More about the Tolman-Oppenheimer-Volkoff equations for the generalized Chaplygin gas
Journal Article
·
· Physical Review. D, Particles Fields
- Dipartimento di Fisica e Matematica, Universita dell'Insubria, Via Valleggio 11, 22100 Como, Italy and INFN, sezione di Milano, Via Celoria 16, 20133 Milano (Italy)
- Dipartimento di Fisica and INFN, Via Irnerio 46, 40126 Bologna (Italy)
- L. D. Landau Institute for Theoretical Physics, Kosygin Street 2, 119334 Moscow (Russian Federation)
We investigate the Tolman-Oppenheimer-Volkoff equations for the generalized Chaplygin gas with the aim of extending the findings of V. Gorini, U. Moschella, A. Y. Kamenshchik, V. Pasquier, and A. A. Starobinsky [Phys. Rev. D 78, 064064 (2008)]. We study both the standard case, where we reproduce some previous results, and the phantom case. In the phantom case we show that even a superluminal group velocity arising for {alpha}>1 cannot prevent the divergence of the pressure at a finite radial distance. Finally, we investigate how a modification of the generalized Chaplygin gas equation of state, required by causality arguments at densities very close to {lambda}, affects the results found so far.
- OSTI ID:
- 21313389
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 80, Issue 10; Other Information: DOI: 10.1103/PhysRevD.80.104038; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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