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Dark energy in motion

dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-20T10:47:24Z
dc.date.available2023-06-20T10:47:24Z
dc.date.issued2006-12
dc.description© World Scientific. This work has been partially supported by the DGICYT (Spain) under the project numbers FPA 2004-02602 and FPA 2005-02327.
dc.description.abstractRecent large-scale peculiar velocity surveys suggest that large matter volumes could be moving with appreciable velocity with respect to the CMB rest frame. If confirmed, such results could conflict with the Cosmological Principle according to which the matter and CMB rest frames should converge on very large scales. In this work, we explore the possibility that such large-scale bulk flows are due, not to the motion of matter with respect to the CMB, but to the flow of dark energy with respect to matter. Indeed, when dark energy is moving, the usual definition of the CMB rest frame as that in which the CMB dipole vanishes is not appropriate. We find instead that the dipole vanishes for observers at rest with respect to the cosmic center of mass, i.e. in motion with respect to the background radiation.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipDGICYT (Spain)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/27160
dc.identifier.doi10.1142/S0218271806009492
dc.identifier.issn0218-2718
dc.identifier.officialurlhttp://dx.doi.org/10.1142/S0218271806009492
dc.identifier.relatedurlhttp://www.worldscientific.com
dc.identifier.relatedurlhttp://arxiv.org/abs/astro-ph/0605381
dc.identifier.urihttps://hdl.handle.net/20.500.14352/51225
dc.issue.number12
dc.journal.titleInternational journal of modern physics. D, Gravitation, astrophysics, cosmology
dc.language.isoeng
dc.page.final2170
dc.page.initial2165
dc.publisherWorld Scientific
dc.relation.projectIDFPA 2004-02602
dc.relation.projectIDFPA 2005-02327
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordVelocity-field
dc.subject.keywordAnisotropy
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleDark energy in motion
dc.typejournal article
dc.volume.number15
dcterms.references[1] P.J.E. Peebles and D.T. Wilkinson, Phys. Rev. 174, 2168 (1968); P.J.E. Peebles, Principles of Physical Cosmology, Princeton University Press (1993); A. Kogut et al., Astrophys.J. 419, 1 (1993) [2] A.G. Riess et al., Astrophys. J. 488, L1 (1997); D.A. Dale et al. Astrophys. J. 510, L11 (1999); M. Colles et al., MNRAS, 321, 277 (2001); T.R. Lauer and M. Postman, Astrophys.J. 425, 418 (1994); M.J. Hudson et al. Astrophys.J. 512, L79 (1999); J.A. Willick, Astrophys.J. 522, 647 (1999); M.J. Hudson et al., Mon. Not. Roy. Astron. Soc. 352, 61 (2004); M.J. Hudson, astro-ph/0311072 [3] S. Zaroubi, astro-ph/0206052. Contribution to XIII Recontres de Blois ”Frontiers of the Universe”, 17-23 June 2001 [4] A. L. Maroto, astro-ph/0512464. To be published in JCAP [5] M. Giovannini, Int. J. Mod. Phys. D14, 363, (2005)
dspace.entity.typePublication
relation.isAuthorOfPublicatione14691a1-d3b0-47b7-96d5-24d645534471
relation.isAuthorOfPublication.latestForDiscoverye14691a1-d3b0-47b7-96d5-24d645534471

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