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Title: Sterile neutrinos as dark matter

Technical Report ·
DOI:https://doi.org/10.2172/10146636· OSTI ID:10146636
 [1];  [2]
  1. Fermi National Accelerator Lab., Batavia, IL (United States)
  2. Queen`s Univ., Kingston, ON (Canada). Dept. of Physics

The simplest model that can accommodate a viable nonbaryonic dark matter candidate is the standard electroweak theory with the addition of right-handed or sterile neutrinos. This model has been studied extensively in the context of the hot dark matter scenario. We reexamine this model and find that hot, warm, and cold dark matter are all possibilities. We focus on the case where sterile neutrinos are the dark matter. Since their only direct coupling is to left-handed or active neutrinos, the most efficient production mechanism is via neutrino oscillations. If the production rate is always less than the expansion rate, then these neutrinos will never be in thermal equilibrium. However, they may still play a significant role in the dynamics of the Universe and possibly provide the missing mass necessary for closure. We consider a single generation of neutrino fields ({nu}{sub L}, {nu}{sub R}) with a Dirac mass, {mu}, and a Majorana mass for the right-handed components only, M. For M {much_gt} {mu} we show that the number density of sterile neutrinos is proportional to {mu}{sup 2}/M so that the energy density today is independent of M. However M is crucial in determining the large scale structure of the Universe. In particular, M {approx_equal} 0.1--1.0 key leads to warm dark matter and a structure formation scenario that may have some advantages over both the standard hot and cold dark matter scenarios.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Toronto Univ., ON (Canada). Canadian Inst. for Theoretical Astrophysics
Sponsoring Organization:
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
DOE Contract Number:
AC02-76CH03000
OSTI ID:
10146636
Report Number(s):
FNAL/Pub-93/057-A; ON: DE93012533; IN: HEP-PH-9303287; CNN: Grant NAGW-2381
Resource Relation:
Other Information: PBD: Mar 1993
Country of Publication:
United States
Language:
English

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