Self-modulational formation of pulsar microstructures |
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| Authors: | A C -L Chian C F Kennel |
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| Institution: | 1. Astronomy Group, Physics Department, Queen's University at Kingston, Ontario, Canada
3. Graduate School, China University of Science and Technology, Beijing, People's Republic of China
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| Abstract: | In this paper, we used the more rigorous general relativistic viscous hydrodynamical equation to discuss and calculate the temperature profile in the accreting disk around a Kerr black hole. It is found that for an accreting disk around a Kerr black hole, the occurrence of extremum values in the temperature profile is indeed possible. Furthermore, the temperature profile is always the same—no matter what kind of viscous mechanism is adopted—if the radiative mechanism of the materials in the disk is black-body radiation. For free-free radiation, we adopted the so-called α-viscosity law model to get a solution analogous to that obtained earlier (Fanget al. 1980). The calculations show that there exists a fast cooling ring region lying just inside the temperature maximum. In this ring region, there are probably some pecularities which do not exist in the usual temperature profile calculation (Fang, 1981). |
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