Atomic Data and Nuclear Data Tables

By P. Bogdanovich, R. Kisielius. 2013

3,509 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/09f65ff17b14489fe03ef4a56418f96f3675f54d

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Citations in the corpus

Precision big bang nucleosynthesis with improved Helium-4 predictions (2018, background): “…obvious that experimental data are scarce at BBN energies and slightly below the scaled S–factor (an overall 9% systematic uncertainty is not shown however), while the empirical fit by Adelberger et al. (2011) or (Descouvemont et al., 2004) follows closely, by construction, the experimental data.”
Constraints on the symmetry energy and neutron skins from experiments and theory (2012, background): “Many such states called the Isobaric Analog states (IAS), have been identified [63].”
Angle-resolved photoemission studies of quantum materials (2020, unknown): “As an experimental technique, ARPES owes much of its utility to the fact that the photoelectric cross-section is at least five to six orders of magnitude higher than other processes such as inelastic light and neutron scattering (Thompson and Vaughan, 2001; Yeh and Lindau, 1985).”
Violent mergers of nearly equal-mass white dwarf as progenitors of subluminous Type Ia supernovae (2011, methodology): “The nuclear reaction rates are taken from the latest (2009) release of the REACLIB database (Rauscher & Thielemann 2000).”
Strongly Constrained and Appropriately Normed Semilocal Density Functional. (2015, methodology): “) Our calculations to construct and test the SCAN meta-GGA are described next: For the rare-gas atoms, we use accurate Hartree-Fock orbitals [67].”
Neutrino-driven wind simulations and nucleosynthesis of heavy elements (2012, unknown): “, FRDM [81], ETFSI [82], Duflo & Zuker [83], HFB-x [84, 85]).”
Direct Detection of Sub-GeV Dark Matter (2011, methodology): “We use the tabulated numerical RHF wavefunctions from [39],”
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars (2017, methodology): “The r-process nucleosynthesis and radioactive heating are computed using the nuclear network code WinNet (Thielemann et al. 2011; Korobkin et al. 2012; Winteler et al. 2012) with a reaction rates compilation for the finite range droplet model (FRDM; Möller et al. 1995; Rauscher & Thielemann 2000).”
SYSTEMATICS OF DYNAMICAL MASS EJECTION, NUCLEOSYNTHESIS, AND RADIOACTIVELY POWERED ELECTROMAGNETIC SIGNALS FROM NEUTRON-STAR MERGERS (2013, background): “These inputs include i) different mass models for the estimate of the β-decay and neutron capture rates, namely the recent microscopic Skyrme (Goriely et al. 2010) and Gogny (Goriely et al. 2009a) Hartree-Fock-Bogolyubov (HFB) mass models as well as the macroscopic-microscopic finite-range droplet m”
A COMPACT DEGENERATE PRIMARY-STAR PROGENITOR OF SN 2011fe (2011, methodology): “…(Itoh et al. 1996), opacities (Iglesias & Rogers 1996), equation of state (Timmes & Swesty 2000; Rogers & Nayfonov 2002), and nuclear reactions (Caughlan & Fowler 1988; Angulo et al. 1999) were employed, including recently updated triple−α (Fynbo et al. 2005), α+12C (Kunz et al. 2002), and…”
CORE-COLLAPSE SUPERNOVA EQUATIONS OF STATE BASED ON NEUTRON STAR OBSERVATIONS (2012, methodology): “Here the finite range droplet model of Möller et al. (1995) was chosen because of its excellent reproduction of experimental binding energies, with a rms deviation of only 0.669 MeV.”
New potentialities of the Liege intranuclear cascade (INCL) model for reactions induced by nucleons and light charged particles (2012, background): “These effects are rather well identified in macroscopic models for the reaction cross sections [57, 58].”