414 citations · 800 across the 7 of their papers we have counts for
7 papers
Equation of state at neutron-star densities and beyond from perturbative QCD
Oleg Komoltsev, Rahul Somasundaram, Tyler Gorda +3
We explore the consequences of imposing robust thermodynamic constraints arising from perturbative Quantum Chromodynamics (QCD) when inferring the dense-matter equation-of-state (E…
What can we learn about the unstable equation-of-state branch from neutron-star mergers?
Maximiliano Ujevic, Rahul Somasundaram, Tim Dietrich +2
The Equation of State (EOS) of dense strongly-interacting matter can be probed by astrophysical observations of neutron stars (NS), such as X-ray detections of pulsars or the measu…
Revealing the strength of three-nucleon interactions with the Einstein Telescope
Henrik Rose, Nina Kunert, Tim Dietrich +5
Three-nucleon forces are crucial for the accurate description of nuclear systems, including dense matter probed in neutron stars. We explore nuclear Hamiltonians that reproduce two…
Quantum Monte Carlo calculations of light nuclei with local chiral two- and three-nucleon interactions
J. E. Lynn, I. Tews, J. Carlson +4
Local chiral effective field theory interactions have recently been developed and used in the context of quantum Monte Carlo few- and many-body methods for nuclear physics. In this…
Spectrum of shear modes in the neutron-star crust: Estimating the nuclear-physics uncertainties
Ingo Tews
I construct a model of the inner crust of neutron stars using interactions from chiral effective field theory (EFT) in order to calculate its equation of state (EOS), shear propert…
Local chiral effective field theory interactions and quantum Monte Carlo applications
A. Gezerlis, I. Tews, E. Epelbaum +5
We present details of the derivation of local chiral effective field theory interactions to next-to-next-to-leading order, and show results for nucleon-nucleon phase shifts and deu…