activity
19982022
most citedSignatures of quark-hadron phase transitions in general-relativistic neutron-star mergers

389 citations · 2.2k across the 26 of their papers we have counts for

collaborators

26 papers

nucl-th2022★ 43 cited

Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions

Elias R. Most, Anton Motornenko, Jan Steinheimer +4

Binary neutron-star mergers and heavy-ion collisions are related through the properties of the hot and dense nuclear matter formed during these extreme events. In particular, low-e…

gr-qc2019★ 190 cited

Postmerger Gravitational-Wave Signatures of Phase Transitions in Binary Mergers

Lukas R. Weih, Matthias Hanauske, Luciano Rezzolla

With the first detection of gravitational waves from a binary system of neutron stars, GW170817, a new window was opened to study the properties of matter at and above nuclear-satu…

astro-ph.HE2019★ 96 cited

On the Deconfinement Phase Transition in Neutron-Star Mergers

Elias R. Most, L. Jens Papenfort, Veronica Dexheimer +3

We study in detail the nuclear aspects of a neutron-star merger in which deconfinement to quark matter takes place. For this purpose, we make use of the Chiral Mean Field (CMF) mod…

nucl-th2019

Neutron-Star-Merger Equation of State

Veronica Dexheimer, Constantinos Constantinou, Elias R. Most +5

In this work, we discuss the dense matter equation of state (EOS) for the extreme range of conditions encountered in neutron stars and their mergers. The calculation of the propert…

astro-ph.HE2018★ 177 cited

Constraining twin stars with GW170817

Gloria Montana, Laura Tolos, Matthias Hanauske +1

If a phase transition is allowed to take place in the core of a compact star, a new stable branch of equilibrium configurations can appear, providing solutions with the same mass a…

astro-ph.HE2018★ 389 cited

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…