Inflation and B-L breaking scale

Details Inflation and B-L breaking scale Inflation and B-L breaking scale

1998-02-16

arxiv.org/abs/hep-ph/9802332v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

3 pages; to be published in the Proceedings of COSMO-97, International Workshop on "Particle Physics and the Early Universe",

Scientific paper

Inflation arises in supersymmetric grand unified theories (susy GUTs) without
fine tuning and cosmic strings usually form at the end of inflation. Hence both
strings and inflation contribute to the density perturbations in the very early
universe which lead to structure formation and to CMB anisotropies. This may
give us a hint as to the $B-L$ breaking scale.

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