H
Hans-Thomas Janka
Researcher at Max Planck Society
Publications - 273
Citations - 24766
Hans-Thomas Janka is an academic researcher from Max Planck Society. The author has contributed to research in topics: Supernova & Neutrino. The author has an hindex of 86, co-authored 263 publications receiving 21791 citations. Previous affiliations of Hans-Thomas Janka include Maine Principals' Association.
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Journal ArticleDOI
High-resolution supernova neutrino spectra represented by a simple fit
TL;DR: In this paper, a spherically symmetric supernova model with full Boltzmann neutrino transport was used to test the fit quality of supernova neutrinos.
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A New Multi-dimensional General Relativistic Neutrino Hydrodynamic Code for Core-collapse Supernovae. I. Method and Code Tests in Spherical Symmetry
TL;DR: In this article, a general relativistic code for hydrodynamical supernova simulations with neutrino transport in spherical and azimuthal symmetry (one dimension and two dimensions, respectively) is presented.
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Core-collapse supernovae: Reflections and directions
Hans-Thomas Janka,Florian Hanke,Lorenz Hüdepohl,Andreas Marek,Bernhard Müller,Martin Obergaulinger +5 more
TL;DR: In this paper, a short overview of the sequence of stages of stellar core-collapse events, the general properties of progenitor-dependent neutrino emission will be briefly described.
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3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state.
Christian D. Ott,Harald Dimmelmeier,Andreas Marek,Hans-Thomas Janka,Ian Hawke,Burkhard Zink,Erik Schnetter +6 more
TL;DR: This work focuses on gravitational wave (GW) emission from rotating collapse, bounce, and early postbounce phases and indicates that the GW signature of these phases is much more generic than previously estimated.
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Neutron-star merger ejecta as obstacles to neutrino-powered jets of gamma-ray bursts
Oliver Just,Martin Obergaulinger,Hans-Thomas Janka,Andreas Bauswein,Andreas Bauswein,N. Schwarz,N. Schwarz +6 more
TL;DR: In this article, a special relativistic, axisymmetric hydrodynamic simulation of black hole-torus systems is presented, in which the viscously driven evolution of the accretion torus is followed with self-consistent energy-dependent neutrino transport and the interaction with the cloud of dynamical ejecta expelled during the NS-NS merging is taken into account.