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Cosmography using strongly lensed gravitational waves from binary black holes
Souvik Jana, Shasvath J. Kapadia, Tejaswi Venumadhav +1
Third generation gravitational wave (GW) detectors are expected to detect millions of binary black hole (BBH) mergers during their operation period. A small fraction of them ($\sim…
Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
Soummyadip Basak, Aditya Kumar Sharma, Shasvath J. Kapadia +1
We study the prospects of detecting continuous gravitational waves (CGWs) from spinning neutron stars (NSs), gravitationally lensed by the galactic supermassive black hole. Assumin…
Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
Aditya Vijaykumar, Shasvath J. Kapadia, Parameswaran Ajith
The postmerger gravitational-wave (GW) signal of a binary neutron star (BNS) merger is expected to contain valuable information that could shed light on the equation of state (EOS)…
Improved early-warning estimates of luminosity distance and orbital inclination of compact binary mergers using higher modes of gravitational radiation
Mukesh Kumar Singh, Divyajyoti, Shasvath J. Kapadia +2
The pre-merger (early-warning) gravitational-wave (GW) detection and localization of a compact binary merger would enable astronomers to capture potential electromagnetic (EM) emis…