Skip to Main content Skip to Navigation
Journal articles

Systematic thermal reduction of neutronization in core-collapse supernovae

Abstract : We investigate to what extent the temperature dependence of the nuclear symmetry energy can affect the neutronization of the stellar core prior to neutrino trapping during gravitational collapse. To this end, we implement a one-zone simulation to follow the collapse until beta-equilibrium is reached and the lepton fraction remains constant. Since the strength of electron capture on the neutron-rich nuclei associated to the supernova scenario is still an open issue, we keep it as a free parameter. We find that the temperature dependence of the symmetry energy consistently yields a small reduction of deleptonization, which corresponds to a systematic effect on the shock wave energetics: the gain in dissociation energy of the shock has a small yet non-negligible value of about 0.4 foe (1 foe = 10(51) erg) and this result is almost independent from the strength of nuclear electron capture. The presence of such a systematic effect and its robustness under changes of the parameters of the one-zone model are significant enough to justify further investigations with detailed numerical simulations of supernova explosions.
Complete list of metadata

http://hal.in2p3.fr/in2p3-00424569
Contributor : Sophie Heurteau <>
Submitted on : Friday, October 16, 2009 - 2:10:49 PM
Last modification on : Wednesday, September 16, 2020 - 4:07:54 PM

Links full text

Identifiers

Collections

Citation

A.F. Fantina, P. Donati, P. M. Pizzochero. Systematic thermal reduction of neutronization in core-collapse supernovae. Physics Letters B, Elsevier, 2009, 676, pp.140-145. ⟨10.1016/j.physletb.2009.04.075⟩. ⟨in2p3-00424569⟩

Share

Metrics

Record views

131