403 citations · 8.9k across the 314 of their papers we have counts for
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Mapping the QCD Phase Transition with Accreting Compact Stars
David Blaschke, Gevorg Poghosyan, Hovik Grigorian
We discuss an idea for how accreting millisecond pulsars could contribute to the understanding of the QCD phase transition in the high-density nuclear matter equation of state (EoS…
Constraints on the High-Density Nuclear Equation of State from Neutron Star Observables
David Blaschke, Thomas Klaehn, Fridolin Weber
Depending on the density reached in the cores of neutron stars, such objects may contain stable phases of novel matter found nowhere else in the Universe. This article gives a brie…
Single-flavor CSL phase in compact stars
David Blaschke, Fredrik Sandin, Thomas Klahn +1
We suggest a scenario where the three light quark flavors are sequentially deconfined under increasing pressure in cold asymmetric nuclear matter as e.g. in neutron stars. The basi…
Ab initio Equation of State data for hydrogen, helium, and water and the internal structure of Jupiter
N. Nettelmann, B. Holst, A. Kietzmann +3
The equation of state of hydrogen, helium, and water effects interior structure models of giant planets significantly. We present a new equation of state data table, LM-REOS, gener…
The quark core of protoneutron stars in the phase diagram of quark matter
F. Sandin, D. Blaschke
We study the effect of neutrino trapping in new-born quark stars within a three-flavor Nambu - Jona-Lasinio (NJL) model with self-consistently calculated quark masses. The phase di…
Compact star constraints on the high-density EoS
H. Grigorian, D. Blaschke, T. Klaehn
A new scheme for testing the nuclear matter (NM) equation of state (EoS) at high densities using constraints from compact star (CS) phenomenology is applied to neutron stars with a…