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Polarizing bubble collisions

delete2010-12-23
delete30
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OA
AI
B
Bartłomiej Czech *
M
Matthew Kleban
K
Klaus Larjo
T
Thomas S Levi
K
Kris Sigurdson
DOI:10.1088/1475-7516/2010/12/023delete
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摘要

摘要

En 中文
We predict the polarization of cosmic microwave background (CMB) photons that results from a cosmic bubble collision. The polarization is purely E-mode, symmetric around the axis pointing towards the collision bubble, and has several salient features in its radial dependence that can help distinguish it from a more conventional explanation for unusually cold or hot features in the CMB sky. The anomalous cold spot detected by the Wilkinson Microwave Anisotropy Probe (WMAP) satellite is a candidate for a feature produced by such a collision, and the Planck satellite and other proposed surveys will measure the polarization on it in the near future. The detection of such a collision would provide compelling evidence for the string theory landscape.
Keyword:
CMBR polarisation
string theory and cosmology
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期刊

Journal of Cosmology and Astroparticle Physics 封面图
Journal of Cosmology and Astroparticle Physics
IF:
5.9
论文数:
1.3W
被引数:
4.7W

机构

N
New York University
学者数:
4.4W
论文数: 3.9W
被引数: 5.8W
U
University of British Columbia
学者数:
7.0W
论文数: 6.1W
被引数: 8.6W
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