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arXiv 2007.00874hep-phhep-ex
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The KSVZ Axion and Pseudo-Nambu-Goldstone Boson Models for the XENON1T Excess

Tianjun Li

英文摘要:

The XENON1T excess can be explained by the Axion Like Particle (ALP) dark matter with mass around 2.5 keV. However, there are three problems needed to be solved: suppressing the coupling $g_{aγ}$ between the ALP and photon, and generating the proper coupling $g_{ae}$ between the ALP and electron as well as the correct ALP mass. We propose three models to solve these problems. In our models, the $g_{ae}$ couplings are produced by integrating out the vector-like leptons, and the correct ALP masses arise from high-dimensional operators. In the KSVZ axion model, the coupling $g_{aγ}$ can be suppressed by choosing proper sets of vector-like fermions, but we need some fine-tunings to obtain the ALP mass. Similarly, one can study the DFSZ axion model. In the $Z_8$ and $ U(1)_X$ models with approximate Pseudo-Nambu-Goldstone Bosons (PNGBs), the coupling $g_{aγ}$ is suppressed due to $SU(3)_C \times U(1)_{\rm EM}$ anomaly free. In the $Z_8$ model, the PNGB mass can be generated naturally at the keV scale via the dimension-8 operator. To solve the PNGB quality problem in the $ Z_8$ model, we embed it into the model with $ U(1)_X$ gauge symmetry.

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