2023年
07/21
開催
開催日時
2023/07/21（金）15:00〜16:00
開催場所
ハイブリッド：研究本館 セミナールーム、オンライン(Zoom)
講演者
須山 輝明 准教授（東京工業大学）
言語
English
詳細ページ
お問い合わせ
伊藤 飛鳥 / asuka.ito-AT-kek.jp
概要
Gravitational lensing (GL) has been a powerful method to probe matter inhomogeneities in the Universe. GL of gravitational waves, which will be detected in the near future, will enable us to gain more information of the nature of dark matter and further boost the significance of GL. In light of this situation, it is important to have understanding of basic properties of GL. In my talk, I show that gravitational lensing obeys the causality in the sense that (electromagnetic/gravitational) waves emitted from the source arrive at an observer only after the arrival of the signal in geometrical optics. This leads to the Kramers-Kronig relation, a well-known relation in the field of optics, in GL, as the relation between real and imaginary parts of the amplification factor. I will also show some relations which hold as consequence of the Kramers-Kronig relation. Finally, I argue that examining the violation of the Kramers-Kronig relation may be used for correctly extracting the lensing signal in the gravitational wave observations.