Cryogenic suspension design for a kilometer-scale gravitational-wave detector
نویسندگان
چکیده
Abstract We report the mirror suspension design for large-scale cryogenic gravitational wave telescope, KAGRA, during bKAGRA phase 1. Mirror thermal noise is one of fundamental noises room-temperature gravitational-wave detectors such as Advanced LIGO and Virgo. Thus, reduction required further improvement their sensitivity. One effective approach reducing to cool mirrors. There are many technical challenges that must be overcome mirrors, cryocooler induced vibrations, drift in suspensions, duty cycling due increased number potential failure mechanisms. Our has a black coating makes radiative cooling more efficient. For conduction cooling, we developed ultra high purity aluminum heat links, which yield conductivity while keeping spring constant sufficiently small. A unique inclination adjustment system, called moving mass, used aligning orientation pitch. Photo-reflective displacement sensors, have large range, installed damping control on marionette recoil mass intermediate mass. Samarium cobalt magnets coil-magnet actuators prevent significant change magnetism between room temperature temperature. In this paper, our first payload its performance 1 discussed.
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ژورنال
عنوان ژورنال: Classical and Quantum Gravity
سال: 2021
ISSN: ['1361-6382', '0264-9381']
DOI: https://doi.org/10.1088/1361-6382/abe9f3