations of fuzzy dark matter. The simulations reproduce the observed image positions of a well-studied lensed quasar more closely than commonly used modelling approaches, highlighting the potential of high-resolution gravitational-lensing observations to probe the nature of dark matter. The findings of this research study have been published in The Astrophysical Journal Letters.   For nearly a century, physicists have grappled with the mystery of dark matter, a substance thought to comprise 85% of all matter in the Universe. Despite its prevalence, it does not emit, absorb or reflect light and is detected through its gravitational effects. Dark matter is also absent from the Standard Model of particle physics, our currently accepted framework for describing the fundamental particles and three of the four fundamental forces of the Universe, a framework that underpins much of modern technology.   Over the past decade, growing astronomical evidence has raised the possibility that dark matter may consist of ultralight particles. Owing to their extremely low masses, these particles can behave collectively like waves, producing complex interference patterns similar to those formed when waves meet on a beach. Such patterns could leave traces in multiple images of galaxies, which arise when the gravity of a massive object bends and distorts light from a more distant source, as predicted by Einstein's theory of gravity.   In the quest to unravel the mystery of dark matter, the research team, including Professor Jeremy Lim and Dr Amruth Alfred from HKU’s Department of Physics and The Hong Kong Institute of Astronomy and Astrophysics (HKIAA), made predictions for the properties of gravitationally lensed images if galaxies are indeed composed of ultralight dark matter. This is the first time such predictions have been made using direct computer simulations to accurately capture the wave-like mass patterns produced by interactions between ultralight particles. The simulations reproduced the observed positions of the lensed images more closely than the comparison models used in the study. The results suggest that gravitationally lensed systems could provide a way to test ultralight-dark-matter models. The researchers are now investigating other effects, including changes in the brightness of gravitationally lensed images.   The project grew out of research visits by the HKU researchers to BNU, where they collaborated closely with members of Professor Zong-Hong Zhu’s group, Dr Zhengxiang Li and PhD student Jiajun Zhou, the lead author of the study. "We were very excited to see what the simulations predicted as we did not know beforehand what observable signatures to expect. Jiajun worked very hard to rapidly get out these remarkable results and we believe this has opened entirely new avenues for future research on the nature of Dark Matter using lensing."   These visits were supported by multiple research grants and awards and helped lay the groundwork for the collaboration. The recent inauguration of HKIAA at HKU has set the stage for closer collaboration with colleagues in the Chinese Mainland and will open the doors to further cutting-edge astrophysics research.   For details of the research, please refer to the journal paper “Gravitational Lensing Predictions from Wave Simulations of Fuzzy Dark Matter”; DOI: 10.3847/2041-8213/ae9a9e

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HKU Science Scholars Rank Among World’s Top 10 in Their Fields in Stanford’s 2026 List

More than 40 current Faculty members of the Faculty of Science at the University of Hong Kong (HKU) have been recognised in Stanford University's 2026 Top 2% Scientists List, with several ranking among the world's top 10 in their fields.  In the 2026 rankings, Professor Bing Zhang, Global STEM Scholar and Chair of Astrophysics in the Department of Physics, ranked 4th globally in Astronomy & Astrophysics. Professor Guochun Zhao, Mok Sau-King Professor and Chair of Earth Sciences in the Department of Earth and Planetary Sciences, secured 6th place globally in Geochemistry and Geophysics. Professor Peng Gong, Vice-President and Pro-Vice-Chancellor (Academic Development) and Chair of Global Sustainability, with appointments in the Department of Geography and the Department of Earth and Planetary Sciences, ranked 9th globally in Geological and Geomatics Engineering. In the global career-long impact ranking, Professor Guochun Zhao also ranked 6th globally in Geochemistry and Geophysics, reflecting his sustained contributions to the field. Professor Hongjie Dai, Sapientia Eminence Professor and Chair of Chemistry in the Department of Chemistry, ranked 9th globally in Nanoscience and Nanotechnology. These achievements form part of HKU's outstanding performance, with 597 scholars recognised across the University. HKU recorded the highest number of scholars among local universities in both the "single-year impact" and "career-long impact" categories, with 502 and 406 scholars respectively. Stanford University's Top 2% Scientists List recognises influential researchers across scientific disciplines based on their research impact. The latest results underscore the breadth and strength of HKU Science's contributions to scientific research worldwide.

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Figure 1. Conceptual model of coastal groundwater phosphorus driving the global acceleration of algal blooms. Image credit: Cheng et al., Nature Communications (2026), CC BY 4.0.

Hidden phosphorus in coastal groundwater fuels global rise in algal blooms

Professor Jiu Jimmy JIAO and Dr Xin LUO from the HKU Department of Earth and Planetary Sciences, together with Dr Kaihao CHENG from the Chinese University of Hong Kong, have published a research paper in Nature Communications titled “Coastal groundwater phosphorus drives global acceleration of algal blooms”. The study reveals that excessive dissolved inorganic phosphorus (DIP) in coastal groundwater is a long-overlooked key driver of the global acceleration of coastal algal blooms (CABs), providing a new scientific basis for understanding the ecological paradox of worsening algal blooms despite nitrogen control measures. Coastal algal blooms pose significant threats to marine ecosystems, fisheries, and human health, causing billions of dollars in economic losses worldwide each year. Although many regions have reduced nitrogen inputs over the past decades in an effort to curb blooms, their frequency and intensity have continued to rise, creating a well-known “ecological paradox”. To investigate this paradox, the study combined a process-oriented physical-chemical framework with a global multi-decadal dataset, systematically analysing coastal chlorophyll-a concentrations, nutrients, and water column stability from 1998 to 2022. The analysis covered 237,540 coastal sites worldwide and integrated 1,533 paired groundwater-seawater DIP observations from 140 coastal groundwater sites. The study found that phosphorus, rather than nitrogen or physical water conditions, was most closely linked to the worsening of coastal algal blooms worldwide. While dissolved inorganic nitrogen (DIN) declined over the study period, dissolved inorganic phosphorus (DIP) continued to rise, driving down the N:P ratio and creating conditions that favour algal blooms. Among the factors examined, chlorophyll-a showed the strongest correlation with DIP (r=0.74). The researchers further traced this excess phosphorus to coastal groundwater. Their global analysis showed a strong link between groundwater and adjacent seawater DIP levels, revealing that groundwater can deliver phosphorus-rich, nitrogen-poor nutrients to coastal waters. In oxygen-depleted aquifers, phosphorus is released from iron oxides while denitrification removes nitrogen, producing groundwater with a particularly low N:P ratio. High-resolution observations from Hong Kong and Delaware Bay provided further evidence: pulses of groundwater phosphorus occurred shortly before algal bloom events, temporarily pushing seawater N:P ratios below 16 and creating favourable conditions for blooms. The researchers describe this combined spatial and temporal control as a “spatio-temporal gating” mechanism, which helps explain why coastal algal blooms can continue to intensify even as nitrogen pollution declines. The study establishes a new mechanistic framework linking groundwater, nutrient balance, and algal blooms, challenging the traditional focus on surface nutrient inputs alone. The findings show that even when surface nitrogen inputs are reduced, groundwater can continue to deliver dissolved inorganic phosphorus (DIP) to coastal waters and sustain algal blooms. The researchers therefore highlight the need to incorporate groundwater flow and aquifer redox conditions into future monitoring and management strategies. Aquifer redox state may also indicate regional vulnerability, particularly as climate change and human activities could drive more aquifers toward reductive conditions and increase the risk of phosphorus-driven blooms. The study further calls for incorporating groundwater DIP and its redox-driven release mechanisms into the next generation of coastal biogeochemical models, which currently tend to overlook the role of groundwater nutrient stoichiometry. The first author, Dr Kaihao Cheng, graduated from the research group of Professor Jiu Jimmy Jiao at The University of Hong Kong and is currently a Research Assistant Professor in the School of Life Sciences at the Chinese University of Hong Kong. The co-corresponding authors are Dr Kaihao Cheng (CUHK), Professor Jiu Jimmy Jiao (HKU), Professor Jin Wu (HKU), and Dr Xin Luo (HKU). Collaborative institutions include the Chinese University of Hong Kong, the University of Hong Kong, the Macau University of Science and Technology, the University of California, Santa Cruz, the Woods Hole Oceanographic Institution, the University of Delaware, and Hainan University. This study was supported by multiple research funds. Click here to read the journal paper.     

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Artist’s impression of satellites observing high-energy prompt emission from a binary neutron star merger. Image credit: Yi-Han Iris Yin; reference images: EPSC, SVOM collaboration, NSSDC.

HKU PhD Student Reveals New Insights into Hidden X-ray Phase Following a Compact Star Merger

An international team of astronomers, including researchers from the Department of Physics and the Hong Kong Institute for Astronomy and Astrophysics (HKIAA) at The University of Hong Kong (HKU), has discovered a previously hidden phase of high-energy activity following the merger of compact stars. This fleeting cosmic explosion, known as EP250704a in X-rays and GRB 250704B in gamma rays, was jointly captured by the China-led Einstein Probe (EP), the Space Variable Objects Monitor (SVOM) and Insight-Hard X-ray Modulation Telescope (HXMT). EP’s wide-field X-ray telescope detected the event from its onset and continued to observe several episodes of soft X-ray emission after the gamma-ray signal disappeared. While the gamma-ray burst lasted only about 0.4 seconds, the source continued to shine in soft X-rays for nearly ten minutes, revealing a phase of activity that conventional gamma-ray observations would likely have missed. These findings have been published as a cover article in Science Bulletin. How Einstein Probe Revealed the Hidden X-ray Phase Short gamma-ray bursts are commonly associated with the merger of compact objects such as neutron stars. As the two objects spiral together and collide, they release an intense burst of high-energy radiation. Traditionally, astronomers have identified these events mainly through gamma rays. Most X-ray telescopes can only turn to a burst after a gamma-ray detector has first located it, meaning the earliest X-ray emission may already be over by the time observations begin. Einstein Probe changes this picture by continuously monitoring a wide area of the sky at soft X-ray energies. In this case, it revealed that what appeared to be a brief gamma-ray event was accompanied by much longer-lasting X-ray activity. Yi-Han Iris Yin, a PhD student at the HKU Department of Physics and the Hong Kong Institute for Astronomy and Astrophysics (HKIAA), is a co-corresponding author of the study. She led the analysis of the high-energy prompt emission and contributed to the physical interpretation of the event. Yin’s analysis of the X-ray signal revealed key insights into the merger’s aftermath: The source remained active long after the gamma-ray burst. The soft X-ray emission continued for nearly ten minutes after the brief gamma-ray flash. The X-rays point to continued central engine activity. Their rapid variability and changing spectrum indicate that the central engine created by the merger continued to release energy. The remnant may be a magnetar. One possible explanation is a rapidly rotating, highly magnetised neutron star that continued to power the X-ray emission. Similar X-ray activity may have been missed before. This suggests prolonged soft X-ray emission could be more common in compact-object mergers than previously recognised and may provide another way to study gravitational-wave sources. Working with an international team led by An LI of Beijing Normal University (BNU) and Professor Bin-Bin ZHANG of Nanjing University (NJU), the researchers found that similar soft X-ray emission may have been present in previous short gamma-ray bursts but remained undetected because it was too soft and faint for conventional gamma-ray instruments.   “Einstein Probe is allowing us to uncover a part of compact star mergers that was hidden from previous gamma-ray observations,” said Yin. “The short gamma-ray flash may represent only the beginning of the high-energy activity. By observing the Universe at soft X-ray energies, we can now follow these systems for much longer and obtain a more complete view of what happens during and after the merger.” Professor Bing ZHANG, Founding Director of HKIAA and Chair of Astrophysics at HKU Department of Physics, co-authored the study and contributed to the physical interpretation of the event. He has long proposed that binary neutron star mergers could produce fast X-ray transients detectable by missions such as Einstein Probe. Beyond the scientific findings, Professor Zhang highlighted the significance of the study in nurturing young researchers and strengthening international collaboration.   Fostering Young Scientific Leadership “One of our goals at HKIAA is to create an environment where talented young researchers can take on scientific leadership and work at the forefront of international astronomy,” Professor Zhang said. “It is particularly encouraging to see our PhD student Yi-Han Iris Yin taking a leading role as one of the corresponding authors in this international collaboration. Her contribution reflects the quality and potential of the young researchers we are training at HKIAA, and this collaboration also demonstrates how Hong Kong can connect with major scientific facilities and research teams in mainland China and around the world.” International Collaboration The study brought together researchers from HKU, Nanjing University, the University of Rome “Tor Vergata”, the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), the Institute of High Energy Physics of the Chinese Academy of Sciences, and many other institutions worldwide. The co-first authors include BNU’s An Li and colleagues from the Institute of High Energy Physics, the University of Rome “Sapienza”, and the University of Chinese Academy of Sciences. The corresponding authors include NJU’s Professor Bin-Bin Zhang, Professor Eleonora Troja from the University of Rome “Tor Vergata”, HKU’s PhD student Yi-Han Iris Yin, and colleagues from NAOC. About the Missions Einstein Probe (EP) Einstein Probe is a space mission led by the Chinese Academy of Sciences (CAS), with international partners including the European Space Agency (ESA), the Max Planck Institute for Extraterrestrial Physics (MPE) in Germany, and the French National Centre for Space Studies (CNES). Space Variable Objects Monitor (SVOM) SVOM is a China–France joint mission led by the China National Space Administration (CNSA), CNES and CAS. It observes gamma-ray bursts and other transient phenomena in the high-energy Universe. Insight-HXMT Insight-HXMT is China’s first space X-ray telescope and was jointly funded by CNSA and CAS. For details, please refer to the journal paper “Minutes-long soft X-ray prompt emission from a compact object merger” published in Science Bulletin.  

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HKU and BNU Astrophysicists Use Wave Simulations to Open a New Window on Dark Matter

Figure 1. Artist’s impression illustrating how wave-like density patterns produced by ultralight dark matter could warp space and alter the path of light from a distant source. As the light travels past the lensing object on its way to Earth, it follows a distorted path shaped by the surrounding mass distribution. The reflective sphere symbolises the still-unknown nature of dark matter. The image was created using 3D computer graphics software. (Photo courtesy: Amruth Alfred)   Astrophysicists from The University of Hong Kong (HKU), working with a research team led by Beijing Normal University (BNU), have developed a more physically realistic approach to testing how ultralight, or “fuzzy”, dark matter could influence gravitationally lensed images. The study is the first to make gravitational-lensing predictions directly from three-dimensional wave simulations of fuzzy dark matter. The simulations reproduce the observed image positions of a well-studied lensed quasar more closely than commonly used modelling approaches, highlighting the potential of high-resolution gravitational-lensing observations to probe the nature of dark matter. The findings of this research study have been published in The Astrophysical Journal Letters.   For nearly a century, physicists have grappled with the mystery of dark matter, a substance thought to comprise 85% of all matter in the Universe. Despite its prevalence, it does not emit, absorb or reflect light and is detected through its gravitational effects. Dark matter is also absent from the Standard Model of particle physics, our currently accepted framework for describing the fundamental particles and three of the four fundamental forces of the Universe, a framework that underpins much of modern technology.   Over the past decade, growing astronomical evidence has raised the possibility that dark matter may consist of ultralight particles. Owing to their extremely low masses, these particles can behave collectively like waves, producing complex interference patterns similar to those formed when waves meet on a beach. Such patterns could leave traces in multiple images of galaxies, which arise when the gravity of a massive object bends and distorts light from a more distant source, as predicted by Einstein's theory of gravity.   In the quest to unravel the mystery of dark matter, the research team, including Professor Jeremy Lim and Dr Amruth Alfred from HKU’s Department of Physics and The Hong Kong Institute of Astronomy and Astrophysics (HKIAA), made predictions for the properties of gravitationally lensed images if galaxies are indeed composed of ultralight dark matter. This is the first time such predictions have been made using direct computer simulations to accurately capture the wave-like mass patterns produced by interactions between ultralight particles. The simulations reproduced the observed positions of the lensed images more closely than the comparison models used in the study. The results suggest that gravitationally lensed systems could provide a way to test ultralight-dark-matter models. The researchers are now investigating other effects, including changes in the brightness of gravitationally lensed images.   The project grew out of research visits by the HKU researchers to BNU, where they collaborated closely with members of Professor Zong-Hong Zhu’s group, Dr Zhengxiang Li and PhD student Jiajun Zhou, the lead author of the study. "We were very excited to see what the simulations predicted as we did not know beforehand what observable signatures to expect. Jiajun worked very hard to rapidly get out these remarkable results and we believe this has opened entirely new avenues for future research on the nature of Dark Matter using lensing."   These visits were supported by multiple research grants and awards and helped lay the groundwork for the collaboration. The recent inauguration of HKIAA at HKU has set the stage for closer collaboration with colleagues in the Chinese Mainland and will open the doors to further cutting-edge astrophysics research.   For details of the research, please refer to the journal paper “Gravitational Lensing Predictions from Wave Simulations of Fuzzy Dark Matter”; DOI: 10.3847/2041-8213/ae9a9e

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Giving Scientific Creativity Room to Thrive

  An international research team, including Emeritus Professor David Dudgeon from HKU’s School of Biological Sciences, warns that short-term funding, precarious career pathways and mounting publication pressures are making it increasingly difficult for scientists to pursue high-risk, innovative research. These pressures may not only slow scientific progress, but also place a disproportionate burden on early-career researchers and ultimately narrow the pool of motivated, creative scientists who remain in academia.   Recent controversies surrounding plagiarism allegations, data fabrication, and AI usage have put an uncomfortable question in the spotlight: are modern academic systems getting better at identifying genuinely original thinkers, or merely better at rewarding those who learn how to succeed within the system? In a new Perspective article published in Nature Human Behaviour, a global team of researchers reviews how funding, peer review, publishing costs, employment insecurity, and academic hierarchies can favour safe and predictable research over bold ideas that challenge established thinking. They argue that contemporary academic systems systematically discourage high-risk, innovative research and place the greatest burden on early-career researchers.     Modern science increasingly depends on short-term funding cycles, productivity-based evaluation and intense competition for permanent positions. At the same time, major scientific advances often require intellectual freedom, tolerance of uncertainty, sufficient time and the possibility of failure. The researchers argue that this conflict particularly affects early-career researchers whose employment, funding, publications and future careers largely depend on decisions made by more established academics and institutions. Concomitantly, the number of PhD graduates and postdoctoral researchers has grown faster than the availability of stable academic positions in many systems. Peer review and research funding can add further pressure by favouring methodological familiarity, predictable outcomes and short-term feasibility over conceptual novelty. For researchers who depend on their next publication or grant to secure an income in science, pursuing safe and predictable research can therefore become a rational career strategy.    Publication costs, journal prestige and institutional inequalities reinforce these pressures. High article processing charges can favour researchers at wealthy institutions and in well-funded countries, while administrative work, teaching, peer review and fundraising reduce the uninterrupted time available for exploratory thinking. Early-career researchers may also remain dependent on senior investigators for employment, resources, publications and professional opportunities. The consequences are both scientific and personal. More than one third of PhD students have reported symptoms of depression and around one third have reported symptoms of anxiety in studies cited by the authors. At the same time, early-career researchers may increasingly carry out narrowly defined work within projects controlled by senior investigators rather than developing independent research programmes. Others may leave academia altogether, potentially removing innovative talent from the academic system.    The authors stress that early career researchers, senior academics, editors, administrators and funders all operate under institutional constraints. However, the consequences of intellectual risk-taking fall most heavily on researchers without permanent positions, independent funding or durable institutional autonomy. The Perspective therefore calls for longer funding periods and dedicated support for high-risk research, evaluation criteria that explicitly reward conceptual novelty, greater use of double-blind peer review, reduced administrative workloads and more stable research career pathways. The Perspective also argues that research assessment should place greater value on originality, collaboration, persistence and non-linear careers rather than relying heavily on publication counts and journal prestige.    Maintaining scientific creativity, the authors conclude, requires more than individual resilience. It requires anacademic system that gives early-career researchers the autonomy, time and security needed to pursue ambitious ideas, including ideas that may fail. Without these conditions, science risks rewarding strategic conformity over scientific creativity, potentially undermining the innovation needed to address the challenges posed by accelerating global Anthropogenic change.    Publication  “How contemporary academic structures constrain scientific creativity and hold back Early Career Researchers“, Nature Human Behaviour https://www.nature.com/articles/s41562-026-02575-5  

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The average number of days of marine heatwaves annually projected for mid-century. Image courtesy Prof. Ben Harvey.

HKU Ecologists Warn That Marine Heatwaves Pose an Underestimated Threat to Public Health

Researchers from the School of Biological Sciences and Swire Institute of Marine Science (SWIMS) at The University of Hong Kong (HKU), in collaboration with Adelaide University, have called for marine heatwaves to be recognised as a public health issue.  The research, published in Nature Sustainability, highlights that marine heatwaves not only damage marine ecosystems but can also intensify extreme weather, disrupt fisheries and aquaculture, reduce seafood supplies and threaten coastal livelihoods, ultimately posing significant risks to human physical and mental health. How Marine Heatwaves Affect Human Health  Marine heatwaves, prolonged periods of unusually high ocean temperatures, are becoming more frequent, longer-lasting and more intense as the climate warms. While their impacts on marine ecosystems are well documented, their consequences for human health remain largely overlooked. Key Impacts Identified Extreme weather: Higher ocean temperatures can contribute to more intense storms and flooding, increasing the risk of injury, death, and displacement. Food safety: Marine heatwaves can increase harmful algal blooms that contaminate seafood and pose health risks. Food security and nutrition: Damage to fisheries and aquaculture can reduce seafood supplies, particularly affecting communities that rely heavily on marine resources. Livelihoods and mental health: Damage to marine ecosystems and loss of income can contribute to stress, anxiety, grief and uncertainty. Ocean-dependent communities: The impacts are particularly relevant in Asia, where hundreds of millions of people depend on the ocean for food, livelihoods and cultural practices.   “The devastating effects of marine heatwaves on marine ecosystems have been recognised for some time. What has been missing from the conversation is what these events mean for people. We are only just beginning to understand how these environmental impacts can have large negative effects on human health,” said Professor Bayden RUSSELL, Associate Professor of Ecology & Biodiversity and senior author of the paper. He added: “For many people, the ocean is much more than a place for recreation. It provides food, income, cultural identity and a sense of place.” These close connections to the ocean mean that damage to marine ecosystems can also have significant psychological impacts. “When marine heatwaves damage coral reefs, fisheries and other marine resources, communities can experience grief, anxiety and uncertainty about the future. These mental health impacts are likely to be substantial, but they remain largely unrecognised and understudied.” The researchers argue that governments and public health agencies should begin treating marine heatwaves much like land-based heatwaves. This includes incorporating marine heatwave forecasts into public health planning, considering health impacts in marine and coastal management, and strengthening collaboration between ocean scientists, health authorities and resource managers. Dr Laura FALKENBERG of Adelaide University said: “Recognising these health impacts is the first step towards better protecting communities.” “As marine heatwaves become increasingly common, we need to move from simply documenting impacts after they occur to preparing communities in advance. Better planning today can reduce future health risks.” For details of the research, please refer to the journal paper “Recognising the human health impacts of marine heatwaves”.    

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