Nuclear Science References (NSR)

NUCLEAR STRUCTURE ⁶He; calculated binding energy of double-Λ ⁶He hypernucleus as a calibrant using several different models, and compared to experimental data. Construction of unified hyperonic EoS for massive neutron stars with limited number of constraints set by phenomenological models.

doi: 10.1103/PhysRevC.95.065803
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2016FA14 Phys.Rev. C 94, 062801 (2016)

J.Fang, H.Pais, S.Avancini, C.Providencia

Larger and more heterogeneous neutron star crusts: A result of strong magnetic fields

doi: 10.1103/PhysRevC.94.062801
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2016FU12 Eur.Phys.J. A 52, 290 (2016)

U.J.Furtado, S.S.Avancini, J.R.Marinelli, W.Martarello, C.Providencia

Neutrino diffusion in the pasta phase matter within the Thomas-Fermi approach

doi: 10.1140/epja/i2016-16290-y
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2014DU14 Phys.Rev. C 90, 055203 (2014)

M.Dutra, O.Lourenco, S.S.Avancini, B.V.Carlson, A.Delfino, D.P.Menezes, C.Providencia, S.Typel, J.R.Stone

Relativistic mean-field hadronic models under nuclear matter constraints

doi: 10.1103/PhysRevC.90.055203
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2014GR14 Phys.Rev. C 90, 045803 (2014)

F.Grill, H.Pais, C.Providencia, Is.Vidana, S.S.Avancini

Equation of state and thickness of the inner crust of neutron stars

doi: 10.1103/PhysRevC.90.045803
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2014PR02 Eur.Phys.J. A 50, 44 (2014)

C.Providencia, S.S.Avancini, R.Cavagnoli, S.Chiacchiera, C.Ducoin, F.Grill, J.Margueron, D.P.Menezes, A.Rabh, I.Vidana

Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars

doi: 10.1140/epja/i2014-14044-7
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2013AV04 Eur.Phys.J. A 49, 75 (2013)

S.S.Avancini, B.V.Carlson, J.R.Marinelli

Nuclear monopole charge form factor calculation for relativistic models including center-of-mass corrections

NUCLEAR STRUCTURE ⁴He, ¹²C; calculated charge formfactor, charge radius using Peierls-Yoccoz projection method for relativistic approaches with reparameterization of the coupling constants. Compared with available data.

doi: 10.1140/epja/i2013-13075-x
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2013DE29 Phys.Rev. C 88, 035804 (2013)

R.C.R.de Lima, S.S.Avancini, C.Providencia

Effect of strong magnetic fields on the nuclear "pasta" phase structure

doi: 10.1103/PhysRevC.88.035804
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2012AV03 Phys.Rev. C 85, 035806 (2012)

S.S.Avancini, C.C.Barros, L.Brito, S.Chiacchiera, D.P.Menezes, C.Providencia

Light clusters in nuclear matter and the "pasta" phase

doi: 10.1103/PhysRevC.85.035806
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2012GR10 Phys.Rev. C 85, 055808 (2012)

F.Grill, C.Providencia, S.S.Avancini

Neutron star inner crust and symmetry energy

doi: 10.1103/PhysRevC.85.055808
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2011AV05 Phys.Rev. C 83, 065805 (2011)

S.S.Avancini, D.P.Menezes, C.Providencia

Finite temperature quark matter under strong magnetic fields

doi: 10.1103/PhysRevC.83.065805
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2010AV06 Phys.Rev. C 82, 025808 (2010)

S.S.Avancini, C.C.Barros, D.P.Menezes, C.Providencia

α particles and the "pasta" phase in nuclear matter

doi: 10.1103/PhysRevC.82.025808
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2010AV08 Phys.Rev. C 82, 055807 (2010); Erratum Phys.Rev. C 85, 059904 (2012)

S.S.Avancini, S.Chiacchiera, D.P.Menezes, C.Providencia

Warm "pasta" phase in the Thomas-Fermi approximation

doi: 10.1103/PhysRevC.82.055807
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2009AV02 Phys.Rev. C 79, 035804 (2009)

S.S.Avancini, L.Brito, J.R.Marinelli, D.P.Menezes, M.M.W.de Moraes, C.Providencia, A.M.Santos

Nuclear "pasta" phase within density dependent hadronic models

doi: 10.1103/PhysRevC.79.035804
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2009ME03 Phys.Rev. C 79, 035807 (2009)

D.P.Menezes, M.B.Pinto, S.S.Avancini, A.Perez Martinez, C.Providencia

Quark matter under strong magnetic fields in the Nambu-Jona-Lasinio model

doi: 10.1103/PhysRevC.79.035807
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2009ME19 Phys.Rev. C 80, 065805 (2009)

D.P.Menezes, M.B.Pinto, S.S.Avancini, C.Providencia

Quark matter under strong magnetic fields in the su(3) Nambu-Jona-Lasinio model

doi: 10.1103/PhysRevC.80.065805
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2009ME21 Eur.Phys.J. A 42, 97 (2009)

D.P.Menezes, S.S.Avancini, C.Z.Vasconcellos, M.Razeira

φ meson effects in the Nolen-Schiffer anomaly

NUCLEAR STRUCTURE ⁴¹Ca, ⁴¹Sc; calculated binding energy, radii, surface energy, proton skin thickness. ¹⁷O, ¹⁷F, ²⁷Al, ²¹Si, ³⁹K, ³⁹Ca, ⁴¹Ca, ⁴¹Sc, ⁸¹Zr, ⁸¹Nb; A=501; calculated mass differences between mirror nuclei pairs. Comparison of four relativistic models and data.

doi: 10.1140/epja/i2009-10848-8
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2008AV04 Phys.Rev. C 78, 015802 (2008)

S.S.Avancini, D.P.Menezes, M.D.Alloy, J.R.Marinelli, M.M.W.Moraes, C.Providencia

Warm and cold pasta phase in relativistic mean field theory

doi: 10.1103/PhysRevC.78.015802
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2008DU05 Phys.Rev. C 77, 035201 (2008)

M.Dutra, O.Lourenco, A.Delfino, J.S.Sa Martins, C.Providencia, S.S.Avancini, D.P.Menezes

Skyrme forces versus relativistic models: Reexamining instabilities

doi: 10.1103/PhysRevC.77.035201
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2007AL30 Phys.Rev. C 75, 054324 (2007)

P.Alberto, S.S.Avancini, M.Fiolhais, J.R.Marinelli

Center-of-mass correction in a relativistic Hartree approximation including meson degrees of freedom

NUCLEAR STRUCTURE ⁴He, ¹⁶O, ⁴⁰Ca; calculated ground state energies and center of mass correction using Peierls_Yoccoz projection method applied to the Hartree solution of the Walecka σ-ω model.

doi: 10.1103/PhysRevC.75.054324
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2007AV03 Phys.Rev. C 75, 055805 (2007)

S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.W.Moraes, C.Providencia

Density dependent hadronic models and the relation between neutron stars and neutron skin thickness

doi: 10.1103/PhysRevC.75.055805
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2007AV06 Phys.Rev. C 76, 064318 (2007)

S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.W.Moraes, A.S.Schneider

Reexamining the neutron skin thickness within a density dependent hadronic model

NUCLEAR STRUCTURE ^40,48Ca, ⁶⁶Ni, ⁹⁰Zr, ²⁰⁸Pb; calculated neutron skin thickness, binding energy, surface energy, density, electron scattering cross sections, asymmetry using Walecka Model.

doi: 10.1103/PhysRevC.76.064318
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2006AL33 Braz.J.Phys. 36, 1375 (2006)

P.Alberto, M.Fiolhais, S.S.Avancini, J.R.Marinelli

Center-of-Mass Correction in a Relativistic Hartree Approximation

NUCLEAR STRUCTURE ⁴He, ¹⁶O, ⁴⁰Ca calculated ground-state energies, center-of-mass corrections. Relativistic Hartree approximation.

doi: 10.1590/S0103-97332006000800009
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2006AV05 Phys.Rev. C 74, 015201 (2006)

S.S.Avancini, D.P.Menezes

Density dependent parametrization models: Formalism and applications

doi: 10.1103/PhysRevC.74.015201
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2006AV07 Phys.Rev. C 74, 024317 (2006)

S.S.Avancini, L.Brito, Ph.Chomaz, D.P.Menezes, C.Providencia

Spinodal instabilities and the distillation effect in relativistic hadronic models

doi: 10.1103/PhysRevC.74.024317
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2006BR23 Phys.Rev. C 74, 045801 (2006)

L.Brito, C.Providencia, A.M.Santos, S.S.Avancini, D.P.Menezes, Ph.Chomaz

Unstable modes in relativistic neutron-electron-proton (npe) matter at finite temperature

doi: 10.1103/PhysRevC.74.045801
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2006PR04 Phys.Rev. C 73, 025805 (2006)

C.Providencia, L.Brito, S.S.Avancini, D.P.Menezes, Ph.Chomaz

Low-density instabilities in relativistic asymmetric matter of compact stars

doi: 10.1103/PhysRevC.73.025805
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2006PR21 Phys.Rev. C 74, 045802 (2006)

C.Providencia, L.Brito, A.M.S.Santos, D.P.Menezes, S.S.Avancini

Coupling of nuclear and electron modes in relativistic stellar matter

doi: 10.1103/PhysRevC.74.045802
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2005AV05 Phys.Rev. C 71, 044323 (2005)

S.S.Avancini, L.Brito, D.P.Menezes, C.Providencia

Collective modes in relativistic asymmetric nuclear matter

doi: 10.1103/PhysRevC.71.044323
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2005AV07 Braz.J.Phys. 35, 832 (2005)

S.S.Avancini, D.P.Menezes, L.Brito, C.Providencia

Asymmetric Nuclear Matter and its Instabilities

doi: 10.1590/S0103-97332005000500031
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2005AV08 Braz.J.Phys. 35, 861 (2005)

S.S.Avancini, F.F.de Souza Cruz, J.R.Marinelli, D.P.Menezes, M.M.Watanabe de Moraes

Analytical Treatment for the Deuteron-Deuteron Interaction

doi: 10.1590/S0103-97332005000500039
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2004AV01 J.Phys.(London) G30, 27 (2004)

S.S.Avancini, M.E.Bracco, M.Chiapparini, D.P.Menezes

On the density-dependent hadron field theory at finite temperature and its thermodynamical consistency

doi: 10.1088/0954-3899/30/2/003
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2004AV04 Phys.Rev. C 70, 015203 (2004)

S.S.Avancini, L.Brito, D.P.Menezes, C.Providencia

Instabilities in asymmetric nuclear matter

doi: 10.1103/PhysRevC.70.015203
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2003AV01 Phys.Rev. C 67, 024301 (2003)

S.S.Avancini, M.E.Bracco, M.Chiapparini, D.P.Menezes

Relativistic mean-field approximation in a density dependent parametrization model at finite temperature

doi: 10.1103/PhysRevC.67.024301
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2003AV06 Braz.J.Phys. 33, 177 (2003)

S.S.Avancini

Some Unusual Algebraic Structures and their Applications in Many-Body Problems

doi: 10.1590/s0103-97332003000200004
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2000AV03 Phys.Rev. C62, 024312 (2000)

S.S.Avancini, F.F.de Souza Cruz, J.R.Marinelli, D.P.Menezes

Quonic Expansion and Its Random-Phase Approximation Counterpart

doi: 10.1103/PhysRevC.62.024312
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1999AV06 J.Phys.(London) G25, 1829 (1999)

S.S.Avancini, J.R.Marinelli, D.P.Menezes

Boson Mapping for a Single j-Shell within the Quon Statistics

doi: 10.1088/0954-3899/25/9/306
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1998AV01 Int.J.Mod.Phys. E7, 379 (1998)

S.S.Avancini, J.R.Marinelli, D.P.Menezes, M.M.Watanabe de Moraes, N.Yoshinaga

Exact Dyson Expansion for a Single J-Shell within the Quon Algebra

doi: 10.1142/S0218301398000178
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1995AV01 J.Phys.(London) G21, 63 (1995)

S.S.Avancini, E.J.V.de Passos

Electron Scattering by ¹²C in the Microscopic Sp(Perpendicular)(1, R) Model

NUCLEAR STRUCTURE ¹²C; calculated levels, B(λ), longitudinal, elastic form factors. Microscopic Sp(1, R) model.

NUCLEAR REACTIONS ¹²C(e, e), (e, e'), E not given; calculated longitudinal, elastic form factors. Microscopic Sp(1, R) model.

doi: 10.1088/0954-3899/21/1/008
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1993AV01 J.Phys.(London) G19, 125 (1993)

S.S.Avancini, E.J.V.de Passos

The Physical Content of the Sp(1, R) Model

NUCLEAR STRUCTURE ¹²C; calculated levels, B(λ), quadrupole moments. Deformed harmonic oscillator wave functions, Sp(1, R) model.

doi: 10.1088/0954-3899/19/1/009
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