Results 21 to 30 of about 75,914 (210)
Quantum metrology for gravitational wave astronomy [PDF]
Nature Communications, 2010 Einstein's general theory of relativity predicts that accelerating mass distributions produce gravitational radiation, analogous to electromagnetic radiation from accelerating charges. These gravitational waves (GWs) have not been directly detected to date, but are expected to open a new window to the Universe once the detectors, kilometre-scale laser ...Schnabel, Roman, Mavalvala, Nergis, McClelland, David, Lam, Ping Koy +3 moreopenaire +5 more sourcesFirst Low-Latency LIGO+Virgo Search for Binary Inspirals and their
Electromagnetic Counterparts [PDF]
, 2012 Aims. The detection and measurement of gravitational-waves from coalescing
neutron-star binary systems is an important science goal for ground-based
gravitational-wave detectors.A. A. van Veggel, A. Basti, A. Belletoile, A. Bertolini, A. Brillet, A. Buonanno, A. C. Melissinos, A. Chincarini, A. Chiummo, A. Colla, A. Conte, A. Corsi, A. Cumming, A. Di Lieto, A. Di Virgilio, A. Dietz, A. E. Villar, A. Effler, A. F. Brooks, A. Freise, A. G. Wiseman, A. Gennai, A. Giazotto, A. Grant, A. Heidmann, A. Ivanov, A. J. Stein, A. J. Weinstein, A. Khalaidovski, A. Królak, A. L. Stuver, A. Lazzarini, A. M. Cruise, A. M. Gretarsson, A. M. Sintes, A. Marandi, A. Markosyan, A. Masserot, A. Melatos, A. Morgia, A. Mullavey, A. Mytidis, A. Nishizawa, A. Nitz, A. P. Lundgren, A. Page, A. Pasqualetti, A. Perreca, A. Rocchi, A. Rüdiger, A. S. Bell, A. S. Stroeer, A. Sergeev, A. Sibley, A. Singer, A. Stochino, A. Thüring, A. Toncelli, A. Vecchio, A. Viceré, A. W. Heptonstall, A. Wade, A. Wanner, A. Zadrożny, Abadie, Abadie, Abadie, Abbott, Abbott, Abbott, Acernese, Arun, B. Allen, B. Barr, B. Behnke, B. Bland, B. Bouhou, B. Canuel, B. Daudert, B. E. Aylott, B. F. Farr, B. F. Schutz, B. F. Whiting, B. Hughey, B. J. J. Slagmolen, B. J. Owen, B. K Kim, B. Krishnan, B. Lantz, B. Machenschalk, B. Moe, B. Mours, B. O’Reilly, B. P. Abbott, B. Rankins, B. S. Sathyaprakash, B. Sassolas, B. Schulz, B. Shapiro, B. Sorazu, B. Swinkels, B. Willke, Beauville, Berger, Berger, Blanchet, Bloom, Buonanno, C. A. Costa, C. Adams, C. Affeldt, C. Aulbert, C. Bogan, C. Bradaschia, C. Buy, C. C. Wipf, C. C. Yancey, C. Cepeda, C. D. Capano, C. D. Ott, C. Gill, C. Graef, C. Gray, C. Greverie, C. Guido, C. H. Lee, C. Hanna, C. I. Torrie, C. Kim, C. L. Mueller, C. Lawrie, C. M. Mow-Lowry, C. M. Reed, C. Messenger, C. Michel, C. N. Colacino, C. Osthelder, C. Palomba, C. Pankow, C. Robinson, C. Rodriguez, C. Röver, C. T. Y. Chung, C. Tomlinson, C. Torres, C. Van Den Broeck, C. Veltkamp, C. Vorvick, C. Wilkinson, C. Zhao, D. A. Brown, D. A. Shaddock, D. Amariutei, D. Atkinson, D. B. Tanner, D. Barker, D. Beck, D. Blair, D. Buskulic, D. C. Coyne, D. Cook, D. DeBra, D. E. Clark, D. E. McClelland, D. Fazi, D. Feldbaum, D. Friedrich, D. G. Keppel, D. H. Reitze, D. H. Shoemaker, D. Hammer, D. Hoak, D. I. Jones, D. J. A. McKechan, D. J. Hosken, D. J. Ottaway, D. J. White, D. Kelley, D. Kozak, D. L. Kinzel, D. Lodhia, D. M. Coward, D. M. Macleod, D. Moraru, D. Murphy, D. Nolting, D. O. Bridges, D. Passuello, D. R. Ingram, D. Rosińska, D. S. Rabeling, D. Sellers, D. Sentenac, D. Sigg, D. Talukder, D. Ugolini, D. Verkindt, D. Yeaton-Massey, Droz, E. A. Khazanov, E. Amador Ceron, E. Black, E. Calloni, E. Cesarini, E. Chassande-Mottin, E. Coccia, E. Cuoco, E. D. Harstad, E. Forsi, E. Genin, E. Goetz, E. J. Daw, E. J. Howell, E. James, E. Jesse, E. K. Gustafson, E. Katsavounidis, E. L. Robinson, E. Macdonald, E. Majorana, E. Maros, E. Ochsner, E. Oelker, E. Schreiber, E. Steinert, E. Thrane, E. Tournefier, F. Acernese, F. Barone, F. Bondu, F. C. Speirits, F. Carbognani, F. Cavalier, F. Clara, F. Cleva, F. Donovan, F. Feroz, F. Fidecaro, F. Frasconi, F. Garufi, F. J. Raab, F. Kawazoe, F. Marchesoni, F. Marion, F. Martelli, F. Matichard, F. Nocera, F. Paoletti, F. Piergiovanni, F. Postiglione, F. Ricci, F. Robinet, F. Salemi, F. Seifert, F. Travasso, F. Vetrano, F. Y. Khalili, F. Zhang, Fielding, G. A. Prodi, G. Ballardin, G. Billingsley, G. Cagnoli, G. Cella, G. Ciani, G. D. Meadors, G. Debreczeni, G. Endrőczi, G. Gemme, G. González, G. H. Ogin, G. Hammond, G. Jones, G. Kang, G. Kuehn, G. Losurdo, G. M. Guidi, G. M. Harry, G. Mazzolo, G. McIntyre, G. Mendell, G. Mitselmakher, G. Moreno, G. Mueller, G. Newton, G. Pagliaroli, G. Persichetti, G. R. Skelton, G. Santostasi, G. Traylor, G. Vajente, G. Vedovato, G. Woan, H. Daveloza, H. Fehrmann, H. Grote, H. Heitmann, H. J. Bulten, H. J. Pletsch, H. K. Lee, H. Kaufer, H. Kim, H. Lück, H. M. Lee, H. Miao, H. Müller-Ebhardt, H. Overmier, H. Radkins, H. S. Cho, H. Vahlbruch, H. Vocca, H. Wittel, H. Yamamoto, H. Yang, I. A. Bilenko, I. Bartos, I. Belopolski, I. Di Palma, I. Ferrante, I. Fiori, I. Kowalska, I. Leonor, I. M. Pinto, I. Maksimovic, I. Mandel, I. Neri, I. Rácz, I. S. Heng, I. Santiago-Prieto, I. W. Harry, I. W. Martin, I. Yakushin, J. A. Giaime, J. Abadie, J. B. Camp, J. B. Kanner, J. Batch, J. Bauchrowitz, J. Betzwieser, J. Birch, J. Breyer, J. Burguet-Castell, J. C. B. Barayoga, J. C. Driggers, J. Cannizzo, J. Cao, J. Chow, J. Clark, J. Colas, J. D. E. Creighton, J. D. Romano, J. E. Brau, J. F. J. van den Brand, J. Franc, J. G. Rollins, J. Gair, J. Garcia, J. Gleason, J. H. Clayton, J. H. Romie, J. Hanks, J. Hanson, J. Harms, J. Heefner, J. Hough, J. J. Oh, J. K. Blackburn, J. Li, J. Lough, J. Luan, J. M. Berliner, J. M. Hallam, J. Marque, J. McIver, J. Miller, J. Munch, J. N. Marx, J. Nelson, J. O’Dell, J. Pöld, J. R. Leong, J. R. Smith, J. R. Taylor, J. S. Kissel, J. Scott, J. Slutsky, J. Soto, J. Steinlechner, J. T. Whelan, J. Veitch, J. Worden, J. Zweizig, J.-C. Dumas, J.-D. Fournier, J.-F. Hayau, J.-P. Coulon, J.-P. Zendri, J.-Y. Vinet, K. A. Hodge, K. A. Strain, K. A. Thorne, K. Agatsuma, K. Arai, K. Cannon, K. D. Giardina, K. Dahl, K. Danzmann, K. Evans, K. Haughian, K. Hayama, K. Holt, K. Izumi, K. Kawabe, K. Kim, K. Kokeyama, K. L. Dooley, K. Mailand, K. Mason, K. Mossavi, K. Redwine, K. Riles, K. Ryan, K. S. Thorne, K. Somiya, K. Tseng, K. V. Tokmakov, K. Wette, K. Yamamoto, Kopparapu, L. A. Forte, L. Barsotti, L. Blackburn, L. Bonelli, L. Bosi, L. C. Stein, L. Cadonati, L. Carbone, L. Cunningham, L. Di Fiore, L. G. Prokhorov, L. Gammaitoni, L. Ju, L. M. Goggin, L. Matone, L. Milano, L. Naticchioni, L. Nuttall, L. Palladino, L. Pekowsky, L. Pinard, L. R. Price, L. Rolland, L. S. Finn, L. Sammut, L. Santamaría, L. Singer, L. Sperandio, L. Taffarello, L. Wade, L. Wallace, L. Wen, L. Williams, L. Winkelmann, L. Zhang, L. Á. Gergely, Li, M. A. Arain, M. A. Barton, M. A. Bizouard, M. A. Hendry, M. A. Papa, M. Abernathy, M. Agathos, M. Barsuglia, M. Bastarrika, M. Bebronne, M. Bejger, M. Benacquista, M. 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Christensen, N. Cornish, N. D. Smith-Lefebvre, N. Fotopoulos, N. Gray, N. Kim, N. Lastzka, N. Leroy, N. Letendre, N. Liguori, N. Man, N. Mavalvala, N. Morgado, N. Zotov, Nakar, O. Bock, O. Chaibi, O. Kranz, O. Miyakawa, O. Puncken, O. Torre, P. A. Willems, P. Ajith, P. Astone, P. Aufmuth, P. B. Graff, P. Baker, P. Campsie, P. Charlton, P. Couvares, P. E. Lindquist, P. Ehrens, P. Fritschel, P. G. Murray, P. Hello, P. J. Fulda, P. J. King, P. J. Sutton, P. J. Veitch, P. Jaranowski, P. K. Lam, P. Kalmus, P. Kwee, P. Leaci, P. Patel, P. Peiris, P. Puppo, P. R. Brady, P. R. Saulson, P. Raffai, P. Rapagnani, P. Ruggi, P. Sainathan, P. Schwinberg, P. Shawhan, P. T. Beyersdorf, P. Thomas, P. Wessels, P. Yu, P.-F. Cohadon, Pan, R. A. Matzner, R. A. Mercer, R. Abbott, R. Adhikari, R. Bassiri, R. Biswas, R. Bondarescu, R. Bonnand, R. Bork, R. Cavalieri, R. Conte, R. Dannenberg, R. Day, R. De Rosa, R. DeRosa, R. DeSalvo, R. Engel, R. Flaminio, R. Frey, R. Geng, R. Gouaty, R. Grosso, R. Gupta, R. 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Winkler, W. Z. Korth, W. Zhang, X. Chen, X. Siemens, X. Wang, Y. Chen, Y. Fan, Y. J. Jang, Y. Liu, Y. M. Kim, Y. Minenkov, Y. Pan, Y. Wan, Z. Du, Z. Frei, Z. Keresztes, Z. Liu, Z. Márka, Z. Wang +815 morecore +9 more sourcesTriangulation of gravitational wave sources with a network of detectors [PDF]
, 2009 There is significant benefit to be gained by pursuing multi-messenger
astronomy with gravitational wave and electromagnetic observations. In order to
undertake electromagnetic follow-ups of gravitational wave signals, it will be
necessary to accurately ..., , , , , , Abbott B (LIGO Scientific), Abbott B (LIGO Scientific), Acernese F, Ajith P, Ajith P Bose S, Allen B, Allen B Anderson W G Brady P R Brown D A Creighton J D E, Aylott B, Beauville F, Beauville F, Birindelli S, Blair D G, Blanchet L, Bloom J S, Brady P R, Dhurandhar S V Tinto M, Dietz A Garofoli J González G Landry M O'Reilly B Sung M, Fender R, Hannam M, Hurley K, Jaynes E T, King A Cannon K, Kopparapu R K, Lindblom L, Lindblom L, Lorimer D R Bailes M McLaughlin M A Narkevic D J Crawford F, Phinney E S, Pretorius F, Prince T A, Searle A, Searle A C, Searle A C, Stamatikos M Gehrels N Halzen F Meszaros P Roming P W A, Stephen Fairhurst, Sutton P Poprocki S, Van Den Broeck C, Van Den Broeck C, Wen L +43 morecore +2 more sourcesIntroduction to Gravitational Wave Astronomy [PDF]
, 2021 This chapter provides an overview of gravitational wave (GW) astronomy, providing background material that underpins the other, more specialized chapters in this handbook. It starts with a brief historical review of the development of GW astronomy, from Einstein's prediction of GWs in 1916 to the first direct detection in 2015.openaire +2 more sourcesCompact Binary Coalescences in the Band of Ground-based
Gravitational-Wave Detectors
, 2010 As the ground-based gravitational-wave telescopes LIGO, Virgo, and GEO 600
approach the era of first detections, we review the current knowledge of the
coalescence rates and the mass and spin distributions of merging neutron-star
and black-hole binaries. , , , Abbott B, Acernese F, Amaro-Seoane P, Aylott B, Belczynski K, Belczynski K, Belczynski K, Belczynski K Bulik T Fryer C L Ruiter A Vink J S Hurley J R, Brady P R, Bulik T, Bulik T Belczynski K, Bulik T Belczynski K Prestwich A, Dietz A, Fregeau J M, Freise A, Gair J R, Gair J R Mandel I Miller M C Volonteri M, Grishchuk L P, Grote H, Hinderer T Lackey B D Lang R N Read J S, Hopman C, Ilya Mandel, Kalogera V, Kalogera V, Kim C, Kim C Kalogera V Lorimer D R, Kopparapu R K, Lee W H Ramirez-Ruiz E van de Ven G, Lorimer D R, Manchester R N, Mandel I, Mandel I, Miller M C, Miller M C, Narayan R, Nelemans G, Nissanke S Hughes S A Holz D E Dalal N Sievers J L, O'Shaughnessy R, O'Shaughnessy R, O'Shaughnessy R, O'Shaughnessy R Kalogera V Belczynski K, O'Shaughnessy R Kim C, O'Shaughnessy R Kopparapu R Belczynski K, Phinney E S, Postnov K, Raymond V, Richard O'Shaughnessy, Röver C, Sadowski A, Sengupta A S (for the LIGO Scientific Collaboration, Sesana A, Sigg D, Smith J R (for the LIGO Scientific Collaboration), Stamatikos M, Thorsett S E, van der Sluys M, van der Sluys M, van der Sluys M V, Veitch J, Veitch J Vecchio A, Vigeland S J Hughes S A, Virgili F J Zhang B O'Brien P Troja E +64 morecore +1 more sourceTeV Particle Astrophysics II: Summary comments [PDF]
, 2006 A unifying theme of this conference was the use of different approaches to
understand astrophysical sources of energetic particles in the TeV range and
above., Abassi R U, Abraham J, Achterberg A (IceCube Collaboration), Allard D, Aloisio R, Blas Cabrera, Bouwhuis M, Budnev N M, Charles Dermer, Coyle P, Dieter Horns, Eckart Lorenz, Eiichiro Komatsu, Elena Aprile, Elisa Bernardini (IceCube), Elisa Resconi, Frank Krennrich, Gabriella Catanesi, Gary Varner, Haino Falcke, Han T, Haungs A, Hillas A M, James Cronin, Jordan Goodman, Julia Becker, Kael Hanson, McKee F, Muraishi H, Neil Cornish, Nicolas Busca, Pasquale Blasi, Peters B, Piero Ullio, Scott Wakely, Shigeru Yoshida, Simon Swordy, Sommers P, Thomas K Gaisser, Thomas K Gaisser, Thomson G B, Tom Weiler +42 morecore +2 more sourcesGravitational wave astronomy with TianQin
Reports on Progress in PhysicsAbstract The opening of the gravitational wave window has significantly enhanced our capacity to explore the Universe’s most extreme and dynamic sector. In the mHz frequency range, a diverse range of compact objects, from the most massive black holes at the farthest reaches of the Universe to the lightest white dwarfs in our cosmic ...En-Kun 恩坤 Li 李, Shuai 帅 Liu 刘, Alejandro Torres-Orjuela, Xian 弦 Chen 陈, Kohei Inayoshi, Long 龙 Wang 王, Yi-Ming 一鸣 Hu 胡, Pau Amaro-Seoane, Abbas Askar, Cosimo Bambi, Pedro R Capelo, Hong-Yu 洪昱 Chen 陈, Alvin J K 靖康 Chua 蔡, Enrique Condés-Breña, Lixin 丽心 Dai 戴, Debtroy Das, Andrea Derdzinski, Hui-Min 会敏 Fan 范, Michiko 井通子 Fujii 藤, Jie 洁 Gao 高, Mudit Garg, Hongwei 宏伟 Ge 葛, Mirek Giersz, Shun-Jia 顺佳 Huang 黄, Arkadiusz Hypki, Zheng-Cheng 正程 Liang 梁, Bin 彬 Liu 刘, Dongdong 栋栋 Liu 刘, Miaoxin 淼昕 Liu 刘, Yunqi 云旗 Liu 刘, Lucio Mayer, Nicola R Napolitano, Peng 朋 Peng 彭, Yong 勇 Shao 邵, Swarnim Shashank, Rongfeng 荣锋 Shen 申, Hiromichi 寛通 Tagawa 田川, Ataru 衝 Tanikawa 谷川, Martina Toscani, Verónica Vázquez-Aceves, Hai-Tian 海天 Wang 王, Han 晗 Wang 王, Shu-Xu 疏序 Yi 易, Jian-dong 建东 Zhang 张, Xue-Ting 雪婷 Zhang 张, Lianggui 良贵 Zhu 朱, Lorenz Zwick, Song 崧 Huang 黄, Jianwei 健伟 Mei 梅, Yan 炎 Wang 王, Yi 懿 Xie 谢, Jiajun 佳骏 Zhang 张, Jun 俊 Luo 罗 +52 moreopenaire +3 more sourcesThe damping of gravitational waves in dust
, 2008 We examine a simple model of interaction of gravitational waves with matter
(primarily represented by dust). The aim is to investigate a possible damping
effect on the intensity of gravitational wave when passing through media., Ehlers J, Ehlers J, Grishchuk L P, Misner C W, Otakar Svítek, Polnarev A G +6 morecore +1 more source
