density region 3.1x10 11 to 2x10 15 g/cm 3/ A2165 Nuclear matter A9760J Neutron starsThe equation of state and the structure and composition of neutron star matter are investigated in the density region 3.1 × 10 112 × 10 15g/cm 3. Below the density 3.1 × 10 11 g/cm 3 the ...
arXiv:1301.5189v1 [astro-ph.CO] 22 Jan 2013General Relativity and Gravitation manuscript No.(will be inserted by the editor)Structure of neutron stars in R-squared gravityMariana Orellana1,2,∗· Federico Garc´ıa1,2,∗∗· Florencia A. TeppaPannia2,∗∗· Gustavo E. Romero1,...
a matter of fact, neutron star crusts seem to be just about the only other places in the entire Universe, apart fromplanets, where one can find condensed matter, in particular a solid phase [2]. Moving from the neutron star surface inward, one finds at first a ...
Electromagnetic field analysis of an YBCO coated conductor exposed to the non-uniform magnetic field in superconducting cables 热度: Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field,Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field,of,in,In,Stars,Field,stars,field...
We study relationships between the neutron-rich skin of a heavy nucleus and the properties of neutron-star crusts. Relativistic effective field theories with a thicker neutron skin in $^{208}$Pb have a larger electron fraction and a lower liquid-to-solid
Neutron starsWe study the internal structure of a static and spherically symmetric neutron star in the framework of an in-medium modified chiral soliton model. The Equations of State describing an infinite and asymmetric nuclear matter are obtained introducing the density dependent functions into the ...
equations of stategravitational collapseneutron starsstellar evolutionstellar modelsstellar structure/ relativistic structuregravitational collapsecharged neutron starsCharged stars have the potential of becoming charged black holes or even naked singularities. It is presented a set of numerical solutions of the...
We compare their respective predictions regarding the structure of neutron stars, in particular the mass-radius relation.关键词: Nuclear matter Nuclear matter aspects of neutron stars Many-body theory Neutron stars DOI: 10.1103/PhysRevC.69.018801 被引量: 321 ...
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Generally speaking, conventional neutron stars and non-mainstream quark stars are two types of models to describe the inner structure of pulsars, with the former composed mainly of hadrons and the latter of a peculiar kind of matter whose state equation should be understood in the level of ...