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Darkon (unparticle)

In this article we are going to analyze Darkon (unparticle) in detail, a topic that has gained great relevance in recent years. Darkon (unparticle) is a concept widely studied in various areas, from psychology to economics, including sociology and politics. Throughout history, Darkon (unparticle) has been the subject of debate and reflection by experts and academics, as well as public opinion in general. In this sense, it is of utmost importance to deepen the knowledge and understanding of Darkon (unparticle), in order to achieve a broader and clearer vision of its impact on society and daily life. Through this article, we propose to explore the multiple dimensions and facets of Darkon (unparticle), with the aim of enriching the debate and promoting critical reflection on this topic.

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For other uses, see Darkon.

Darkon is a hypothetical scalar unparticle to introduce to the Minimal Supersymmetric Standard Model, a dark matter candidate.[1][2][3][4]

History

A. Zee and V. Silveira were the first to consider the darkon field as dark matter in 1985. This approach was then used by several others groups of physicists.[2][5][6]

Concept

In addition to the Standard Model particles, It contains the darkon, a real singlet field. To play the role of dark matter, the darkon field must interact weakly with the standard matter field sector and should not rapidly decay into particles. The simplest way of introducing the darkon is to demand that they can only be annihilated or created in pairs and to make it stable against decay.[2]

See also

References

  1. ^ Jia, Lian-Bao; Li, Xue-Qian (13 February 2014). "Study of a WIMP dark matter model with the updated results of CDMS II". Physical Review D. 89 (3) 035006. arXiv:1309.6029. Bibcode:2014PhRvD..89c5006J. doi:10.1103/PhysRevD.89.035006. ISSN 1550-7998. S2CID 118570160.
  2. ^ a b c Xiao-Gang, He (June 2009). "Darkon dark matter, unparticle effects and collider physics". Chinese Physics C. 33 (6): 451–455. doi:10.1088/1674-1137/33/6/010. ISSN 1674-1137. S2CID 250794700. Retrieved 7 January 2023.
  3. ^ Cai, Yi; He, Xiao-Gang; Ren, Bo (28 April 2011). "Low Mass Dark Matter and Invisible Higgs Width In Darkon Models". Physical Review D. 83 (8) 083524. arXiv:1102.1522. Bibcode:2011PhRvD..83h3524C. doi:10.1103/PhysRevD.83.083524. S2CID 119204162.
  4. ^ Stichel, P. C.; Zakrzewski, Wojtek J. (1 September 2012). "Darkon fluid — a model for the dark sector of the universe?". International Journal of Geometric Methods in Modern Physics. 09 (6): 1261014. arXiv:1202.4895. doi:10.1142/S0219887812610142. ISSN 0219-8878. S2CID 119210010. Retrieved 7 January 2023.
  5. ^ He, Xiao-Gang; Li, Tong; Li, Xue-Qian; Tandean, Jusak; Tsai, Ho-Chin (January 2011). "Constraints on Scalar Dark Matter from Direct Experimental Searches". International Journal of Modern Physics: Conference Series. 01: 257–265. arXiv:0811.0658. Bibcode:2011IJMPS...1..257H. doi:10.1142/S2010194511000377. Retrieved 7 January 2023.
  6. ^ Cheung, Kingman; Tsai, Yue-Lin S.; Tseng, Po-Yan; Yuan, Tzu-Chiang; Zee, A. (1 January 2014). "Global Constraints of the Simplest Darkon Model". Nuclear Physics B - Proceedings Supplements. 246–247: 116–126. Bibcode:2014NuPhS.246..116C. doi:10.1016/j.nuclphysbps.2013.10.074. ISSN 0920-5632. Retrieved 7 January 2023.

Further reading


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