https://doi.org/10.1051/epjconf/201611308003
Low-energy calculations for nuclear photodisintegration
1 Dipartimento di Fisica, Università di Trento, I-38123 Trento, Italy
2 Istituto Nazionale di Fisica Nucleare, TIFPA, I-38123 Trento, Italy
3 Russian Research Centre “Kurchatov” Institute, Kurchatov Square, 123182 Moscow, Russia
a e-mail: s.deflorian.2@unitn.it
Published online: 25 March 2016
In the Standard Solar Model a central role in the nucleosynthesis is played by reactions of the kind 
, which enter the proton-proton chains. These reactions can also be studied through the inverse photodisintegration reaction. One option is to use the Lorentz Integral Transform approach, which transforms the continuum problem into a bound state-like one. A way to check the reliability of such methods is a direct calculation, for example using the Kohn Variational Principle to obtain the scattering wave function and then directly calculate the response function of the reaction.
© Owned by the authors, published by EDP Sciences, 2016
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