Authors: George Rajna
The rareness of this decay is due to the coincidence of two factors: First, the decay requires quantum loops with several weak interaction vertices, some of which have a low probability to occur; second, angular momentum conservation constrains the decay products of the scalar B 0 or Bs meson into a highly unlikely configuration.  A team of Ohio University nuclear physicists has proposed a new theoretical model for calculating pairing properties of atomic nuclei including those found in extreme astrophysical environments.  In nature, the nuclear reactions that form stars are often accompanied by astronomically high amounts of energy, sometimes over billions of years.  Dark matter halos are theoretical bodies inside which galaxies are suspended; the halo's mass dominates the total mass.  An international team of researchers extended their results from a previous study to directly measure the cosmic-ray all-electron (electron + positron) spectrum in an energy range from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope (CALET).  Mysterious radiation emitted from distant corners of the galaxy could finally be explained with efforts to recreate a unique state of matter that blinked into existence in the first moments after the Big Bang.  Researchers at Oregon State University have confirmed that last fall's union of two neutron stars did in fact cause a short gamma-ray burst.  Quark matter – an extremely dense phase of matter made up of subatomic particles called quarks – may exist at the heart of neutron stars.  When a massive astrophysical object, such as a boson star or black hole, rotates, it can cause the surrounding spacetime to rotate along with it due to the effect of frame dragging.  Rotating black holes and computers that use quantum-mechanical phenomena to process information are topics that have fascinated science lovers for decades, but even the most innovative thinkers rarely put them together. 
Comments: 29 Pages.
[v1] 2018-09-26 10:57:42
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