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Jürgen Schaffner-Bielich

Researcher at Goethe University Frankfurt

Publications -  54
Citations -  2923

Jürgen Schaffner-Bielich is an academic researcher from Goethe University Frankfurt. The author has contributed to research in topics: Neutron star & Strange matter. The author has an hindex of 23, co-authored 54 publications receiving 2468 citations. Previous affiliations of Jürgen Schaffner-Bielich include Brookhaven National Laboratory & Heidelberg University.

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New Constraints on Radii and Tidal Deformabilities of Neutron Stars from GW170817.

Elias R. Most, +3 more
- 25 Jun 2018 - 
TL;DR: A parameterized manner a very large range of physically plausible equations of state (EOSs) for compact stars for matter that is either purely hadronic or that exhibits a phase transition is explored, finding the radius that is statistically most probable for any value of the stellar mass.
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Astrophysics: quark matter in compact stars?

M. Alford, +6 more
- 18 Jan 2007 - 
TL;DR: This paper compares Özel's observational limits with predictions based on a more comprehensive set of proposed quark-matter equations of state from the literature, and concludes that the presence of quark matter in EXO 0748–676 is not ruled out.
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Constraining Neutron Star Matter with Quantum Chromodynamics

Aleksi Kurkela, +5 more
- 23 Jun 2014 - 
TL;DR: In this paper, the authors demonstrate that significant further restrictions can be placed by additionally requiring the pressure to approach that of deconfined quark matter at high densities, which turns out to be highly insensitive to the amount of quark atoms inside the stars.
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Hypernuclear Physics for Neutron Stars

Jürgen Schaffner-Bielich
- 15 May 2008 - 
TL;DR: The role of hypernuclear physics for the physics of neutron stars is delineated in this paper, where hypernuclear potentials in dense matter control the hyperon composition of dense neutron star matter.
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Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase

Tobias Fischer, +10 more
- 27 May 2011 - 
TL;DR: In this article, a quark-hadron hybrid equation of state was constructed for core-collapse supernova simulations, based on general relativistic radiation hydrodynamics and three-flavor Boltzmann neutrino transport in spherical symmetry.