Constança Providência

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Débora Peres MenezesUniversidade Federal de Santa CatarinaZweryfikowany adres z ufsc.br
Joao da ProvidenciaProfessor de Física,Universidade de CoimbraZweryfikowany adres z uc.pt
Sidney dos Santos AvanciniProfessor titularZweryfikowany adres z ufsc.br
Márcio FerreiraUniversity of CoimbraZweryfikowany adres z uc.pt
Helena PaisCFisUC, University of Coimbra, PortugalZweryfikowany adres z uc.pt
Isaac VidanaIstituto Nazionale di Fisica Nucleare (INFN), Sezione di CataniaZweryfikowany adres z ct.infn.it
Prafulla K PandaDepartment of Physics, Utkal UniversityZweryfikowany adres z utkaluniversity.ac.in
Tuhin MalikCFisUC, Department of Physics, University of Coimbra, PTZweryfikowany adres z uc.pt
Pedro CostaUniversidade de CoimbraZweryfikowany adres z uc.pt
Aziz RabhiDocteur de Physique, Universite de CoimbraZweryfikowany adres z fis.uc.pt
Alexandre Magno Silva SantosProfessor de Física Adjunto 2, Departamento de Física-UFSCZweryfikowany adres z ufsc.br
Morgane FortinFormerly N. Copernicus Astronomical Center, WarsawZweryfikowany adres z camk.edu.pl
Bijay Kumar AgrawalSaha Institute of Nuclear PhysicsZweryfikowany adres z saha.ac.in
Domenico LogotetaINFN PisaZweryfikowany adres z pi.infn.it
Ignazio BombaciUniversita` di PisaZweryfikowany adres z unipi.it
Philippe chomazCEAZweryfikowany adres z cea.fr
Jérôme MargueronIRL Nuclear Physics and Nuclear Astrophysics, MSU FRIB, USAZweryfikowany adres z cnrs.fr
Mariana DutraInstituto Tecnológico de AeronáuticaZweryfikowany adres z ita.br
Marina NielsenInstituto de Física, Universidade de São PauloZweryfikowany adres z if.usp.br

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Constança Providência

CFisUC, Department of Physics, University of Coimbra, Portugal

Zweryfikowany adres z uc.pt - Strona główna

neutron stars equation of state symmetry energy QCD phase diagram ultrastrong magnetic field


Tytuł Sortuj wg cytatów Sortuj wg roku Sortuj wg tytułu	Cytowane przez Cytowane przez	Rok
A compilation of charged-particle induced thermonuclear reaction rates C Angulo, M Arnould, M Rayet, P Descouvemont, D Baye, ... Nuclear Physics A 656 (1), 3-183, 1999	3032	1999
Relativistic mean-field hadronic models under nuclear matter constraints M Dutra, O Lourenço, SS Avancini, BV Carlson, A Delfino, DP Menezes, ... Physical Review C 90 (5), 055203, 2014	519	2014
Neutron star radii and crusts: Uncertainties and unified equations of state M Fortin, C Providência, AR Raduta, F Gulminelli, JL Zdunik, P Haensel, ... Physical Review C 94 (3), 035804, 2016	342	2016
Quark matter under strong magnetic fields in the Nambu–Jona-Lasinio Model DP Menezes, MB Pinto, SS Avancini, AP Martinez, C Providencia Physical Review C—Nuclear Physics 79 (3), 035807, 2009	338	2009
GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability T Malik, N Alam, M Fortin, C Providência, BK Agrawal, TK Jha, B Kumar, ... Physical Review C 98 (3), 035804, 2018	300	2018
Density dependence of the nuclear symmetry energy: A microscopic perspective I Vidana, C Providência, A Polls, A Rios Physical Review C—Nuclear Physics 80 (4), 045806, 2009	263	2009
Inverse magnetic catalysis in the -flavor Nambu–Jona-Lasinio and Polyakov–Nambu–Jona-Lasinio models M Ferreira, P Costa, O Lourenço, T Frederico, C Providência Physical Review D 89 (11), 116011, 2014	256	2014
Core-crust transition in neutron stars: Predictivity of density developments C Ducoin, J Margueron, C Providência, I Vidana Physical Review C—Nuclear Physics 83 (4), 045810, 2011	215	2011
Hyperons in neutron star matter within relativistic mean-field models M Oertel, C Providência, F Gulminelli, AR Raduta Journal of Physics G: Nuclear and Particle Physics 42 (7), 075202, 2015	186	2015
Estimation of the effect of hyperonic three-body forces on the maximum mass of neutron stars I Vidana, D Logoteta, C Providência, A Polls, I Bombaci Europhysics Letters 94 (1), 11002, 2011	184	2011
Quark matter under strong magnetic fields in the su (3) Nambu–Jona-Lasinio model DP Menezes, MB Pinto, SS Avancini, C Providência Physical Review C—Nuclear Physics 80 (6), 065805, 2009	184	2009
Warm and cold pasta phase in relativistic mean field theory SS Avancini, DP Menezes, MD Alloy, JR Marinelli, MMW Moraes, ... Physical Review C—Nuclear Physics 78 (1), 015802, 2008	166	2008
Deconfinement and chiral restoration within the SU (3) Polyakov–Nambu–Jona-Lasinio and entangled Polyakov–Nambu–Jona-Lasinio models in an external magnetic field M Ferreira, P Costa, DP Menezes, C Providência, NN Scoccola Physical Review D 89 (1), 016002, 2014	147	2014
Hypernuclei and massive neutron stars M Fortin, SS Avancini, C Providência, I Vidaña Physical Review C 95 (6), 065803, 2017	138	2017
Equation of state and thickness of the inner crust of neutron stars F Grill, H Pais, C Providência, I Vidana, SS Avancini Physical Review C 90 (4), 045803, 2014	129	2014
QCD critical end point under strong magnetic fields SS Avancini, DP Menezes, MB Pinto, C Providencia Physical Review D—Particles, Fields, Gravitation, and Cosmology 85 (9), 091901, 2012	123	2012
Nuclear “pasta” phase within density dependent hadronic models SS Avancini, L Brito, JR Marinelli, DP Menezes, MMW de Moraes, ... Physical Review C—Nuclear Physics 79 (3), 035804, 2009	117	2009
Neutron star properties and the symmetry energy R Cavagnoli, DP Menezes, C Providencia Physical Review C—Nuclear Physics 84 (6), 065810, 2011	115	2011
Warm “pasta” phase in the Thomas-Fermi approximation SS Avancini, S Chiacchiera, DP Menezes, C Providência Physical Review C—Nuclear Physics 82 (5), 055807, 2010	115	2010
Quark–hadron phase transition in a neutron star under strong magnetic fields A Rabhi, H Pais, PK Panda, C Providencia Journal of Physics G: Nuclear and Particle Physics 36 (11), 115204, 2009	111	2009

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