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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 astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2025★ 3 cited

Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations

Brendan T. Reed, Cassandra L. Armstrong, Rahul Somasundaram +4

The observation of neutron star mergers with gravitational waves (GWs) has provided a new method to constrain the dense-matter equation of state (EOS) and to better understand its…

astro-ph.HE2025

Leveraging differentiable programming in the inverse problem of neutron stars

Thibeau Wouters, Peter T. H. Pang, Hauke Koehn +5

Neutron stars (NSs) probe the high-density regime of the nuclear equation of state (EOS). However, inferring the EOS from observations of NSs is a computationally challenging task.…

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…

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…

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…