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Phantom crossing dark energy in Horndeski's theory

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dc.contributor.author Matsumoto J.
dc.date.accessioned 2019-01-22T20:58:48Z
dc.date.available 2019-01-22T20:58:48Z
dc.date.issued 2018
dc.identifier.issn 2470-0010
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/149721
dc.description.abstract © 2018 American Physical Society. The ΛCDM model is a remarkably successful model which is consistent with the observations of cosmic microwave background radiation (CMB), baryon acoustic oscillation (BAO), and the large scale structure of the Universe. However, the discrepancy in the value of H0 between the local observations and PLANCK observation of CMB was recently pointed out. One of the ways to ease the discrepancy is to introduce phantom dark energy instead of the cosmological constant. However, phantom dark energy often suffers from instabilities. We will investigate the general solution to overcome the difficulty of phantom dark energy and construct some particular models which have a phantom crossing and can be consistent with the observations.
dc.relation.ispartofseries Physical Review D
dc.title Phantom crossing dark energy in Horndeski's theory
dc.type Article
dc.relation.ispartofseries-issue 12
dc.relation.ispartofseries-volume 97
dc.collection Публикации сотрудников КФУ
dc.source.id SCOPUS24700010-2018-97-12-SID85049526933


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  • Публикации сотрудников КФУ Scopus [17617]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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