Pseudo-Newtonian Simulation of a Thin Accretion Disk Around a Reissner–Nordström Naked Singularity
We present the first numerical simulations of a thin accretion disk around a Reissner–Nordström (RN) naked singularity (NkS; a charged point mass). The gravity of the RN NkS is modeled with a pseudo-Newtonian potential that reproduces exactly the radial dependence of the RN Keplerian orbital frequen...
Main Authors: | , , , |
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格式: | 文件 |
语言: | English |
出版: |
IOP Publishing
2025-01-01
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丛编: | The Astrophysical Journal |
主题: | |
在线阅读: | https://doi.org/10.3847/1538-4357/adb421 |