Cosmological Inhomogeneities with Bose-Einstein Condensate Dark Matter - INSPIRE

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Cosmological Inhomogeneities with Bose-Einstein Condensate Dark Matter

Ben Kain
(
- Holy Cross Coll.
)
,
Hong Y. Ling
(
- Rowan U., Glassboro
)

Dec, 2011

16 pages

Published in:

Phys.Rev.D 85 (2012) 023527

e-Print:

1112.4169 [hep-ph]

DOI:

10.1103/PhysRevD.85.023527

View in:

ADS Abstract Service

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Abstract: (arXiv)

We consider the growth of cosmological perturbations to the energy density of dark matter during matter domination when dark matter is a scalar field that has undergone Bose-Einstein condensation. We study these inhomogeneities within the framework of both Newtonian gravity, where the calculation and results are more transparent, and General Relativity. The direction we take is to derive analytical expressions, which can be obtained in the small pressure limit. Throughout we compare our results to those of the standard cosmology, where dark matter is assumed pressureless, using our analytical expressions to showcase precise differences. We find, compared to the standard cosmology, that Bose-Einstein condensate dark matter leads to a scale factor, gravitational potential and density contrast that increase at faster rates.

Note:

17 pages, 2 figures; typos corrected, references added

05.30.Jp
98.80.-k
95.35.+d
dark matter
condensation: Bose-Einstein
perturbation theory
gravitation
curvature: perturbation
cosmological model

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