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Neutrino statistics and big bang nucleosynthesis

A D Dolgov1,2, S H Hansen3 and A Yu Smirnov4,5

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Neutrinos may possibly violate the spin-statistics theorem, and hence obey Bose statistics or mixed statistics despite having spin half. We find the generalized equilibrium distribution function of neutrinos which depends on a single Fermi–Bose parameter, κ, and interpolates continuously between the bosonic and fermionic distributions when κ changes from −1 to +1. We consider modification of the big bang nucleosynthesis (BBN) in the presence of bosonic or partly bosonic neutrinos. For pure bosonic neutrinos the abundances change (in comparison with the usual Fermi–Dirac case) by −3.2% for 4He (which is equivalent to a decrease of the effective number of neutrinos by ΔNν≈−0.6), +2.6% for 2H, and −7% for 7Li. These changes provide a better fit to the BBN data. Future BBN studies will be able to constrain the Fermi–Bose parameter to κ>0.5, if no deviation from fermionic nature of neutrinos is found. We also evaluate the sensitivity of future CMB and LSS observations to the Fermi–Bose parameter.


Keywords

big bang nucleosynthesis

neutrino properties

cosmological neutrinos

PACS

95.30.Cq Elementary particle processes

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

98.80.Ft Origin, formation, and abundances of the elements

Subjects

Gravitation and cosmology

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 06 (June 2005)

Received 11 April 2005, accepted for publication 1 June 2005

Published 9 June 2005



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