activity
20092026
most citedFundamental Physics with the Square Kilometre Array

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

collaborators

79 papers

gr-qc2026

Nonlinear Perturbations of Relativistic Stars

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

We extend the general relativistic Lagrangian perturbation formalism of Friedman and Schutz [Astrophys. J. 200, 204 (1975)] beyond linear order, retaining full time dependence of t…

math.AG2026

The non-abelian Hodge correspondence for extensions on quasi-projective curves

Quoc-Anh Tran

Let be a smooth projective connected complex curve, be a finite set of reduced points, and . We give a moduli-theoretic constructi…

astro-ph.HE2026

A Multi-Mission Detection Framework for High-Energy Transients: Application to a 13-year Fermi/GBM and Swift/BAT Sample

Ariel Perera, Barak Zackay, Tejaswi Venumadhav

The detection of faint high-energy transients is becoming increasingly important in time-domain and multi-messenger astronomy, particularly for identifying electromagnetic counterp…

gr-qc2026

Probing Dark Matter with Strongly Lensed Binary Black Hole Mergers: Prospects in the Near Future

Koustav N. Maity, Souvik Jana, Ankur Barsode +2

Gravitational-wave~(GW) transients, strongly lensed by intervening galaxies and clusters, are expected to constitute a small fraction (-) of the events detectable…

gr-qc2026

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions

Hang Yu, Giorgio Nicolini, Shu Yan Lau +6

We study tides during the inspiral of a binary neutron star system, including nonlinear hydrodynamical interactions. Using an affine approximation that treats the perturbed neutron…

astro-ph.CO2026

The diffraction-lensing interpretation of GW231123 with astrophysical priors

Mark Ho-Yeuk Cheung, Digvijay Wadekar, Matias Zaldarriaga +3

GW231123, if unlensed, is a rare binary black hole merger with high masses and high spins for both progenitors. We show that the signal is better fitted by a lower-mass, lower-spin…

gr-qc2026

Discovery of Interpretable Surrogates via Agentic AI: Application to Gravitational Waves

Tousif Islam, Digvijay Wadekar, Tejaswi Venumadhav +4

Fast surrogate models for expensive simulations are now essential across the sciences, yet they typically operate as black boxes. We present \texttt{GWAgent}, a large language mode…

gr-qc2026

The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response

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

Time-dependent tidal interactions during the late inspiral of binary neutron stars encode valuable information about neutron-star structure, but systematically extending the famili…

astro-ph.HE2026★ 1 cited

Expanding the Population of Short Gamma-Ray Transients with a Coherent Fermi/GBM Search. A 13-year catalog of short GRBs

Ariel Perera, Barak Zackay, Tejaswi Venumadhav

In this paper, we present an archival search for short gamma-ray bursts (sGRBs) over 13 years (2013-2025) of Fermi/GBM data using a Poisson matched-filter pipeline that performs a…

astro-ph.HE2026

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog

Tousif Islam, Tejaswi Venumadhav, Digvijay Wadekar +6

We provide a comprehensive analysis of GW190711_030756 and GW200114_020818, two of the most significant binary black hole merger candidates in the IAS catalog, with probabilities o…

gr-qc2026

Searching for precessing binary systems with mode-by-mode filtering and marginalization

Zihan Zhou, Digvijay Wadekar, Javier Roulet +8

Nearly all previous binary black hole searches in LIGO--Virgo--KAGRA (LVK) gravitational wave data have assumed that the component spins are aligned with the orbital angular moment…

astro-ph.HE2026

Progenitor of the recoiling super-massive black hole RBH-1 identified using HST/JWST imaging

Tousif Islam, Tejaswi Venumadhav, Digvijay Wadekar

Using a combination of \textit{Hubble Space Telescope} and \textit{James Webb Space Telescope} imaging, a runaway supermassive black hole (RBH-1) was recently identified with an in…

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…