Loop quantum gravity and cosmological constant
A one-parameter regularization freedom of the Hamiltonian constraint for loop quantum gravity is analyzed. The corresponding spatially flat, homogenous and isotropic model includes the two well-known models of loop quantum cosmology as special cases. The quantum bounce nature is tenable in the gener...
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Elsevier
2021
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oai:doaj.org-article:8ef54a8d0f0e4b2eb11053d42cc152492021-12-04T04:32:41ZLoop quantum gravity and cosmological constant0370-269310.1016/j.physletb.2021.136770https://doaj.org/article/8ef54a8d0f0e4b2eb11053d42cc152492021-12-01T00:00:00Zhttp://www.sciencedirect.com/science/article/pii/S0370269321007103https://doaj.org/toc/0370-2693A one-parameter regularization freedom of the Hamiltonian constraint for loop quantum gravity is analyzed. The corresponding spatially flat, homogenous and isotropic model includes the two well-known models of loop quantum cosmology as special cases. The quantum bounce nature is tenable in the generalized cases. For positive value of the regularization parameter, the effective Hamiltonian leads to an asymptotic de-Sitter branch of the Universe connecting to the standard Friedmann branch by the quantum bounce. Remarkably, by suitably choosing the value of the regularization parameter, the observational cosmological constant can emerge at large volume limit from the effect of quantum gravity, and the effective Newtonian constant satisfies the experimental restrictions in the meantime.Xiangdong ZhangGaoping LongYongge MaElsevierarticleCosmological constantLoop quantum cosmologyEffective equationPhysicsQC1-999ENPhysics Letters B, Vol 823, Iss , Pp 136770- (2021) |
institution |
DOAJ |
collection |
DOAJ |
language |
EN |
topic |
Cosmological constant Loop quantum cosmology Effective equation Physics QC1-999 |
spellingShingle |
Cosmological constant Loop quantum cosmology Effective equation Physics QC1-999 Xiangdong Zhang Gaoping Long Yongge Ma Loop quantum gravity and cosmological constant |
description |
A one-parameter regularization freedom of the Hamiltonian constraint for loop quantum gravity is analyzed. The corresponding spatially flat, homogenous and isotropic model includes the two well-known models of loop quantum cosmology as special cases. The quantum bounce nature is tenable in the generalized cases. For positive value of the regularization parameter, the effective Hamiltonian leads to an asymptotic de-Sitter branch of the Universe connecting to the standard Friedmann branch by the quantum bounce. Remarkably, by suitably choosing the value of the regularization parameter, the observational cosmological constant can emerge at large volume limit from the effect of quantum gravity, and the effective Newtonian constant satisfies the experimental restrictions in the meantime. |
format |
article |
author |
Xiangdong Zhang Gaoping Long Yongge Ma |
author_facet |
Xiangdong Zhang Gaoping Long Yongge Ma |
author_sort |
Xiangdong Zhang |
title |
Loop quantum gravity and cosmological constant |
title_short |
Loop quantum gravity and cosmological constant |
title_full |
Loop quantum gravity and cosmological constant |
title_fullStr |
Loop quantum gravity and cosmological constant |
title_full_unstemmed |
Loop quantum gravity and cosmological constant |
title_sort |
loop quantum gravity and cosmological constant |
publisher |
Elsevier |
publishDate |
2021 |
url |
https://doaj.org/article/8ef54a8d0f0e4b2eb11053d42cc15249 |
work_keys_str_mv |
AT xiangdongzhang loopquantumgravityandcosmologicalconstant AT gaopinglong loopquantumgravityandcosmologicalconstant AT yonggema loopquantumgravityandcosmologicalconstant |
_version_ |
1718373043412140032 |