KEK素粒子原子核研究所・理論セミナー(中村 康二 氏)

カテゴリ
開始2018/06/07(木)15:00
終了2018/06/07(木)16:30
会場研究本館3階セミナールーム
講演タイトルExtension of the input–output relation for a Michelson interferometer to arbitrary coherent-state light sources: --- Gravitational-wave detector and weak-value amplification ---
講演者中村 康二 氏(国立天文台)
言語英語/English
連絡先yuichiro-AT-post.kek.jp
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食堂・売店利用予定なし/0

概要

An extension of the input-output relation for a conventional Michelson interferometric gravitational-wave detector is carried out to treat an arbitrary coherent state for the injected optical beam. This extension is one of necessary researches toward the clarification of the relation between conventional gravitational-wave detectors and a simple model of a gravitational-wave detector inspired by weak-measurements in [Nishizawa, Phys. Rev. A vol.92 (2015), 032123.]. The derived input-output relation describes not only a conventional Michelson-interferometric gravitational-wave detector but also the situation of weak measurements. As a result, we may say that a conventional Michelson gravitational-wave detector already includes the essence of the weak-value amplification as the reduction of the quantum noise from the light source through the measurement at the dark port.

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