MISC

1994年8月

CHAOTIC INFLATION AND BARYOGENESIS IN SUPERGRAVITY

PHYSICAL REVIEW D
  • H MURAYAMA
  • ,
  • H SUZUKI
  • ,
  • T YANAGIDA
  • ,
  • J YOKOYAMA

50
4
開始ページ
R2356
終了ページ
R2360
記述言語
英語
掲載種別
記事・総説・解説・論説等(学術雑誌)
出版者・発行元
AMER PHYSICAL SOC

We propose a Kahler potential in supergravity which successfully accommodates chaotic inflation. This model can have a large gravitino mass without giving a large mass to squarks and sleptons, and thus is free from both the gravitino problem and entropy crisis. In this model baryogenesis takes places naturally, identifying the inflaton with a right-handed sneutrino with its mass M congruent-to 10(13) GeV, which is consistent with the COBE data and the Mikheyev-Smirnov-Wolfenstein solution to the solar neutrino problem. The model can also accommodate the matter content appropriate for the mixed dark matter scenario.

リンク情報
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:A1994PC89100002&DestApp=WOS_CPL
ID情報
  • ISSN : 2470-0010
  • eISSN : 2470-0029
  • Web of Science ID : WOS:A1994PC89100002

エクスポート
BibTeX RIS