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Studying supernova neutrinos through nuclear structure calculations

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Hellenic Nuclear Physics Society   

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Studying supernova neutrinos through nuclear structure calculations (EN)
Tsakstara, V.
Sinatkas, J.
Kosmas, T. S.
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
2019-11-23
Differential and integrated cross section calculations are performed in the context of the quasi particle random phase approximation (QRPA) by utilizing realistic two- nucleon forces, for the 64,66 Zn isotopes, contents of the COBRA double beta decay detector. For these isotopes the response to supernova neutrinos is of current inter- est. The response of the 66 Zn isotope to the energy-spectra of supernova neutrinos is also explored by convoluting the original results for the differential cross sections by employing: (i) a two-parameter Fermi-Dirac (FD) and (ii) a Power-Law (PL) neutrino energy distribution. Such folded cross sections are useful in low-energy astrophysical-neutrino detection in underground terrestrial experiments. (EN)
Neutrino-nucleus reactions (EN)
Supernovae (EN)
Annual Symposium of the Hellenic Nuclear Physics Society
English
Hellenic Nuclear Physics Society (HNPS) (EN)
2654-0088
2654-007X
Annual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 18 (2010): HNPS2010; 193-199 (EL)
HNPS Advances in Nuclear Physics; Vol. 18 (2010): HNPS2010; 193-199 (EN)
Πνευματική ιδιοκτησία (c) 2019 V. Tsakstara, T. S. Kosmas, J. Sinatkas (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



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