Aksino (born axino ) is a hypothetical neutral elementary particle with spin 1/2 predicted by some theories of particle physics. The Peccei theory - Quinn is trying to explain the observed phenomenon, known as the strong CP problem , by introducing hypothetical real pseudoscalar particles, the so-called axions . Adding supersymmetry to this model makes it necessary to have a fermion superpartner for the axion β axino (with R parity β1), as well as a bosonic superpartner β saxion (with R parity +1). All of them form one chiral superfield. [one]
| Axino | |
|---|---|
| Structure | Elementary particle |
| A family | Fermion |
| Group | Neutral particle , super partner |
| Involved in interactions | Gravity |
| Status | Hypothetical |
| Quantum numbers | |
| Spin | 1/2 Δ§ |
| R parity | -one |
In some models, axino may be the lightest supersymmetric particle [2] , which is supposed to be stable. In particular, in connection with this property, axino is considered as one of the candidates for the role of particles that make up dark matter . [3] [4] [5] [6]
Notes
- β David H. Lyth (1993) " Dilution of Cosmological Densities by Saxino Decay ."
- β Abe, Nobutaka, Takeo Moroi and Masahiro Yamaguchi. Anomaly-Mediated Supersymmetry Breaking with Axion // Russian Journal of High Energy Physics : journal. - 2002 .-- January ( vol. 1 ). - P. 10 . - DOI : 10.1088 / 1126-6708 / 2002/01/010 .
- β Hooper, Dan and Lian-Tao Wang. Possible evidence for axino dark matter in the galactic bulge ( Physical ) // Physical Review D : journal. - 2004 .-- 3 September ( vol. 70 ). - P. 063506 . - DOI : 10.1103 / PhysRevD.70.063506 .
- β Arnd Brandenberg and Frank D. Steffen (2004) β Axinos As Dark Matter In The Universe (link not available) β
- β Arnd Brandenberg and Frank D. Steffen (2004) β Axino Dark Matter From Thermal Production β
- β Laura Covi, Leszek Roszkowski, Roberto Ruiz de Austri and Michael Small (2004) β Axino Dark Matter and the CMSSM β