Calculations of Maxwellian-averaged cross sections and astrophysical reaction rates using the ENDF/B-VII.0, JEFF-3.1, JENDL-3.3, and ENDF/B-VI.8 evaluated nuclear reaction data libraries [PDF]
We calculated the Maxwellian-averaged cross sections (MACS) and astrophysical reaction rates of the stellar nucleosynthesis reactions (n,$\gamma$), (n,fission), (n,p), (n,$\alpha$) and (n,2n) using the ENDF/B-VII.0-, JEFF-3.1-, JENDL-3.3-, and ENDF/B-VI ...
B. Pritychenko +2 more
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TABLES OF NUCLEAR CROSS SECTIONS AND REACTION RATES: AN ADDENDUM TO THE PAPER “ASTROPHYSICAL REACTION RATES FROM STATISTICAL MODEL CALCULATIONS” [PDF]
In a previous publication [Atomic Data and Nuclear Data Tables 75, 1 (2000)], we had given seven parameter analytical fits to theoretical reaction rates derived from nuclear cross sections calculated in the statistical model (Hauser-Feshbach formalism ...
T. Rauscher, F.‐K. Thielemann
openalex +4 more sources
Underground Measurements of Nuclear Reaction Cross-Sections Relevant to AGB Stars [PDF]
Nuclear reaction cross sections are essential ingredients to predict the evolution of AGB stars and understand their impact on the chemical evolution of our Galaxy.
Chemseddine Ananna +13 more
doaj +6 more sources
Measurement of nuclear reaction cross sections by using Cherenkov radiation toward high-precision proton therapy. [PDF]
Masuda T +9 more
europepmc +3 more sources
MEASUREMENT OF 182,184,186W (N, N’ γ) CROSS SECTIONS AND WHAT WE CAN LEARN FROM IT [PDF]
Today’s development of nuclear installations rely on numerical simulation for which the main input are evaluated nuclear data. Inelastic neutron scattering (n, xn) is a reaction of importance because it modifies the neutron population, the neutron energy
Henning Greg +17 more
doaj +1 more source
Reinvestigating the Gamow Factor of Reactions on Light Nuclei
We present a modified Gamow factor by reinvestigating the conventional assumptions used in its derivation. The conventional Gamow factor, factorized from the total cross section, effectively describes the penetration probabilities (PPs) in low-energy ...
Eunseok Hwang +4 more
doaj +1 more source
The 26Al abundance holds a special role in present-day astrophysics, since it is a probe of active nucleosynthesis in the Galaxy and a valuable constraint of Galactic core-collapse supernovae rate.
M. La Cognata +21 more
doaj +1 more source
The Nuclear Reaction Network WinNet
We present the state-of-the-art single-zone nuclear reaction network WinNet , which is capable of calculating the nucleosynthetic yields of a large variety of astrophysical environments and conditions.
M. Reichert +15 more
doaj +1 more source
Transfer Reactions As a Tool in Nuclear Astrophysics
Nuclear reaction rates are one of the most important ingredients in describing how stars evolve. The study of the nuclear reactions involved in different astrophysical sites is thus mandatory to address most questions in nuclear astrophysics.
Faïrouz Hammache +1 more
doaj +1 more source
Investigation of (p,xd) reaction on 120Sn nucleus at proton energy of 30 MeV
For the first time, the double-differential and integral cross-sections of the reaction (p,xd) on the 120Sn nucleus were measured at the energy of the bombarding protons of 30 MeV. Tin is the structural material of the nuclear power plants being designed,
Zh.K. Kerimkulov +4 more
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