The DOI matches its Crossref record; 26 of the 26 references it cites were found in a registry or an index.
Black Hole Mass Decreasing due to Phantom Energy Accretion
Open accessAbstract
Solution for a stationary spherically symmetric accretion of the relativistic perfect fluid with an equation of state p(rho) onto the Schwarzschild black hole is presented. This solution is a generalization of Michel solution and applicable to the problem of dark energy accretion. It is shown that accretion of phantom energy is accompanied by the gradual decrease of the black hole mass. Masses of all black holes tend to zero in the phantom energy Universe approaching the Big Rip.
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Cites
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Cosmological Imprint of an Energy Component with General Equation of State
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Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
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Cited by
Khlopov, M. Y. (2010) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/10/6/001 · Cited by 681
Phantom energy traversable wormholes
Lobo, F. S. N. (2005) · Physical Review D · doi:10.1103/physrevd.71.084011 · Cited by 549
Wormholes supported by a phantom energy
Sushkov, S. (2005) · Physical Review D · doi:10.1103/physrevd.71.043520 · Cited by 470
Metadata
- Authors
- Babichev, E., Dokuchaev, V., & Eroshenko, Y.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2004-07-08
- Volume
- 93
- Issue
- 2
- Pages
- 021102-021102
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2076374996
- Cited by
- 489
- References
- 26
- FWCI
- 14.77
- Type
- journal article
- Language
- en
- Open access
- green
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
