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個人經歷

2001~2006 華中科技大學博士

2006~2008 中科院上海天文台博士後

2008~2010 韓國國立忠南大學博士後

主講課程

大學物理

研究領域

黑洞吸積盤理論；高能輻射過程；宇宙學激波與高能宇宙射線

學術成果

在研基金

“Blazar伽瑪輻射起源的重子模型”，國家自然科學基金主任基金項目

“Blazar的高能輻射機制及套用”，福建省自然科學基金面上項目

發表文章

1. 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)

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

3. 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)

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

5. 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)

6. 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)

7. 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)

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基本介紹