Keresés
1 találatból megjelenítve: 1-1
Cím: LIGO: the Laser Interferometer Gravitational-Wave Observatory
Szerző: ; ; ; ; ; ; ; ; ; ; Araya, M; Armandula, H; Armor, P; Aso, Y; Aston, S; Aufmuth, P; Aulbert, C; Babak, S; Baker, P; Ballmer, S; Barker, C; Barker, D; Barr, B; Barriga, P; Barsotti, L; Barton, MA; Bartos, I; Bassiri, R; Bastarrika, M; Behnke, B; Benacquista, M; Betzwieser, J; Beyersdorf, PT; Bilenko, IA; Billingsley, G; Biswas, R; Black, E; Blackburn, JK; Blackburn, L; Blair, D; Bland, B; Bodiya, TP; Bogue, L; Bork, R; Boschi, V; Bose, S; Brady, PR; Braginsky, VB; Brau, JE; Bridges, DO; Brinkmann, M; Brooks, AF; Brown, DA; Brummit, A; Brunet, G; Bullington, A; Buonanno, A; Burmeister, O; Byer, RL; Cadonati, L; Camp, JB; Cannizzo, J; Cannon, KC; Cao, J; Cardenas, L; Caride, S; Castaldi, G; Caudill, S; Cavaglia, M; Cepeda, C; Chalermsongsak, T; Chalkley, E; Charlton, P; Chatterji, S; Chelkowski, S; Chen, Y; Christensen, N; Chung, CTY; Clark, D; Clark, J; Clayton, JH; Cokelaer, T; Colacino, CN; Conte, R; Cook, D; Corbitt, TRC; Cornish, N; Coward, D; Coyne, DC; Creighton, JDE; Creighton, TD; Cruise, AM; Culter, RM; Cumming, A; Cunningham, L; Danilishin, SL; Danzmann, K; Daudert, B; Davies, G; Daw, EJ; DeBra, D; Degallaix, J; Dergachev, V; Desai, S; DeSalvo, R; Dhurandhar, S; Diaz, M; Dietz, A; Donovan, F; Dooley, KL; Doomes, EE; Drever, RP; Dueck, J; Duke, I; Dumas, JC; Dwyer, JG; Echols, C; Edgar, M; Effler, A; Ehrens, P; Espinoza, E; Etzel, T; Evans, M; Evans, T; Fairhurst, S; Faltas, Y; Fan, Y; Fazi, D; Fehrmenn, H; Finn, LS; Flasch, K; Foley, S; Forrest, C; Fotopoulos, N; Franzen, A; Frede, M; Frei, M; Frei, Z; Freise, A; Frey, R; Fricke, T; Fritschel, P; Frolov, VV; Fyffe, M; Galdi, V; Garofoli, JA; Gholami, I; Giaime, JA; Giampanis, S; Giardina, KD; Goda, K; Goetz, E; Goggin, LM; Gonzalez, G; Gorodetsky, ML; Gossler, S; Gouaty, R; Grant, A; Gras, S; Gray, C; Gray, M; Greenhalgh, RJS; Gretarsson, AM; Grimaldi, F; Grosso, R; Grote, H; Grunewald, S; Guenther, M; Gustafson, EK; Gustafson, R; Hage, B; Hallam, JM; Hammer, D; Hammond, GD; Hanna, C; Hanson, J; Harms, J; Harry, GM; Harry, IW; Harstad, ED; Haughian, K; Hayama, K; Heefner, J; Heng, IS; Heptonstall, A; Hewitson, M; Hild, S; Hirose, E; Hoak, D; Hodge, KA; Holt, K; Hosken, DJ; Hough, J; Hoyland, D; Hughey, B; Huttner, SH; Ingram, DR; Isogai, T; Ito, M; Ivanov, A; Johnson, B; Johnson, WW; Jones, DI; Jones, G; Jones, R; Ju, L; Kalmus, P; Kalogera, V; Kandhasamy, S; Kanner, J; Kasprzyk, D; Katsavounidis, E; Kawabe, K; Kawamura, S; Kawazoe, F; Kells, W; Keppel, DG; Khalaidovski, A; Khalili, FY; Khan, R; Khazanov, E; King, P; Kissel, JS; Klimenko, S; Kokeyama, K; Kondrashov, V; Kopparapu, R; Koranda, S; Kozak, D; Krishnan, B; Kumar, R; Kwee, P; Lam, PK; Landry, M; Lantz, B; Lazzarini, A; Lei, H; Lei, M; Leindecker, N; Leonor, I; Li, C; Lin, H; Lindquist, PE; Littenberg, TB; Lockerbie, NA; Lodhia, D; Longo, M; Lormand, M; Lu, P; Lubinski, M; Lucianetti, A; Luck, H; Machenschalk, B; MacInnis, M; Mageswaran, M; Mailand, K; Mandel, I; Mandic, V; Marka, S; Marka, Z; Markosyan, A; Markowitz, J; Maros, E; Martin, IW; Martin, RM; Marx, JN; Mason, K; Matichard, F; Matone, L; Matzner, RA; Mavalvala, N; McCarthy, R; McClelland, DE; McGuire, SC; McHugh, M; McIntyre, G; McKechan, DJA; McKenzie, K; Mehmet, M; Melatos, A; Melissinos, AC; Menendez, DF; Mendell, G; Mercer, RA; Meshkov, S; Messenger, C; Meyer, MS; Miller, J; Minelli, J; Mino, Y; Mitrofanov, VP; Mitselmakher, G; Mittleman, R; Miyakawa, O; Moe, B; Mohanty, SD; Mohapatra, SRP; Moreno, G; Morioka, T; Mors, K; Mossavi, K; MowLowry, C; Mueller, G; Muller-Ebhardt, H; Muhammad, D; Mukherjee, S; Mukhopadhyay, H; Mullavey, A; Munch, J; Murray, PG; Myers, E; Myers, J; Nash, T; Nelson, J; Newton, G; Nishizawa, A; Numata, K; O'Dell, J; O'Reilly, B; O'Shaughnessy, R; Ochsner, E; Ogin, GH; Ottaway, DJ; Ottens, RS; Overmier, H; Owen, BJ; Pan, Y; Pankow, C; Papa, MA; Parameshwaraiah, V; Patel, P; Pedraza, M; Penn, S; Perraca, A; Pierro, V; Pinto, IM; Pitkin, M; Pletsch, HJ; Plissi, MV; Postiglione, F; Principe, M; Prix, R; Prokhorov, L; Punken, O; Quetschke, V; Raab, FJ; Rabeling, DS; Radkins, H; Raffai, P; Raics, Z; Rainer, N; Rakhmanov, M; Raymond, V; Reed, CM; Reed, T; Rehbein, H; Reid, S; Reitze, DH; Riesen, R; Riles, K; Rivera, B; Roberts, P; Robertson, NA; Robinson, C; Robinson, EL; Roddy, S; Rover, C; Rollins, J; Romano, JD; Romie, JH; Rowan, S; Rudiger, A; Russell, P; Ryan, K; Sakata, S; de la, Jordana LS; Sandberg, V; Sannibale, V; Santamaria, L; Saraf, S; Sarin, P; Sathyaprakash, BS; Sato, S; Satterthwaite, M; Saulson, PR; Savage, R; Savov, P; Scanlan, M; Schilling, R; Schnabel, R; Schofield, R; Schulz, B; Schutz, BF; Schwinberg, P; Scott, J; Scott, SM; Searle, AC; Sears, B; Seifert, F; Sellers, D; Sengupta, AS; Sergeev, A; Shapiro, B; Shawhan, P; Shoemaker, DH; Sibley, A; Siemens, X; Sigg, D; Sinha, S; Sintes, AM; Slagmolen, BJJ; Slutsky, J; Smith, JR; Smith, MR; Smith, ND; Somiya, K; Sorazu, B; Stein, A; Stein, LC; Steplewski, S; Stochino, A; Stone, R; Strain, KA; Strigin, S; Stroeer, A; Stuver, AL; Summerscales, TZ; Sun, KX; Sung, M; Sutton, PJ; Szokoly, GP; Talukder, D; Tang, L; Tanner, DB; Tarabrin, SP; Taylor, JR; Taylor, R; Thacker, J; Thorne, KA; Thuring, A; Tokmakov, KV; Torres, C; Torrie, C; Traylor, G; Trias, M; Ugolini, D; Ulmen, J; Urbanek, K; Vahlbruch, H; Vallisneri, M; Van, den Broeck C; van der Sluys, MV; van Veggel, AA; Vass, S; Vaulin, R; Vecchio, A; Veitch, J; Veitch, P; Veltkamp, C; Villar, A; Vorvick, C; Vyachanin, SP; Waldman, SJ; Wallace, L; Ward, RL; Weidner, A; Weinert, M; Weinstein, AJ; Weiss, R; Wen, L; Wen, S; Wette, K; Whelan, JT; Whitcomb, SE; Whiting, BF; Wilkinson, C; Willems, PA; Williams, HR; Williams, L; Willke, B; Wilmut, I; Winkelmann, L; Winkler, W; Wipf, CC; Wiseman, AG; Woan, G; Wooley, R; Worden, J; Wu, W; Yakushin, I; Yamamoto, H; Yan, Z; Yoshida, S; Zanolin, M; Zhang, J; Zhang, L; Zhao, C; Zotov, N; Zucker, ME; zur, Muhlen H; Zweizig, J
Dátum: 2009
Feltöltve: 2020-08-11
(2009)
The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves (GWs) of astrophysical origin. Direct detection of GWs holds the promise of testing general relativity ...