Conformal Hamiltonian dynamics of general relativity

被引：12
|
作者：
Arbuzov, A. B. [1 ]
Barbashov, B. M. [1 ]
Nazmitdinov, R. G. [1 ,2 ]
Pervushin, V. N. [1 ]
Borowiec, A. [3 ]
Pichugin, K. N. [4 ]
Zakharov, A. F. [5 ]
机构：
[1] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
[2] Univ Illes Balears, Dept Fis, E-07122 Palma de Mallorca, Spain
[3] Univ Wroclaw, Inst Theoret Phys, PL-50204 Wroclaw, Poland
[4] LV Kirenskii Inst Phys, Krasnoyarsk 660036, Russia
[5] Inst Theoret & Expt Phys, Moscow 117259, Russia
来源：
PHYSICS LETTERS B | 2010年 / 691卷 / 05期
关键词：
General relativity; Cosmology; Dilaton gravity; COSMOLOGICAL CONSTANT; UNIVERSE; GRAVITATION; SUPERNOVAE; MODEL;
D O I：
10.1016/j.physletb.2010.06.042
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The General Relativity formulated with the aid of the spin connection coefficients is considered in the finite space geometry of similarity with the Dirac scalar dilaton. We show that the redshift evolution of the General Relativity describes the vacuum creation of the matter in the empty Universe at the electroweak epoch and the dilaton vacuum energy plays a role of the dark energy. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码：230 / 233
页数：4
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