activity
20242026
collaborators

6 papers

gr-qc2026

Dynamical tidal response of neutron stars via scattering amplitudes

M. V. S. Saketh, Suprovo Ghosh, Nils Andersson

A key challenge of gravitational-wave physics is distinguishing the nature of compact objects in binary coalescences, in particular whether they are black holes or neutron stars. N…

gr-qc2026

Dynamical tidal Love numbers of black holes under generic perturbations: Connecting black hole perturbation theory with effective field theory

Sumanta Chakraborty, M. V. S Saketh, Tanja Hinderer +1

The foundation for modeling the coupling of the internal structure of compact objects in binary systems to their dynamics and emitted gravitational waves is a systematic effective…

gr-qc2025

Strong-field Gravitational Wave Lensing in the Kerr Background

M. V. S. Saketh, Rajes Ghosh, Anuj Mishra

Gravitational-wave (GW) lensing can encode valuable information about the properties of the intervening lens, but most existing studies remain restricted to the small-deflection, w…

gr-qc2025

Kerr-Newman quasinormal modes and Seiberg-Witten theory

Hector O. Silva, Jung-Wook Kim, M. V. S. Saketh

It was recently suggested the quasinormal-mode spectrum of black holes is related to a class of four-dimensional super Yang-Mills theories described by Seiberg-Witt…

gr-qc2024

Investigating tidal heating in neutron stars via gravitational Raman scattering

M. V. S. Saketh, Zihan Zhou, Suprovo Ghosh +2

We present a scattering amplitude formalism to study the tidal heating effects of nonspinning neutron stars incorporating both worldline effective field theory and relativistic ste…

gr-qc2024

Quasinormal modes of slowly-spinning horizonless compact objects

M. V. S. Saketh, Elisa Maggio

One of the main predictions of general relativity is the existence of black holes featuring a horizon beyond which nothing can escape. Gravitational waves from the remnants of comp…