389 citations · 3.8k across the 122 of their papers we have counts for
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Hyperons and quarks in proto-neutron stars
J. Roark, X. Du, C. Constantinou +3
In this work, we study matter in the cores of proto-neutron stars, focusing on the impact of their composition on the stellar structure. We begin by examining the effects of finite…
Can magnetic fields stabilize or destabilize twin stars?
R. O. Gomes, V. Dexheimer, S. Han +1
Sharp phase transitions described by stiff equations of state allow for the existence of a third family of stable compact stars (besides white dwarfs and neutron stars), twin stars…
What do we learn about vector interactions from GW170817?
Veronica Dexheimer, Rosana de Oliveira Gomes, Stefan Schramm +1
We analyze the role played by vector-isovector meson interaction in dense matter present in the interior of neutron stars in the light of new measurements made during the double ne…
Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
Elias R. Most, L. Jens Papenfort, Veronica Dexheimer +4
Merging binaries of neutron stars are not only strong sources of gravitational waves, but also have the potential of revealing states of matter at densities and temperatures not ac…
Modeling magnetic neutron stars: a short overview
R. O. Gomes, S. Schramm, V. Dexheimer
Neutron stars are the endpoint of the life of intermediate mass stars and posses in their cores matter in the most extreme conditions in the universe. Besides their extremes of tem…
Cooling of Small and Massive Hyperonic Stars
Rodrigo Negreiros, Laura Tolos, Mario Centelles +2
We perform cooling simulations for isolated neutron stars using recently developed equations of state for their core. The equations of state are obtained from new parametrizations…