NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 26, 2024.

Search: Author = L.Huther

Found 3 matches.

Back to query form

2016MA12      Phys.Rev. C 93, 025805 (2016)

T.Marketin, L.Huther, G.Martinez-Pinedo

Large-scale evaluation of β-decay rates of r-process nuclei with the inclusion of first-forbidden transitions

RADIOACTIVITY Z=8-110, N=11-236, A=19-339(β^-); calculated decay rates for Gamow-Teller and first-forbidden transitions, total decay rates, P_0n, P_1n, P_3n, P_4n, P_5n delayed-neutron emission probabilities, average energies of electrons antineutrinos and photons after decay. Z=47-48, A=114-154; calculated Q(β^-). Z=36-43, A=93-117; Z=37-50, N=65-88; Z=24-32, N=50; Z=42-49, N=82; Z=6-73, N=126; ^194,195,196Re, ^199,200Os, ^{198,199,201,202}Ir, ^203,204Pt, ²⁰⁴Au, ^211,212,213Tl, ^218,219Bi(β^-); calculated half-lives for β^- decay. Fully self-consistent covariant density functional theory (CDFT) framework with the ground states calculated with relativistic Hartree-Bogoliubov (RHB) model, and excited states within the proton-neutron relativistic quasiparticle random phase approximation (pn-RQRPA). Comparison with experimental Q values and half-lives. Calculated abundances of heavy nuclei, and evolution of neutron-to-seed ratio resulting from hot and cold r-processes using half-lives from the FRDM and the current model. Supplementary file contains theoretical values of half-lives and P_xn for 5409 neutron-rich nuclei.

doi: 10.1103/PhysRevC.93.025805
Citations: PlumX Metrics

2014MA04      J.Phys.(London) G41, 044008 (2014)

G.Martinez-Pinedo, T.Fischer, L.Huther

Supernova neutrinos and nucleosynthesis

doi: 10.1088/0954-3899/41/4/044008
Citations: PlumX Metrics

2011HU03      Eur.Phys.J. A 47, 10 (2011)

L.Huther, H.P.Loens, G.Martinez-Pinedo, K.Langanke

s-process stellar enhancement factors obtained within the statistical model with parity-dependent level densities

NUCLEAR REACTIONS ²⁰⁴Pb(n, γ), E=0.086 eV-860 keV; calculated σ, reaction rates. A=24-210(n, γ), E=8, 30, 90 keV; calculated s-process reaction rates, stellar enhancement factors. Hilaire-Goriely and BSFG densities with parity.

doi: 10.1140/epja/i2011-11010-y
Citations: PlumX Metrics