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  • 25.40  (2)
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    The European physical journal 327 (1987), S. 71-74 
    ISSN: 1434-601X
    Keywords: 23.20 ; 25.40 ; 25.88
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We have studied the14N(p, γ)15O reaction leading into thej π=1/2+ resonance atE cm =260 keV in the proton channel. Our calculation is based on a potential model for nuclear bremsstrahlung allowing both fragments to have non-vanishing spins. Our study reproduces consistently the total width of the final resonance as well as the capture cross sections into this state thereby not confirming a contradiction between these two experimental data sets as discussed recently.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    The European physical journal 325 (1986), S. 309-315 
    ISSN: 1434-601X
    Keywords: 25.40 ; 97.10
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We have updated and recalculated the21Na(p, γ)22Mg and22Na(p, γ)23Mg reaction rates for temperatures 107–109 K relevant for explosive hydrogen burning in stellar environment. We find the21Na(p, γ)22Mg rate lower than recently suggested. Considering various uncertainties in spin and parity assignments of the low energy22Na+p resonances we present upper and lower limits for the22Na(p, γ)23Mg reaction rate which, however, allows for a meaningful discussion of the consequences of the new rates on the Ne - Na cycle under various stellar conditions.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
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