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Late time transitions in the quintessence field and the H-0 tension
Univ Manchester, Sch Phys & Astron, Jodrell Bank, Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England.
KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, S-10691 Stockholm, Sweden;Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Physics. KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, S-10691 Stockholm, Sweden;Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden; Univ Amsterdam, Inst Theoret Phys Amsterdam, Gravitat Astroparticle Phys Amsterdam GRAPPA, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands;Univ Amsterdam, Delta Inst Theoret Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands.ORCID iD: 0000-0001-7958-8940
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Physics.
2019 (English)In: Physics of the Dark Universe, ISSN 0953-8585, E-ISSN 2212-6864, Vol. 26, article id UNSP 100385Article in journal (Refereed) Published
Abstract [en]

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.

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ELSEVIER , 2019. Vol. 26, article id UNSP 100385
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Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:uu:diva-400050DOI: 10.1016/j.dark.2019.100385ISI: 000499696200023OAI: oai:DiVA.org:uu-400050DiVA, id: diva2:1380079
Funder
EU, European Research Council, 681431Swedish Research Council, 638-2013-8993Swedish Research Council, 2015-04814Available from: 2019-12-18 Created: 2019-12-18 Last updated: 2019-12-18Bibliographically approved

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Visinelli, LucaDanielsson, Ulf

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