(Anti)Evaporation of Schwarzschildde Sitter Black Holes

Related identifiers: doi: 10.1103/PhysRevD.57.2436 
Subject: Astrophysics  High Energy Physics  Theoryarxiv: General Relativity and Quantum Cosmology  Astrophysics::High Energy Astrophysical Phenomena

References
(13)
13 references, page 1 of 2
 1
 2
[1] S. W. Hawking: Particle creation by black holes. Commun. Math. Phys. 43, 199 (1974).
[2] C. G. Callan, S. B. Giddings, J. A. Harvey and A. Strominger: Evanescent black holes. Phys. Rev. D 45, 1005 (1992), hepth/9111056.
[3] J. G. Russo, L. Susskind and L. Thorlacius: Black hole evaporation in 1 + 1 dimensions. Phys. Lett. B292, 13 (1992), hepth/9201074.
[4] J. G. Russo, L. Susskind and L. Thorlacius: The endpoint of Hawking radiation. Phys. Rev. D 46, 3444 (1992), hepth/9206070.
[5] R. Bousso and S. W. Hawking: Trace anomaly of dilaton coupled scalars in two dimensions. Submitted to Phys. Rev. Lett.; preprint no. DAMTP/R97/25, hepth/9705236.
[6] H. Nariai: On a new cosmological solution of Einstein's field equations of gravitation. Sci. Rep. Tohoku Univ. Ser. I 35, 62 (1951).
[7] P. Ginsparg and M. J. Perry: Semiclassical perdurance of de Sitter space. Nucl. Phys. B222, 245 (1983).
[8] R. Bousso and S. W. Hawking: Pair creation of black holes during inflation. Phys. Rev. D 54, 6312 (1996), grqc/9606052.
[9] J. D. Hayward: Entropy in the RST model . Phys. Rev. D 52, 2239 (1995), grqc/9412065.
[10] S. Nojiri and S. D. Odintsov: Trace anomaly and nonlocal effective action for 2D conformally invariant scalar interacting with dilaton. Eprint no. hepth/9706009.

Metrics
1views in OpenAIRE0views in local repository0downloads in local repository

 Download from


Cite this publication