Current status of KAGRA
暂无分享,去创建一个
[1] Takayuki Tomaru,et al. The CLIO project , 2006 .
[2] T. Akutsu,et al. Molecular adsorbed layer formation on cooled mirrors and its impacts on cryogenic gravitational wave telescopes , 2018, Physical Review D.
[3] C. Broeck,et al. Advanced Virgo: a second-generation interferometric gravitational wave detector , 2014, 1408.3978.
[4] R. Poggiani. Multi-messenger Observations of a Binary Neutron Star Merger , 2019, Proceedings of Frontier Research in Astrophysics – III — PoS(FRAPWS2018).
[5] N. Kimura,et al. A study of cooling time reduction of interferometric cryogenic gravitational wave detectors using a high-emissivity coating , 2013, 1309.4836.
[6] M. M. Casey,et al. Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts , 2005 .
[7] T. Akutsu,et al. Performance test of pipe-shaped radiation shields for cryogenic interferometric gravitational wave detectors , 2015 .
[8] The Ligo Scientific Collaboration,et al. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral , 2017, 1710.05832.
[9] N. Kimura,et al. Cryogenic system for the interferometric cryogenic gravitationalwave telescope, KAGRA - design, fabrication, and performance test - , 2014 .
[10] A. Rüdiger,et al. Resonant sideband extraction: a new configuration for interferometric gravitational wave detectors , 1993 .
[11] Optical design and suspension system of the KAGRA output mode-cleaner , 2018 .
[12] Hiroaki Yamamoto,et al. Interferometer design of the KAGRA gravitational wave detector , 2013, 1306.6747.
[13] O. Miyakawa,et al. Length sensing and control strategies for the LCGT interferometer , 2011, 1111.7147.
[14] The Ligo Scientific Collaboration,et al. Observation of Gravitational Waves from a Binary Black Hole Merger , 2016, 1602.03837.
[15] K. Kuroda,et al. Cryogenic contamination speed for cryogenic laser interferometric gravitational wave detector , 2001 .
[16] Y. Wang,et al. Exploring the sensitivity of next generation gravitational wave detectors , 2016, 1607.08697.
[17] S. Oh,et al. An arm length stabilization system for KAGRA and future gravitational-wave detectors , 2019, Classical and Quantum Gravity.
[18] S. Miyoki,et al. SMALL VIBRATION CRYOCOOLER SYSTEM FOR CRYOGENIC GRAVITATIONAL WAVE INTERFEROMETER , 2005 .
[19] B. J. Meers,et al. Recycling in laser-interferometric gravitational-wave detectors. , 1988, Physical review. D, Particles and fields.
[20] Shinji Miyoki. Large scale cryogenic gravitational wave telescope , 2005 .
[21] K. Kuroda,et al. Optical properties measurement of an Al2O3 mirror substrate for the Large-Scale Cryogenic Gravitational Wave Telescope (LCGT) , 2010 .
[22] B. A. Boom,et al. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA , 2013, Living Reviews in Relativity.
[23] J. Steinlechner. Development of mirror coatings for gravitational-wave detectors , 2018, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[24] Hiroaki Yamamoto,et al. Sapphire mirror for the KAGRA gravitational wave detector , 2014 .
[25] B. J. Meers,et al. Automatic alignment of optical interferometers. , 1994, Applied optics.
[26] A. Araya,et al. Ultrastable performance of an underground-based laser interferometer observatory for gravitational waves , 2004, gr-qc/0403080.
[27] Joshua R. Smith,et al. LIGO: The laser interferometer gravitational-wave observatory , 2006, QELS 2006.
[28] C. Kim,et al. First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA , 2019, Classical and Quantum Gravity.
[29] F. Travasso,et al. Cryogenic suspension design for a kilometer-scale gravitational-wave detector , 2020, Classical and Quantum Gravity.
[30] Cryogenic measurement of the optical absorption coefficient in sapphire crystals at 1.064 μm for the large-scale cryogenic gravitational wave telescope , 2001, physics/0101075.
[31] Mechanical quality factor of a sapphire fiber at cryogenic temperatures , 2000, gr-qc/0007071.
[32] Shinji Miyoki,et al. LARGE-SCALE CRYOGENIC GRAVITATIONAL WAVE TELESCOPE , 1999 .
[33] E. Hirose,et al. Influence of nonuniformity in sapphire substrates for a gravitational wave telescope , 2019, Physical Review D.
[34] T. Akutsu,et al. Vacuum and cryogenic compatible black surface for large optical baffles in advanced gravitational-wave telescopes , 2016 .
[35] B. J. Meers. The frequency response of interferometric gravitational wave detectors , 1989 .
[36] Takayuki Tomaru,et al. MECHANICAL QUALITY FACTOR OF A CRYOGENIC SAPPHIRE TEST MASS FOR GRAVITATIONAL WAVE DETECTORS , 1999 .
[37] O. Miyakawa,et al. Excavation of an underground site for a km-scale laser interferometric gravitational-wave detector , 2014 .
[38] S. Klimenko,et al. Advanced LIGO , 2014, 1411.4547.