activity
20242026
collaborators

12 papers

nucl-th2026

Universality and variability of the heavy r-process element abundance pattern from a nonequilibrium approach

David Blaschke, Friedrich K. Röpke, Gerd Röpke

A striking feature in the observed chemical composition of the majority of stars is the universality of the relative abundances of the heavy elements, although some outliers exist.…

cond-mat.mes-hall2026

Generalized Beth-Uhlenbeck Approach to the 2+1D Gross-Neveu Model

Biplab Mahato, David Blaschke

We study the thermodynamics of the (2+1) dimensional Gross-Neveu model inspired from graphene. We focus on the entropy density of the Gaussian fluctuation beyond the mean field. Th…

nucl-th2025

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement

Christoph Gärtlein, Violetta Sagun, Oleksii Ivanytskyi +2

We study rotating hybrid stars, with particular emphasis on the effect of spin on the deconfinement phase transition and star properties. Our analysis is based on a hybrid equation…

nucl-th2025

Generalized Beth--Uhlenbeck entropy formula from the derivable approach

David Blaschke, Gerd Röpke, Gordon Baym

We derive a generalized Beth-Uhlenbeck formula for the entropy of a dense fermion system with strong two-particle correlations, including scattering states and bound states. We wor…

nucl-th2025

Bayesian inference favors quark matter in neutron star interiors

Alexander Ayriyan, Oleksii Ivanytskyi, David Blaschke

We perform a physics-informed Bayesian analyses of the equation of state of hybrid neutron stars that incorporates color-flavor-locked quark matter modeled by a three-flavor non-lo…

nucl-th2025

Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?

Christoph Gärtlein, Violetta Sagun, Oleksii Ivanytskyi +2

We study rotating hybrid stars, with a particular emphasis on the effect of a deconfinement phase transition on their properties at high spin. Our analysis is based on a hybrid equ…