activity
20002019
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 · 2.5k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2019★ 78 cited

ALIS: An efficient method to compute high spectral resolution polarized solar radiances using the Monte Carlo approach

C. Emde, R. Buras, B. Mayer

An efficient method to compute accurate polarized solar radiance spectra using the (three-dimensional) Monte Carlo model MYSTIC has been developed. Such high resolution spectra are…

astro-ph2008★ 1 cited

Nucleosynthesis in Early Neutrino Driven Winds

R. D. Hoffman, J. L. Fisker, J. Pruet +3

Nucleosynthesis in early neutrino winds is investigated. Presented is a brief overview of two recent problems of supernova nucleosynthesis. In the first part we investigate the eff…

astro-ph2007★ 133 cited

Dynamics of shock propagation and nucleosynthesis conditions in O-Ne-Mg core supernovae

H. -Th. Janka, B. Mueller, F. S. Kitaura +1

It has been recently proposed that the shocked surface layers of exploding O-Ne-Mg cores provide the conditions for r-process nucleosynthesis, because their rapid expansion and hig…

astro-ph2006★ 2 cited

Nucleosynthesis in neutrino heated matter: The vp-process and the r-process

G. Martínez-Pinedo, A. Kelic, K. Langanke +11

This manuscript reviews recent progress in our understanding of the nucleosynthesis of medium and heavy elements in supernovae. Recent hydrodynamical models of core-collapse supern…

astro-ph2005★ 293 cited

Two-Dimensional Hydrodynamic Core-Collapse Supernova Simulations with Spectral Neutrino Transport II. Models for Different Progenitor Stars

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

1D and 2D supernova simulations for stars between 11 and 25 solar masses are presented, making use of the Prometheus/Vertex neutrino-hydrodynamics code, which employs a full spectr…

astro-ph2005★ 246 cited

Nucleosynthesis in Early Supernova Winds II: The Role of Neutrinos

J. Pruet, R. D. Hoffman, S. E. Woosley +2

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 nucle…