Glampedakis: How viscous is a su- perfluid neutron star core? Nuclear Physics A, 763:212 - 229, 2005, ISSN 0375-9474. http://www.sciencedirect.com/science/article/pii/ S0375947405010572. vN. Anderson, G. L. Comer, K. Glampedakis. How viscous is a superfluid neutron star core?
A neutron star's almost incomprehensible density causes protons and electrons to combine into neutrons—the process that gives such stars their name. The composition of their cores is unknown, but they may consist of a neutron superfluid or some unknown state of matter. ...
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Our results raise the possibility that (some) pulsar glitches could originate within a quark matter core deep within a neutron star... M Mannarelli,K Rajagopal,R Sharma - 《High Energy Physics Phenomenology》 被引量: 111发表: 2007年 Earthquake-like behaviour of soft |[gamma]|-ray repeaters...
How Hot is That Star This resource is part of the Science Education Gateway (SEGway) project, funded by NASA, which is a national consortium of scientists, museums, and educato... J Meunier,J Lehman 被引量: 0发表: 0年 Observational evidence for supernova-induced star formation - Canis Ma...
Edward Farhi, an MIT physicist who researched strangelets, thinks the most likely place to find strange matter is in neutron stars. These collapsing stars compress their interiors forcefully. "At the core, you have densities and pressures large enough to form strange matter. If strange matter for...
motion or spinning and there is not a visible reason for this motion and the invisible reason has an effect that appears to be caused by an object with a mass greater than three solar masses (too big to be a neutron star), then it is possible that a black hole is causing the motion...
That is huge because it points to FRBs as not a one-off event but something continuous, a reoccurring event. Suddenly, options such as active neutron stars are back in play while neutron star collisions and black holes are out, at least forthisFRB. Averaging 11 bursts measured and using ...
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star collapses by its own gravity and the iron core heats up. The core becomes so tightly packed that protons and electrons merge to form neutrons. In less than a second, the iron core, which is about the size ofEarth, shrinks to a neutron core with a radius of about 6 miles (10 ...