Neutron stars are studied in the framework of relativistic interacting field theory of nucleons, hyperons, and mesons. A large component of strange baryons is found, and in the interior the neutron population is minor.doi:10.1016/0370-2693(82)90078-8Norman K. Glendenning...
Besides their intrinsic nuclear-structure value, nuclear mass models areessential for astrophysical applications, such as r-process nucleosynthesis andneutron-star structure. To overcome the intrinsic limitations of existing"state-of-the-art" mass models, we propose a refinement based on a Bayesian...
equation of statestars: individual: EXO 0748−676stars: neutronX-rays: binariesRecently, the neutron star X-ray binary EXO 0748676 underwent a transition to quiescence. We analysed an XMMNewton observation of this source in quiescence, where we fitted the spectrum with two different neutron star...
Its prime scientific focus is an in-depth investigation of neutron stars—objects that compress up to two Solar masses into a volume the size of a city—accomplished through observations in 0.2-12 keV X-rays, the electromagnetic band into which the stars radiate significant fractions of their ...
The extreme kinetic energy required for exothermic nuclear fusion and the complex interplay of neutron capture and radioactive decay, the principal nucleosynthesis processes, translate into an abundance profile (see Fig. 1.1) that embodies the relative stability of each nuclide. Show moreView chapter...
Neutron Stars as a Source of the Short-Lived Nuclides in Ap-star Atmospheres. We propose a new explanation of some magnetic chemically peculiar (MCP) star anomalies, which is based on an assumption that such stars be the close binary... Gopka,F Vera,Ulyanov,... - 《Aip Conference Proceed...
GCs are dense, gravitationally bound collections of thousands to millions of ancient stars that orbit in the fringes of large galaxies; many GCs formed early in the history of the Universe. Because they contain some of the oldest stars in a galaxy, GCs provide astronomers wit...
Upper limits on the observational effects of nuclear pasta in neutron stars The effects of the existence of exotic nuclear shapes at the bottom of the neutron star inner crust - nuclear `pasta' - on observational phenomena are esti... M Gearheart,WG Newton,J Hooker,... - 《Monthly Notices...
Like a dried-up lemon from the back of the fridge, neutron stars are less squeezable than expected. E Conover - 《Science News》 被引量: 0发表: 2021年 Squeezable, Cross-Linked, Grease-Like Electromagnetic Wave Absorber The present invention provides a squeezable, cross-linked, grease-like ...
Detailed elaboration and general model of the electron treatment of surfaces of charged plasmoids (from atomic nuclei to white dwarves, neutron stars, and ... because of forcing the electrons out of the structures leads to sputtering (bouncing) of neutral structures that were gravitating before. ...