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Autor:
Yoshida, Sanichiro1 (AUTHOR) sanichiro.yoshida@selu.edu, Pappalettera, Giovanni2 (AUTHOR)
Publikováno v:
Materials (1996-1944). Mar2023, Vol. 16 Issue 5, p2123. 4p.
Autor:
Hayama, Kazuhiro, Desai, Shantanu, Kotake, Kei, Mohanty, Soumya D., Rakhmanov, Malik, Summerscales, Tiffany, Yoshida, Sanichiro
Publikováno v:
Class. Quantum Grav. 25 (2008) 184022
Significant progress has been made in the development of an international network of gravitational wave detectors, such as TAMA300, LIGO, VIRGO, and GEO600. For these detectors, one of the most promising sources of gravitational waves are core collap
Externí odkaz:
http://arxiv.org/abs/0807.4514
Autor:
Hayama, Kazuhiro, Desai, Shantanu, Mohanty, Soumya D., Rakhmanov, Malik, Summerscales, Tiffany, Yoshida, Sanichiro
Publikováno v:
Class. Quant. Grav.25:184021, 2008
Sco X-1, the brightest low mass X-ray binary, is likely to be a source for gravitational wave emission. In one mechanism, emission of a gravitational wave arrests the increase in spin frequency due to the accretion torque in a low mass X-ray binary.
Externí odkaz:
http://arxiv.org/abs/0807.4171
Autor:
Hayama, Kazuhiro, Desai, Shantanu, Mohanty, Soumya D., Rakhmanov, Malik, Summerscales, Tiffany, Yoshida, Sanichiro
Publikováno v:
Class.Quant.Grav.25:184016,2008
Pulsar glitches are a potential source of gravitational waves for current and future interferometric gravitational wave detectors. Some pulsar glitch events were observed by radio and X-ray telescopes during the fifth LIGO science run. It is expected
Externí odkaz:
http://arxiv.org/abs/0807.3983
Autor:
Desai, Shantanu, Hayama, Kazuhiro, Mohanty, Soumya, Rakhmanov, Malik, Summerscales, Tiffany, Yoshida, Sanichiro
Publikováno v:
Class.Quant.Grav.25:184024,2008
We propose to search for gravitational waves from PKS 2155-304 as well as other blazars. PKS 2155-304 emitted a long duration energetic flare in July 2006, with total isotropic equivalent energy released in TeV gamma rays of approximately $10^{45}$ e
Externí odkaz:
http://arxiv.org/abs/0804.3393
Publikováno v:
In Ultrasonics April 2017 76:166-176