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,...
al. Structure of neutron, quark and exotic stars in Eddington-inspired Born-Infeld gravity, Phys. Rev. D 88 (2013) 044032.T. Harko, F. S. N. Lobo, M. K. Mak and S. V. Sushkov, "Structure of neutron, quark and exotic stars in Eddington-inspired Born-Infeld gravity," Phys. Rev....
Through extensive model calculations, physicists at Goethe University Frankfurt have reached general conclusions about the internal structure of neutron stars, where matter reaches enormous densities: depending on their mass, the stars can have a core that is either very stiff or very soft. The findin...
One of the most intriguing consequence of the extreme conditions inside neutron stars is the possibility of the natural existence of a deconfined strange quark matter phase in the high density interior of the star. The equation of state (EOS) of strange quark matter (SQM) was recently improved...
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: 320 ...
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 ...
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
Electric and magnetic properties of a semiconductor in the field of a strong electromagnetic wave 热度: Analysis of rotary electrical discharge machining characteristics in reversal magnetic field for copper-en8 steel system 热度: Structure of Rotating Neutron Stars in Uniform Strong Magnetic Field,Struct...
We will discuss the properties of equilibrium models of magnetized neutron stars, and we will show how internal and external currents can be related. These magnetic field configurations will be discussed considering also their stability, relevant for their origin and possibly connected to events like ...