The 79th JSAP Autumn Meeting, 2018

Presentation information

Oral presentation

3 Optics and Photonics » 3.5 Laser system and materials

[19p-431B-1~18] 3.5 Laser system and materials

Wed. Sep 19, 2018 1:45 PM - 6:45 PM 431B (431-2)

Shigeki Tokita(Osaka Univ.), Masaki Tokurakawa(UEC), Hiroaki Furuse(Kitami Inst. of Tech.)

4:45 PM - 5:00 PM

[19p-431B-12] Thermal lens effect in Input Mode Cleaner of the gravitational-wave detector KAGRA

Issei Sugai1, Masashi Ohkawa2, Kentaro Somiya3, Seiji Kawamura4, Keiko Kokeyama5, Takamasa Suzuki1, Takashi Sato2 (1.Grad. School of Sci. and Tech., Niigata Univ., 2.Fac. of Eng., Niigata Univ., 3.Dept. of Phys., Tokyo Tech., 4.Grad. School of Sci., Nagoya Univ., 5.ICRR, Univ. of Tokyo)

Keywords:thermal lens effect, gravitational wave detector, KAGRA

A Japanese gravitational-wave antenna, called KAGRA, is a 3-km Michelson-type laser interferometer to detect gravitational waves. In the input optics system of the KAGRA, the input mode cleaner (IMC) plays important roles to stabilize the pre-stabilized laser beam in TEM00 mode content and position. Since the IMC is a three-mirror triangular ring cavity, power density in the IMC is extremely high due to resonance. The high power density can bring unnecessary heating, which causes thermal lens effect, to the mirrors. So, in this study, influence of the thermal lensing on transmitted light from the IMC was considered by numerical simulation using FINESSE.