activity
20182026
most citedA "no-hair" test for binary black holes

53 citations · 66 across the 11 of their papers we have counts for

collaborators

12 papers

physics.chem-ph2026

Electronic Density versus Geometry for Machine-Learned Molecular Absorption Spectra

Siddharth Dhanpal, Peter Elliott, Paolo Emilio Trevisanutto +2

Molecular optical absorption spectroscopy provides a direct probe of electronic structure and is widely used for molecular identification, interpretation of photophysical behaviour…

quant-ph2026

Physics-Informed Graph-Neural Decoding of the Surface Code: the Logical Signal as an Exact Topological Pairing

P. E. Trevisanutto, S. Dhanpal, S. Basak +2

We develop a physics-informed graph neural network (GNN) decoder for the surface code that solves a discrete Poisson equation on the syndrome graph, with the syndrome as the charge…

astro-ph.SR2026

Period spacings and global seismic parameters for K2 red giants using deep learning

Nipun Ghanghas, Siddharth Dhanpal, Shravan Hanasoge +2

Gravity-mode period spacings (DPi_1) of red giants probe the stellar core directly, constraining its structure, mass and evolutionary state. Their measurement requires resolving na…

astro-ph.SR2026

Potential of Gaia XP Spectra in Red Giant Star Asteroseismology: A Deep-Learning Approach

Rajarshi Barman, Shatanik Bhattacharya, Shravan M. Hanasoge +1

Red giants are tracers of stellar evolution & Galactic structure & their asteroseismic properties, particularly large frequency separation, frequency of maximum oscillation power &…

astro-ph.SR2025

Anomalously fast core and envelope rotation in red giants

Siddharth Dhanpal, Othman Benomar, Shravan Hanasoge +1

Red giants undergo dramatic and complex structural transformations as they evolve. Angular momentum is transported between the core and envelope during this epoch, a poorly underst…

astro-ph.SR2025

Seismic constraints on the spin evolution of slowly rotating young intermediate-mass stars

K. H. Singh, S. K. Panda, S. M. Hanasoge +1

Scuti stars are hot, rapid rotators and are a poorly understood class of pulsators. Asteroseismology provides the only means with which to probe their interior dynamics. Howeve…

astro-ph.SR2024

Quadratic frequency dispersion in the oscillations of intermediate-mass stars

Subrata Kumar Panda, Shravan Hanasoge, Siddharth Dhanpal +1

Asteroseismology, the study of stellar vibration, has met with great success, shedding light on stellar interior structure, rotation, and magnetism. Prominently known as Scutis…

astro-ph.SR2024

Magnetic flux in the Sun emerges unaffected by supergranular-scale surface flows

Prasad Mani, Chris S. Hanson, Siddarth Dhanpal +3

Magnetic flux emergence from the convection zone into the photosphere and beyond is a critical component of the behaviour of large-scale solar magnetism. Flux rarely emerges amid f…

astro-ph.SR2023

Asteroseismology applied to constrain structure parameters of δ Scuti stars

Subrata Kumar Panda, Siddharth Dhanpal, Simon J. Murphy +2

Asteroseismology is a powerful tool to probe the structure of stars. Space-borne instruments like CoRoT, Kepler and TESS have observed the oscillations of numerous stars, among whi…

astro-ph.SR2023

Inferring coupling strengths of mixed-mode oscillations in red-giant stars using deep learning

Siddharth Dhanpal, Othman Benomar, Shravan Hanasoge +3

Asteroseismology is a powerful tool that may be applied to shed light on stellar interiors and stellar evolution. Mixed modes, behaving as acoustic waves in the envelope and buoyan…

astro-ph.SR2022★ 13 cited

Measuring frequency and period separations in red-giant stars using machine learning

Siddharth Dhanpal, Othman Benomar, Shravan Hanasoge +4

Asteroseismology is used to infer the interior physics of stars. The \textit{Kepler} and TESS space missions have provided a vast data set of red-giant light curves, which may be u…

gr-qc2018★ 53 cited

A "no-hair" test for binary black holes

Siddharth Dhanpal, Abhirup Ghosh, Ajit Kumar Mehta +2

One of the consequences of the black-hole "no-hair" theorem in general relativity (GR) is that gravitational radiation (quasi-normal modes) from a perturbed Kerr black hole is uniq…