Restudy on Dark Matter Time-Evolution in the Littlest Higgs model with T-parity
arXiv:0711.3254 · doi:10.1088/0253-6102/50/5/40
Abstract
Following previous study, in the Littlest Higgs model (LHM), the heavy photon is supposed to be a possible dark matter candidate and its relic abundance of the heavy photon is estimated in terms of the Boltzman-Lee-Weinberg time-evolution equation. The effects of the T-parity violation is also considered. Our calculations show that when Higgs mass taken to be 300 GeV and don't consider T-parity violation, only two narrow ranges GeV and GeV are tolerable with the current astrophysical observation and if GeV, there must at least exist another species of heavy particle contributing to the cold dark matter. As long as the T-parity can be violated, the heavy photon can decay into regular standard model particles and would affect the dark matter abundance in the universe, we discuss the constraint on the T-parity violation parameter based on the present data. Direct detection prospects are also discussed in some detail.
13 pages, 11 figures included
References in corpus (10)
- Dark Matter from new Technicolor Theories
- Towards Working Technicolor: Effective Theories and Dark Matter
- Sneutrino cold dark matter, a new analysis: relic abundance and detection rates
- Right-Handed Sneutrino as Cold Dark Matter of the Universe
- Novel Collider Signatures for Little Higgs Dark Matter Models
- Unparticle Dark Matter
- Cosmological constraints on neutrino plus axion hot dark matter
- Supersymmetric Unparticle Effects on Higgs Boson Mass and Dark Matter
- Indirect Detection of Little Higgs Dark Matter
- Dark Matter in the Simplest Little Higgs Model