720 citations · 9.8k across the 105 of their papers we have counts for
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Quarkyonic Matter and Neutron Stars
Larry McLerran, Sanjay Reddy
We consider Quarkyonic Matter to naturally explain the observed properties of neutron stars. We argue that such matter might exist at densities close to that of nuclear matter and…
A critical examination of constraints on the equation of state of dense matter obtained from GW170817
I. Tews, J. Margueron, S. Reddy
The correlation of the tidal polarizabilities - for GW170817 is predicted by combining dense-matter equations of state (EOSs) that satisfy nuclear physics constraints wit…
Neutrino-nucleon scattering in the neutrino-sphere
Paulo F. Bedaque, Sanjay Reddy, Srimoyee Sen +1
We calculate the differential scattering rate for thermal neutrinos in a hot and dilute gas of interacting neutrons using linear response theory. The dynamical structure factors fo…
Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations
Ingo Tews, Joseph Carlson, Stefano Gandolfi +1
The dense matter equation of state (EOS) determines neutron star (NS) structure but can be calculated reliably only up to one to two times the nuclear saturation density, using acc…