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The top documents tagged [infn laboratori nazionali]
Carlo Broggini, INFN-Padova Nuclear Burning in Stars (E star ) ( E ) = S(E) e –2 E -1 2 cm m m m m Astrophysical Factor Gamow Factor Reaction Rate(star)
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Coulomb excitation of the 42 Ca with AGATA Demonstrator K. Hadyńska-Klęk 1,2 P.J. Napiorkowski 1, A. Maj 3, F. Azaiez 4, J.J. Valiente Dobon 5 on behalf
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Andrea Candelori - Irradiation facilities at the INFN National Laboratory of Legnaro – Irradiation facilities for semiconductor
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Nuclear Burning in Stars (E star ) ( E ) = S(E) e –2 E -1 Reaction Rate(star) (E) (E) dE Gamow Peak Maxwell Boltzmann Extrap.Meas. LUNA results Men in
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Maria Grazia Pia, INFN Genova Epistemic and systematic uncertainties in Monte Carlo simulation: Epistemic and systematic uncertainties in Monte Carlo simulation:
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Maria Grazia Pia, INFN Genova Conceptual challenges and computational progress in X-ray simulation Maria Grazia Pia INFN Genova, Italy Maria Grazia Pia
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Maria Grazia Pia, INFN Genova New techniques in Monte Carlo simulation: experience with a prototype of generic programming application to Geant4 physics
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51 Disintegration of 12C nuclei by 700–1500 MeV photons - Nuclear Physics A, August 2015
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S. Belogurov, ITEP/INR Moscow GERDA experiment 21.10.04 New experiment for the search of neutrinoless double beta decay of 76 Ge at LNGS GERmanium Detector
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Incontro con i referee di CNS3 Milano 28 Febbraio 2014 Isospin dependence of compound nucleus formation and decay ISODEC – Scientific Program LOI@SPES
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Maria Grazia Pia Experimental validation of models in the pre-equilibrium and nuclear de-excitation phase G.A.P. Cirrone 1, G. Cuttone 1, F. Di Rosa 1,
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J. Marton / IMEPRECFA Meeting, Innsbruck, March 26, 2004 EXOTIC ATOM RESEARCH AT DAΦNE J. Marton Institute for Medium Energy Physics Austrian Academy of
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