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Investigation of the environment influence for the underground and - - PowerPoint PPT Presentation

Investigation of the environment influence for the underground and cryogenic gravitational wave detector, KAGRA 16th International Conference on TAUP 2019 2019/09/10, Toyama International Conference Center, Toyama, Japan Takaaki Yokozawa(ICRR)


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SLIDE 1

Investigation of the environment influence for the underground and cryogenic gravitational wave detector, KAGRA

16th International Conference on TAUP 2019 2019/09/10, Toyama International Conference Center, Toyama, Japan Takaaki Yokozawa(ICRR) on the behalf of the KAGRA collaboration

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Contents

  • Underground and cryogenic GW detector, KAGRA
  • Environmental noise and its measurement
  • Physical environmental monitors
  • Example of the noise hunting
  • Toward joining international network observation O3
  • Summary and future plan

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SLIDE 3

KAGRA

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Kamland CLIO

Super Kamiokande

Toyama City Toyama Bay

KA KAGRA in Ka Kamioka, , Ja Japan

KAGRA Entrance SK Entrance

KAGRA

  • 3km arm length
  • Underground
  • Cryogenic(20K)
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SLIDE 4

Commissioning

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One of the important task is

Possible upgrade of VT

  • V : Volume, try to achieve the good sensitivity
  • Search the origin of noises which make the noise floor dirty and

make the glitch and line noises

  • Line noise characterization, time variance of noise floor, glitch

noisy period search, veto, …

  • T : Time, try to achieve the stable operation
  • Reducing the problems which cause the unlock, quick recovery
  • Safety interferometer control system
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SLIDE 5

Commissioning

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  • First sensitivity curve by the Fabry-Perot Michelson interferometer
  • Inspiral range : 102pc(BNS), 1157pc(BBH30Msum)
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SLIDE 6

Commissioning

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  • iKAGRA (Apr.2016)
  • First 3km interferometer
  • bKAGRA phase1 (May.2018)
  • First 3km cryogenic

interferometer

  • FPMichelson (Sep.2019)
  • O3 target
  • bKAGRA design sensitivity
  • Very challenging, but we

must reduce the noise!

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SLIDE 7

PEM : Monitors

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  • PEM : Physical Environmental Monitors
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SLIDE 8

PEM : Monitors

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SLIDE 9

PEM : Monitors

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  • http://gwwiki.icrr.u-tokyo.ac.jp/JGWwiki/KAGRA/Subgroups/PEM
  • https://www.icrr.u-tokyo.ac.jp/~washimi/KAGRA/PEM/PEMmap/
  • We provided the PEM information in the web page
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SLIDE 10

PEM : Portable PEMs

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  • Portable PEMs will accelerate the

noise hunting!

  • We introduced a Chromebook(ASUS Flip C101PA) for the underground work
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SLIDE 11

PEM evaluation

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  • There are so many activities for evaluating the environmental

noise of the KAGRA interferometer

  • Ground motion with seasonal, microseismic, earthquake, …
  • Vibration and magnetic field evaluation for cryochamber and vacuum pump
  • DC and AC power supply
  • Photon calibrator noise evaluation
  • Sound reverberation time for evaluating the Newtonian noise
  • Making sound and magnetic field map
  • Effect of the weather environment
  • temperature, humidity, pressure, earthquake, lightning, …
  • Coherent channel with PEM channels
  • Investigate the lock loss reason
  • etc, etc, etc, …
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SLIDE 12

PEM noise hunting

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  • One example of the noise hunting, called 44Hz noise

44Hz

  • There was the serious noise at 44Hz
  • Bruco, coherence finding tool, found

the coherence with accelerometer in the Laser room

  • We found the origin of the vibration

by portable PEM and removed it.

  • Succeeded in the noise hunting!
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SLIDE 13

Future : PEM injection

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  • Sound injection to Laser room
  • Sound injection to BS chamber
  • Preliminary results for the sound injection during the engineering run2
  • PEM injection : One of the important measurements to

evaluate the effect of the environment(sound, vibration, magnetic field, RF signal, …) to the interferometer signals.

  • KAGRA, LIGO, Virgo PEM injectors
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SLIDE 14

Future : ET location study

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  • Cryogenic and underground environments are important

advanced features for future GW detectors

  • We started the investigation of their environmental noise with

Virgo PEM team.

  • Advanced noise measurement
  • Discussing about the location of the Einstein Telescope
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SLIDE 15

Summary

  • We are in the phase of the commissioning toward joining the

international network observation, O3 run.

  • For joining O3, improve the sensitivity is one of the important task
  • PEM : Physical environmental monitor plays an important role
  • Investigating the environmental noises for the cryogenic and

underground gravitational detector. 15