Quantum Creation of a Schwarzschild-de Sitter Black Hole

Chin. Phys. Lett.

1997, Vol. 14

Issue (4): 317-320 DOI:

Original Articles

Quantum Creation of a Schwarzschild-de Sitter Black Hole

WU Zhong-chao

Department of Physics, Beijing Normal University, Beijing 100875

Cite this article:

WU Zhong-chao 1997 Chin. Phys. Lett. 14 317-320

Download: PDF(185KB)
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks

Abstract Using the Hartle-Hawking no-boundary proposal for the wave function of the universe, we can study the wave function and probability of a single Schwarzschild-de Sitter black hole created at the birth of the universe. The black hole originates from a gravitational instanton with conical singularities. The probability of a black hole creation is the exponential of one quarter of the sum of areas of the black hole and cosmological horizons. One quarter of this sum is the total entropy of the universe.

Keywords: 98.80.Hw 98.80.Bp 04.60.Kz

Published: 01 April 1997

PACS:	98.80.Hw
	98.80.Bp	(Origin and formation of the Universe)
	04.60.Kz	(Lower dimensional models; minisuperspace models)

TRENDMD:

URL:

https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1997/V14/I4/0317

Service
	E-mail this article
	E-mail Alert
	RSS
Articles by authors
	WU Zhong-chao

Related articles from Frontiers Journals

[1]	XIONG Hua-Hui, ZHU Jian-Yang* . Effect of the Inverse Volume Modification in Loop Quantum Cosmology[J]. Chin. Phys. Lett., 2011, 28(3): 317-320
[2]	CAO Guang-Tao, WANG Yong-Jiu . Interference Phase of Mass Neutrino in Schwarzschild de Sitter Field**[J]. Chin. Phys. Lett., 2011, 28(2): 317-320
[3]	Ujjal Debnath . Modified Chaplygin Gas with Variable G and Λ[J]. Chin. Phys. Lett., 2011, 28(11): 317-320
[4]	Raj Bali, Seema Tinker. Bianchi Type III Bulk Viscous Barotropic Fluid Cosmological Models with Variable G and Λ[J]. Chin. Phys. Lett., 2009, 26(2): 317-320
[5]	Mahamat Saleh, Bouetou Bouetou Thomas, , Timoleon Crepin Kofane,. Quasi-Normal Modes of Gravitational Perturbation around a Reissner-Nordström Black Hole Surrounded by Quintessence[J]. Chin. Phys. Lett., 2009, 26(10): 317-320
[6]	Raj Bali, Seema Tinker. Bianchi Type-V Bulk Viscous Barotropic Fluid Cosmological Model with Variable G and Λ[J]. Chin. Phys. Lett., 2008, 25(8): 317-320
[7]	HU Ping-Hui, WANG Yong-Jiu. Sagnac Effect in the Kerr--Newman and Reissner--Nordström Fields[J]. Chin. Phys. Lett., 2006, 23(8): 317-320
[8]	GAO Shan. A Conjecture on the Origin of Dark Energy[J]. Chin. Phys. Lett., 2005, 22(3): 317-320
[9]	ZHANG Yang,. Dark Energy Coupled with Dark Matter in the Accelerating Universe[J]. Chin. Phys. Lett., 2004, 21(6): 317-320
[10]	XU Li-Xin, LIU Hong-Ya, WANG Bei-Li. Big Bounce Singularity of a Simple Five-Dimensional Cosmological Model[J]. Chin. Phys. Lett., 2003, 20(7): 317-320
[11]	CHEN Ju-Hua, WANG Yong-Jiu. Chaos in Einstein-Maxwell-Dust System[J]. Chin. Phys. Lett., 2003, 20(6): 317-320
[12]	LIU Liao, PEI Shou-Yong. Can Higgs Field Have a Cosmological Origin?[J]. Chin. Phys. Lett., 2003, 20(5): 317-320
[13]	ZHANG Yang. Dark Energy Coupled with Relativistic Dark Matter in Accelerating Universe[J]. Chin. Phys. Lett., 2003, 20(10): 317-320
[14]	CHEN Li. Dependence of X-Ray Luminosity on Temperature for Groups and Clusters with the Moving Median Statistics[J]. Chin. Phys. Lett., 2002, 19(2): 317-320
[15]	QIU Wei-Gang, WANG Bin, SU Ru-Keng. Perturbation of Massive Scalar Field in Three-Dimensional Spherical de Sitter Space-time[J]. Chin. Phys. Lett., 2002, 19(11): 317-320

Viewed

Full text

Abstract