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Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014 @ Toyama Univ. 1

Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

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Page 1: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

Coating development and plans for filter

cavity tests at TAMA

Daisuke TATSUMINational Astronomical Observatory of Japan

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 1

Page 2: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 2

Filter cavity

Page 3: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 3

Squeezing Light and Filter cavity

Squeezed vacuum injection is one of promising way to reduce the detector noises.

As a R&D activity for beyond the KAGRA detector, we have a plan to develop the filter cavity at TAMA.

Page 4: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 4

A demonstration by eLIGO

2dB

Page 5: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 5

Frequency independent squeezing

Page 6: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 6

Solution: Filter Cavity

Page 7: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 7

Frequency dependent squeezing

Page 8: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 8

Loss requirement (2)

Page 9: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 9

Loss requirements

Page 10: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 10

Rough design of the filter cavity

Cavity pole freq. = 40Hz

Roundtrip Loss < 1ppm/m

Cavity length 10m 300m

Finesse 4E+5 4E+4Mirror reflectance 5N=99.999% 4N=99.99%

Cavity Loss 10ppm 300ppm

Page 11: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 11

Coating developments

Page 12: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 12

Low loss mirror developments

NAOJ and UEC

(Univ. of Electro-Communications)

collaborate with Japanese coating companies

for low-loss mirror coating

developments.

Page 13: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

Cross section of the multi-layered coating

Pictures are taken by TEM microscopein Univ. of Tokyo

The films have clear edges.Each layer is dense and uniform.

Page 14: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

X-ray Photoelectron Spectroscopy : XPS

Argon ion gun

Neutralizer

Soft X-ray

Soft X-ray

Page 15: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

O K

LL

O 1

s

Ta 4

d5

O 2

s

Ta2O5 film

X-ray Photoelectron Spectroscopy : XPS

measured by A. Ueda at Institute of Engineering Innovations,

University of Tokyo

Page 16: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

Ave.   8.0ppm

Scattering Loss

coated by SigmaKoki

world top class quality!

Page 17: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

At least the best performance in Japan

446 J/cm2 with 10nsec pulse

44.6 GW/cm2 (peak power density)

This is tolerance for one shot pulse.

KAGRA IOO requireshigh power density (> 1 MW/cm2) tolerance for 10 year continuous operation.

Damage Threshold

Page 18: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

2014/08/02 KAGRA f2f   August 2014 @ Toyama Univ. 18

SUMMARY

Recent few years we develop

low-loss mirror

with Japanese companies.

By using the mirror

the filter cavity tests at TAMA

are planned.

Page 19: Coating development and plans for filter cavity tests at TAMA Daisuke TATSUMI National Astronomical Observatory of Japan 2014/08/02 KAGRA f2f August 2014

End