
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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