Late time transitions in the quintessence field and the H0 tension

被引：47

作者：

Di Valentino, Eleonora ^{[1
]}

Ferreira, Ricardo Z. ^{[2
,3
]}

Visinelli, Luca ^{[2
,3
,4
,5
,6
]}

Danielsson, Ulf ^{[4
]}

机构：

[1] Univ Manchester, Sch Phys & Astron, Jodrell Bank, Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England

[2] KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, S-10691 Stockholm, Sweden

[3] Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden

[4] Uppsala Univ, Dept Phys & Astron, Lagerhyddsvagen 1, S-75120 Uppsala, Sweden

[5] Univ Amsterdam, Inst Theoret Phys Amsterdam, Gravitat Astroparticle Phys Amsterdam GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[6] Univ Amsterdam, Delta Inst Theoret Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

来源：

PHYSICS OF THE DARK UNIVERSE | 2019年 / 26卷

基金：

欧洲研究理事会; 瑞典研究理事会;

关键词：

MICROWAVE BACKGROUND ANISOTROPIES; CFHTLENS; OSCILLATIONS; PLANCK;

D O I：

10.1016/j.dark.2019.100385

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We consider a quintessence field which transitions from a matter-like to a cosmological constant behaviour between recombination and the present time. We aim at easing the tension in the measurement of the present Hubble rate, and we assess the Lambda CDM model properly enlarged to include our quintessence field against cosmological observations. The model does not address the scope we proposed. This result allows us to exclude a class of quintessential models as a solution to the tension in the Hubble constant measurements. (c) 2019 Elsevier B.V. All rights reserved.

引用

页数：13

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