activity
20092026
most citedFundamental Physics with the Square Kilometre Array

385 citations · 3.2k across the 77 of their papers we have counts for

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Showing 2025Show all

14 papers · 1 filter

gr-qc2025

Strong lensing cosmography using binary-black-hole mergers: Prospects for the near future

Koustav N. Maity, Souvik Jana, Tejaswi Venumadhav +2

A small fraction of gravitational-wave (GW) signals from binary black holes (BBHs) will be gravitationally lensed by intervening galaxies and galaxy clusters. Strong lensing will p…

gr-qc2025

Data-driven extraction and phenomenology of eccentric harmonics in eccentric spinning binary black hole mergers

Tousif Islam, Tejaswi Venumadhav, Ajit Kumar Mehta +6

Newtonian and post-Newtonian (PN) calculations indicate that the phenomenology of eccentric binary black hole (BBH) merger waveforms is significantly more complex than that of thei…

astro-ph.HE2025★ 1 cited

A New Search Pipeline for Short Gamma Ray Bursts in Fermi/GBM Data -- A 50% Increase in the Number of Detections

Ariel Perera, Barak Zackay, Tejaswi Venumadhav

In this paper, we present the development and the results of a new search pipeline for short gamma-ray bursts (sGRBs) in the publicly available data from the Gamma-Ray Burst Monito…

gr-qc2025★ 2 cited

Binary black hole population inference combining confident and marginal events from the search pipeline

Ajit Kumar Mehta, Digvijay Wadekar, Isha Anantpurkar +6

We present the population properties of binary black hole mergers identified by the pipeline (which incorporates higher-order modes in the search templates) du…

gr-qc2025

Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation

Digvijay Wadekar, Arush Pimpalkar, Mark Ho-Yeuk Cheung +9

We introduce a machine learning (ML) framework called for improving the sensitivity of gravitational wave search pipelines. Typically, search pipelines only use a s…

gr-qc2025

Sampler-free gravitational wave inference using matrix multiplication

Jonathan Mushkin, Javier Roulet, Barak Zackay +5

Parameter estimation (PE) for compact binary coalescence (CBC) events observed by gravitational wave (GW) laser interferometers is a core task in GW astrophysics. We present a meth…

gr-qc2025

Relativistic and Dynamical Love

Abhishek Hegade K. R., K. J. Kwon, Tejaswi Venumadhav +2

Gravitational waves emitted in the late inspiral of binary neutron stars are affected by their tidal deformation. We study the tidal dynamics in full general relativity through mat…

gr-qc2025

Searching for intermediate mass ratio binary black hole mergers in the third observing run of LIGO-Virgo-KAGRA

Mark Ho-Yeuk Cheung, Digvijay Wadekar, Ajit Kumar Mehta +6

Intermediate mass ratio inspirals (IMRIs) of binary black holes with mass ratios are astrophysically interesting sources of gravitational waves. Me…

astro-ph.CO2025

Primordial magnetic fields and modified recombination histories

Jonathan Schiff, Tejaswi Venumadhav

Recent cosmological data and astrophysical observations, such as the Hubble tension and the increasing preference from galaxy surveys for dynamical dark energy, have begun to chall…

astro-ph.HE2025

gwharmone: first data-driven surrogate for eccentric harmonics in binary black hole merger waveforms

Tousif Islam, Tejaswi Venumadhav, Ajit Kumar Mehta +6

We present gwharmone, the first data-driven surrogate model for eccentric harmonics (as well as the full radiation content) of the dominant quadrupolar mode in eccentric, non-spinn…

gr-qc2025★ 7 cited

Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms

Tousif Islam, Tejaswi Venumadhav, Ajit Kumar Mehta +6

Newtonian and post-Newtonian (PN) calculations suggest that each spherical harmonic mode of the gravitational waveforms (radiation) emitted by eccentric binaries can be further dec…

gr-qc2025

Resonance locking: radian-level phase shifts due to nonlinear hydrodynamics of -modes in merging neutron star binaries

K. J. Kwon, Hang Yu, Tejaswi Venumadhav

A neutron star (NS) in a binary system deforms due to the companion's tidal gravitational field. As the binary inspirals due to gravitational wave (GW) emission, the NS's deformati…

gr-qc2025

Significant increase in sensitive volume of a gravitational wave search upon including higher harmonics

Ajit Kumar Mehta, Digvijay Wadekar, Javier Roulet +6

Most gravitational wave searches to date have included only the quadrupole mode in their search templates. Here, we demonstrate that incorporating higher harmonics improves the sea…

gr-qc2025★ 7 cited

Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms

Tousif Islam, Tejaswi Venumadhav

Characterizing eccentricity in gravitational waveforms in a consistent manner is crucial to facilitate parameter estimation, astrophysical population studies, as well as searches f…