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pro vyhledávání: '"Lo, Rico Ka Lok"'
Publikováno v:
journal = {Phys. Rev. D}, volume = {105}, issue = {2}, pages = {024016}, numpages = {36}, year = {2022}, month = {Jan}
The gravitational radiation from the ringdown of a binary black hole merger is described by the solution of the Teukolsky equation, which predicts both the temporal dependence and the angular distribution of the emission. Many studies have explored t
Externí odkaz:
http://arxiv.org/abs/2110.03116
Autor:
Sachdev, Surabhi, Magee, Ryan, Hanna, Chad, Cannon, Kipp, Singer, Leo, SK, Javed Rana, Mukherjee, Debnandini, Caudill, Sarah, Chan, Chiwai, Creighton, Jolien D. E., Ewing, Becca, Fong, Heather, Godwin, Patrick, Huxford, Rachael, Kapadia, Shasvath, Li, Alvin K. Y., Lo, Rico Ka Lok, Meacher, Duncan, Messick, Cody, Mohite, Siddharth R., Nishizawa, Atsushi, Ohta, Hiroaki, Pace, Alexander, Reza, Amit, Sathyaprakash, B. S., Shikauchi, Minori, Singh, Divya, Tsukada, Leo, Tsuna, Daichi, Tsutsui, Takuya, Ueno, Koh
Binary neutron stars (BNSs) will spend $\simeq 10$ -- 15 minutes in the band of Advanced LIGO and Virgo detectors at design sensitivity. Matched-filtering of gravitational-wave (GW) data could in principle accumulate enough signal-to-noise ratio (SNR
Externí odkaz:
http://arxiv.org/abs/2008.04288
Akademický článek
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Autor:
Xiang Li1 xiangli@tapir.caltech.edu, Ling Sun2,3, Lo, Rico Ka Lok2, Payne, Ethan2,3,4,5, Yanbei Chen1
Publikováno v:
Physical Review D: Particles, Fields, Gravitation & Cosmology. 1/15/2022, Vol. 105 Issue 2, p1-1. 1p.
