Tests of Fundamental Discrete Symmetries at the NICA Facility: Addendum to the Spin Physics Programme

2021 ◽  
Vol 52 (4) ◽  
pp. 549-554
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I. A. Koop ◽  
A. I. Milstein ◽  
N. N. Nikolaev ◽  
A. S. Popov ◽  
S. G. Salnikov ◽  
...  
1985 ◽  
Vol 46 (C2) ◽  
pp. C2-421-C2-425
Author(s):  
F . Bradamante
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2012 ◽  
Vol 182 (8) ◽  
pp. 869 ◽  
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Eugeniyus L. Ivchenko
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2016 ◽  
Vol 902 ◽  
pp. 1-57 ◽  
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I. Girardi ◽  
S.T. Petcov ◽  
Alexander J. Stuart ◽  
A.V. Titov

2021 ◽  
Vol 103 (10) ◽  
Author(s):  
Michele Arzano ◽  
Andrea Bevilacqua ◽  
Jerzy Kowalski-Glikman ◽  
Giacomo Rosati ◽  
Josua Unger
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1989 ◽  
Vol 232 (1) ◽  
pp. 104-112 ◽  
Author(s):  
D. Kapetanakis ◽  
G. Zoupanos

1999 ◽  
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Author(s):  
Walter Bonivento
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2014 ◽  
Vol 45 (1) ◽  
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A. Rakotozafindrabe ◽  
M. Anselmino ◽  
R. Arnaldi ◽  
S. J. Brodsky ◽  
V. Chambert ◽  
...  

2008 ◽  
Vol 23 (39) ◽  
pp. 3271-3283 ◽  
Author(s):  
HYE-SUNG LEE

Supersymmetry is one of the best motivated new physics scenarios. To build a realistic supersymmetric standard model, however, a companion symmetry is necessary to address various issues. While R-parity is a popular candidate that can address the proton and dark matter issues simultaneously, it is not the only option for such a property. We review how a TeV scale U(1)′ gauge symmetry can replace the R-parity. Discrete symmetries of the U(1)′ can make the model still viable and attractive with distinguishable phenomenology. For instance, with a residual discrete symmetry of the U(1)′, Z6 = B3 × U2, the proton can be protected by the baryon triality (B3) and a hidden sector dark matter candidate can be protected by the U-parity (U2).


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