activity
19982011
most citedSignals of the QCD phase transition in core-collapse supernovae

276 citations · 580 across the 14 of their papers we have counts for

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Showing 2008Show all

6 papers · 1 filter

astro-ph2008

NuGrid: s process in massive stars

Raphael Hirschi, Urs Frischknecht, F. -K. Thielemann +10

The s-process production in massive stars at very low metallicities is expected to be negligible due to the low abundance of the neutron source 22Ne, to primary neutron poisons and…

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-ph20087 cited

Stellar Evolution in the Early Universe

R. Hirschi, U. Frischknecht, F. -K. Thielemann +5

Massive stars played a key role in the early evolution of the Universe. They formed with the first halos and started the re-ionisation. It is therefore very important to understand…

astro-ph2008

New Stellar Cross Sections and The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars"

I. Dillmann, R. Plag, C. Domingo-Pardo +4

Since April 2005 a regularly updated stellar neutron cross section compilation is available online at http://nuclear-astrophysics.fzk.de/kadonis. This online-database is called the…

astro-ph20082 cited

KADoNiS- The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars

I. Dillmann, M. Heil, F. Käppeler +3

The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" (KADoNiS) project is an online database for experimental cross sections relevant to the s process and p process.…

astro-ph200823 cited

Experimental (n,) cross sections of the p-process nuclei Se and Sr

I. Dillmann, M. Heil, F. Käppeler +2

The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capt…