TY - JOUR
T1 - Supersymmetric inflation, baryon asymmetry and the gravitino problem
AU - Ovrut, Burt A.
AU - Steinhardt, Paul J.
N1 - Funding Information:
We wouldl ike to thankS . Raby and M. Turnerf or theirm anyv aluablec ommentsT.h is work was sup-portedin partb y DOE grantD E-AC02-81ER4 0033 B.000 at RockefelleUr niversity(B AO), DOE Grant EY-76-C-020307a1t the Universityo f Pennsylvania (BAO and PJS), and the Alfred P. SloanF oundation (PJS).
PY - 1984/11/8
Y1 - 1984/11/8
N2 - A special class of locally supersymmetric models has been found which can produce a phase transition that meets all the conditions necessary for the inflationary universe scenario and which sets, via spontaneous supersymmetry breaking, a mass hierarchy consistent with the electroweak unification scale. In this paper we show that the same models can produce a baryon asymmetry after inflation that is consistent with astrophysical observations and can avoid the cosmological problems caused by gravitinos that appear in almost in all other locally supersymmetric models.
AB - A special class of locally supersymmetric models has been found which can produce a phase transition that meets all the conditions necessary for the inflationary universe scenario and which sets, via spontaneous supersymmetry breaking, a mass hierarchy consistent with the electroweak unification scale. In this paper we show that the same models can produce a baryon asymmetry after inflation that is consistent with astrophysical observations and can avoid the cosmological problems caused by gravitinos that appear in almost in all other locally supersymmetric models.
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U2 - 10.1016/0370-2693(84)90113-8
DO - 10.1016/0370-2693(84)90113-8
M3 - Article
AN - SCOPUS:33748844041
VL - 147
SP - 263
EP - 268
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
SN - 0370-2693
IS - 4-5
ER -