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Can the QCD Axion Feed a Dark Energy Component?

Kristjan Müürsepp,Enrico Nardi,Clemente Smarra

arXiv · Phenomenology(2024)

HEPC-NICPB Laboratory of High Energy and Computational Physics | INFN Laboratory of High Energy and Computational Physics | INFN SISSA International School for Advanced Studies

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Abstract
A pseudo Nambu-Goldstone boson (PNGB) coupled to a confining gauge group viaan anomalous term is characterised, during the confining phase transition, by atemperature dependent mass m^2(T) ∝ T^-n. For n>2, anon-relativistic population of such particles dominating the cosmologicalenergy density would act as dark energy (DE), accelerating the expansion. Westudy the possibility that a PNGB φ_b coupled to a hidden gauge groupthat is presently undergoing confinement could realise this scenario. To obtainthe observed amount of DE, the number density of φ_b must be boosted bysome mechanism. Assuming that the QCD axion φ_a constitutes the darkmatter (DM), a non-adiabatic level crossing between φ_a and φ_bshortly before matter-DE equality can convert a small fraction of DM into DE,providing such mechanism and explaining the coincidence puzzle.
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要点】:论文探讨了QCD轴子通过非绝热水平交叉转化为暗能量(DE)的可能性,从而解决宇宙加速膨胀和暗能量与暗物质巧合问题。

方法】:通过分析伪Nambu-Goldstone玻色子(PNGB)与隐 gauge 群通过异常项耦合,在相变过程中质量随温度变化的行为,以及QCD轴子与PNGB之间的相互作用。

实验】:论文主要基于理论模型和计算,未提及具体实验。使用的数据集为宇宙学参数,如暗能量和暗物质的观测值,得到的结果表明该机制能够解释暗能量与暗物质的比例巧合问题。