研究领域
黑洞吸积盘理论；高能辐射过程；宇宙学激波与高能宇宙射线

个人简历
2001~2006 华中科技大学 博士

2006~2008 中科院上海天文台 博士后

2008~2010 韩国国立忠南大学 博士后

在研基金
“Blazar伽玛辐射起源的重子模型”，国家自然科学基金主任基金项目

“Blazar的高能辐射机制及应用”，福建省自然科学基金面上项目

发表文章

[1] Hang-Ying Shui, Fu-Guo Xie, Zhen Yan, Ren-Yi Ma, “The Width–Flux Relation of the Broad Iron Kα Line during the State Transitions of the Black Hole X-Ray Binaries”, 2023, Research in Astronomy and Astrophysics, 23, 065020

[2] Ren-Yi Ma, Shawn Roberts, Ya-Ping Li, Q. Daniel Wang, “Spectral energy distribution of the inner accretion flow around Sgr A* - clue for a weak outflow in the innermost region”, 2019, MNRAS, 483, 5614

[3] Xiao-Di Yu, Ren-Yi Ma, Ya-Ping Li, Hui Zhang, Tao-Tao Fang, “The profiles of Fe K alpha line from the inhomogeneous accretion flow”, 2018, MNRAS, 476, 2045

[4] Xiao-Di Yu, Ya-Ping Li, Fu-Guo Xie, Ren-Yi Ma, “A Monte Carlo study of the spectra from inhomogeneous accretion flow”, 2017, Research in Astronomy and Astrophysics, 17, 86

[5] Tong Liu, Bing Zhang, Ye Li, Ren-Yi Ma, Li Xue, “Detectable MeV neutrinos from black hole neutrino-dominated accretion flows”, 2016, PRD, 93, 123004

[6] Fu-Guo Xie, Andrzej A. Zdziarski, Ren-Yi Ma, & Qi-Xiang Yang, “A Luminous Hot Accretion Flow in The Low-luminosity Active Galactic Nucleus NGC 7213”, 2016, MNRAS, 463, 2287-2295

[7] Wei-Min Gu, Yi-Ze Dong, Tong Liu, Ren-Yi Ma, & Jun-Feng Wang, “A Neutron Star-White Dwarf Binary Model for Repeating Fast Radio Burst 121102”, 2016, ApJ, 823, L28

[8] Xiao-Fei Yu, Wei-Min Gu, Ren-Yi Ma, Ju-Fu Lu, “Thermal Stability of Magnetized Optically Thin Radiative Cooling-dominated Accretion Disks”, 2015, ApJ, 801, 47

[9] Fu-Guo Xie, Qi-Xiang Yang, Renyi Ma, “Jet-dominated Quiescent States in Black Hole X-ray Binaries: the case of V404 Cyg”, 2014, MNRAS, 442, L110-L114

[10] Renyi Ma, Fu-Guo Xie, Shu-Jin Hou, “Relationship Between the Kinetic Power and Bolometric Luminosity of Jets: limitation from black hole X-ray binaries, active galactic nuclei, and gamma-ray bursts”, 2014, ApJ, 780, L14-L18

[11] Renyi Ma, “Modeling the Multi-band Spectrum of IGR J17177-3656”, 2012, MNRAS, 423, L87-L91

[12] Gong, X. L., Li, L. X., & Ma, R. Y. "A Disc-Corona Model for a Rotating Black Hole", Monthly Notices of the Royal Astronomical Society (Accepted)

[13] Ma, R. Y., Ryu, D., & Kang, H. "Cosmic Rays Accelerated at Cosmological Shock Waves", J. Astrophys. Astr., 32, 301 (2011)

[14] Edmon. P. P., Kang, H., Jones, T., & Ma, R. Y. "Non-thermal radiation from Type Ia supernova remnants", Monthly Notices of the Royal Astronomical Society, 414, 3521 (2011)

[15] Yuan, F., Ma, R. Y., & Narayan, R. "A Simplified Global Solution for an Advection-dominated Accretion Flow", Astrophys. J., 679, 984 (2008)

[16] Ma, R. Y., Yuan, F., & Wang, D. X. "Influence of the Magnetic Coupling Process on the Advection Dominated Accretion Flows around Black Holes", Astrophys. J., 671, 1981 (2007)

[17] Ye, Y. C., Wang, D. X., & Ma, R. Y. "Magnetic coupling of a rotating black hole with advection-dominated accretion flows", New Astron., 12, 471 (2007)

[18] Ma, R. Y., Wang, D. X., & Zuo, X. Q. "Influences of the magnetic coupling process on the spectrum of a disk covered by the corona", Astron. and Astrop., 453, 1 (2006)

[19] Lei, W. H., Wang, D. X., & Ma, R. Y. "A Toy Model for Gamma-Ray Bursts in Type Ib/c Supernovae", Astrophys. J., 619, 420 (2005)

More information may be found at https://astro.xmu.edu.cn/new_en/info/1036/1086.htm

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