期刊
CHINESE PHYSICS LETTERS
卷 29, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0256-307X/29/1/010401
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资金
- Higher Education Commission, Islamabad, Pakistan
We investigate the dynamical behavior of phantom energy near a stringy magnetically charged black hole. For this purpose, we derive equations of motion for steady-state spherically symmetric flow of phantom energy onto the stringy magnetically charged black hole. It is found that phantom energy accreting onto a black hole decreases its mass. Further, the location of the critical points of accretion is explored, which yields a mass to charge ratio. This ratio implies that accretion process cannot transform a black hole into an extremal black hole or a naked singularity, hence cosmic censorship hypothesis remains valid here.
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