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| Content Provider | Springer Nature Link |
|---|---|
| Author | Jamil, Mubasher Qadir, Asghar |
| Copyright Year | 2010 |
| Abstract | We investigate the effects of accretion of phantom energy onto primordial black holes. Since Hawking radiation and phantom energy accretion contribute to a decrease of the mass of the black hole, the primordial black hole that would be expected to decay now due to the Hawking process would decay earlier due to the inclusion of the phantom energy. Equivalently, to have the primordial black hole decay now it would have to be more massive initially. We find that the effect of the phantom energy is substantial and the black holes decaying now would be much more massive—over ten orders of magnitude! This effect will be relevant for determining the time of production and hence the number of evaporating black holes expected in a universe accelerating due to phantom energy. |
| Starting Page | 1069 |
| Ending Page | 1082 |
| Page Count | 14 |
| File Format | |
| ISSN | 00017701 |
| Journal | General Relativity and Gravitation |
| Volume Number | 43 |
| Issue Number | 4 |
| e-ISSN | 15729532 |
| Language | English |
| Publisher | Springer US |
| Publisher Date | 2010-02-12 |
| Publisher Place | Boston |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Black hole Dark energy Phantom energy Hawking radiation Astronomy, Astrophysics and Cosmology Differential Geometry Theoretical, Mathematical and Computational Physics Quantum Physics Classical and Quantum Gravitation, Relativity Theory Cosmology |
| Content Type | Text |
| Resource Type | Article |
| Subject | Physics and Astronomy |
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