activity
20202025
most citedNeutron Star Equation of State in light of GW190814

143 citations · 475 across the 8 of their papers we have counts for

collaborators

8 papers

nucl-th2025★ 1 cited

Building Neutron Stars with the MUSES Calculation Engine

Mateus Reinke Pelicer, Nikolas Cruz-Camacho, Carlos Conde +25

Exploring the equation of state of dense matter is an essential part of interpreting the observable properties of neutron stars. We present here the first results for dense matter…

nucl-th2023★ 87 cited

Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter

Rajesh Kumar, Veronica Dexheimer, Johannes Jahan +57

This review aims at providing an extensive discussion of modern constraints relevant for dense and hot strongly interacting matter. It includes theoretical first-principle results…

astro-ph.HE2022★ 63 cited

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…

nucl-th2022

Mirror Neutron Stars: How QCD can be used to study dark matter through gravitational waves

Maurício Hippert, Jack Setford, Hung Tan +3

Given the lack of empirical evidence of weakly interacting dark matter, it is reasonable to look to other candidates such as a confining dark sector with a similar number of partic…

astro-ph.HE2021★ 57 cited

The slope, the hill, the drop, and the swoosh: Learning about the nuclear matter equation of state from the binary Love relations

Hung Tan, Veronica Dexheimer, Jacquelyn Noronha-Hostler +1

Analyses that connect astrophysical observations of neutron stars with nuclear matter properties sometimes rely on equation-of-state insensitive relations. We show that the slope o…

astro-ph.HE2021★ 78 cited

Extreme Matter meets Extreme Gravity: Ultra-heavy neutron stars with crossovers and first-order phase transitions

Hung Tan, Travis Dore, Veronica Dexheimer +2

The speed of sound of the matter within neutron stars may contain non-smooth structure related to first-order phase transitions or or crossovers. Here we investigate what are the o…

astro-ph.HE2021★ 46 cited

Mirror Neutron Stars

Maurício Hippert, Jack Setford, Hung Tan +3

The fundamental nature of dark matter is entirely unknown. A compelling candidate is Twin Higgs mirror matter, invisible hidden-sector cousins of the Standard Model particles and f…

astro-ph.HE2020★ 143 cited

Neutron Star Equation of State in light of GW190814

Hung Tan, Jacquelyn Noronha-Hostler, Nico Yunes

The observation of gravitational waves from an asymmetric binary opens the possibility for heavy neutron stars, but these pose challenges to models of the neutron star equation of…