Publication:
Dark energy in motion

Loading...
Thumbnail Image
Full text at PDC
Publication Date
2006-12
Advisors (or tutors)
Editors
Journal Title
Journal ISSN
Volume Title
Publisher
World Scientific
Citations
Google Scholar
Research Projects
Organizational Units
Journal Issue
Abstract
Recent 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.
Description
© World Scientific. This work has been partially supported by the DGICYT (Spain) under the project numbers FPA 2004-02602 and FPA 2005-02327.
Unesco subjects
Keywords
Citation
[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)
Collections