TY - GEN
T1 - Disappearing inflaton potential
AU - Kitajima, Naoya
N1 - Publisher Copyright:
© Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015. All rights reserved.
PY - 2015
Y1 - 2015
N2 - Inflaton potential may disappear by heavy field dynamics I. Chaotic inflation in SUGRA - Mass parameter is promoted to be a dynamical field: S - <S> ≠ 0 during inflation & <S> = 0 after inflation, and then inflaton becomes (almost) massless. => Dark matter / dark radiation / searched by some experiments II. New inflation in SUGRA - Inflaton may return to the origin after reheating and rolls down to the electroweak vacuum => Inflaton can be MSSM Higgs field.
AB - Inflaton potential may disappear by heavy field dynamics I. Chaotic inflation in SUGRA - Mass parameter is promoted to be a dynamical field: S - <S> ≠ 0 during inflation & <S> = 0 after inflation, and then inflaton becomes (almost) massless. => Dark matter / dark radiation / searched by some experiments II. New inflation in SUGRA - Inflaton may return to the origin after reheating and rolls down to the electroweak vacuum => Inflaton can be MSSM Higgs field.
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M3 - Conference contribution
AN - SCOPUS:85092222955
T3 - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
SP - 908
EP - 922
BT - Proceedings of the 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
PB - Kyoto University, Yukawa Institute for Theoretical Physics
T2 - 25th Workshop on General Relativity and Gravitation in Japan, JGRG 2015
Y2 - 7 December 2015 through 11 December 2015
ER -