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20032008
most citedSignals of the QCD phase transition in core-collapse supernovae

276 citations · 563 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph2008276 cited

Signals of the QCD phase transition in core-collapse supernovae

I. Sagert, M. Hempel, G. Pagliara +5

We explore the implications of the QCD phase transition during the postbounce evolution of core-collapse supernovae. Using the MIT bag model for the description of quark matter and…

astro-ph2007202 cited

The isotropic diffusion source approximation for supernova neutrino transport

M. Liebendoerfer, S. C. Whitehouse, T. Fischer

Astrophysical observations originate from matter that interacts with radiation or transported particles. We develop a pragmatic approximation in order to enable multi-dimensional s…

astro-ph200785 cited

Gravitational waves from 3D MHD core collapse simulations

S. Scheidegger, T. Fischer, S. C. Whitehouse +1

We present the gravitational wave analysis from rotating (model s15g) and nearly non-rotating (model s15h) 3D MHD core collapse supernova simulations at bounce and the first couple…

astro-ph2006

Efficient approximations of neutrino physics for three-dimensional simulations of stellar core collapse

M. Liebendoerfer, U. -L. Pen, C. Thompson

Neutrino transport in spherically symmetric models of stellar core collapse and bounce has achieved a technically complete level, rewarded by the agreement among independent groups…

astro-ph2005

Neutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process

C. Fröhlich, G. Martínez-Pinedo, M. Liebendörfer +5

We present a new nucleosynthesis process, that we denote nu p-process, which occurs in supernovae (and possibly gamma-ray bursts) when strong neutrino fluxes create proton-rich eje…

astro-ph2005

A simple parameterization of the consequences of deleptonization for simulations of stellar core collapse

M. Liebendoerfer

A simple and computationally efficient parameterization of the deleptonization, the entropy changes, and the neutrino stress is presented for numerical simulations of stellar core…