Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2008-02-04
Phys.Rev.D77:123516,2008
Physics
High Energy Physics
High Energy Physics - Phenomenology
14 pages, no figure, to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.77.123516
We present a new model of D-term dominated chaotic inflation in supergravity. The F-flat direction present in this model is lifted by the dominant D-term, which leads to chaotic inflation and subsequent reheating. No cosmic string is formed after inflation because the U(1) gauge symmetry is broken during inflation. The leptogenesis scenario via the inflaton decay in our D-term chaotic inflation scenario is also discussed.
Kadota Kenji
Kawano Teruhiko
Yamaguchi Masahide
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