Speaker
Kan Nakazono
(The University of Tokyo)
Description
We propose and experimentally demonstrate a novel method for cavity frequency tuning in cavity haloscope experiments by coupling with a superconducting qubit. Compared to the existing tuning-rod approach, this alternative method addresses a few advantages: (a) easy implementation, (b) reduction of electromagnetic wave leakage, and (c) fast scanning because there is no thermal noise derived from the friction while tuning. In this presentation, I will summarize our detection setup, data analysis method, and the first results of our search for the dark photon around 36.1 μeV.
Primary authors
Kan Nakazono
(The University of Tokyo)
Karin Watanabe
(Tokyo University)
Koji Terashi
(Tokyo University)
Ryu Sawada
(University of Tokyo, Project assistant professor)
Shion Chen
Tatsumi Nitta
(The University of Tokyo)
Toshiaki Inada
(Tokyo University)
