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- Publications
- Influence
Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
- T. Sukhbold, T. Ertl, S. Woosley, J. M. Brown, H.-T. Janka
- Physics
- 15 October 2015
Nucleosynthesis, light curves, explosion energies, and remnant masses are calculated for a grid of supernovae resulting from massive stars with solar metallicity and masses from 9.0 to 120 solar… Expand
Formation of Double Neutron Star Systems
- T. Tauris, M. Kramer, +11 authors D. Champion
- Physics
- 28 June 2017
Double neutron star (DNS) systems represent extreme physical objects and the endpoint of an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems and their mergers… Expand
Nucleosynthesis in Early Supernova Winds. II. The Role of Neutrinos
- J. Pruet, R. D. Hoffman, S. Woosley, H.-T. Janka, R. Buras
- Physics
- 7 November 2005
One of the outstanding unsolved riddles of nuclear astrophysics is the origin of the so-called p-process nuclei from A = 92 to 126. Both the lighter and heavier p-process nuclei are adequately… Expand
Nucleosynthesis in the hot convective bubble in core-collapse supernovae
- J. Pruet, S. Woosley, R. Buras, H.-T. Janka, R. D. Hoffman
- Physics
- 17 September 2004
As an explosion develops in the collapsed core of a massive star, neutrino emission drives convection in a hot bubble of radiation, nucleons, and pairs just outside a proto-neutron star. Shortly… Expand
Equation-of-state dependence of the gravitational-wave signal from the ring-down phase of neutron-star mergers
- A. Bauswein, H.-T. Janka, +7 authors Technische Universitaat Darmstadt
- Physics
- 9 April 2012
Neutron-star (NS) merger simulations are conducted for 38 representative microphysical descriptions of high-density matter in order to explore the equation-of-state dependence of the postmerger… Expand
Axisymmetric general relativistic simulations of the accretion-induced collapse of white dwarfs
- E. Abdikamalov, C. Ott, +4 authors H.-T. Janka
- Physics
- 14 October 2009
The accretion-induced collapse (AIC) of a white dwarf may lead to the formation of a protoneutron star
and a collapse-driven supernova explosion. This process represents a path alternative to… Expand
Neutrino signatures of supernova forward and reverse shock propagation
- R. Tomàs, M. Kachelriess, G. Raffelt, A. Dighe, H.-T. Janka, L. Scheck
- Physics
- 7 July 2004
A few seconds after bounce in a core-collapse supernova, the shock wave passes the density region corresponding to resonant neutrino oscillations with the 'atmospheric' neutrino mass difference. The… Expand
Neutrino-driven supernovae: An accretion instability in a nuclear physics controlled environment
- H.-T. Janka, R. Buras, F. K. Joyanes, A. Marek, M. Rampp, L. Scheck
- Physics
- 12 November 2004
New simulations demonstrate that low-mode, nonradial hydrodynamic instabilities of the accretion shock help starting hot-bubble convection in supernovae and thus support explosions by the… Expand
Neutrino emission from type II supernovae: an analysis of the spectra
- H.-T. Janka, W. Hillebrandt
- Physics
- 1989
Une methode de Monte Carlo est utilisee pour calculer le spectre des neutrinos de tous types, pour 2 stades differents apres l'effondrement du noyau de fer d'une etoile de 20 M ○. . Les resultats… Expand
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