| Expressions for the ~(18)F(p,α) ~(15)O and ~(18)F(p,γ) ~(19)Ne Astrophysical Reaction Rates |
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| 作者单位： | Physics,Physics,Physics,Physics,Department,Physics,A.W.Wright Division,Oak Ridge National Laboratory,Oak Ridge,Tennessee 37831,Division,Oak Ridge National Laboratory,Oak Ridge,Tennessee 37831,Division,Oak Ridge National Laboratory,Oak Ridge,Tennessee 37831,Division,Oak Ridge National Laboratory,Oak Ridge,Tennessee 37831,of Physics and Astronomy,University of North Carolina,Chapel Hill,North Carolina 27599,Department,Tennessee Technological University,Cookeville,Tennessee 38505,Nuclear Structure Laboratory,Yale University,New Haven,Connecticut 05511 |
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| 摘 要： | Hydrogen is burned explosively in stellar explosions such as novae, X-ray bursts, X-ray pulsars, and supemovae, as well as possibly in other exotic astrophysical environments such as accretion disks around black holes, Thorne-Zytkow objects, and supermassive stars. Temperatures in these environments range from 107 to 109 K and above, and densities from 102 to 106g/cm3. In such sites,
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