A cosmological concordance model with dynamical vacuum term

被引：54

作者：

Alcaniz, J. S. ^{[2
]}

Borges, H. A. ^{[1
]}

Carneiro, S. ^{[1
]}

Fabris, J. C. ^{[3
]}

Pigozzo, C. ^{[1
]}

Zimdahl, W. ^{[3
]}

机构：

[1] Univ Fed Bahia, Inst Fis, Salvador, BA, Brazil

[2] Observ Nacl, Rio De Janeiro, RJ, Brazil

[3] Univ Fed Espirito Santo, Dept Fis, Vitoria, ES, Brazil

来源：

PHYSICS LETTERS B | 2012年 / 716卷 / 01期

关键词：

DARK ENERGY; THERMODYNAMICS; SINGULARITY; DENSITY;

D O I：

10.1016/j.physletb.2012.08.014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We demonstrate that creation of dark-matter particles at a constant rate implies the existence of a cosmological term that decays linearly with the Hubble rate. We discuss the cosmological model that arises in this context and test it against observations of the first acoustic peak in the cosmic microwave background (CMB) anisotropy spectrum, the Hubble diagram for supernovas of type la (SNIa), the distance scale of baryonic acoustic oscillations (BAO) and the distribution of large scale structures (LSS). We show that a good concordance is obtained, albeit with a higher value of the present matter abundance than in the ACDM model. We also comment on general features of the CMB anisotropy spectrum and on the cosmic coincidence problem. (C) 2012 Elsevier B.V. All rights reserved.

引用

页码：165 / 170

页数：6

共 46 条

[1]

Alcaniz JS, 1999, ASTRON ASTROPHYS, V349, P729

[2]

[Anonymous], ARXIVHEPTH0110007

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