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Astronomy

A brief history of the Universe (adapted from NASA)

The astrophysical studies at Xiamen University (hosted by theDepartment of Astronomy) use observations of multi-messenger signals (i.e., the radio, millimeter/submillimeter, infrared, optical, ultraviolet, X-ray and Gamma-ray emission, gravitational wave, neutrino, and time-domain facilities), theoretical modeling and numerical simulations to tackle the most important questions about the 13.79± 0.02 billion-years-old (Planck2018) universe. These questions include the formation and evolution of multi-scale astronomical objects and the physical laws under extreme conditions.

Current research areas include large-scale structure of the Universe, cosmological simulation, galaxy formation and evolution, intergalactic/circumgalactic/interstellar medium, active galactic nucleus and supermassive black hole, black-hole accretion at various mass scales, neutron star, stellar outburst phenomenon (i.e., gamma ray burst and fast radio burst), modeling and detection of dark matter, neutrino etc.

Our faculty also involves in a number of domestic and international collaborations/projects, including the Five-hundred-meter Aperture Spherical Telescope (FAST), the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), the Hard X-ray Modulation Telescope (HXMT), the Subaru Prime Focus Spectrograph project (PFS), theEast Asian Observatory’sJames Clark Maxwell Telescope(JINGLEandMALATANGprojects), theIRAM telescopes, the Jiangmen Underground Neutrino Observatory (JUNO) and future facilities the Thirty Meter Telescope (TMT), the Chinese Space Station Telescope (CSST), the Square Kilometer Array (SKA), the Taiji program in space gravitational physics and the Legacy Survey of Space and Time (LSST).


  • 高煜

  • 孙谋远

    msun88@xmu.edu.cn

    活动星系核、星系与大质量黑洞的共同演化、黑洞天体物理学

  • 武剑锋

    wujianfeng AT xmu.edu.cn

    海韵园物理与机电航空大楼564

    黑洞天体物理学;黑洞和星系的宇宙学演化;高能天体物理;多波段观测分析;大规模巡天

  • 于浩然

    haoran@xmu.edu.cn

    宇宙大尺度结构;N体数值模拟;中微子宇宙学;星系角动量;高性能计算

  • Fang Taotao

    Professor

    fangt@xmu.edu.cn

    Physics Building 539, Haiyun Campus, Xiamen University

    Galaxy formation and evolution; Observational extragalactic astronomy; Large scale structure

  • Gu Weimin

    Professor

    guwm@xmu.edu.cn

    540, Physics Building, Haiyun Campus

    accretion disks, X-ray binaries, gamma-ray bursts, ultraluminous X-ray sources

  • Huang Feng

    Associate Professor

    fenghuang@xmu.edu.cn

    Physics Building 571, Xiamen University (Haiyun Campus)

    Dark Matter Detection, Astroparticle Physics, Multi-wavelength Observation

  • Li Ang

    Associate Professor

    liang@xmu.edu.cn

    Physics Building 571, Xiamen University (Haiyun Campus)

    Nuclear astrophysics; High energy astrophysics related to compact stars, dark matter, gamma-ray bursts and supernova; Finite nuclei/hypernuclei, and the underlying nucleon interaction and hyperon interaction.

  • Liu Tong

    Associate Professor

    tongliu@xmu.edu.cn

    Physics Building 543, Xiamen University (Haiyun Campus)

    Black hole accretion disks and relativistic jets  Gamma-ray bursts, fast radio bursts, and supernovae Gravitational waves Neutrino astrophysics and nucleosynthesis Tidal disruption events Protoplanetary disks

  • Luo Shu

    Associate Professor

    luoshu@xmu.edu.cn

    Physics Building 542, Xiamen University (Haiyun Campus)

    Neutrino Astrophysics & Neutrino Cosmology Phenomenology of Neutrino Oscillation

  • Ma Renyi

    Associate Professor

    ryma@xmu.edu.cn

    Physics Building 542, Haiyun Campus, Xiamen University

    Black hole accretion disks Jets Cosmic rays

  • Wang Junfeng

    Prof.

    jfwang@xmu.edu.cn

    Physics Building 541 Haiyun Campus

    co-evolution of galaxies and super massive black holes, star formation, multi-wavelength imaging observation

  • Xue Li

    Associate Professor

    lixue@xmu.edu.cn

    Physics Building 544, Hai-Yun Campus

    Accretion Disk, Instability, QPO, NDAF Numerical Method, Spectral Method, Computational technique, MPI, GPU

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