New calculations of grossβ-decay properties for astrophysical applications: Speeding-up the classicalrprocess

By P. Möller, B. Pfeiffer, K. Kratz. 2003

288 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/032c93ed74be10f8531abafd6d39b30a5250d461

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In Nuclear and High Energy Physics

Citations in the corpus

r-PROCESS LANTHANIDE PRODUCTION AND HEATING RATES IN KILONOVAE (2015, background): “For example, REACLIB gives a half-life of 300 ns for 216Pb because the Nuclear Wallet Cards state the half-life is “> 300 ns”, but Möller et al. (2003) gives a half-life of about 850 s, which is much closer to the half-lives of similar nuclides.”
The Intermediate r-process in Core-collapse Supernovae Driven by the Magneto-rotational Instability (2016, methodology): “Theoretical reaction rates (e.g. for neutron-capture) for neutron-rich nuclei are based on mass predictions by Möller et al. (1995) and the theoretical β-decay rates are taken from Möller et al. (2003).”
Nucleosynthesis in the Early Galaxy (2007, methodology): “Theoretical β-decay rates were taken from Möller et al. (1997) or when available, from calculations including first forbidden transitions (Möller et al. 2003).”
Production of the entire range of r-process nuclides by black hole accretion disc outflows from neutron star mergers (2016, methodology): “To explore the impact of β-decay rates, we alternatively employ those of Marketin et al. (2016) and Möller et al. (2003).”
Nuclear weak-interaction processes in stars (2002, unknown): “However, a first attempt towards this goal (Möller et al., 2002) has combined first-forbidden transitions estimated in the Gross Theory (Takahashi et al., 1973) with GT results taken from QRPA calculations.”
The impact of individual nuclear properties on $r$-process nucleosynthesis (2015, methodology): “In QRPA based calculations, such as those of Ref.”
Radioactive decays at limits of nuclear stability (2011, methodology): “Several approaches have been employed to reproduce and predict the beta decay halflives in large parts of the nuclear chart (Borzov and Goriely, 2000; Homma et al., 1996; Möller et al., 2003; Nakata et al., 1997).”
Origin of the heaviest elements: The rapid neutron-capture process (2019, methodology): “, 2012) (open triangles) and the predictions of the models: Finite Range Droplet Model with Quasi Random Phase Approximation FRDM-QRPA (dark blue) (Möller et al., 2003), Gross Theory KTUY-GT2 (light green) (Tachibana et al.”
ELECTROMAGNETIC TRANSIENTS POWERED BY NUCLEAR DECAY IN THE TIDAL TAILS OF COALESCING COMPACT BINARIES (2011, methodology): “Experimental values are taken for nuclear masses where available, elsewhere theoretical masses are taken from Möller et al. (2003).”
NEUTRINO-DRIVEN WINDS IN THE AFTERMATH OF A NEUTRON STAR MERGER: NUCLEOSYNTHESIS AND ELECTROMAGNETIC TRANSIENTS (2015, background): “Weak interaction rates including neutrino absorption on nucleons are taken into account (Möller et al. 2003; Fröhlich et al. 2006).”
THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS (2010, background): “…database includes updated terrestrial half-lives, both experimental (Audi et al. 2003a; Tuli & National Nuclear Data Center 2007) and theoretical (Möller et al. 2003), which can be used as a default, but are then superseded in the burst model with temperature- and density-dependent rates when…”