Hawking Radiation Spectra for Scalar Fields by a HigherDimensional SchwarzschilddeSitter Black Hole

Related identifiers: doi: 10.1103/PhysRevD.94.024035 
Subject: High Energy Physics  Phenomenology  High Energy Physics  Theory  Astrophysics  Cosmology and Nongalactic Astrophysicsarxiv: General Relativity and Quantum Cosmology

References
(51)
0.0 0.2 0.4 0.6 0.8 1.0 1.2 ω rh (a)
[1] N. ArkaniHamed, S. Dimopoulos and G. R. Dvali, Phys. Lett. B 429, 263 (1998); Phys. Rev. D 59, 086004 (1999); I. Antoniadis, N. ArkaniHamed, S. Dimopoulos and G. R. Dvali, Phys. Lett. B 436, 257 (1998).
[2] L. Randall and R. Sundrum, Phys. Rev. Lett. 83 (1999) 3370; Phys. Rev. Lett. 83 (1999) 4690.
[3] F. Tangherlini, Nuovo Cim. 27 (1963) 636.
[4] S. W. Hawking, Commun. Math. Phys. 43, 199{220 (1975)
[5] P. Kanti and J. MarchRussell, Phys. Rev. D 66, 024023 (2002); Phys. Rev. D 67, 104019 (2003).
[6] C. M. Harris and P. Kanti, JHEP 0310, 014 (2003).
[7] A. S. Cornell, W. Naylor and M. Sasaki, JHEP 0602, 012 (2006); V. Cardoso, M. Cavaglia and L. Gualtieri, Phys. Rev. Lett. 96, 071301 (2006); JHEP 0602, 021 (2006); S. Creek, O. Efthimiou, P. Kanti and K. Tamvakis, Phys. Lett. B 635, 39 (2006).
[8] C. M. Harris and P. Kanti, Phys. Lett. B 633 (2006) 106; G. Du y, C. Harris, P. Kanti and E. Winstanley, JHEP 0509, 049 (2005).
[9] M. Casals, P. Kanti and E. Winstanley, JHEP 0602, 051 (2006).

Metrics
No metrics available

 Download from


Cite this publication