Isocurvature, Black Holes, and the Maximum Temperature of our Universe

開催日時

2021/09/28 11:00 – 12:00

開催場所

Online (Zoom)

講演者

Dr. Samuel Charles Passaglia ( Kavli IPMU)

言語

日本語

詳細ページ

お問い合わせ

伊形 尚久 / igata-AT-post.kek.jp


概要

The isocurvature component of the primordial perturbations has been largely ignored ever since CMB experiments established that on large-scales the adiabatic mode dominates. On small scales, however, isocurvature can still play a role. I present a new signal of small-scale isocurvature, the formation of primordial black holes, which I use to derive new model-independent isocurvature constraints. I then discuss the isocurvature we expect in the Standard Model from the evolution of the Higgs field during reheating.