UMich: Researchers Look for Dark Matter Close to Home

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UMich: Researchers Look for Dark Matter Close to Home

Post by bystander » Fri Mar 27, 2020 3:31 pm

Researchers Look for Dark Matter Close to Home
University of Michigan, Ann Arbor | 2020 Mar 26
Eighty-five percent of (matter in) the universe is composed of dark matter, but we don’t know what, exactly, it is.

A new study from the University of Michigan, Lawrence Berkeley National Laboratory (Berkeley Lab) and University of California, Berkeley has ruled out dark matter being responsible for mysterious electromagnetic signals previously observed from nearby galaxies. Prior to this work there were high hopes that these signals would give physicists hard evidence to help identify dark matter.

Dark matter can’t be observed directly because it does not absorb, reflect or emit light, but researchers know it exists because of the effect it has on other matter. We need dark matter to explain gravitational forces that hold galaxies together, for example.

Physicists have suggested dark matter is a closely related cousin of the neutrino, called the sterile neutrino. Neutrinos—subatomic particles with no charge and which rarely interact with matter—are released during nuclear reactions taking place inside the sun. They have a tiny amount of mass, but this mass isn’t explained by the Standard Model of Particle Physics. Physicists suggest that the sterile neutrino, a hypothetical particle, could account for this mass and also be dark matter. ...

New Technique Looks for Dark Matter Traces in Dark Places
Lawrence Berkeley National Laboratory | 2020 Mar 26

The Dark Matter Interpretation of the 3.5-keV Line Is Inconsistent with
Blank-Sky Observations
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Re: UMich: Researchers Look for Dark Matter Close to Home

Post by neufer » Mon Oct 04, 2021 7:01 pm wrote:
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<<Sterile neutrinos (or inert neutrinos) are hypothetical particles (neutral leptons – neutrinos) that are believed to interact only via gravity and do not interact via any of the fundamental interactions of the Standard Model. The term sterile neutrino is used to distinguish them from the known active neutrinos in the Standard Model, which carry an isospin charge of ±1/2 under the weak interaction. It typically refers to neutrinos with right-handed chirality, which may be added to the Standard Model. Particles that possess the quantum numbers of sterile neutrinos and masses great enough such that they do not interfere with the current theory of Big Bang Nucleosynthesis are often called neutral heavy leptons (NHLs) or heavy neutral leptons (HNLs).

The existence of right-handed neutrinos is theoretically well-motivated because all other known fermions have been observed with both left and right chirality. They could also explain in a natural way the small active neutrino masses inferred from neutrino oscillation. The mass of the right-handed neutrinos themselves is unknown and could have any value between 1015 GeV and less than 1 eV. To comply with theories of leptogenesis and dark matter, there must be at least 3 types of sterile neutrinos (if they exist). This is in contrast to the number of active neutrino types required to ensure the electroweak interaction is free of anomalies, which must be exactly 3: The number of charged leptons and quark generations.

Due to the lack of electric charge, hypercharge, and color charge, sterile neutrinos would not interact electromagnetically, weakly, or strongly, making them extremely difficult to detect. They have Yukawa interactions with ordinary leptons and Higgs bosons, which via the Higgs mechanism leads to mixing with ordinary neutrinos. In experiments involving energies larger than their mass, sterile neutrinos would participate in all processes in which ordinary neutrinos take part, but with a quantum mechanical probability that is suppressed by a small mixing angle. That makes it possible to produce them in experiments, if they are light enough to be within the reach of current particle accelerators.

They would also interact gravitationally due to their mass, and if they are heavy enough, could explain cold dark matter or warm dark matter. In some grand unification theories they also interact via gauge interactions which are extremely suppressed at ordinary energies because their gauge boson is extremely massive. For a particle to be considered a dark matter candidate, it must have non-zero mass and no electromagnetic charge. Naturally, neutrinos and neutrino-like particles are a source of interest in the search for dark matter due to the possession of these two properties. It is more common today that theories rely on cold dark matter models (dark matter in the early universe is non-relativistic) as opposed to hot dark matter models (dark matter in the early universe is relativistic).

Since the mass of sterile neutrinos is not currently known, the possibility that it is dark matter has not been ruled out. If dark matter consists of sterile neutrinos then certain constraints can be applied to their properties. Firstly, the mass of the sterile neutrino would need to be on the keV scale to produce the structure of the universe observed today. Secondly, while its not required that the dark matter be stable, the lifetime of the particles must be longer than the current age of the universe. This places an upper bound on the strength of the mixing between sterile and active neutrinos. From what is known about the particle thus far, the sterile neutrino is a promising dark matter candidate, but, as with every other proposed dark matter particle, it has yet to be confirmed to exist.

The search for sterile neutrinos is an active area of particle physics. If they exist and their mass is smaller than the energies of particles in the experiment, they can be produced in the laboratory, either by mixing between active and sterile neutrinos or in high energy particle collisions. If they are heavier, the only directly observable consequence of their existence would be the observed active neutrino masses. They may, however, be responsible for a number of unexplained phenomena in physical cosmology and astrophysics, including dark matter, baryogenesis or hypothetical dark radiation.>>
Art Neuendorffer