Research and Development for Large- Scale Cryogenic ...
Transcript of Research and Development for Large- Scale Cryogenic ...
Research and Development for Large-Scale Cryogenic Gravitational Wave Telescope (LCGT)
Norikatsu MioDepartment of Advanced
Materials Science,University of Tokyo
LCGT: Japanese future project
3-km interferometer at Kamioka mineCryogenic system to reduce thermal noise
Budget for LCGT has not been approved!
Key technologies to LCGT
Cryogenic mirrors Cooling technology (Next talk)
Operation of cryogenic interferometerCLIO: 100-m cryogenic interferometer (ICRR)
High-power laser100-W Nd:YAG laser (U-Tokyo)
etc
Target sensitivity of CLIO
Laser: Nd:YAG
1064nm, 2W
Finesse: 7500
Mirror: Sapphire
20 K, 1.8 kg, Q ~108
SQL at 100 Hz
High-power laser
Quantum-noise limited sensitivityAchieve the required detection level
Cooling capabilityAbsorbed power < refrigerating power
1kW at BS of interferometerRecycling gain of 10 and input optics efficiency of 33% are assumed
Necessary laser power => 300W
Design of laser system
LD-pumped Nd:YAG laser system (1.06µm)100-W Master-Slave Injection Lock laser
Master(2W)->1st Slave (10W)->2nd Slave 100WSaturated power amplifier (100W->300W)
Second slave laser and amplifier
Under development P > 100WStanford (USA) (slab)Laser Zentrum Hannovor (Germany) (rod)Adelaide (Australia) (slab)U-Tokyo+Mitsubishi (Japan) (rod)
High-quality & high-power laser
Thermal birefringence compensation
Uniform pumpingby diffusive reflector
Two rods and rotatorBy Mitsubishi
Linear cavity configuration
Convex mirrors (Curvature: 20cm)R=85% Output couplerP =60 W and M2 =1.12
Double-module cavity for 100-W output power
Ring cavity with two laser modulesSecond module will be installed, next year