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Neutrinos in Cosmology
I give an overview of the effects of neutrinos on cosmology, focussing in particular on the role played by neutrinos in the evolution of cosmological perturbations. I discuss how recent observations o...
I give an overview of the effects of neutrinos on cosmology, focussing in particular on the role played by neutrinos in the evolution of cosmological perturbations. I discuss how recent observations o...
Astrophysical S-factor of the 12N(p,
)13O Reaction Determined from the (12N,13O) Proton Transfer Reaction
The reaction cross section of the radiative proton capture on the drip line nucleus 12N was studied at the Cyclotron Institute at Texas A&M University. We have employed the indirect Asymptotic Nor...
)13O Reaction Determined from the (12N,13O) Proton Transfer ReactionThe reaction cross section of the radiative proton capture on the drip line nucleus 12N was studied at the Cyclotron Institute at Texas A&M University. We have employed the indirect Asymptotic Nor...
Extracting the Asymptotic Normalization Coefficients in Neutron Transfer Reactions to Determine the Astrophysical Reaction Rates for 22Mg(p,)23Al and 17F(p,)18Ne
AIP Conf. Proc. -- January 24, 2008 -- Volume 972, pp. 439-443
EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (II): Proceedings of the Carpathian Summer School of Physics 2007;
doi:10.1063/1.2870381
Issue Date: 24 January 2008
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T. Al.-Abdullah,a F. Cârstoiu,b X. Chen,a H. Clark,a C. Fu,a C. A. Gagliardi,a Y.-W. Lui,a A. M. Mukhamedzhanov,a G. T
bcaru,a Y. Tokimoto,a L. Trache,a R. E. Tribble,a and Y. Zhaia
aCyclotron Institute, Texas A&M University, College Station, TX 77843, U.S.A.
bNational Institute for Nuclear Physics and Engineering, P.O. Box MG-6, Bucharest, Romania
aCyclotron Institute, Texas A&M University, College Station, TX 77843, U.S.A.
bNational Institute for Nuclear Physics and Engineering, P.O. Box MG-6, Bucharest, Romania
It was expected that rays from 18F and 22Na would be observed in massive One novae, but neither has been to date. The 17F(p,)18Ne and 22Mg(p,)23Al reactions may play important roles in the production and destruction of 18F and 22Na. We have determined the asymptotic normalization coefficients for 18Ne and 23Al through measurements of peripheral neutron transfer reactions in the mirror nuclear systems. We use the ANCs to calculate the astrophysical S-factors and reaction rates for these two reactions.
©2008 American Institute of Physics
rays from 18F and 22Na would be observed in massive One novae, but neither has been to date. The 17F(p,)18Ne and 22Mg(p,)23Al reactions may play important roles in the production and destruction of 18F and 22Na. We have determined the asymptotic normalization coefficients for 18Ne and 23Al through measurements of peripheral neutron transfer reactions in the mirror nuclear systems. We use the ANCs to calculate the astrophysical S-factors and reaction rates for these two reactions.
©2008 American Institute of Physics
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BibSonomy
KEYWORDS and PACS
- 26.50.+x
Nuclear physics aspects of novae, supernovae, and other explosive environments - 26.20.Cd
Stellar hydrogen burning - 26.30.-k
Nucleosynthesis in novae, supernovae and other explosive environments - 95.55.Ka
X- and γ-ray telescopes and instrumentation - 25.70.Hi
Heavy ion-induced transfer reactions - YEAR: 2008
PUBLICATION DATA
0094-243X (print)
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