scholarly journals Simple theory of chiral fermion dark matter

2021 ◽  
Vol 103 (1) ◽  
Author(s):  
Tomohiro Abe ◽  
K. S. Babu

I review the observational situation concerning the existence of dark matter in the outer parts of galaxies. Observation now leaves little doubt of its presence, and both observation and simple theory suggest that the dark matter is probably bound to galaxies, and furthermore is present around both spirals and ellipticals. New evidence concerning the rotation curve of the Galaxy shows that the distribution of the halo stuff in our own system is roughly spherical, as seems natural from existing dynamical data on the nature of the halo material.


2020 ◽  
Vol 809 ◽  
pp. 135757
Author(s):  
A.E. Cárcamo Hernández ◽  
José W.F. Valle ◽  
Carlos A. Vaquera-Araujo
Keyword(s):  

2021 ◽  
Vol 2021 (12) ◽  
Author(s):  
B. Fu ◽  
S.F. King

Abstract We consider the possibility that dark matter is stabilised by a discrete Z2 symmetry which arises from a subgroup of a U(1)′ gauge symmetry, spontaneously broken by integer charged scalars, and under which the chiral quarks and leptons do not carry any charges. A chiral fermion χ with half-integer charge is odd under the preserved Z2, and hence becomes a stable dark matter candidate, being produced through couplings to right-handed neutrinos with vector-like U(1)′ charges, as in the type Ib seesaw mechanism. We calculate the relic abundance in such a low energy effective seesaw model containing few parameters, then consider a high energy renormalisable model with a complete fourth family of vector-like fermions, where the chiral quark and lepton masses arise from a seesaw-like mechanism. With the inclusion of the fourth family, the lightest vector-like quark can contribute to the dark matter production, enlarging the allowed parameter space that we explore.


Nature ◽  
2010 ◽  
Author(s):  
Melissa Lee Phillips
Keyword(s):  

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