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Probing the nature of dark matter using strongly lensed gravitational waves from binary black holes
Souvik Jana, Shasvath J. Kapadia, Tejaswi Venumadhav +2
Next-generation ground-based gravitational-wave (GW) detectors are expected to detect millions of binary black hole mergers during their operation period. A small fraction ($\sim 0…
Rates and beaming angles of GRBs associated with compact binary coalescences
Shasvath J. Kapadia, Dimple, Dhruv Jain +3
Some, if not all, binary neutron star (BNS) coalescences, and a fraction of neutron - star black hole (NSBH) mergers, are thought to produce sufficient mass-ejection to power Gamma…
Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
Tathagata Ghosh, Bhaskar Biswas, Sukanta Bose +1
Gravitational waves (GWs) from binary neutron stars (BNSs) are expected to be accompanied by electromagnetic (EM) emissions, which help identify the host galaxy. Since GWs directly…
Profiling stellar environments of gravitational wave sources
Avinash Tiwari, Aditya Vijaykumar, Shasvath J. Kapadia +2
Gravitational waves (GWs) have enabled direct detections of compact binary coalescences (CBCs). However, their poor sky localisation and the typical lack of observable electromagne…
Can the Near-Horizon Black Hole Memory be detected through Binary Inspirals?
Sajad A. Bhat, Srijit Bhattacharjee, Shasvath J. Kapadia
The memory effect, in the context of gravitational-waves (GWs), manifests itself in the permanent relative displacement of test masses when they encounter the GWs. A number of work…
Constraints on compact dark matter from the non-observation of gravitational-wave strong lensing
A. Barsode, S. J. Kapadia, P. Ajith
We use the non-observation of strong lensing of gravitational waves (GWs) in the first three observation runs of LIGO-Virgo detectors to constrain the fraction of dark matter in th…