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. [29] 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. [28] In nature, the nuclear reactions that form stars are often accompanied by astronomically high amounts of energy, sometimes over billions of years. [27] Dark matter halos are theoretical bodies inside which galaxies are suspended; the halo's mass dominates the total mass. [26] 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). [25] 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. [24] 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. [23] Quark matter – an extremely dense phase of matter made up of subatomic particles called quarks – may exist at the heart of neutron stars. [22] 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. [21] 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. [20]
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