Matter (PhysicsExtraterrestrial MatterEquations Of StateDegrees Of FreedomQuantum ChromodynamicsThe equation of state of hadronic matter in neutron stars is briefly reviewed. Uncertainties regarding the stiffness and composition of hadronic matter are discussed. Importance of poorly known short range ...
The physics of neutron stars is a remarkable combination of Einstein’s theory of general relativity and nuclear physics. Their interiors harbour extreme matter that cannot be probed in the laboratory. At such high densities and pressures, their cores ma
《海外直订The Physics and Astrophysics of Neutron Stars 中子星的物理学和天体物理学》,作者:海外直订The Physics and Astrophysics of Neutron Stars 中子星的物理学和天体物理学Rezzolla 著,出版社:Springer,ISBN:9783319976150。
An All-Union Seminar on the Physics of Neutron Stars was held at the Ioffe Physial-Technical Institute from March 15 to 18, 1988. Papers presented at this seminar are briefly reviewed, with attention given to the following topics: neutron-star (NS) formation and structure; NS evolution in ...
If it can be interpreted aas neutron star rotation, then thoery seems to indicate that it provides very stringent conditions on the equation of state when combines with the mass constraint. The physics of supernova invloves so many factors of comparable importance but high uncertainty, that they...
neutron in Physics topic From Longman Dictionary of Contemporary Englishneu‧tron /ˈnjuːtrɒn $ ˈnuːtrɑːn/ noun [countable] technical a part of an atom that has no electrical chargeExamples from the Corpusneutron• First, then, what about neutron decay?• These stars ...
Nuclear Physics of the Outer Crust of Accreting Neutron Stars*This project is funded by the NSF through Grants No. PHY-0822648, PHY-1102511, PHY-1404442, and No. PHY-1430152.Meisel, Zach... Z Meisel - American Physical Society 被引量: 0发表: 2015年 Neutron physics of the Re/Os clock...
The death of that star is the birth of a neutron star: 那个星体的死亡,成了一个中子星的诞生: one of the densest known objects in the universe, 中子星是全宇宙最高密度的已知物体之一, and a laboratory for the strange physics of supercondensed matter. ...
Proto-neutron stars (PNSs) are basic labs for the physics of hot dense matter. These compact objects can be formed at the last stage of a type-II supernova collapse [1], [2], [3], [4], [5]. Some minutes after the core bounce, a hot and lepton-rich baryonic structure is consti...
The purpose of this letter is to add a new aspect to this discussion, which focuses on the connection between proton superconductivity and the masses of neutron stars. Assuming (as is currently the case) that the temperature evolution of Cas A is largely controlled by superconducting protons, ...