KEK素粒子原子核研究所・宇宙物理セミナー(嵯峨 承平氏)

 
分類宇宙物理セミナー
開始2019/07/11 (木) 15:30
終了2019/07/11 (木) 16:30
会場研究本館 1階 会議室1
講演タイトルThe vector mode in the observational cosmology
講演者嵯峨 承平氏(京都大学 基礎物理学研究所 学振特別研究員)
言語英語/English
連絡先wangsai-AT-post.kek.jp
ウェブサイト
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概要

In the inflation theory with a dilatonic coupling between the inflaton and the U(1) gauge field, a persistent electric field (and then an anisotropic inflation) is obtained as a solution of the classical field equations. We studied the pair production of charged scalar particles in the inflaton-driven electric field. In particular, we evaluated the induced current due to the pair production. Solving the field equations with the induced current, we showed that the first-order backreaction screens the electric field with the cosmic expansion. This result indicates that the no-go theorem of anisotropic inflations holds true regardless of whether the dilatonic coupling is present or not. If time allows, we also comment on future directions of this topic, i.e. i) induced current on general backgrounds, ii) pair productions of charged fermions. This talk is based on Phys. Rev. D98 (2018) 103512 and work in progress.

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