[1] A. Einstein, “Approximative Integration of the Field Equations of Gravitation”, Sitzungsber.Preuss.Akad.Wiss.Berlin (Math.Phys.) 1916, 688 (1916).
[2] G. M. Clemence, “The Relativity Effect in Planetary Motions”, Reviews of Modern Physics 19, 361 (1947).
[3] F. W. Dyson, A. S. Eddington, and C. Davidson, “A Determination of the Deflection of Light by the Sun’s Gravitational Field, from Observations Made at the Total Eclipse of May 29, 1919”, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 220, 291 (1920).
[4] A. Einstein, “LENS-LIKE ACTION OF A STAR BY THE DEVIATION OF LIGHT IN THE GRAVITATIONAL FIELD”, Science 84, 506 (1936).
[5] D. Walsh, R. F. Carswell, and R. J. Weymann, “0957 + 561 A, B: twin quasistellar objects or gravitational lens?”, Nature 279, 381 (1979).
[6] M. D. Kruskal, “Maximal Extension of Schwarzschild Metric”, Physical Review 119, 1743 (1960).
[7] S. W. Hawking, “Black Holes in General Relativity”, Communications in Mathematical Physics 25, 152 (1972).
[8] J. Weber, “Detection and Generation of Gravitational Waves”, Physical Review 117, 306 (1960).
[9] H. Hirakawa and K. Narihara, “Search for Gravitational Radiation at 145 Hz”, Physical Review Letters 35, 330 (1975).
[10] P. Astone et al., “IGEC2: A 17-month search for gravitational wave bursts in 2005–2007”, Physical Review D 82, 022003 (2010).
[11] N. Yunes and X. Siemens, “Gravitational-Wave Tests of General Relativity with Ground-Based Detectors and Pulsar-Timing Arrays”, Living Reviews in Relativity 16, 9 (2013).
[12] C. M. Will, “The Confrontation between General Relativity and Experiment”, Living Reviews in Relativity 17, 4 (2014).
[13] W. H. Press and K. S. Thorne, “Gravitational-Wave Astronomy”, Annual Review of Astronomy and Astrophysics 10, 335 (1972).
[14] B. F. Schutz, “Gravitational wave astronomy”, Classical and Quantum Gravity 16, A131 (1999).
[15] S. Kobayashi and P. Meszaros, “Gravitational Radiation from Gamma-Ray Burst Progenitors”, The Astrophysical Journal 589, 861 (2003).
[16] E. Muller, M. Rampp, R. Buras, H.-T. Janka, and D. H. Shoemaker, “Toward Gravitational Wave Signals from Realistic Core-Collapse Supernova Models”, The Astrophysical Journal 603, 221 (2004).
[17] C. D. Ott, A. Burrows, L. Dessart, and E. Livne, “A New Mechanism for Gravitational-Wave Emission in Core-Collapse Supernovae”, Physical Review Letters 96, 201102 (2006).
[18] R. A. Hulse and J. H. Taylor, “Discovery of a pulsar in a binary system”, The Astrophysical Journal 195, L51 (1975).
[19] A. A. Michelson and E. W. Morley, “On the Relative Motion of the Earth and the Luminiferous Ether”, American Journal of Science s3-34, 333 (1887).
[20] A. Perot and C. Fabry, “On the Application of Interference Phenomena to the Solution of Various Problems of Spectroscopy and Metrology”, The Astrophysical Journal 9, 87 (1899).
[21] R. W. P. Drever et al., “Gravitational Wave Detectors Using Laser Interferometers and Optical Cavities: Ideas, Principles and Prospects”, in Quantum Optics, Experimental Gravity, and Measurement Theory, edited by P. Meystre and M. O. Scully, NATO Advanced Science Institutes Series, pages 503–514, Springer US, Boston, MA, 1983.
[22] A. J. Aasi et al., “Advanced LIGO”, Classical and Quantum Gravity 32, 074001 (2015).
[23] F. Acernese et al., “Advanced Virgo: a second-generation interferometric gravitational wave detector”, Classical and Quantum Gravity 32, 024001 (2014).
[24] H. Grote and LIGO Scientific Collaboration, “The status of GEO 600”, Classical and Quantum Gravity 25, 114043 (2008).
[25] H. Grote and the LIGO Scientific Collaboration, “The GEO 600 status”, Classical and Quantum Gravity 27, 084003 (2010).
[26] K. L. Dooley et al., “GEO 600 and the GEO-HF upgrade program: successes and challenges”, Classical and Quantum Gravity 33, 075009 (2016).
[27] K. Somiya, “Detector configuration of KAGRA–the Japanese cryogenic gravitational-wave detector”, Classical and Quantum Gravity 29, 124007 (2012).
[28] Y. Aso et al., “Interferometer design of the KAGRA gravitational wave detector”, Physical Review D 88, 043007 (2013).
[29] B. P. Abbott et al., “Observation of Gravitational Waves from a Binary Black Hole Merger”, Physical Review Letters 116, 061102 (2016).
[30] B. P. Abbott et al., “GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs”, Physical Review X 9, 031040 (2019).
[31] B. P. Abbott et al., “Tests of General Relativity with GW150914”, Physical Review Letters 116, 221101 (2016).
[32] B. P. Abbott et al., “Tests of General Relativity with GW170817”, Physical Review Letters 123, 011102 (2019).
[33] B. P. Abbott et al., “GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral”, Physical Review Letters 119, 161101 (2017).
[34] B. P. Abbott et al., “Multi-messenger Observations of a Binary Neutron Star Merger”, The Astrophysical Journal 848, L12 (2017).
[35] B. P. Abbott et al., “Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A”, The Astrophysical Journal 848, L13 (2017).
[36] T. Matsubayashi, H. Shinkai, and T. Ebisuzaki, “Gravitational Waves from Merging Intermediate-Mass Black Holes”, The Astrophysical Journal 614, 864 (2004).
[37] C. Reisswig et al., “Formation and Coalescence of Cosmological Supermassive-Black-Hole Binaries in Supermassive-Star Collapse”, Physical Review Letters 111, 151101 (2013).
[38] B. Allen, “The stochastic gravity-wave background: sources and detection”, arXiv:gr-qc/9604033 (1996).
[39] D. Langlois, R. Maartens, and D. Wands, “Gravitational waves from inflation on the brane”, Physics Letters B 489, 259 (2000).
[40] T. L. Smith, M. Kamionkowski, and A. Cooray, “Direct detection of the inflationary gravitational-wave background”, Physical Review D 73, 023504 (2006).
[41] J. R. Gair, M. Vallisneri, S. L. Larson, and J. G. Baker, “Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors”, Living Reviews in Relativity 16, 7 (2013).
[42] A. Stroeer and A. Vecchio, “The LISA verification binaries”, Classical and Quantum Gravity 23, S809 (2006).
[43] B. F. Schutz, “Fundamental physics with LISA”, Classical and Quantum Gravity 26, 094020 (2009).
[44] K. Yagi and T. Tanaka, “DECIGO/BBO as a Probe to Constrain Alternative Theories of Gravity”, Progress of Theoretical Physics 123, 1069 (2010).
[45] J. Garc´ıa-Bellido, D. G. Figueroa, and A. Sastre, “Gravitational wave background from reheating after hybrid inflation”, Physical Review D 77, 043517 (2008).
[46] L. Alabidi, K. Kohri, M. Sasaki, and Y. Sendouda, “Observable spectra of induced gravitational waves from inflation”, Journal of Cosmology and Astroparticle Physics 2012, 017 (2012).
[47] M. Punturo et al., “The Einstein Telescope: a third-generation gravitational wave observatory”, Classical and Quantum Gravity 27, 194002 (2010).
[48] B. P. Abbott et al., “Exploring the sensitivity of next generation gravitational wave detectors”, Classical and Quantum Gravity 34, 044001 (2017).
[49] P. Amaro-Seoane et al., “Laser Interferometer Space Antenna”, arXiv:1702.00786 [astro-ph] (2017).
[50] G. M. Harry, P. Fritschel, D. A. Shaddock, W. Folkner, and E. S. Phinney, “Laser interferometry for the Big Bang Observer”, Classical and Quantum Gravity 23, 4887 (2006).
[51] J. Luo et al., “TianQin: a space-borne gravitational wave detector”, Classical and Quantum Gravity 33, 035010 (2016).
[52] W.-R. Hu and Y.-L. Wu, “The Taiji Program in Space for gravitational wave physics and the nature of gravity”, National Science Review 4, 685 (2017).
[53] K. A. Kuns, H. Yu, Y. Chen, and R. X. Adhikari, “Astrophysics and cosmology with a deci-hertz gravitational-wave detector: TianGO”, arXiv:1908.06004 [astro-ph, physics:gr-qc] (2019).
[54] S. Kawamura et al., “The Japanese space gravitational wave antenna: DECIGO”, Classical and Quantum Gravity 28, 094011 (2011).
[55] S. A. Hughes and K. S. Thorne, “Seismic gravity-gradient noise in interferometric gravitational-wave detectors”, Physical Review D 58, 122002 (1998).
[56] R. Abbott et al., “Seismic isolation enhancements for initial and advanced LIGO”, Classical and Quantum Gravity 21, S915 (2004).
[57] W. Fichter, P. Gath, S. Vitale, and D. Bortoluzzi, “LISA Pathfinder dragfree control and system implications”, Classical and Quantum Gravity 22, S139 (2005).
[58] F. Acernese et al., “Performances of the Virgo interferometer longitudinal control system”, Astroparticle Physics 33, 75 (2010).
[59] L. Barsotti, M. Evans, and P. Fritschel, “Alignment sensing and control in advanced LIGO”, Classical and Quantum Gravity 27, 084026 (2010).
[60] C. Cutler, “Angular resolution of the LISA gravitational wave detector”, Physical Review D 57, 7089 (1998).
[61] A. Freise et al., “Triple Michelson interferometer for a third-generation gravitational wave detector”, Classical and Quantum Gravity 26, 085012 (2009).
[62] L. D. Landau and E. M. Lifshits, The classical theory of fields, Number v. 2 in Course of theoretical physics, Pergamon Press, Oxford ; New York, 4th rev. english ed edition, 1975.
[63] M. Maggiore, Gravitational Waves, Oxford University Press, Oxford, 2008.
[64] H.-T. Janka, T. Eberl, M. Ruffert, and C. L. Fryer, “Black Hole–Neutron Star Mergers as Central Engines of Gamma-Ray Bursts”, The Astrophysical Journal 527, L39 (1999).
[65] S. Rosswog, “Mergers of Neutron Star–Black Hole Binaries with Small Mass Ratios: Nucleosynthesis, Gamma-Ray Bursts, and Electromagnetic Transients”, The Astrophysical Journal 634, 1202 (2005).
[66] G. Nelemans, L. R. Yungelson, and S. F. Portegies Zwart, “The gravitational wave signal from the Galactic disk population of binaries containing two compact objects”, Astronomy & Astrophysics 375, 890 (2001).
[67] E. Garc´ıa-Berro et al., “The merging of white dwarf and neutron star systems: gravitational radiation”, Journal of Physics: Conference Series 66, 012040 (2007).
[68] C. L. Fryer, S. E. Woosley, M. Herant, and M. B. Davies, “Merging White Dwarf/Black Hole Binaries and Gamma-Ray Bursts”, The Astrophysical Journal 520, 650 (1999).
[69] K. N. Yakunin et al., “Gravitational waves from core collapse supernovae”, Classical and Quantum Gravity 27, 194005 (2010).
[70] C. Grupen, Astroparticle Physics, Springer, Berlin ; New York, 2005.
[71] P. Jaranowski, A. Kr´olak, and B. F. Schutz, “Data analysis of gravitationalwave signals from spinning neutron stars: The signal and its detection”, Physical Review D 58, 063001 (1998).
[72] A. Vilenkin, “Gravitational radiation from cosmic strings”, Physics Letters B 107, 47 (1981).
[73] T. Damour and A. Vilenkin, “Gravitational radiation from cosmic (super)strings: Bursts, stochastic background, and observational windows”, Physical Review D 71, 063510 (2005).
[74] A. Kosowsky, M. S. Turner, and R. Watkins, “Gravitational waves from first-order cosmological phase transitions”, Physical Review Letters 69, 2026 (1992).
[75] M. Gleiser and R. Roberts, “Gravitational Waves from Collapsing Vacuum Domains”, Physical Review Letters 81, 5497 (1998).
[76] R. Easther and E. A. Lim, “Stochastic gravitational wave production after inflation”, Journal of Cosmology and Astroparticle Physics 2006, 010 (2006).
[77] N. Yunes and F. Pretorius, “Fundamental theoretical bias in gravitational wave astrophysics and the parametrized post-Einsteinian framework”, Physical Review D 80, 122003 (2009).
[78] T. G. F. Li et al., “Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence”, Physical Review D 85, 082003 (2012).
[79] M. Isi, M. Giesler, W. M. Farr, M. A. Scheel, and S. A. Teukolsky, “Testing the No-Hair Theorem with GW150914”, Physical Review Letters 123, 111102 (2019).
[80] C. Brans and R. H. Dicke, “Mach’s Principle and a Relativistic Theory of Gravitation”, Physical Review 124, 925 (1961).
[81] H. A. Buchdahl, “Non-Linear Lagrangians and Cosmological Theory”, Monthly Notices of the Royal Astronomical Society 150, 1 (1970).
[82] M. Visser, “Mass for the Graviton”, General Relativity and Gravitation 30, 1717 (1998).
[83] D. M. Eardley, D. L. Lee, A. P. Lightman, R. V. Wagoner, and C. M. Will, “Gravitational-Wave Observations as a Tool for Testing Relativistic Gravity”, Physical Review Letters 30, 884 (1973).
[84] A. Nishizawa, A. Taruya, K. Hayama, S. Kawamura, and M.-a. Sakagami, “Probing nontensorial polarizations of stochastic gravitational-wave backgrounds with ground-based laser interferometers”, Physical Review D 79, 082002 (2009).
[85] K. Hayama and A. Nishizawa, “Model-independent test of gravity with a network of ground-based gravitational-wave detectors”, Physical Review D 87, 062003 (2013).
[86] P. S. Cowperthwaite et al., “The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models”, The Astrophysical Journal 848, L17 (2017).
[87] R. W. Klebesadel, I. B. Strong, and R. A. Olson, “Observations of GammaRay Bursts of Cosmic Origin”, The Astrophysical Journal 182, L85 (1973).
[88] J. van Paradijs, C. Kouveliotou, and R. A. M. J. Wijers, “Gamma-Ray Burst Afterglows”, Annual Review of Astronomy and Astrophysics 38, 379 (2000).
[89] C. S. Kochanek and T. Piran, “Gravitational Waves and γ-Ray Bursts”, The Astrophysical Journal 417, L17 (1993).
[90] M. Tanaka et al., “Kilonova from post-merger ejecta as an optical and near-Infrared counterpart of GW170817”, Publications of the Astronomical Society of Japan 69 (2017).
[91] K. Sato, “First-order phase transition of a vacuum and the expansion of the Universe”, Monthly Notices of the Royal Astronomical Society 195, 467 (1981).
[92] A. H. Guth, “Inflationary universe: A possible solution to the horizon and flatness problems”, Physical Review D 23, 347 (1981).
[93] P. A. R. Ade et al., “Joint Analysis of BICEP2/Keck Array and Planck Data”, Physical Review Letters 114, 101301 (2015).
[94] Planck Collaboration, “Planck 2018 results. X. Constraints on inflation”, Astronomy & Astrophysics (2019).
[95] F. A. Jenet et al., “Upper Bounds on the Low-Frequency Stochastic Gravitational Wave Background from Pulsar Timing Observations: Current Limits and Future Prospects”, The Astrophysical Journal 653, 1571 (2006).
[96] R. van Haasteren et al., “Placing limits on the stochastic gravitationalwave background using European Pulsar Timing Array data: EPTA GWB limit”, Monthly Notices of the Royal Astronomical Society 414, 3117 (2011).
[97] Z. Arzoumanian et al., “The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background”, The Astrophysical Journal 859, 47 (2018).
[98] J. W. Armstrong, L. Iess, P. Tortora, and B. Bertotti, “Stochastic Gravitational Wave Background: Upper Limits in the 10-6 to 10-3 Hz Band”, The Astrophysical Journal 599, 806 (2003).
[99] K. Ishidoshiro et al., “Upper Limit on Gravitational Wave Backgrounds at 0.2 Hz with a Torsion-Bar Antenna”, Physical Review Letters 106, 161101 (2011).
[100] Y. Kuwahara, A. Shoda, K. Eda, and M. Ando, “Search for a stochastic gravitational wave background at 1–5 Hz with a torsion-bar antenna”, Physical Review D 94, 042003 (2016).
[101] B. P. Abbott et al., “Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run”, Physical Review Letters 118, 121101 (2017).
[102] A. Nishizawa et al., “Laser-interferometric detectors for gravitational wave backgrounds at 100 MHz: Detector design and sensitivity”, Physical Review D 77, 022002 (2008).
[103] T. Akutsu et al., “Search for a Stochastic Background of 100-MHz Gravitational Waves with Laser Interferometers”, Physical Review Letters 101, 101101 (2008).
[104] A. Ito, T. Ikeda, K. Miuchi, and J. Soda, “Probing GHz Gravitational Waves with Graviton-magnon Resonance”, arXiv:1903.04843 [astro-ph, physics:gr-qc, physics:hep-ph] (2019).
[105] S. Kuroyanagi, S. Tsujikawa, T. Chiba, and N. Sugiyama, “Implications of the B -mode polarization measurement for direct detection of inflationary gravitational waves”, Physical Review D 90, 063513 (2014).
[106] A. Sesana, “Prospects for Multiband Gravitational-Wave Astronomy after GW150914”, Physical Review Letters 116, 231102 (2016).
[107] S. Vitale, “Multiband Gravitational-Wave Astronomy: Parameter Estimation and Tests of General Relativity with Space- and Ground-Based Detectors”, Physical Review Letters 117, 051102 (2016).
[108] S. Isoyama, H. Nakano, and T. Nakamura, “Multiband gravitationalwave astronomy: Observing binary inspirals with a decihertz detector, BDECIGO”, Progress of Theoretical and Experimental Physics 2018 (2018).
[109] N. Seto and J. Yokoyama, “Probing the Equation of State of the Early Universe with a Space Laser Interferometer”, Journal of the Physical Society of Japan 72, 3082 (2003).
[110] A. Albrecht, P. J. Steinhardt, M. S. Turner, and F. Wilczek, “Reheating an Inflationary Universe”, Physical Review Letters 48, 1437 (1982).
[111] K. Nakayama, S. Saito, Y. Suwa, and J. Yokoyama, “Space-based gravitational-wave detectors can determine the thermal history of the early Universe”, Physical Review D 77, 124001 (2008).
[112] S. Kuroyanagi, T. Chiba, and N. Sugiyama, “Precision calculations of the gravitational wave background spectrum from inflation”, Physical Review D 79, 103501 (2009).
[113] C. Grojean and G. Servant, “Gravitational waves from phase transitions at the electroweak scale and beyond”, Physical Review D 75, 043507 (2007).
[114] J. J. Blanco-Pillado, K. D. Olum, and X. Siemens, “New limits on cosmic strings from gravitational wave observation”, Physics Letters B 778, 392 (2018).
[115] H. J. Kimble, Y. Levin, A. B. Matsko, K. S. Thorne, and S. P. Vyatchanin, “Conversion of conventional gravitational-wave interferometers into quantum nondemolition interferometers by modifying their input and/or output optics”, Physical Review D 65, 022002 (2001).
[116] A. Buonanno and Y. Chen, “Quantum noise in second generation, signalrecycled laser interferometric gravitational-wave detectors”, Physical Review D 64, 042006 (2001).
[117] P. R. Saulson, “Thermal noise in mechanical experiments”, Physical Review D 42, 2437 (1990).
[118] V. Braginsky, M. Gorodetsky, and S. Vyatchanin, “Thermodynamical fluc tuations and photo-thermal shot noise in gravitational wave antennae”, Physics Letters A 264, 1 (1999).
[119] M. Cerdonio, L. Conti, A. Heidmann, and M. Pinard, “Thermoelastic effects at low temperatures and quantum limits in displacement measurements”, Physical Review D 63, 082003 (2001).
[120] N. Nakagawa, A. M. Gretarsson, E. K. Gustafson, and M. M. Fejer, “Thermal noise in half-infinite mirrors with nonuniform loss: A slab of excess loss in a half-infinite mirror”, Physical Review D 65, 102001 (2002).
[121] G. M. Harry et al., “Titania-doped tantala/silica coatings for gravitationalwave detection”, Classical and Quantum Gravity 24, 405 (2007).
[122] K. Somiya and K. Yamamoto, “Coating thermal noise of a finite-size cylindrical mirror”, Physical Review D 79, 102004 (2009).
[123] R. Del Fabbro et al., “Low frequency behaviour of the Pisa seismic noise super-attenuator for gravitational wave detection”, Physics Letters A 133, 471 (1988).
[124] T. Sekiguchi, A Study of Low Frequency Vibration Isolation System for Large Scale Gravitational Wave Detectors, Ph.D. thesis, The University of Tokyo, 2016.
[125] P. R. Saulson, “Terrestrial gravitational noise on a gravitational wave antenna”, Physical Review D 30, 732 (1984).
[126] D. Fiorucci, J. Harms, M. Barsuglia, I. Fiori, and F. Paoletti, “Impact of infrasound atmospheric noise on gravity detectors used for astrophysical and geophysical applications”, Physical Review D 97, 062003 (2018).
[127] A. Yariv and P. Yeh, Photonics: Optical Electronics in Modern Communications, Oxford University Press, 2007.
[128] D. H. Reitze, P. R. Saulson, and H. Grote, editors, Advanced interferometric gravitational-wave detectors, World Scientific, New Jersey, 2019.
[129] R. W. P. Drever et al., “Laser phase and frequency stabilization using an optical resonator”, Applied Physics B 31, 97 (1983).
[130] D. Z. Anderson, “Alignment of resonant optical cavities”, Applied Optics 23, 2944 (1984).
[131] S. Solimeno et al., “Fabry-P´erot resonators with oscillating mirrors”, Physical Review A 43, 6227 (1991).
[132] N. M. Sampas and D. Z. Anderson, “Stabilization of laser beam alignment to an optical resonator by heterodyne detection of off-axis modes”, Applied Optics 29, 394 (1990).
[133] E. Morrison, B. J. Meers, D. I. Robertson, and H. Ward, “Experimental demonstration of an automatic alignment system for optical interferometers”, Applied Optics 33, 5037 (1994).
[134] E. Morrison, B. J. Meers, D. I. Robertson, and H. Ward, “Automatic alignment of optical interferometers”, Applied Optics 33, 5041 (1994).
[135] J. Mizuno et al., “Resonant sideband extraction: a new configuration for interferometric gravitational wave detectors”, Physics Letters A 175, 273 (1993).
[136] T. Robson, N. Cornish, and C. Liu, “The construction and use of LISA sensitivity curves”, Classical and Quantum Gravity 36, 105011 (2019).
[137] L. Barsotti, S. Gras, M. Evans, and P. Fritschel, “The updated Advanced LIGO design curve”, LIGO Document T1800044-v5, 2018.
[138] D. Bortoluzzi et al., “Testing LISA drag-free control with the LISA technology package flight experiment”, Classical and Quantum Gravity 20, S89 (2003).
[139] A. Schleicher et al., “In-orbit performance of the LISA Pathfinder drag-free and attitude control system”, CEAS Space Journal 10, 471 (2018).
[140] B. L. Schumaker, “Disturbance reduction requirements for LISA”, Classical and Quantum Gravity 20, S239 (2003).
[141] G. Noci et al., “Cold Gas Micro Propulsion System for Scientific Satellite Fine Pointing: Review of Development and Qualification Activities at Thales Alenia Space Italia”, in 45th AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit, Denver, Colorado, 2009, American Institute of Aeronautics and Astronautics.
[142] G. Anderson et al., “Experimental results from the ST7 mission on LISA Pathfinder”, Physical Review D 98, 102005 (2018).
[143] M. Armano et al., “LISA Pathfinder micronewton cold gas thrusters: Inflight characterization”, Physical Review D 99, 122003 (2019).
[144] J. Pap et al., “Variations in total solar and spectral irradiance as measured by the VIRGO experiment on SOHO”, Advances in Space Research 24, 215 (1999).
[145] S. Kuroyanagi, K. Nakayama, and S. Saito, “Prospects for determination of thermal history after inflation with future gravitational wave detectors”, Physical Review D 84, 123513 (2011).
[146] P. L. Bender and D. Hils, “Confusion noise level due to galactic and extragalactic binaries”, Classical and Quantum Gravity 14, 1439 (1997).
[147] M. R. Adams and N. J. Cornish, “Detecting a stochastic gravitational wave background in the presence of a galactic foreground and instrument noise”, Physical Review D 89, 022001 (2014).
[148] A. J. Farmer and E. S. Phinney, “The gravitational wave background from cosmological compact binaries”, Monthly Notices of the Royal Astronomical Society 346, 1197 (2003).
[149] C. C. Yancey et al., “MULTI-MESSENGER ASTRONOMY OF GRAVITATIONAL-WAVE SOURCES WITH FLEXIBLE WIDE-AREA RADIO TRANSIENT SURVEYS”, The Astrophysical Journal 812, 168 (2015).
[150] A. Nishizawa, A. Taruya, and S. Saito, “Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens”, Physical Review D 83, 084045 (2011).
[151] N. Seto, S. Kawamura, and T. Nakamura, “Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space”, Physical Review Letters 87, 221103 (2001).
[152] S. Hawking, “Gravitationally Collapsed Objects of Very Low Mass”, Monthly Notices of the Royal Astronomical Society 152, 75 (1971).
[153] R. Saito and J. Yokoyama, “Gravitational-Wave Background as a Probe of the Primordial Black-Hole Abundance”, Physical Review Letters 102, 161101 (2009).
[154] H. Niikura et al., “Microlensing constraints on primordial black holes with the Subaru/HSC Andromeda observation”, Nature Astronomy 3, 524 (2019).
[155] K. Nagano, T. Fujita, Y. Michimura, and I. Obata, “Axion Dark Matter Search with Interferometric Gravitational Wave Detectors”, Physical Review Letters 123, 111301 (2019).
[156] T. Nakamura et al., “Pre-DECIGO can get the smoking gun to decide the astrophysical or cosmological origin of GW150914-like binary black holes”, Progress of Theoretical and Experimental Physics 2016, 093E01 (2016).
[157] B. Bertotti, L. Iess, and P. Tortora, “A test of general relativity using radio links with the Cassini spacecraft”, Nature 425, 374 (2003).
[158] K. Yagi, N. Yunes, and T. Tanaka, “Gravitational Waves from Quasicircular Black-Hole Binaries in Dynamical Chern-Simons Gravity”, Physical Review Letters 109, 251105 (2012).
[159] K. Yagi, “SCIENTIFIC POTENTIAL OF DECIGO PATHFINDER AND TESTING GR WITH SPACE-BORNE GRAVITATIONAL WAVE INTERFEROMETERS”, International Journal of Modern Physics D 22, 1341013 (2013).
[160] G. Gnocchi, A. Maselli, T. Abdelsalhin, N. Giacobbo, and M. Mapelli, “Bounding alternative theories of gravity with multiband GW observations”, Physical Review D 100, 064024 (2019).
[161] T. Kinugawa, H. Takeda, and H. Yamaguchi, “Probe for Type Ia supernova progenitor in decihertz gravitational wave astronomy”, arXiv:1910.01063 [astro-ph] (2019).
[162] D. Shaddock, B. Ware, P. G. Halverson, R. E. Spero, and B. Klipstein, “Overview of the LISA Phasemeter”, in AIP Conference Proceedings, volume 873, pages 654–660, Greenbelt, Maryland (USA), 2006, AIP.
[163] I. Bykov, J. J. E. Delgado, A. F. G. Mar´ın, G. Heinzel, and K. Danzmann, “LISA phasemeter development: Advanced prototyping”, Journal of Physics: Conference Series 154, 012017 (2009).
[164] B. P. Abbott et al., “LIGO: the Laser Interferometer Gravitational-Wave Observatory”, Reports on Progress in Physics 72, 076901 (2009).
[165] D. V. Martynov et al., “Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy”, Physical Review D 93, 112004 (2016).
[166] A. Abramovici et al., “Improved sensitivity in a gravitational wave interferometer and implications for LIGO”, Physics Letters A 218, 157 (1996).
[167] M. Ohashi et al., “Design and construction status of CLIO”, Classical and Quantum Gravity 20, S599 (2003).
[168] J. A. Sidles and D. Sigg, “Optical torques in suspended Fabry–Perot interferometers”, Physics Letters A 354, 167 (2006).
[169] A. Suemasa, A. Shimo-oku, K. Nakagawa, and M. Musha, “Developments of high frequency and intensity stabilized lasers for space gravitational wave detector DECIGO/B-DECIGO”, CEAS Space Journal 9, 485 (2017).
[170] M. Musha, T. Kanaya, K. Nakagawa, and K.-I. Ueda, “Intensity and frequency noise characteristics of two coherently-added injection-locked Nd:YAG lasers”, Applied Physics B 73, 209 (2001).
[171] L.-W. Wei, F. Cleva, and C. N. Man, “Coherently combined master oscillator fiber power amplifiers for Advanced Virgo”, Optics Letters 41, 5817 (2016).
[172] E. A. Donley, T. P. Heavner, F. Levi, M. O. Tataw, and S. R. Jefferts, “Double-pass acousto-optic modulator system”, Review of Scientific Instruments 76, 063112 (2005).
[173] G. P. Barwood, P. Gill, and W. R. C. Rowley, “High-accuracy length metrology using multiple-stage swept-frequency interferometry with laser diodes”, Measurement Science and Technology 9, 1036 (1998).
[174] A. Araya et al., “Absolute-length determination of a long-baseline Fabry–Perot cavity by means of resonating modulation sidebands”, Applied Optics 38, 2848 (1999).
[175] A. Stochino, K. Arai, and R. X. Adhikari, “Technique for in situ measurement of free spectral range and transverse mode spacing of optical cavities”, Applied Optics 51, 6571 (2012).
[176] K. A. Strain, “Electrostatic drive (ESD) results from GEO and application in Advanced LIGO”, LIGO Document T060015-x0, 2006.
[177] O. Jennrich, “LISA technology and instrumentation”, Classical and Quantum Gravity 26, 153001 (2009).
[178] D. I. Robertson et al., “Construction and testing of the optical bench for LISA Pathfinder”, Classical and Quantum Gravity 30, 085006 (2013).
[179] M. Musha (private communication).
[180] F. Wei et al., “Subkilohertz linewidth reduction of a DFB diode laser using self-injection locking with a fiber Bragg grating Fabry-Perot cavity”, Optics Express 24, 17406 (2016).
[181] E. Canuto, A. Molano, and L. Massotti, “Drag-Free Control of the GOCE Satellite: Noise and Observer Design”, IEEE Transactions on Control Systems Technology 18, 501 (2010).
[182] M. Armano et al., “LISA Pathfinder platform stability and drag-free performance”, Physical Review D 99, 082001 (2019).
[183] W. J. Weber et al., “Position sensors for flight testing of LISA dragfree control”, in Astronomical Telescopes and Instrumentation, edited by M. Cruise and P. Saulson, page 31, Waikoloa, Hawai’i, United States, 2003.
[184] C. C. Speake and S. M. Aston, “An interferometric sensor for satellite drag-free control”, Classical and Quantum Gravity 22, S269 (2005).
[185] S. J. Cooper et al., “A compact, large-range interferometer for precision measurement and inertial sensing”, Classical and Quantum Gravity 35, 095007 (2018).
[186] I. Funaki, Y. Nakayama, H. Horisawa, and M. Ando, “Micro-thruster Options for the Japanese Space Gravitational Wave Observatory Missions”, International Electric Propulsion Conference, IEPC-2011-308 (2011).
[187] P. J. Wass et al., “Testing of the UV discharge system for LISA Pathfinder”, in AIP Conference Proceedings, volume 873, pages 220–224, Greenbelt, Maryland (USA), 2006, AIP.
[188] K. Yagi and N. Seto, “Detector configuration of DECIGO/BBO and identification of cosmological neutron-star binaries”, Physical Review D 83, 044011 (2011).
[189] D. G. Enzer, R. T. Wang, and W. M. Klipstein, “GRAIL – A microwave ranging instrument to map out the lunar gravity field”, in 2010 IEEE International Frequency Control Symposium, pages 572–577, Newport Beach, CA, USA, 2010, IEEE.
[190] F. Cirillo and P. F. Gath, “Control system design for the constellation acquisition phase of the LISA mission”, Journal of Physics: Conference Series 154, 012014 (2009).
[191] P. G. Maghami and T. T. Hyde, “Laser interferometer space antenna dynamics and controls model”, Classical and Quantum Gravity 20, S273 (2003).
[192] Y. Michimura, Y. Kuwahara, T. Ushiba, N. Matsumoto, and M. Ando, “Optical levitation of a mirror for reaching the standard quantum limit”, Optics Express 25, 13799 (2017).
[193] P. Fritschel et al., “Alignment of an interferometric gravitational wave detector”, Applied Optics 37, 6734 (1998).
[194] N. Smith-Lefebvre et al., “Optimal alignment sensing of a readout mode cleaner cavity”, Optics Letters 36, 4365 (2011).
[195] S. Kawamura and M. E. Zucker, “Mirror-orientation noise in a Fabry–Perot interferometer gravitational wave detector”, Applied Optics 33, 3912 (1994).
[196] T. Abel, G. L. Bryan, and M. L. Norman, “The Formation of the First Star in the Universe”, Science 295, 93 (2002).
[197] A. Buonanno and Y. Chen, “Signal recycled laser-interferometer gravitational-wave detectors as optical springs”, Physical Review D 65, 042001 (2002).
[198] H. Rehbein et al., “Double optical spring enhancement for gravitationalwave detectors”, Physical Review D 78, 062003 (2008).
[199] K. Somiya et al., “Development of a frequency-detuned interferometer as a prototype experiment for next-generation gravitational-wave detectors”, Applied Optics 44, 3179 (2005).
[200] O. Miyakawa et al., “Measurement of optical response of a detuned resonant sideband extraction gravitational wave detector”, Physical Review D 74, 022001 (2006).
[201] R. O. R. Y. Thompson, “Coherence Significance Levels”, Journal of Atmospheric Sciences 36, 2020 (1979).
[202] R. D. Peccei and H. R. Quinn, “CP Conservation in the Presence of Pseudoparticles”, Physical Review Letters 38, 1440 (1977).
[203] P. Svrcek and E. Witten, “Axions in string theory”, Journal of High Energy Physics 06, 051 (2006).
[204] A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. MarchRussell, “String axiverse”, Physical Review D 81, 123530 (2010).
[205] L. Visinelli and S. Vagnozzi, “Cosmological window onto the string axiverse and the supersymmetry breaking scale”, Physical Review D 99, 063517 (2019).
[206] J. P. Conlon, “The QCD Axion and Moduli Stabilisation”, Journal of High Energy Physics 2006, 078 (2006).
[207] P. Sikivie, “Experimental Tests of the ”Invisible” Axion”, Physical Review Letters 51, 1415 (1983).
[208] M. B. Schneider, F. P. Calaprice, A. L. Hallin, D. W. MacArthur, and D. F. Schreiber, “Limit on Im ( C S C A * ) from a Test of T Invariance in Ne 19 Beta Decay”, Physical Review Letters 51, 1239 (1983).
[209] G. Raffelt and L. Stodolsky, “Mixing of the photon with low-mass particles”, Physical Review D 37, 1237 (1988).
[210] A. G. Dias, A. C. B. Machado, C. C. Nishi, A. Ringwald, and P. Vaudrevange, “The quest for an intermediate-scale accidental axion and further ALPs”, Journal of High Energy Physics 2014, 37 (2014).
[211] P. W. Graham, I. G. Irastorza, S. K. Lamoreaux, A. Lindner, and K. A. van Bibber, “Experimental Searches for the Axion and Axion-Like Particles”, Annual Review of Nuclear and Particle Science 65, 485 (2015).
[212] I. G. Irastorza and J. Redondo, “New experimental approaches in the search for axion-like particles”, Progress in Particle and Nuclear Physics 102, 89 (2018).
[213] M. Y. Khlopov, “Probes for dark matter physics”, International Journal of Modern Physics D 27, 1841013 (2018).
[214] K. Zioutas et al., “First Results from the CERN Axion Solar Telescope”, Physical Review Letters 94, 121301 (2005).
[215] V. Anastassopoulos et al., “New CAST limit on the axion–photon interaction”, Nature Physics 13, 584 (2017).
[216] A. Payez et al., “Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles”, Journal of Cosmology and Astroparticle Physics 02, 006 (2015).
[217] A. C. Melissinos, “Search for Cosmic Axions using an Optical Interferometer”, Physical Review Letters 102, 202001 (2009).
[218] W. DeRocco and A. Hook, “Axion interferometry”, Physical Review D 98, 035021 (2018).
[219] I. Obata, T. Fujita, and Y. Michimura, “Optical Ring Cavity Search for Axion Dark Matter”, Physical Review Letters 121, 161301 (2018).
[220] H. Liu, B. D. Elwood, M. Evans, and J. Thaler, “Searching for axion dark matter with birefringent cavities”, Physical Review D 100, 023548 (2019).
[221] S. M. Carroll, G. B. Field, and R. Jackiw, “Limits on a Lorentz- and parity-violating modification of electrodynamics”, Physical Review D 41, 1231 (1990).
[222] S. M. Carroll, “Quintessence and the Rest of the World: Suppressing Long-Range Interactions”, Physical Review Letters 81, 3067 (1998).
[223] A. Andrianov, D. Espriu, F. Mescia, and A. Renau, “The axion shield”, Physics Letters B 684, 101 (2010).
[224] D. Espriu and A. Renau, “Photon propagation in a cold axion background with and without magnetic field”, Physical Review D 85, 025010 (2012).
[225] T. Fujita, R. Tazaki, and K. Toma, “Hunting Axion Dark Matter with Protoplanetary Disk Polarimetry”, Physical Review Letters 122, 191101 (2019).
[226] D. Budker, P. W. Graham, M. Ledbetter, S. Rajendran, and A. O. Sushkov, “Proposal for a Cosmic Axion Spin Precession Experiment (CASPEr)”, Physical Review X 4, 021030 (2014).
[227] B. J. Meers, “Recycling in laser-interferometric gravitational-wave detectors”, Physical Review D 38, 2317 (1988).
[228] T. T. Fricke et al., “DC readout experiment in Enhanced LIGO”, Classical and Quantum Gravity 29, 065005 (2012).
[229] 久村 富持, 『制御システム論の基礎』, 共立出版, 1988.
[230] M. Araki, B. Kondo, and K. Yamamoto, “GG-Pseudo-Band Method for the Design of Multivariable Control Systems”, IFAC Proceedings Volumes 14, 393 (1981).
[231] C. M. Caves, “Quantum-mechanical noise in an interferometer”, Physical Review D 23, 1693 (1981).
[232] K. Aki and P. G. Richards, Quantitative Seismology, Univ. Science Books, Sausalito, Calif, 2. ed., corr. print edition, 2009.
[233] N. K. Pavlis, S. A. Holmes, S. C. Kenyon, and J. K. Factor, “The development and evaluation of the Earth Gravitational Model 2008 (EGM2008): THE EGM2008 EARTH GRAVITATIONAL MODEL”, Journal of Geophysical Research: Solid Earth 117, n/a (2012).
[234] E. Th´ebault et al., “International Geomagnetic Reference Field: the 12th generation”, Earth, Planets and Space 67, 79 (2015).
[235] M. A. Barton, “Models of the Advanced LIGO Suspensions in Mathematica”, LIGO Document T020205-v1, 2014.
[236] T. Sekiguchi, “Suspension rigid-body modeling tool in Mathematica”, JGW-T1503729-v2, 2015.
論文の公開元へ
