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Neutrino number asymmetry and cosmological birefringence

C Q Geng1,2, S H Ho1,2 and J N Ng2

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We study effective interactions of a new type in terms of the CPT-even dimension-6 Chern–Simons-like term, which could originate from superstring theory, to generate the cosmological birefringence. We use the neutrino number asymmetry to induce a sizable rotation polarization angle in the data for the cosmic microwave background radiation polarization. The combined effect of the new term and the neutrino asymmetry provides an alternative way to understand the birefringence.


Keywords

CMBR polarization theory

cosmological neutrinos

baryon asymmetry

 

E-print Number: 0706.0080

Cited: by |

Refers: to

PACS

98.80.Cq Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)

11.15.-q Gauge field theories

14.60.Lm Ordinary neutrinos (nue, numu, nutau)

11.25.-w Strings and branes

11.30.Er Charge conjugation, parity, time reversal, and other discrete symmetries

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 09 (September 2007)

Received 13 July 2007, accepted for publication 20 August 2007

Published 11 September 2007



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