Results 41 to 50 of about 2,866,947 (383)

Probing supermassive black hole binaries with orbital resonances of laser-ranged satellites

European Physical Journal C: Particles and Fields, 2023
Coalescing supermassive black hole binaries (SMBHBs) are the primary source candidates for low frequency gravitational wave (GW) detections, which could bring us deep insights into galaxy evolutions over cosmic time and violent processes of spacetime ...
Minghui Du, Qiong Deng, Yifan Bian, Ziren Luo, Peng Xu   +4 more
doaj   +1 more source

Gravitational-wave physics and astronomy in the 2020s and 2030s

Nature Reviews Physics, 2021
The 100 years since the publication of Albert Einstein’s theory of general relativity saw significant development of the understanding of the theory, the identification of potential astrophysical sources of sufficiently strong gravitational waves and ...
M. Bailes, B. Berger, P. Brady, M. Branchesi, K. Danzmann, M. Evans, K. Holley-Bockelmann, B. Iyer, T. Kajita, S. Katsanevas, M. Kramer, A. Lazzarini, L. Lehner, G. Losurdo, H. Lück, D. McClelland, M. Mclaughlin, M. Punturo, S. Ransom, Somak Raychaudhury, D. Reitze, F. Ricci, S. Rowan, Y. Saito, G. Sanders, B. Sathyaprakash, B. Schutz, A. Sesana, H. Shinkai, X. Siemens, D. Shoemaker, J. Thorpe, J. V. D. van den Brand, S. Vitale   +33 more
semanticscholar   +1 more source

Review of closed drift thruster neutral flow dynamics

AIP Advances, 2023
Operation of closed drift thruster (CDT) relies mainly on neutral gas, whose trajectory and distribution in the flow field have a significant influence on performance.
Shixu Lu, Liexiao Dong, Wei Luo, Shengtao Liang, Jianfei Long, Xiaocheng Zhu, Ning Guo, Luxiang Xu   +7 more
doaj   +1 more source

A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses

Galaxies, 2021
Quantum noise limits the sensitivity of laser interferometric gravitational-wave detectors. Given the state-of-the-art optics, the optical losses define the lower bound of the best possible quantum-limited detector sensitivity.
Teng Zhang, Joe Bentley, Haixing Miao
doaj   +1 more source

Advanced Virgo: a second-generation interferometric gravitational wave detector [PDF]

, 2014
Advanced Virgo is the project to upgrade the Virgo interferometric detector of gravitational waves, with the aim of increasing the number of observable galaxies (and thus the detection rate) by three orders of magnitude. The project is now in an advanced
F. Acernese, M. Agathos, K. Agatsuma, D. Aisa, N. Allemandou, A. Allocca, J. Amarni, P. Astone, G. Balestri, G. Ballardin, F. Barone, J. Baronick, M. Barsuglia, A. Basti, F. Basti, T. Bauer, V. Bavigadda, M. Bejger, M. Beker, C. Belczynski, D. Bersanetti, A. Bertolini, M. Bitossi, M. Bizouard, S. Bloemen, M. Blom, M. Boer, G. Bogaert, D. Bondi, F. Bondu, L. Bonelli, R. Bonnand, V. Boschi, L. Bosi, T. Bouedo, C. Bradaschia, M. Branchesi, T. Briant, A. Brillet, V. Brisson, T. Bulik, H. Bulten, D. Buskulic, C. Buy, G. Cagnoli, E. Calloni, C. Campeggi, B. Canuel, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, E. Mottin, A. Chincarini, A. Chiummo, S. Chua, F. Cleva, E. Coccia, P. Cohadon, A. Colla, M. Colombini, A. Conte, J. Coulon, E. Cuoco, A. Dalmaz, S. D’Antonio, V. Dattilo, M. Davier, R. Day, G. Debreczeni, J. Degallaix, S. Del'eglise, W. D. Pozzo, H. Dereli, R. Rosa, L. Fiore, A. Lieto, A. Virgilio, M. Doets, V. Dolique, M. Drago, M. Ducrot, G. Endrőczi, V. Fafone, S. Farinon, I. Ferrante, F. Ferrini, F. Fidecaro, I. Fiori, R. Flaminio, J. Fournier, S. Franco, S. Frasca, F. Frasconi, L. Gammaitoni, F. Garufi, M. Gaspard, A. Gatto, G. Gemme, B. Gendre, Eric Genin, A. Gennai, S. Ghosh, L. Giacobone, A. Giazotto, R. Gouaty, M. Granata, G. Greco, P. Groot, G. Guidi, J. Harms, A. Heidmann, H. Heitmann, P. Hello, G. Hemming, E. Hennes, D. Hofman, P. Jaranowski, R. Jonker, M. Kasprzack, F. K'ef'elian, I. Kowalska, M. Kraan, A. Kr'olak, A. Kutynia, C. Lazzaro, M. Leonardi, N. Leroy, N. Letendre, T. G. F. Li, B. Lieunard, M. Lorenzini, V. Loriette, G. Losurdo, C. Magazzù, E. Majorana, I. Maksimovic, V. Malvezzi, N. Man, V. Mangano, M. Mantovani, F. Marchesoni, F. Marion, J. Marque, F. Martelli, L. Martellini, A. Masserot, D. Meacher, J. Meidam, F. Mezzani, C. Michel, L. Milano, Y. Minenkov, A. Moggi, M. Mohan, M. Montani, N. Morgado, B. Mours, F. Mul, M. Nagy, I. Nardecchia, L. Naticchioni, G. Nelemans, I. Neri, M. Neri, F. Nocera, E. Pacaud, C. Palomba, F. Paoletti, A. Paoli, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Perciballi, S. Petit, M. Pichot, F. Piergiovanni, G. Pillant, A. Piluso, L. Pinard, R. Poggiani, M. Prijatelj, G. Prodi, M. Punturo, P. Puppo, D. Rabeling, I. R'acz, P. Rapagnani, M. Razzano, V. Re, T. Regimbau, F. Ricci, F. Robinet, A. Rocchi, L. Rolland, R. Romano, D. Rosińska, P. Ruggi, E. Saracco, B. Sassolas, F. Schimmel, D. Sentenac, V. Sequino, S. Shah, K. Siellez, N. Straniero, B. Swinkels, M. Tacca, M. Tonelli, F. Travasso, M. Turconi, G. Vajente, N. van Bakel, M. van Beuzekom, J. V. D. van den Brand, C. Van Den Broeck, M. van der Sluys, J. van Heijningen, M. Vas'uth, G. Vedovato, J. Veitch, D. Verkindt, F. Vetrano, A. Vicer'e, J. Vinet, G. Visser, H. Vocca, R. Ward, M. Was, L.-W. Wei, M. Yvert, A. Z. zny, J. Zendri   +233 more
semanticscholar   +1 more source

Gravitational waves [PDF]

Nuclear Physics B - Proceedings Supplements, 1994
In the last few years there have been a number of significant developments in research towards the detection of gravitational radiation from astronomical objects. The construction of 3 large-scale (3- or 4-km) interferometric detectors has been funded; new high-sensitivity bars are under construction; there is a serious proposal using two ...
openaire   +4 more sources

Thermal Gravitational Waves [PDF]

The Open Astronomy Journal, 2011
20 pages, 57 ...
Sivaram, C., Arun, Kenath
openaire   +2 more sources

Mapping the gravitational wave background [PDF]

, 2001
The gravitational wave sky is expected to have isolated bright sources superimposed on a diffuse gravitational wave background. The background radiation has two components: a confusion limited background from unresolved astrophysical sources; and a ...
, Abramovici A, Bender P L, Brink D M, Cornish N J, Cornish N J, Cornish N J, Cornish N J, Giampieri G, Hellings R W, Hogan C J, Neil J Cornish, Peterseim M, Tinto M, Vecchio A   +14 more
core   +3 more sources

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral [PDF]

, 2017
On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral.
The Ligo Scientific Collaboration, The Virgo Collaboration   +1 more
semanticscholar   +1 more source

Evanescent gravitational waves [PDF]

Physical Review D, 2020
We describe the properties of evanescent gravitational waves (EGWs)---wave solutions of Einstein equations which decay exponentially in some direction while propagating in another. Evanescent waves are well-known in acoustics and optics and have recently received much attention due to their extraordinary properties such as their transverse spin and ...
Golat, Sebastian, Lim, Eugene A., Rodríguez-Fortuño, Francisco J.   +2 more
openaire   +4 more sources