Upper Limits on the Peccei-Quinn Scale and on the Reheating Temperature in Axino Dark Matter Scenarios
arXiv:0904.3218 · doi:10.1016/j.physletb.2009.07.047
Abstract
Considering axino cold dark matter scenarios with a long-lived charged slepton, we study constraints on the Peccei-Quinn scale f_a and on the reheating temperature T_R imposed by the dark matter density and by big bang nucleosynthesis (BBN). For an axino mass compatible with large-scale structure, m_axino \gtrsim 100 keV, temperatures above 10^9 GeV become viable for f_a > 3x10^12 GeV. We calculate the slepton lifetime in hadronic axion models. With the dominant decay mode being two-loop suppressed, this lifetime can be sufficiently large to allow for primordial bound states leading to catalyzed BBN of Lithium-6 and Beryllium-9. This implies new upper limits on f_a and on T_R that depend on quantities which will be probed at the Large Hadron Collider.
10 pages, 5 figures; small additions and minor changes, matches published version
References in corpus (8)
- Dark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos
- Big-Bang Nucleosynthesis with Long-Lived Charged Slepton
- Cosmological implications of supersymmetric axion models
- The running fine structure constant alpha(E) via the Adler function
- Determining Reheating Temperature at Colliders with Axino or Gravitino Dark Matter
- Probing the Reheating Temperature at Colliders and with Primordial Nucleosynthesis
- Quintessential Kination and Thermal Production of Gravitinos and Axinos
- CBBN in the CMSSM