Cross sections of the 21Ne(α, n)24Mg and 22Ne(α, n)25Mg reactions at low energies of astrophysical interest
- 1 July 1974
- journal article
- Published by Elsevier in Nuclear Physics A
- Vol. 226 (3) , 493-505
- https://doi.org/10.1016/0375-9474(74)90496-5
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- Advanced Evolution of Massive Stars. IV. Secondary Nucleosynthesis During Helium BurningThe Astrophysical Journal, 1972
- Study of the 22Ne(α, n)25Mg reaction: a possible source of stellar neutronSNuclear Physics A, 1969
- Thermonuclear Reaction RatesAnnual Review of Astronomy and Astrophysics, 1967
- Stellar Neutron SourcesThe Astrophysical Journal, 1966
- Nuclear reactions of Ne21 with protons and α particlesNuclear Physics, 1965
- Neutrino Processes and Pair Formation in Massive Stars and Supernovae.The Astrophysical Journal Supplement Series, 1964
- New Neutron Sources of Possible Astrophysical Importance.The Astronomical Journal, 1960
- Synthesis of the Elements in StarsReviews of Modern Physics, 1957
- Nuclear Reactions with the Neon Isotopes in Stars.The Astrophysical Journal, 1957