Decay branching ratios of excitedMg24
Autor: | A. Czeszumska, Richard Hughes, D. Lee, M. Dag, R. Chyzh, J. J. Ressler, Eric B. Norman, E. McCleskey, T.J. Ross, Jason Burke, R. A. E. Austin, Robert Casperson, J. Munson, M. McCleskey, L. W. Phair, P. Chodash, Antti Saastamoinen, M. S. Basunia, Shuichi Ota, A. Spiridon |
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Rok vydání: | 2017 |
Předmět: |
Physics
Nuclear reaction Range (particle radiation) 010308 nuclear & particles physics Coulomb barrier Inelastic scattering Branching (polymer chemistry) 01 natural sciences Nuclear physics medicine.anatomical_structure Excited state 0103 physical sciences medicine Atomic physics 010306 general physics α particles Nucleus |
Zdroj: | Physical Review C. 95 |
ISSN: | 2469-9993 2469-9985 |
Popis: | Author(s): Munson, JM; Norman, EB; Burke, JT; Casperson, RJ; Phair, LW; McCleskey, E; McCleskey, M; Lee, D; Hughes, RO; Ota, S; Czeszumska, A; Chodash, PA; Saastamoinen, AJ; Austin, RAE; Spiridon, AE; Dag, M; Chyzh, R; Basunia, MS; Ressler, JJ; Ross, TJ | Abstract: The nuclear reactions C12(C12,α)Ne20, C12(C12,p)Na23, and C12(C12,n)Mg23 are the primary reactions in carbon burning, which occurs as part of several stellar processes. The Gamow window, which describes the energy range where most of these reactions take place, is typically around 1.5 MeV in the center-of-mass frame. Direct measurements of the cross sections at this energy are difficult due to the large Coulomb barrier present between the carbon nuclei; however, a successful surrogate measurement can provide the branching ratios between these reactions while avoiding the C12+C12 Coulomb barrier. An experiment was performed using inelastic scattering of 40 MeV α particles on Mg24 as a possible surrogate for the C12+C12 compound nucleus. |
Databáze: | OpenAIRE |
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