Zobrazeno 1 - 10
of 99
pro vyhledávání: '"Mohanty, Soumya D."'
Future space-based laser interferometric detectors, such as LISA, will be able to detect gravitational waves (GWs) generated during the inspiral phase of stellar-mass binary black holes (SmBBHs). The detection and characterization of GWs from SmBBHs
Externí odkaz:
http://arxiv.org/abs/2407.10797
Autor:
Girgaonkar, Raghav, Mohanty, Soumya D.
Publikováno v:
Physical Review D, vol. 110, 023037 (2024)
Transient signals arising from instrumental or environmental factors, commonly referred to as glitches, constitute the predominant background of false alarms in gravitational wave searches with ground-based detectors. Therefore, effective data analys
Externí odkaz:
http://arxiv.org/abs/2401.15237
Neutron star (NS) binaries can be potentially intriguing gravitational wave (GW) sources, with both high- and low-frequency radiations from the possibly aspherical individual stars and the binary orbit, respectively. The successful detection of such
Externí odkaz:
http://arxiv.org/abs/2401.11241
Spinning neutron stars (NSs) can emit continuous gravitational waves (GWs) that carry a wealth of information about the compact object. If such a signal is detected, it will provide us with new insight into the physical properties of matter under ext
Externí odkaz:
http://arxiv.org/abs/2307.01055
We evaluate the prospects for radio follow-up of the double neutron stars (DNSs) in the Galactic disk that could be detected through future space-borne gravitational wave (GW) detectors. We first simulate the DNS population in the Galactic disk that
Externí odkaz:
http://arxiv.org/abs/2305.05202
Transient signals of instrumental and environmental origins ("glitches") in gravitational wave data elevate the false alarm rate of searches for astrophysical signals and reduce their sensitivity. Glitches that directly overlap astrophysical signals
Externí odkaz:
http://arxiv.org/abs/2301.02398
Extracting gravitational wave (GW) signals from individual Galactic binaries (GBs) against their self-generated confusion noise is a key data analysis challenge for space-borne detectors operating in the $\approx 0.1$ mHz to $\approx 10$ mHz range. G
Externí odkaz:
http://arxiv.org/abs/2206.12083
Publikováno v:
Physical Review D Vol. 106, No. 2, 2022
The sensitivity of ongoing searches for gravitational wave (GW) sources in the ultra-low frequency regime ($10^{-9}$ Hz to $10^{-7}$ Hz) using Pulsar Timing Arrays (PTAs) will continue to increase in the future as more well-timed pulsars are added to
Externí odkaz:
http://arxiv.org/abs/2110.14959
Autor:
Songsheng, Yu-Yang, Qian, Yi-Qian, Li, Yan-Rong, Du, Pu, Chen, Jie-Wen, Wang, Yan, Mohanty, Soumya D., Wang, Jian-Min
Detecting continuous nanohertz gravitational waves (GWs) generated by individual close binaries of supermassive black holes (CB-SMBHs) is one of the primary objectives of pulsar timing arrays (PTAs). The detection sensitivity is slated to increase si
Externí odkaz:
http://arxiv.org/abs/2109.00367
Autor:
Zou, Xiao-Bo1,2,3,4 (AUTHOR) zouxb18@lzu.edu.cn, Mohanty, Soumya D.2,5 (AUTHOR) soumya.mohanty@utrgv.edu, Luo, Hong-Gang1,4 (AUTHOR) luohg@lzu.edu.cn, Liu, Yu-Xiao1,3,4 (AUTHOR) liuyx@lzu.edu.cn
Publikováno v:
Universe (2218-1997). Apr2024, Vol. 10 Issue 4, p171. 20p.