New results for radiation ²H³H radiatiVE capture at astrophysical energy | Izvestiya vuzov. Fizika. 2019. № 3. DOI: 10.17223/00213411/62/3/53

New results for radiation ²H³H radiatiVE capture at astrophysical energy

The calculations of the total cross section, astrophysical S-factor and the rates of ²H³H radiative capture reaction at low energies have been carried out within the framework of a modified potential cluster model with forbidden states that follow from the classification of orbital states of clusters according to Young schemes. It is shown that the model used and the methods for classifying cluster states according to Young schemes allow generally to describe correctly the available experimental data for the total cross section and the astrophysical S-factor of this process.

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Keywords

forbidden states, classification of orbital states according to Young schemes, potential cluster model, total cross sections, thermonuclear reactions, ²H³H system , potential description, radiative capture, elastic scattering, low and astrophysical energies, nuclear astrophysics, light atomic nuclei, запрещенные состояния, классификация орбитальных состояний по схемам Юнга, термоядерные реакции, потенциальная кластерная модель, полные сечения, радиационный захват, потенциальное описание, ²H³H-система , упругое рассеяние, низкие и астрофизические энергии, легкие атомные ядра, ядерная астрофизика

Authors

Name	Organization	E-mail
Dubovichenko S.B.	Fesenkov Astrophysical Institute NCSRT ASA MDASI; Al-Farabi Kazakh National University	dubovichenko@mail.ru; dubovichenko@gmail.com
Zazulin D.M.	Al-Farabi Kazakh National University	denis_zazulin@mail.ru

Всего: 2

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