How viscous is a superfluid neutron star core? Nuclear Physics A, 763:212-229, December 2005.Andersson, N., Comer, G.L. and Glampedakis, K., How viscous is a superfluid neutron star core ?, preprint (2004)N. Anderson, G. L. Comer, K. Glampedakis, How viscous is a superfluid ...
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...
This kind of star fuses heavier and heavier elements in its core, eventually becoming so massive that it cannot hold itself up against gravity, Borowski said. The result is a huge explosion called a supernova. The star's core lives on as either a neutron star or a black hole, according ...
the star will consume those layers by fusing them into heavier and heavier elements. If the star doesn't have enough gravity to do that, it will release its cooling outer layers into space.) A white dwarf with enough mass will eventually gosupernova. Its core will collapse, resulting...
How strong gravity is when the neutrons are not together in the neutron star, and how gravity acts when they are separated?Neutron stars:The Neutrons stars have an intense field that can impact the orbits and other planets if they come close...
if a visible star or disk of gas has a "wobbling" 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...
supernovae, they blast their elements to space. The best example of a supernova is the Crab Nebula, in Taurus. The core of the original star is left behind as the rest of its material is blasted to space. Eventually, the core could compress to become a neutron star or a black hole....
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We consider a hot white dwarf, in which the main source of energy loss is plasmon decay. We also regard a U(1)Lµ−Lτ leptophilic dark photon that contributes to the plasmon decay. This novel vector mediator has different contributions for each flavour of neutrino-antineutrino pairs ...
Two protons combine to form a deuterium atom (hydrogen atom with one neutron and one proton), a positron (similar to an electron, but with a positive charge) and a neutrino. A proton and a deuterium atom combine to form a helium-3 atom (two protons with one neutron) and a gamma ray...