On the Realization of MSSM Inflation(Astrophysics and Cosmology)
スポンサーリンク
概要
- 論文の詳細を見る
We study the fine-tuning problem on the initial condition of inflation in the minimal supersymmetric standard model (MSSM), associated with the narrowness of the slow-roll region. We consider two cases before the onset of the MSSM inflation, namely, the radiation-dominated era and preceding inflationary era. We find that thermal dissipation does not induce additional friction to the inflaton; thus it does not help enlarge the slow-roll region. We argue that thermal correction to the potential in the preceding radiation-dominated era and quantum fluctuations in the preceding inflationary era disturb field configuration and prevent the MSSM inflation unless a certain specific preinflation history is realized.
- 2009-10-25
著者
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KAMADA Kohei
Department of Physics, Graduate School of Science, The University of Tokyo
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Kamada Kohei
Department Of Physics Graduate School Of Science The University Of Tokyo:research Center For The Ear
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Yokoyama Jun'ichi
Univ. Tokyo Kashiwa Jpn
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YOKOYAMA Junichi
Research Center for the Early Universe, School of Science, The University of Tokyo
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Kamada Kohei
Department Of Physics Graduate School Of Science The University Of Tokyo:research Center For The Ear
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Yokoyama Jun'ichi
Research Center for the Early Universe (RESCEU), Graduate School of Science, The University of Tokyo
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YOKOYAMA Jun'ichi
Research Center for the Early Universe (RESCEU), Graduate School of Science, The University of Tokyo:Institute for the Physics and Mathematics of the Universe, The University of Tokyo
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Kamada Kohei
Department of Physics, Graduate School of Science, The University of Tokyo:Research Center for the Early Universe (RESCEU), Graduate School of Science, The University of Tokyo
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