TY - JOUR
T1 - After primordial inflation
AU - Nanopoulos, D. V.
AU - Olive, K. A.
AU - Srednicki, M.
PY - 1983/7/21
Y1 - 1983/7/21
N2 - We consider the history of the early universe in the locally supersymmetric model we have previously discussed. We pay particular attention to the requirement of converting the quanta of the field which drives primordial inflation (inflatons) to ordinary particles which can produce the cosmological baryon asymmetry without producing too many gravitinos. An inflaton mass of about 1013 GeV (a natural value in our model) produces a completely acceptable scenario.
AB - We consider the history of the early universe in the locally supersymmetric model we have previously discussed. We pay particular attention to the requirement of converting the quanta of the field which drives primordial inflation (inflatons) to ordinary particles which can produce the cosmological baryon asymmetry without producing too many gravitinos. An inflaton mass of about 1013 GeV (a natural value in our model) produces a completely acceptable scenario.
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U2 - 10.1016/0370-2693(83)91624-6
DO - 10.1016/0370-2693(83)91624-6
M3 - Article
AN - SCOPUS:33645956508
VL - 127
SP - 30
EP - 34
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 - 1-2
ER -