239 citations · 3.9k across the 138 of their papers we have counts for
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Strangeness Transport in Binary Neutron Star Mergers
Melvin Storbacka, Jiaxi Wu, Alexander Haber +5
The presence of hyperons in the cores of neutron stars opens fast strangeness equilibration channels that can produce bulk-viscous dissipation during binary inspiral. Because these…
A finite temperature framework for quark matter with color-superconducting phases
Hosein Gholami, Marco Hofmann, Débora Mroczek +1
Current observations of neutron stars and measurements of gravitational waves only provide constraints on the zero temperature () equation of state (EoS) of dense matter. The…
Validity of a finite temperature expansion for dense nuclear matter
Debora Mroczek, Nanxi Yao, Katherine Zine +5
In this work we provide a new, well-controlled expansion of the equation of state of dense matter from zero to finite temperatures () while covering a wide range of charge fract…
Nontrivial features in the speed of sound inside neutron stars
Debora Mroczek, M. Coleman Miller, Jacquelyn Noronha-Hostler +1
Measurements of neutron star masses, radii, and tidal deformability have direct connections to nuclear physics via the equation of state (EoS), which for the cold, catalyzed matter…
Searching for phase transitions in neutron stars with modified Gaussian processes
Debora Mroczek, M. Coleman Miller, Jacquelyn Noronha-Hostler +1
Gaussian processes provide a promising framework by which to extrapolate the equation of state (EoS) of cold, catalyzed matter beyond times nuclear saturation density. Here w…
Dark Matter or Regular Matter in Neutron Stars? How to tell the difference from the coalescence of compact objects
Maurício Hippert, Emily Dillingham, Hung Tan +3
The mirror twin Higgs model is a candidate for (strongly-interacting) complex dark matter, which mirrors SM interactions with heavier quark masses. A consequence of this model are…