Nuclear Physics of Stars 2015
DOI: 10.1002/9783527692668.refs
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(4 citation statements)
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“…where µ is the reduced mass of the 30 Si+p system, k the Maxwell-Boltzmann constant, T the temperature, and σ(E) the nuclear reaction cross section at energy E. For the 30 Si(p,γ) 31 P reaction, the resonances of interest are narrow and isolated and the thermonuclear reaction rate becomes [14]:…”
Section: A Methodsmentioning
confidence: 99%
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“…where µ is the reduced mass of the 30 Si+p system, k the Maxwell-Boltzmann constant, T the temperature, and σ(E) the nuclear reaction cross section at energy E. For the 30 Si(p,γ) 31 P reaction, the resonances of interest are narrow and isolated and the thermonuclear reaction rate becomes [14]:…”
Section: A Methodsmentioning
confidence: 99%
“…For unbound states the proton width Γ p is expressed as the product of the proton spectroscopic factor and the single-particle proton width: Γ p = C 2 S p × Γ s.p . The single-particle width is calculated with the formula [14]: c The protons are assumed to be transferred to 2p 3/2 , 1d 3/2 and 1f 7/2 orbitals for = 1, 2 and 3 transitions, respectively.…”
Section: B Proton Width and Resonance Strengthmentioning
confidence: 99%
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