Neutrinophilic axion-like dark matter

被引：42

作者：

Huang, Guo-yuan ^{[1
,2
]}

Nath, Newton ^{[1
,2
]}

机构：

[1] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China

[2] Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China

来源：

EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 11期

基金：

中国国家自然科学基金;

关键词：

OSCILLATION EXPERIMENTS; FAMILY SYMMETRY; CP CONSERVATION; CONSTRAINTS; SIMULATION; COSMOLOGY; SEARCHES; MODEL; DECAY; BURST;

D O I：

10.1140/epjc/s10052-018-6391-y

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The axion-like particles (ALPs) are very good candidates of the cosmological dark matter, which can exist in many extensions of the standard model (SM). The mass of the ALPs can be as small as . On the other hand, the neutrinos are found to be massive and the SM must be extended to explain the sub-eV neutrino masses. It becomes very interesting to consider an exclusive coupling between these two low scale frontiers that are both beyond the SM. The propagation of neutrinos inside the Milky Way would undergo the coherent forward scattering effect with the ALP background, and the neutrino oscillation behavior can be modified by the ALP-induced potential. Assuming a derivative coupling between the ALP and the three generations of active neutrinos, possible impacts on the neutrino oscillation experiments have been explored in this paper. In particular, we have numerically studied the sensitivity of the deep underground neutrino experiment (DUNE). The astrophysical consequences of such coupling have also been investigated systematically.

引用

页数：13

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