stars: neutronWe have tested the appropriateness of two-soliton analytic metric to describe the exterior of all types of neutron stars, no matter what their equation of state or rotation rate is. The particular analytic solution of the vacuum Einstein equations proved quite adjustable to mimic the...
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 ...
We calculate static and spherically symmetric solutions for the Rastallmodification of gravity to describe Neutron Stars (NS). The key feature of theRastall gravity is the non-conservation of the energy-momentum tensorproportionally to the space-time curvature. Using realistic equations of statefor ...
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Gravitational-wave measurements of the tidal deformability of neutron stars could reveal important information regarding their internal structure, the equation of state of high-dense nuclear matter and gravity in strong field regime. In this work, we extend the relativistic theory of the tidal deformabi...
Neutron starsRotating starsPulsarsWe summarize the key ingredients of a new neutron star model fulfilling global, but not local, charge neutrality. The model is described by what we have called the Einstein-Maxwell-Thomas-Fermi equations, which account for the strong, weak, electromagnetic, and ...
A normal Neutron star has around the same mass as well. I admit it should be changed to say weight on Earth. Because every source I've ever read in my life on Neutron stars states that they would have a weight of 100 million tons per thimblefull on the earth. To be fair, the ...
Candidate isolated neutron stars and other stellar X -ray sources from the ROSAT All-Sky and Sloan Digital Sky Surveys.作者为Agueros, Marcel A.,于2006发表的Astronomy.类Ph.D.论文。
As stars contracted, it was thought, they would get hotter and hotter, giving off light in the process. This could not be the primary way that stars shine, however. If it were, they would scarcely last a million years, rather than the billions of years in age that we know they are....
New DLC characters are coming to Nickelodeon All-Stars Brawl and they include Jenny the robot, Hugh Neutron, and Rocko.