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Title: |
| Vertical Structure of Neutrino-dominated Accretion Disk and Applications to Gamma-ray Bursts |
Authors: |
| Liu, Tong; Gu, Wei-Min; Dai, Zi-Gao; Lu, Ju-Fu |
Affiliation: |
| AA(Department of Astronomy, Nanjing University, Nanjing, Jiangsu 210093, China tongliu@nju.edu.cn), AB(Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, China guwm@xmu.edu.cn), AC(Department of Astronomy, Nanjing University, Nanjing, Jiangsu 210093, China ), AD(Department of Physics and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, China) |
Publication: |
| The Astrophysical Journal, Volume 709, Issue 2, pp. 851-855 (2010). (ApJ Homepage) |
Publication Date: |
| 02/2010 |
Origin: |
| IOP |
ApJ Keywords: |
| accretion, accretion disks, black hole physics, gamma-ray burst: general |
DOI: |
| 10.1088/0004-637X/709/2/851 |
Bibliographic Code: |
| 2010ApJ...709..851L |
Abstract
We revisit the vertical structure of neutrino-dominated accretion flows in spherical coordinates. We stress that the flow should be geometrically thick when advection becomes dominant. In our calculation, the luminosity of neutrino annihilation is enhanced by 1 or 2 orders of magnitude. The empty funnel along the rotation axis can naturally explain the neutrino annihilable ejection.
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