Literature DB >> 28163609

Physics of Neutron Star Crusts.

Nicolas Chamel1, Pawel Haensel2.   

Abstract

The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.

Year:  2008        PMID: 28163609      PMCID: PMC5255077          DOI: 10.12942/lrr-2008-10

Source DB:  PubMed          Journal:  Living Rev Relativ        ISSN: 1433-8351            Impact factor:   40.429


  26 in total

1.  Superfluidity and thermal response of neutron star crusts.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1996-04-15

2.  Superfluidity and neutron star crust matter.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1996-07-15

3.  Neutrino emissivity from e- synchrotron and e-e+ annihilation processes in a strong magnetic field: General formalism and nonrelativistic limit.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1992-10-15

4.  Neutrino emissivity from e-e+ annihilation in a strong magnetic field: Hot, nondegenerate plasma.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1992-11-15

5.  Specific heat of superfluid matter in the inner crust of neutron stars.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1994-10-15

6.  Neutron star crusts.

Authors: 
Journal:  Phys Rev Lett       Date:  1993-01-25       Impact factor: 9.161

7.  Dynamics of a model of supersolid.

Authors: 
Journal:  Phys Rev Lett       Date:  1994-04-11       Impact factor: 9.161

8.  Direct URCA process in neutron stars.

Authors: 
Journal:  Phys Rev Lett       Date:  1991-05-27       Impact factor: 9.161

9.  Effective mass of neutrons diffracting in crystals.

Authors: 
Journal:  Phys Rev Lett       Date:  1986-12-15       Impact factor: 9.161

10.  Equation of state and the maximum mass of neutron stars.

Authors: 
Journal:  Phys Rev Lett       Date:  1988-11-28       Impact factor: 9.161

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  4 in total

1.  Elastic shocks in relativistic rigid rods and balls.

Authors:  João L Costa; José Natário
Journal:  Proc Math Phys Eng Sci       Date:  2019-05-15       Impact factor: 2.704

2.  A new continuum model for general relativistic viscous heat-conducting media.

Authors:  E Romenski; I Peshkov; M Dumbser; F Fambri
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2020-03-30       Impact factor: 4.226

Review 3.  QCD and strongly coupled gauge theories: challenges and perspectives.

Authors:  N Brambilla; S Eidelman; P Foka; S Gardner; A S Kronfeld; M G Alford; R Alkofer; M Butenschoen; T D Cohen; J Erdmenger; L Fabbietti; M Faber; J L Goity; B Ketzer; H W Lin; F J Llanes-Estrada; H B Meyer; P Pakhlov; E Pallante; M I Polikarpov; H Sazdjian; A Schmitt; W M Snow; A Vairo; R Vogt; A Vuorinen; H Wittig; P Arnold; P Christakoglou; P Di Nezza; Z Fodor; X Garcia I Tormo; R Höllwieser; M A Janik; A Kalweit; D Keane; E Kiritsis; A Mischke; R Mizuk; G Odyniec; K Papadodimas; A Pich; R Pittau; J-W Qiu; G Ricciardi; C A Salgado; K Schwenzer; N G Stefanis; G M von Hippel; V I Zakharov
Journal:  Eur Phys J C Part Fields       Date:  2014-10-21       Impact factor: 4.590

4.  The influence of the enhanced vector meson sector on the properties of the matter of neutron stars.

Authors:  Ilona Bednarek; Ryszard Manka; Monika Pienkos
Journal:  PLoS One       Date:  2014-09-04       Impact factor: 3.240

  4 in total

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