COSMOLOGICAL BARYOGENESIS IN SUPERSTRING MODELS WITH STABLE PROTONS

Author:

CAMPBELL B.A.1,ELLIS J.1,NANOPOULOS D.V.1,OLIVE K.A.2

Affiliation:

1. CERN, CH-1211 Geneva 23, Switzerland

2. Physics Department, Univ. of Minnesota, Minneapolis, MN 55455, USA

Abstract

We discuss cosmological baryogenesis in phenomenological low-energy models inspired by the superstring which have an unobservably long baryon lifetime. The Affleck-Dine mechanism of baryogenesis in a cold (≲104 GeV ) universe is shown to be feasible, with a large baryon density being produced by the decays of large expectation values for squark and slepton fields after inflation. We catalogue the gauge-invariant quartic scalar operators in the low-energy effective action which could appear once supersymmetry is broken, show that the D-terms in the potential can vanish, and discuss the possibility that the F-terms have flat directions allowing large values for these scalar fields.

Publisher

World Scientific Pub Co Pte Lt

Subject

General Physics and Astronomy,Astronomy and Astrophysics,Nuclear and High Energy Physics

Cited by 24 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Preserving flat directions during inflation;Physics Letters B;1995-07

2. On preserving a B + L asymmetry produced in the early universe;Physics Letters B;1994-06

3. Lepto-baryogenesis;Nuclear Physics B - Proceedings Supplements;1994-05

4. Inflation, neutrino baryogenesis, and (s)neutrino-induced baryogenesis;Nuclear Physics B;1993-06

5. Supersymmetric (s)neutrino-mass induced baryogenesis;Physics Letters B;1993-04

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