activity
20232026
most citedMaximally local two-nucleon interactions at NLO in -less chiral effective field theory

16 citations · 101 across the 19 of their papers we have counts for

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Showing 2024Show all

10 papers · 1 filter

gr-qc2024★ 2 cited

Can Neutron Star Tidal Effects Obscure Deviations from General Relativity?

Stephanie M. Brown, Badri Krishnan, Rahul Somasundaram +1

One of the main goals of gravitational-wave astrophysics is to study gravity in the strong-field regime and constrain deviations from general relativity (GR). Any such deviation af…

nucl-th2024★ 7 cited

Inferring three-nucleon couplings from multi-messenger neutron-star observations

Rahul Somasundaram, Isak Svensson, Soumi De +5

Understanding the interactions between nucleons in dense matter is an important challenge in theoretical physics. Effective field theories have emerged as the dominant approach to…

nucl-th2024★ 6 cited

Perturbative treatment of nonlocal chiral interactions in auxiliary-field diffusion Monte Carlo calculations

Ryan Curry, Rahul Somasundaram, Stefano Gandolfi +2

Nuclear many-body systems, ranging from nuclei to neutron stars, are some of the most interesting physical phenomena in our universe, and Quantum Monte Carlo (QMC) approaches are a…

astro-ph.HE2024★ 15 cited

The impact of dark matter on tidal signatures in neutron star mergers with Einstein Telescope

Hauke Koehn, Edoardo Giangrandi, Nina Kunert +3

If dark matter (DM) accumulates inside neutron stars (NS), it changes their internal structure and causes a shift of the tidal deformability from the value predicted by the dense-m…

astro-ph.HE2024

Kilonova Emissions from Neutron Star Merger Remnants: Implications for Nuclear Equation of State

Kelsey A. Lund, Rahul Somasundaram, Gail C. McLaughlin +3

Multi-messenger observation of binary neutron-star mergers can provide valuable information on the nuclear equation of state (EoS). Here, we investigate to which extent electromagn…

nucl-th2024★ 13 cited

Neutron matter from local chiral effective field theory interactions at large cutoffs

I. Tews, R. Somasundaram, D. Lonardoni +6

Neutron matter is an important many-body system that provides valuable constraints for the equation of state (EOS) of neutron stars. Neutron-matter calculations employing chiral ef…

astro-ph.HE2024★ 10 cited

Probe and Prejudice: Classification of compact objects and model comparison using EOS knowledge

Hauke Koehn, Thibeau Wouters, Henrik Rose +4

Nuclear theory and experiments, alongside astrophysical observations, constrain the equation of state (EOS) of supranuclear-dense matter. Conversely, knowledge of the EOS allows an…

astro-ph.HE2024★ 1 cited

Towards accelerated nuclear-physics parameter estimation from binary neutron star mergers: Emulators for the Tolman-Oppenheimer-Volkoff equations

Brendan T. Reed, Rahul Somasundaram, Soumi De +5

Gravitational-wave observations of binary neutron-star (BNS) mergers have the potential to revolutionize our understanding of the nuclear equation of state (EOS) and the fundamenta…

nucl-th2024★ 12 cited

Emulators for scarce and noisy data: application to auxiliary field diffusion Monte Carlo for the deuteron

Rahul Somasundaram, Cassandra L. Armstrong, Pablo Giuliani +3

The validation, verification, and uncertainty quantification of computationally expensive theoretical models of quantum many-body systems require the construction of fast and accur…

astro-ph.HE2024

Measuring Neutron Star Radius with second and third generation Gravitational Wave Detector Networks

Ananya Bandopadhyay, Keisi Kacanja, Rahul Somasundaram +2

The next generation of ground-based interferometric gravitational wave detectors will observe mergers of black holes and neutron stars throughout cosmic time. A large number of the…