NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.E.Mosquera Found 13 matches. 2021SA21 Int.J.Mod.Phys. E30, 2150028 (2021) M.M.Saez, K.J.Fushimi, M.E.Mosquera, O.Civitarese Limits on active-sterile neutrino mixing parameters using heavy nuclei abundances
doi: 10.1142/S0218301321500282
2020FU06 Int.J.Mod.Phys. E29, 2050072 (2020) K.Fushimi, M.E.Mosquera, O.Civitarese MSSM WIMPs-Nucleon cross-section for Ex < 500 GeV
doi: 10.1142/S021830132050072X
2020ME05 Phys.Rev. C 101, 035806 (2020) B.E.Melendez, M.E.Mosquera, O.Civitarese Cross sections of ultrahigh-energy neutrinos: Comparison with ICE-CUBE data
doi: 10.1103/PhysRevC.101.035806
2020MO30 Phys.Rev. C 102, 025803 (2020) Cross section of ultrahigh-energy neutrinos: Estimation of the uncertanties due to parton distribution functions NUCLEAR REACTIONS 12C(ν, ν'), (ν, X), (ν-bar, ν-bar'), (ν-bar, X), E=0.3-32000 TeV; calculated σ(E) for charged and neutral currents, and total neutrino scattering σ(E) by included the uncertainties of the parton distribution function. Comparison with the IceCube experimental data.
doi: 10.1103/PhysRevC.102.025803
2017MO36 Phys.Rev. C 96, 045802 (2017) Time variation of fundamental constants in nonstandard cosmological models
doi: 10.1103/PhysRevC.96.045802
2013CI01 Nucl.Phys. A898, 1 (2013) Nuclear structure constrains on resonant energies: A solution of the cosmological 7Li problem? NUCLEAR REACTIONS 7Be(d, pα), (n, p), (α, γ), E not given (low); calculated freeze-out temperature, resonance energy, 7Li, Be cosmic abundance using semi-analytical solution of balance equations.
doi: 10.1016/j.nuclphysa.2012.11.012
2011MO31 Phys.Rev. C 84, 065803 (2011) Constraints on active-sterile neutrino mixing from primordial abundances NUCLEAR STRUCTURE 2H, 4He, 7Li; calculated primordial abundance using a modified version of Kawano's code by including mixing between active and sterile neutrinos.
doi: 10.1103/PhysRevC.84.065803
2010CI02 Nucl.Phys. A846, 157 (2010) O.Civitarese, M.A.Moline, M.E.Mosquera Cosmological bounds to the variation of the Higgs vacuum expectation value: BBN constraints
doi: 10.1016/j.nuclphysa.2010.06.011
2008CI03 Int.J.Mod.Phys. E17, 493 (2008) O.Civitarese, S.J.Landau, M.E.Mosquera Double beta decay rates as test of the time variation of fundamental constants
doi: 10.1142/S0218301308009847
2008CI04 Int.J.Mod.Phys. E17, 351 (2008) Study of the compatibility of LSND and WMAP data
doi: 10.1142/S0218301308006156
2008CI05 Phys.Rev. C 77, 045806 (2008) Testing primordial abundances with sterile neutrinos NUCLEAR STRUCTURE 2H, 3,4He, 7Li; calculated abundances, big-bang model. Comparison with experimental data.
doi: 10.1103/PhysRevC.77.045806
2008CI06 Phys.Rev. C 78, 064308 (2008) O.Civitarese, R.J.Liotta, M.E.Mosquera Effects of resonant and continuum states on the neutrino-nucleus cross section NUCLEAR REACTIONS 208Pb(ν, e-), E<200 MeV; calculated σ, level energies, multipolarities.
doi: 10.1103/PhysRevC.78.064308
2006LA03 Astrophys.J. 637, 38 (2006) S.J.Landau, M.E.Mosquera, H.Vucetich Primordial nucleosynthesis with varying fundamental constants: A semianalytical approach
doi: 10.1086/431417
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