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NSR database version of April 27, 2024.

Search: Author = A.Lohs

Found 2 matches.

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2020FI02      Phys.Rev. C 101, 025804 (2020)

T.Fischer, G.Guo, A.A.Dzhioev, G.Martinez-Pinedo, M.-R.Wu, A.Lohs, Y.-Z.Qian

Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current-neutrino interactions and inverse neutron decay

NUCLEAR REACTIONS 1H(ν-bar, e+)n, 1n(ν, e-)p, E<100 MeV; derived expressions for medium-dependent charged-current reactions in fully inelastic kinematics, including contribution from weak magnetism; implemented weak reaction rates in the supernova model; simulated core-collapse supernova explosions and proto-neutron star (PNS) deleptonization; analyzed subsequent neutrino signal depending on the treatment of weak interactions; investigated nuclear medium dependence at the mean-field level, with the inverse neutron decay as new opacity source; calculated complete nucleosynthesis outcome from core-collapse supernova explosion simulation.

doi: 10.1103/PhysRevC.101.025804
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2017BO24      Phys.Rev.Lett. 119, 242702 (2017)

R.Bollig, H.-T.Janka, A.Lohs, G.Martinez-Pinedo, C.J.Horowitz, T.Melson

Muon Creation in Supernova Matter Facilitates Neutrino-Driven Explosions

doi: 10.1103/PhysRevLett.119.242702
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