Quantum Cosmology with a Complex ø<sup>6</sup> Field at Finite Temperature

Chin. Phys. Lett.

1999, Vol. 16

Issue (1): 76-78 DOI:

Original Articles

Quantum Cosmology with a Complex ø⁶ Field at Finite Temperature

SHEN You-gen¹;ZHANG Tong-jie¹;XU Chong-ming²

¹Shanghai Observatory, Chinese Academy of Sciences, Shanghai 200030 ²Department of Physics, Nanjing Normal University, Nanjing 210097

Cite this article:

SHEN You-gen, ZHANG Tong-jie, XU Chong-ming 1999 Chin. Phys. Lett. 16 76-78

Download: PDF(177KB)
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks

Abstract Quantum cosmology with complex ø⁶ fields at finite temperature for the Vilenkin boundary conditions and Hartle-Hawking boundary conditions has been studied in this paper. The corresponding Wheeler-DeWitt equations and the Universe wave functions are obtained. At the same time, the probability density distribution is calculated and the effect of temperature on probability density distribution is found.

Keywords: 98.80.Hw 04.60.Kz 98.80.Bp

Published: 01 January 1999

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

TRENDMD:

URL:

https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y1999/V16/I1/076

Service
	E-mail this article
	E-mail Alert
	RSS
Articles by authors
	SHEN You-gen
	ZHANG Tong-jie
	XU Chong-ming

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): 76-78
[2]	CAO Guang-Tao, WANG Yong-Jiu . Interference Phase of Mass Neutrino in Schwarzschild de Sitter Field**[J]. Chin. Phys. Lett., 2011, 28(2): 76-78
[3]	Ujjal Debnath . Modified Chaplygin Gas with Variable G and Λ[J]. Chin. Phys. Lett., 2011, 28(11): 76-78
[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): 76-78
[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): 76-78
[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): 76-78
[7]	HU Ping-Hui, WANG Yong-Jiu. Sagnac Effect in the Kerr--Newman and Reissner--Nordström Fields[J]. Chin. Phys. Lett., 2006, 23(8): 76-78
[8]	GAO Shan. A Conjecture on the Origin of Dark Energy[J]. Chin. Phys. Lett., 2005, 22(3): 76-78
[9]	ZHANG Yang,. Dark Energy Coupled with Dark Matter in the Accelerating Universe[J]. Chin. Phys. Lett., 2004, 21(6): 76-78
[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): 76-78
[11]	CHEN Ju-Hua, WANG Yong-Jiu. Chaos in Einstein-Maxwell-Dust System[J]. Chin. Phys. Lett., 2003, 20(6): 76-78
[12]	LIU Liao, PEI Shou-Yong. Can Higgs Field Have a Cosmological Origin?[J]. Chin. Phys. Lett., 2003, 20(5): 76-78
[13]	ZHANG Yang. Dark Energy Coupled with Relativistic Dark Matter in Accelerating Universe[J]. Chin. Phys. Lett., 2003, 20(10): 76-78
[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): 76-78
[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): 76-78

Viewed

Full text

Abstract