activity
19962026
most citedTwo-dimensional hydrodynamic core-collapse supernova simulations with spectral neutrino transport. I. Numerical method and results for a 15 M_sun star

420 citations · 4k across the 52 of their papers we have counts for

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Showing 2003 · astro-phShow all

5 papers · 2 filters

astro-ph2003★ 313 cited

Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods

M. Liebendoerfer, M. Rampp, H. -Th. Janka +1

Accurate neutrino transport has been built into spherically symmetric simulations of stellar core collapse and postbounce evolution. The results of such simulations agree that sphe…

astro-ph2003★ 191 cited

Towards Gravitational Wave Signals from Realistic Core Collapse Supernova Models

Ewald Mueller, Markus Rampp, Robert Buras +2

We have computed the gravitational wave signal from supernova core collapse using the presently most realistic input physics available. We start from state-of-the-art progenitor mo…

astro-ph2003★ 33 cited

Supernova neutrinos: Flavor-dependent fluxes and spectra

G. G. Raffelt, M. Th. Keil, R. Buras +2

Transporting nu_mu and nu_tau in a supernova (SN) core involves several processes that have been neglected in traditional simulations. Based on a Monte Carlo study we find that the…

astro-ph2003★ 309 cited

Improved Models of Stellar Core Collapse and Still no Explosions: What is Missing?

R. Buras, M. Rampp, H. -Th. Janka +1

Two-dimensional hydrodynamic simulations of stellar core-collapse with and without rotation are presented which for the first time were performed by solving the Boltzmann equation…

astro-ph2003★ 280 cited

Electron capture rates on nuclei and implications for stellar core collapse

K. Langanke, G. Martinez-Pinedo, J. M. Sampaio +7

Supernova simulations to date have assumed that during core collapse electron captures occur dominantly on free protons, while captures on heavy nuclei are Pauli-blocked and are ig…