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20132026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 10.8k across the 78 of their papers we have counts for

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gr-qc2026

Line-of-Sight Acceleration-driven waveform corrections for unequal-mass compact binary coalescences

Mohd Asim Ansari, Avinash Tiwari, Sajad A. Bhat +2

A constant line-of-sight acceleration (LOSA) of the centre-of-mass of a quasi-circular compact binary coalescence (CBC) leads to modulations in the gravitational-wave (GW) waveform…

gr-qc2026

Line-of-sight Acceleration Driven Effects in Eccentric Compact Binary Coalescences

Mohd Asim Ansari, Avinash Tiwari, Sajad A. Bhat +2

The line-of-sight acceleration (LOSA) effect, imprinted in the gravitational wave (GW) signal of an inspiralling compact binary by an external gravitational potential, is one of th…

gr-qc2026

Probing magnetic fields of compact objects with continuous gravitational waves

Gopalkrishna Prabhu, Aditya Kumar Sharma, R. Prasad +2

Spinning, deformed compact objects such as neutron stars are canonical sources of continuous gravitational waves. These objects may be born with magnetic fields that can strongly i…

gr-qc2026

A product template bank to search for compact binary coalescences microlensed by isolated point mass lenses

Sudhir Gholap, Sanjeev V. Dhurandhar, Shasvath J. Kapadia

Gravitational waves (GW) from stellar mass compact binary coalescences (CBCs) that encounter a lens whose Schwarzschild radius is comparable to the GW wavelength, will be microlens…

gr-qc2026

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits

Avinash Tiwari, Shasvath J. Kapadia, Aditya Vijaykumar +1

The centre of mass (CoM) of compact binary coalescences (CBCs) occurring in the vicinity of a supermassive black hole, through interaction with an arbitrary third body (e.g., of st…

gr-qc2025

Probing the spin of compact objects with gravitational microlensing of gravitational waves

Gopalkrishna Prabhu, Uddeepta Deka, Sumanta Chakraborty +1

Propagating gravitational waves (GWs) can encounter a massive object (lens) whose gravitational radius is comparable to the wavelength of the GWs (wave-optics regime). The resultin…