NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = W.M.Spinella Found 4 matches. 2017RA28 Phys.Rev. C 96, 065807 (2017) I.F.Ranea-Sandoval, M.G.Orsaria, S.Han, F.Weber, W.M.Spinella Color superconductivity in compact stellar hybrid configurations
doi: 10.1103/PhysRevC.96.065807
2016SP02 Eur.Phys.J. A 52, 61 (2016) W.M.Spinella, F.Weber, G.A.Contrera, M.G.Orsaria Neutrino emissivity in the quark-hadron mixed phase of neutron stars
doi: 10.1140/epja/i2016-16061-x
2015DE31 Phys.Rev. C 92, 035810 (2015) S.M.de Carvalho, R.Negreiros, M.Orsaria, G.A.Contrera, F.Weber, W.Spinella Thermal evolution of hybrid stars within the framework of a nonlocal Nambu-Jona-Lasinio model
doi: 10.1103/PhysRevC.92.035810
2014SP01 Phys.Rev. C 90, 014315 (2014) Testing the spin-cutoff parametrization with shell-model calculations NUCLEAR STRUCTURE 11,12,13C, 14N, 16,17O, 20Ne, 22,23,24,25,26,27Na, 24,25,26,27,28,29Mg, 26,27,28,29,30Al, 28,29,30,31,32Si, 30,31,32,33P, 32,33,34S, 34,35Cl, 46,47,48,49,50,51,52Ca, 45,46,47,49Sc, 44,45,46,47Ti, 46V; calculated and analyzed level density parameter ρJ/ρ as function of spin and excitation energy. 12,13C, 14N, 17O, 20Ne, 24,26Mg, 26,27,28Al, 28Si, 34,35Cl, 48,49Ca, 45Sc, 44,45,46,47Ti, 46V; calculated spin-cutoff factors as function of excitation energy, in some cases for both positive and negative parities using semirealistic interactions in the interacting shell model. 22Na, 33S, 44Ti; calculated average J(J+1) as function of excitation energy using shell model and from inverting the thermal average.
doi: 10.1103/PhysRevC.90.014315
Back to query form Note: The following list of authors and aliases matches the search parameter W.M.Spinella: , W.M.SPINELLA |