activity
19942025
most citedIdentifying a first-order phase transition in neutron star mergers through gravitational waves

403 citations · 8.9k across the 314 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2017★ 144 cited

Quark deconfinement as supernova explosion engine for massive blue-supergiant stars

Tobias Fischer, Niels-Uwe F. Bastian, Meng-Ru Wu +6

Blue-supergiant stars develop into core-collapse supernovae --- one of the most energetic outbursts in the universe --- when all nuclear burning fuel is exhausted in the stellar co…

astro-ph.HE2017★ 250 cited

Implications from GW170817 and I-Love-Q relations for relativistic hybrid stars

Vasileios Paschalidis, Kent Yagi, David Alvarez-Castillo +2

Gravitational wave observations of GW170817 placed bounds on the tidal deformabilities of compact stars allowing one to probe equations of state for matter at supranuclear densitie…

astro-ph.HE2017★ 44 cited

The state of matter in simulations of core-collapse supernovae -- Reflections and recent developments

Tobias Fischer, Niels-Uwe Bastian, David Blaschke +7

In this review article we discuss selected developments regarding the role of the equation of state (EOS) in simulations of core-collapse supernovae. There are no first-principle c…

astro-ph.HE2017★ 4 cited

Strange matter prospects within the string-flip model

Niels-Uwe F. Bastian, David B. Blaschke, Mateusz Cierniak +4

In this contribution we extend the recently developed two-flavor quark-matter string-flip model by including strange quarks. We discuss implications for compact stars.

astro-ph.HE2017★ 2 cited

Cooling of neutron stars with stiff stellar matter

H. Grigorian, D. N. Voskresensky, D. Blaschke

Recent evidence for high masses () pulsars PSR J1614-2230 and PSR J0348-0432 requires neutron star matter to have a stiff equation of state (EoS). The thermal evol…

astro-ph.HE2017★ 5 cited

Bayesian analysis for a new class of hybrid EoS models using mass and radius data of compact stars

A. Ayriyan, D. E. Alvarez-Castillo, S. Benic +3

We present a Bayesian analysis for a new class of realistic models of two-phase equations of state (EoS) for hybrid stars and demonstrate that the observation of a pair of high-mas…

astro-ph.HE2017★ 102 cited

Quark-Nuclear Hybrid EoS with Excluded Volume Effects

Mark Alexander Randolph Kaltenborn, Niels-Uwe Friedrich Bastian, David Bernhard Blaschke

A two-phase description of the quark-nuclear matter hybrid equation of state that takes into account the effect of excluded volume in both the hadronic and the quark matter phases…