Abstract
We study some of the cosmological imprints of pre-inflationary particles. We show that each such particle provides a seed for a spherically symmetric cosmic defect. The profile of this cosmic defect is fixed and its magnitude is linear in a single parameter that is determined by the mass of the pre-inflationary particle. We study the CMB and peculiar velocity imprints of this cosmic defect and suggest that it could explain some of the large scale cosmological anomalies.
Original language | English |
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Article number | 004 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2010 |
Issue number | 2 |
DOIs | |
State | Published - 15 Feb 2010 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics