NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of May 10, 2024.

Search: Author = C.Providencia

Found 143 matches.

    Showing 1 to 100.


Back to query form

2024PE05      Phys.Rev. C 109, 025206 (2024)

R.C.Pereira, P.Costa, C.Providencia, J.Moreira

New approach to the 3-momentum regularization of the in-medium one- and two-fermion line integrals with applications to cross sections in the Nambu-Jona-Lasinio model

doi: 10.1103/PhysRevC.109.025206
Citations: PlumX Metrics

2022AN24      Eur.Phys.J. A 58, 254 (2022)

D.Antonopoulou, E.Bozzo, C.Ishizuka, D.I.Jones, M.Oertel, C.Providencia, L.Tolos, S.Typel

CompOSE: a repository for neutron star equations of state and transport properties

doi: 10.1140/epja/s10050-022-00908-2
Citations: PlumX Metrics

2022CU05      Phys.Rev. C 105, 065803 (2022)

T.Custodio, H.Pais, C.Providencia

Heavy baryons in hot stellar matter with light nuclei and hypernuclei

NUCLEAR STRUCTURE 1n, 1,2,3,4H, 3,4,6He; calculated unbound nucleon and light cluster fractions as a function of temperature, density, mass fractions of Λ, Σ, and Ξ hyperons, Δ isobars, 1n, 1,2,3H, 3,4,6He light clusters, and 3,4H, 6He hypernuclei clusters as a function of the density; deduced that heavy-baryons, hyperons and Δs favor the formation of clusters, while a larger number of clusters decreases the fraction of free nucleons, favoring processes such as direct Urca reactions. Relativistic mean-field theory (RMF) with DD2 and FSU2H models. Relevance to the production of light nuclei, hypernuclei heavy baryons such as hyperons and Δ baryons in the low-density matter of stellar environments such as supernova or binary mergers.

doi: 10.1103/PhysRevC.105.065803
Citations: PlumX Metrics

2022MA50      Phys.Rev. C 106, L042801 (2022)

T.Malik, B.K.Agrawal, C.Providencia

Inferring the nuclear symmetry energy at suprasaturation density from neutrino cooling

doi: 10.1103/PhysRevC.106.L042801
Citations: PlumX Metrics

2022MA57      Phys.Rev. C 106, 055801 (2022)

K.D.Marquez, D.P.Menezes, H.Pais, C.Providencia

Δ baryons in neutron stars

doi: 10.1103/PhysRevC.106.055801
Citations: PlumX Metrics

2022SU24      Phys.Rev. C 106, 035805 (2022)

L.Suleiman, M.Fortin, J.L.Zdunik, C.Providencia

Polytropic fits of modern and unified equations of state

doi: 10.1103/PhysRevC.106.035805
Citations: PlumX Metrics

2022TY01      Eur.Phys.J. A 58, 221 (2022)

S.Typel, M.Oertel, T.Klahn, D.Chatterjee, V.Dexheimer, C.Ishizuka, M.Mancini, J.Novak, H.Pais, C.Providencia, Ad.R.Raduta, M.Servillat, L.Tolos, for the CompOSE Core Collaboration

CompOSE reference manual

doi: 10.1140/epja/s10050-022-00847-y
Citations: PlumX Metrics

2021BO13      Phys.Rev. C 103, 055804 (2021)

O.Boukari, H.Pais, S.Antic, C.Providencia

Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter

doi: 10.1103/PhysRevC.103.055804
Citations: PlumX Metrics

2021CU03      Phys.Rev. C 104, 035801 (2021)

T.Custodio, H.Pais, C.Providencia

Light hyperclusters and hyperons in low-density hot stellar matter

NUCLEAR STRUCTURE 2,3H, 3,4,6He; calculated mass fractions of light clusters and unbound protons and neutrons in equilibrium versus density for temperature T=10, 30, 50, 100 MeV, unbound nucleon and light cluster fractions with and without hyperons as function of temperature T=10-100 MeV, unbound nucleon and hyperon (Λ, Σ, Ξ) fractions, total mass fraction of the light clusters, and mass fractions of the unbound protons and neutrons, Λ, Σ and Ξ, light clusters, and light hypernuclei as a function of the density, with and without light clusters; deduced that dissolution of the less-abundant clusters occurs at larger densities due to smaller Pauli-blocking effects. Calculations based on relativistic mean-field model (RMF) with density-dependent (DD) couplings in low-density matter. Relevance to the presence of light nuclei in core-collapse supernova matter and in binary neutron star (NS) mergers.

doi: 10.1103/PhysRevC.104.035801
Citations: PlumX Metrics

2021FE10      Eur.Phys.J. A 57, 263 (2021)

M.Ferreira, A.Rabhi, C.Providencia

Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields

doi: 10.1140/epja/s10050-021-00572-y
Citations: PlumX Metrics

2021PA23      Eur.Phys.J. A 57, 193 (2021)

H.Pais, B.Bertolino, J.Fang, X.Wang, C.Providencia

Strong magnetic fields: neutron stars with an extended inner crust

doi: 10.1140/epja/s10050-021-00506-8
Citations: PlumX Metrics

2021RA08      Phys.Rev. C 103, 035811 (2021)

A.Rabhi, C.Providencia, S.A.Moszkowski, J.da Providencia, H.Bohr

Neutron stars within the Bogoliubov quark-meson coupling model

doi: 10.1103/PhysRevC.103.035811
Citations: PlumX Metrics

2020CU05      Eur.Phys.J. A 56, 295 (2020)

T.Custodio, A.Falcao, H.Pais, C.Providencia, F.Gulminelli, G.Ropke

Light clusters in warm stellar matter: calibrating the cluster couplings

doi: 10.1140/epja/s10050-020-00302-w
Citations: PlumX Metrics

2020MA58      Phys.Rev. C 102, 052801(R) (2020)

T.Malik, B.K.Agrawal, C.Providencia, J.N.De

Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters

doi: 10.1103/PhysRevC.102.052801
Citations: PlumX Metrics

2020PA23      Phys.Rev.Lett. 125, 012701 (2020)

H.Pais, R.Bougault, F.Gulminelli, C.Providencia, E.Bonnet, B.Borderie, A.Chbihi, J.D.Frankland, E.Galichet, D.Gruyer, M.Henri, N.Le Neindre, O.Lopez, L.Manduci, M.Parlog, G.Verde

Low Density In-Medium Effects on Light Clusters from Heavy-Ion Data

NUCLEAR REACTIONS 124Sn(136Xe, X), 112Sn(124Xe, X), E not given; analyzed available data; deduced chemical constants from heavy-ion collisions.

doi: 10.1103/PhysRevLett.125.012701
Citations: PlumX Metrics

2019MA35      Phys.Rev. C 99, 052801 (2019)

T.Malik, B.K.Agrawal, J.N.De, S.K.Samaddar, C.Providencia, C.Mondal, T.K.Jha

Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei

doi: 10.1103/PhysRevC.99.052801
Citations: PlumX Metrics

2019PA29      Phys.Rev. C 99, 055806 (2019)

H.Pais, F.Gulminelli, C.Providencia, G.Ropke

Full distribution of clusters with universal couplings and in-medium effects

NUCLEAR STRUCTURE 2,3H, 3,4He; A=4-12; calculated mass fraction of light- and exotic-clusters within nuclear matter using relativistic mean field framework. Relevance to warm nonhomogeneous matter at subsaturation densities in core-collapse supernova or neutron star mergers.

doi: 10.1103/PhysRevC.99.055806
Citations: PlumX Metrics

2018AV04      Phys.Rev. C 98, 025805 (2018)

S.Avancini, B.P.Bertolino, A.Rabhi, J.Fang, H.Pais, C.Providencia

Stability of the neutron-proton-electron matter under strong magnetic fields: The covariant Vlasov approach

doi: 10.1103/PhysRevC.98.025805
Citations: PlumX Metrics

2018MA58      Phys.Rev. C 98, 035804 (2018)

T.Malik, N.Alam, M.Fortin, C.Providencia, B.K.Agrawal, T.K.Jha, B.Kumar, S.K.Patra

GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability

doi: 10.1103/PhysRevC.98.035804
Citations: PlumX Metrics

2018PA17      Phys.Rev. C 97, 045805 (2018)

H.Pais, F.Gulminelli, C.Providencia, G.Ropke

Light clusters in warm stellar matter: Explicit mass shifts and universal cluster-meson couplings

doi: 10.1103/PhysRevC.97.045805
Citations: PlumX Metrics

2017AL21      Phys.Rev. C 95, 055808 (2017)

N.Alam, H.Pais, C.Providencia, B.K.Agrawal

Warm unstable asymmetric nuclear matter: Critical properties and the density dependence of the symmetry energy

NUCLEAR STRUCTURE 208Pb; calculated binding energy per particle, charge radii, neutron radii, and neutron skin thickness for 208Pb along with the maximum mass of a neutron star and corresponding radius using several relativistic mean-field models.

doi: 10.1103/PhysRevC.95.055808
Citations: PlumX Metrics

2017AV02      Phys.Rev. C 95, 045804 (2017)

S.S.Avancini, M.Ferreira, H.Pais, C.Providencia, G.Ropke

Light clusters and pasta phases in warm and dense nuclear matter

doi: 10.1103/PhysRevC.95.045804
Citations: PlumX Metrics

2017FA04      Phys.Rev. C 95, 045802 (2017)

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

Effect of strong magnetic fields on the crust-core transition and inner crust of neutron stars

doi: 10.1103/PhysRevC.95.045802
Citations: PlumX Metrics

2017FA06      Phys.Rev. C 95, 062801 (2017)

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

Crust-core transition of a neutron star: Effects of the symmetry energy and temperature under strong magnetic fields

doi: 10.1103/PhysRevC.95.062801
Citations: PlumX Metrics

2017FO12      Phys.Rev. C 95, 065803 (2017)

M.Fortin, S.S.Avancini, C.Providencia, I.Vidana

Hypernuclei and massive neutron stars

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
Citations: PlumX Metrics

2017GR10      Phys.Rev. C 95, 055807 (2017)

G.Grams, A.M.Santos, P.K.Panda, C.Providencia, D.P.Menezes

Nuclear pasta phases within the quark-meson coupling model

doi: 10.1103/PhysRevC.95.055807
Citations: PlumX Metrics

2017ME12      Phys.Rev. C 96, 045803 (2017)

D.P.Menezes, C.Providencia

Hyperons in the nuclear pasta phase

doi: 10.1103/PhysRevC.96.045803
Citations: PlumX Metrics

2016AL25      Phys.Rev. C 94, 052801 (2016)

N.Alam, B.K.Agrawal, M.Fortin, H.Pais, C.Providencia, Ad.R.Raduta, A.Sulaksono

Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation

doi: 10.1103/PhysRevC.94.052801
Citations: PlumX Metrics

2016BO07      Eur.Phys.J. A 52, 58 (2016)

I.Bombaci, D.Logoteta, I.Vidana, C.Providencia

Quark matter nucleation in neutron stars and astrophysical implications

doi: 10.1140/epja/i2016-16058-5
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2016FO18      Phys.Rev. C 94, 035804 (2016)

M.Fortin, C.Providencia, Ad.R.Raduta, F.Gulminelli, J.L.Zdunik, P.Haensel, M.Bejger

Neutron star radii and crusts: Uncertainties and unified equations of state

doi: 10.1103/PhysRevC.94.035804
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2016OE01      Eur.Phys.J. A 52, 50 (2016)

M.Oertel, F.Gulminelli, C.Providencia, A.R.Raduta

Hyperons in neutron stars and supernova cores

doi: 10.1140/epja/i2016-16050-1
Citations: PlumX Metrics

2016PA15      Phys.Rev. C 93, 045802 (2016)

H.Pais, A.Sulaksono, B.K.Agrawal, C.Providencia

Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness

NUCLEAR STRUCTURE 48Ca, 132Sn, 208Pb; calculated total binding energies, charge and neutron radii for selected parametrizations, skin thickness for 208Pb; investigated correlations of crust-core transition density and pressure in neutron stars with the slope of the symmetry energy and neutron skin thickness using different families of mean-field parametrization in relativistic nonlinear Walecka model (NLWM). Asymmetric nuclear and stellar matter at zero temperature.

doi: 10.1103/PhysRevC.93.045802
Citations: PlumX Metrics

2016PA26      Phys.Rev. C 93, 065805 (2016)

H.Pais, D.P.Menezes, C.Providencia

Neutron stars: From the inner crust to the core with the (extended) Nambu-Jona-Lasinio model

doi: 10.1103/PhysRevC.93.065805
Citations: PlumX Metrics

2016PA30      Phys.Rev. C 94, 015808 (2016)

H.Pais, C.Providencia

Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of state

doi: 10.1103/PhysRevC.94.015808
Citations: PlumX Metrics

2015ME05      Phys.Rev. C 91, 065205 (2015); Erratum Phys.Rev. C 97, 029904 (2018)

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

Anisotropy in the equation of state of magnetized quark matter

doi: 10.1103/PhysRevC.91.065205
Citations: PlumX Metrics

2015PA28      Phys.Rev. C 91, 055801 (2015)

H.Pais, S.Chiacchiera, C.Providencia

Light clusters, pasta phases, and phase transitions in core-collapse supernova matter

doi: 10.1103/PhysRevC.91.055801
Citations: PlumX Metrics

2015RA06      Phys.Rev. C 91, 045803 (2015)

A.Rabhi, M.A.Perez-Garcia, C.Providencia, I.Vidana

Magnetic susceptibility and magnetization properties of asymmetric nuclear matter in a strong magnetic field

doi: 10.1103/PhysRevC.91.045803
Citations: PlumX Metrics

2014CA04      Eur.Phys.J. A 50, 13 (2014)

A.Carbone, A.Polls, C.Providencia, A.Rios, I.Vidana

Tensor force effects and high-momentum components in the nuclear symmetry energy

doi: 10.1140/epja/i2014-14013-2
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2014ME06      Phys.Rev. C 89, 055207 (2014)

D.P.Menezes, M.B.Pinto, L.B.Castro, P.Costa, C.Providencia

Repulsive vector interaction in three-flavor magnetized quark and stellar matter

doi: 10.1103/PhysRevC.89.055207
Citations: PlumX Metrics

2014PA15      Phys.Rev. C 89, 045803 (2014)

P.K.Panda, D.P.Menezes, C.Providencia

Effects of the symmetry energy on the kaon condensates in the quark-meson coupling model

doi: 10.1103/PhysRevC.89.045803
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2013LO11      Nucl.Phys. A914, 433c (2013)

D.Logoteta, I.Vidana, C.Providencia

Two-meson exchange hyperonic three-body forces and consequences for neutron stars

doi: 10.1016/j.nuclphysa.2013.01.022
Citations: PlumX Metrics

2013LO14      Phys.Rev. C 88, 055802 (2013)

D.Logoteta, C.Providencia, I.Vidana

Formation of hybrid stars from metastable hadronic stars

doi: 10.1103/PhysRevC.88.055802
Citations: PlumX Metrics

2013PR04      Phys.Rev. C 87, 055801 (2013)

C.Providencia, A.Rabhi

Interplay between the symmetry energy and the strangeness content of neutron stars

doi: 10.1103/PhysRevC.87.055801
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2012FE07      Phys.Rev. C 85, 055811 (2012)

M.Ferreira, C.Providencia

Description of light clusters in relativistic nuclear models

doi: 10.1103/PhysRevC.85.055811
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2012LO06      Phys.Rev. C 85, 055807 (2012)

D.Logoteta, C.Providencia, I.Vidana, I.Bombaci

Quark matter nucleation with a microscopic hadronic equation of state

doi: 10.1103/PhysRevC.85.055807
Citations: PlumX Metrics

2012PA12      Phys.Rev. C 85, 055802 (2012)

P.K.Panda, A.M.S.Santos, D.P.Menezes, C.Providencia

Compact stars within a soft symmetry energy quark-meson-coupling model

doi: 10.1103/PhysRevC.85.055802
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2011CA09      Phys.Rev. C 83, 045201 (2011)

R.Cavagnoli, C.Providencia, D.P.Menezes

Hadron-quark phase transition in asymmetric matter with boson condensation

doi: 10.1103/PhysRevC.83.045201
Citations: PlumX Metrics

2011CA28      Phys.Rev. C 84, 065810 (2011)

R.Cavagnoli, D.P.Menezes, C.Providencia

Neutron star properties and the symmetry energy

doi: 10.1103/PhysRevC.84.065810
Citations: PlumX Metrics

2011DU13      Phys.Rev. C 83, 045810 (2011)

C.Ducoin, J.Margueron, C.Providencia, I.Vidana

Core-crust transition in neutron stars: Predictivity of density developments

doi: 10.1103/PhysRevC.83.045810
Citations: PlumX Metrics

2011PE25      Phys.Rev. C 84, 045803 (2011)

M.A.Perez-Garcia, C.Providencia, A.Rabhi

Landau parameters for asymmetric nuclear matter with a strong magnetic field

doi: 10.1103/PhysRevC.84.045803
Citations: PlumX Metrics

2011RA09      Phys.Rev. C 83, 055801 (2011)

A.Rabhi, C.Providencia

Quark matter under strong magnetic fields in chiral models

doi: 10.1103/PhysRevC.83.055801
Citations: PlumX Metrics

2011RA28      Phys.Rev. C 84, 035803 (2011)

A.Rabhi, P.K.Panda, C.Providencia

Warm and dense stellar matter under strong magnetic fields

doi: 10.1103/PhysRevC.84.035803
Citations: PlumX Metrics

2011VI07      Phys.Rev. C 84, 062801 (2011)

I.Vidana, A.Polls, C.Providencia

Nuclear symmetry energy and the role of the tensor force

doi: 10.1103/PhysRevC.84.062801
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2010LE10      Phys.Rev. C 82, 015809 (2010)

C.H.Lenzi, A.S.Schneider, C.Providencia, R.M.Marinho

Compact stars with a quark core within the Nambu-Jona-Lasinio (NJL) model

doi: 10.1103/PhysRevC.82.015809
Citations: PlumX Metrics

2010MA09      Phys.Rev. C 81, 024307 (2010)

G.F.Marranghello, C.Providencia, A.M.S.Santos

Isospin constraints on the parametric coupling model for nuclear matter

doi: 10.1103/PhysRevC.81.024307
Citations: PlumX Metrics

2010PA24      Phys.Rev. C 82, 025801 (2010)

H.Pais, A.Santos, L.Brito, C.Providencia

Dynamical properties of nuclear and stellar matter and the symmetry energy

doi: 10.1103/PhysRevC.82.025801
Citations: PlumX Metrics

2010PA31      Phys.Rev. C 82, 045801 (2010)

P.K.Panda, C.Providencia, D.P.Menezes

Warm stellar matter within the quark-meson-coupling model

doi: 10.1103/PhysRevC.82.045801
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2009BO26      Eur.Phys.J. A 41, 355 (2009)

H.Bohr, C.Providencia, J.da Providencia

Color-symmetric superconductivity in a phenomenological QCD model

doi: 10.1140/epja/i2009-10832-4
Citations: PlumX Metrics

2009CH37      Nucl.Phys. A826, 178 (2009)

M.Chiapparini, M.E.Bracco, A.Delfino, M.Malheiro, D.P.Menezes, C.Providencia

Hadron production in non-linear relativistic mean field models

doi: 10.1016/j.nuclphysa.2009.05.002
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2009PA27      Phys.Rev. C 80, 014905 (2009)

P.K.Panda, D.P.Menezes, C.Providencia

Particle production within the quark meson coupling model

doi: 10.1103/PhysRevC.80.014905
Citations: PlumX Metrics

2009PA39      Phys.Rev. C 80, 045808 (2009)

H.Pais, A.Santos, C.Providencia

Dynamical instabilities of warm npe matter: δ meson effects

doi: 10.1103/PhysRevC.80.045808
Citations: PlumX Metrics

2009RA02      Phys.Rev. C 79, 015804 (2009)

A.Rabhi, C.Providencia, J.Da Providencia

Spinodal instabilities and the distillation effect in nuclear matter under strong magnetic fields

doi: 10.1103/PhysRevC.79.015804
Citations: PlumX Metrics

2009RA20      Phys.Rev. C 80, 025806 (2009)

A.Rabhi, C.Providencia, J.Da Providencia

Effect of the δ meson on the instabilities of nuclear matter under strong magnetic fields

doi: 10.1103/PhysRevC.80.025806
Citations: PlumX Metrics

2009SA16      Phys.Rev. C 79, 045805 (2009)

A.M.Santos, C.Providencia, P.K.Panda

Low density instabilities in asymmetric nuclear matter within the quark-meson coupling (QMC) model with the δ meson

doi: 10.1103/PhysRevC.79.045805
Citations: PlumX Metrics

2009VI07      Phys.Rev. C 80, 045806 (2009)

I.Vidana, C.Providencia, A.Polls, A.Rios

Density dependence of the nuclear symmetry energy: A microscopic perspective

NUCLEAR STRUCTURE 132Sn, 208Pb; calculated neutron skin thickness, and transition densities using microscopic Brueckner-Hartree-Fock approach using the realistic AV18 potential plus a three-body force of Urbana type.

doi: 10.1103/PhysRevC.80.045806
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2008DU19      Phys.Rev. C 78, 055801 (2008)

C.Ducoin, C.Providencia, A.M.Santos, L.Brito, Ph.Chomaz

Cluster formation in compact stars: Relativistic versus Skyrme nuclear models

doi: 10.1103/PhysRevC.78.055801
Citations: PlumX Metrics

2008SA15      Phys.Rev. C 77, 045805 (2008)

A.M.Santos, L.Brito, C.Providencia

Dynamical instabilities in density-dependent hadronic relativistic models

doi: 10.1103/PhysRevC.77.045805
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2007BR28      Phys.Rev. C 76, 044316 (2007)

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

Low-density expansion and isospin dependence of nuclear energy functional: Comparison between relativistic and Skyrme models

doi: 10.1103/PhysRevC.76.044316
Citations: PlumX Metrics

2007ME17      Nucl.Phys. A790, 558c (2007)

D.P.Menezes, D.B.Melrose, C.Providencia, K.Wu

The QCD phase diagram and the gamma-ray bursts

doi: 10.1016/j.nuclphysa.2007.03.094
Citations: PlumX Metrics

2007ME26      Phys.Rev. C 76, 064902 (2007)

D.P.Menezes, C.Providencia, M.Chiapparini, M.E.Bracco, A.Delfino, M.Malheiro

Constraining relativistic models through heavy ion collisions

doi: 10.1103/PhysRevC.76.064902
Citations: PlumX Metrics

2007PA28      Phys.Rev. C 75, 065806 (2007)

P.K.Panda, C.Providencia, J.da Providencia

Tensor interaction and short range correlations in relativistic nuclear models

doi: 10.1103/PhysRevC.75.065806
Citations: PlumX Metrics

2007TS03      Prog.Theor.Phys.(Kyoto) 117, 431 (2007)

Y.Tsue, C.Providencia, J.da Providencia, M.Yamamura

Semi-Classical Approach to the Two-Level Pairing Model - Various Aspects of Phase Change -

doi: 10.1143/PTP.117.431
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2006ME05      Phys.Rev. C 73, 025806 (2006)

D.P.Menezes, D.B.Melrose, C.Providencia, K.Wu

γ-ray bursts and the QCD phase diagram

doi: 10.1103/PhysRevC.73.025806
Citations: PlumX Metrics

2006PA14      Phys.Rev. C 73, 035805 (2006)

P.K.Panda, J.da Providencia, C.Providencia

Short range correlations in relativistic nuclear matter models

doi: 10.1103/PhysRevC.73.035805
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2006PR07      Prog.Theor.Phys.(Kyoto) 115, 547 (2006)

C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura

Boson Realization of the su(3)-Algebra. III - Schwinger Representation for the Elliot Model -

doi: 10.1143/PTP.115.547
Citations: PlumX Metrics

2006PR08      Prog.Theor.Phys.(Kyoto) 115, 561 (2006)

C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura

Boson Realization of the su(3)-Algebra. IV - Holstein-Primakoff Representation for the Elliot Model-

doi: 10.1143/PTP.115.561
Citations: PlumX Metrics

2006PR10      Prog.Theor.Phys.(Kyoto) 115, 739 (2006)

C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura

A New Boson Realization of the Two-Level Pairing Model in a Many-Fermion System and Its Classical Counterpart - The Role of the su(2) (x) su(1, 1)-Coherent State in the Schwinger Boson Representation for the su(2) (x) su(2)-Algebra-

doi: 10.1143/PTP.115.739
Citations: PlumX Metrics

2006PR11      Prog.Theor.Phys.(Kyoto) 115, 759 (2006)

C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura

A Note on the Two-Level Pairing Model Obeying the su(2) (x) su(2)-Algebra -Re-formation in Terms of the su(1, 1) (x) su(1, 1)-Algebra

doi: 10.1143/PTP.115.759
Citations: PlumX Metrics

2006PR17      Prog.Theor.Phys.(Kyoto) 116, 87 (2006)

C.Providencia, J.da Providencia, Y.Tsue, M.Yamamura

The Lipkin Model in Many-Fermion System as an Example of the su(1, 1) (X) su(1, 1)-Algebraic Model

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
Citations: PlumX Metrics

Back to query form    [Next]