Matter bispectrum in cubic Galileon cosmologies

dc.contributor.authorBartolo, Nicola
dc.contributor.authorBellini, Emilio
dc.contributor.authorBertacca, Daniele
dc.contributor.authorMatarrese, Sabino
dc.date.accessioned2018-02-16T08:44:57Z
dc.date.available2018-02-16T08:44:57Z
dc.date.issued2013
dc.description.abstractIn this paper we obtain the bispectrum of dark matter density perturbations in the frame of covariant cubic Galileon theories. This result is obtained by means of a semi- analytic approach to second-order perturbations in Galileon cosmologies, assuming Gaussian initial conditions. In particular, we show that, even in the presence of large deviations of the linear growth-rate w.r.t. the CDM one, at the bispectrum level such deviations are reduced to a few percent.en_US
dc.description.accreditationWeb of Science
dc.identifier.citationBartolo, N, et al. (2013). Matter bispectrum in cubic Galileon cosmologies. Journal of Cosmology and Astroparticle Physics, 34en_US
dc.identifier.issn1475-7516
dc.identifier.urihttp://dx.doi.org/10.1088/1475-7516/2013/03/034
dc.identifier.urihttp://hdl.handle.net/10566/3504
dc.language.isoenen_US
dc.privacy.showsubmitterFALSE
dc.publisherIOP Scienceen_US
dc.rightsThis is the pre-print version (From arXiv:1301.4831) of the article published online at: http://dx.doi.org/10.1088/1475-7516/2013/03/034
dc.status.ispeerreviewedTRUE
dc.subjectModi ed gravityen_US
dc.subjectGalileonen_US
dc.subjectMatter Bispectrumen_US
dc.subjectCosmological perturbationsen_US
dc.titleMatter bispectrum in cubic Galileon cosmologiesen_US
dc.typeArticleen_US

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