马任意助理教授的个人主页

 

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. 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)

8. 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)

任教课程
大学物理
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