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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Axion dark matter and cosmological parameters.
1Department of Physics, University of Florida, Gainesville, Florida 32611, USA.
Physical Review Letters
|March 10, 2012
Summary
Photon cooling after the Big Bang can resolve the lithium abundance problem. Colder axions in a Bose-Einstein condensate may enable this cooling, predicting a high effective number of neutrinos.
Area of Science:
- Cosmology
- Particle Physics
Background:
- The primordial abundance of Lithium-7 (⁷Li) shows a significant discrepancy between observational data and theoretical predictions from Big Bang nucleosynthesis.
- Achieving the necessary photon cooling before cosmic recombination is challenging under standard cosmological models.
Purpose of the Study:
- To propose a mechanism for photon cooling that resolves the cosmological lithium abundance problem.
- To investigate the role of dark matter axions in facilitating this cooling process.
Main Methods:
- Investigating the thermal contact between Bose-Einstein condensed axions and photons.
- Analyzing the impact of axion-photon thermalization on early universe thermodynamics.
Main Results:
- Photon cooling after Big Bang nucleosynthesis and before recombination can reconcile the observed and predicted ⁷Li abundances.
- Bose-Einstein condensed axions provide a viable mechanism for achieving this photon cooling through thermal contact.
- The proposed mechanism predicts a higher effective number of neutrinos (N_eff) than currently inferred from cosmic microwave background anisotropy data.
Conclusions:
- The axion Bose-Einstein condensate model offers a potential solution to the cosmic lithium problem.
- This model has testable implications for cosmological parameters, specifically N_eff, which can be constrained by future cosmic microwave background observations.
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