NSR Query Results

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NSR database version of May 3, 2024.

Search: Author = W.M.Spinella

Found 4 matches.

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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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2014SP01      Phys.Rev. C 90, 014315 (2014)

W.M.Spinella, C.W.Johnson

Testing the spin-cutoff parametrization with shell-model calculations

NUCLEAR STRUCTURE ^11,12,13C, ¹⁴N, ^16,17O, ²⁰Ne, ^{22,23,24,25,26,27}Na, ^{24,25,26,27,28,29}Mg, ^{26,27,28,29,30}Al, ^{28,29,30,31,32}Si, ^30,31,32,33P, ^32,33,34S, ^34,35Cl, ^{46,47,48,49,50,51,52}Ca, ^45,46,47,49Sc, ^44,45,46,47Ti, ⁴⁶V; calculated and analyzed level density parameter ρ_J/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
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Note: The following list of authors and aliases matches the search parameter W.M.Spinella: , W.M.SPINELLA