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轴子诱导冷却导致 21cm 吸收信号的自然解释。

Natural Explanation for 21 cm Absorption Signals via Axion-Induced Cooling.

机构信息

CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China.

School of Physical Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, China.

出版信息

Phys Rev Lett. 2018 Sep 14;121(11):111301. doi: 10.1103/PhysRevLett.121.111301.

Abstract

The EDGES Collaboration has reported an anomalously strong 21 cm absorption feature corresponding to the era of first star formation, which may indirectly betray the influence of dark matter during this epoch. We demonstrate that, by virtue of the ability to mediate cooling processes while in the condensed phase, a small amount of axion dark matter can explain these observations within the context of standard models of axions and axionlike particles. The EDGES best-fit result favors an axionlike particle mass in the (10, 450) meV range, which can be compressed for the QCD axion to (100, 450) meV in the absence of fine tuning. Future experiments and large scale surveys, particularly the International Axion Observatory (IAXO) and EUCLID, should have the capability to directly test this scenario.

摘要

EDGES 合作组织报告了一个异常强烈的 21 厘米吸收特征,对应于第一代恒星形成的时代,这可能间接地揭示了暗物质在这个时代的影响。我们证明,在凝聚相下,通过介导冷却过程的能力,少量轴子暗物质可以在轴子和轴子样粒子的标准模型框架内解释这些观测结果。EDGES 的最佳拟合结果有利于在(10,450)meV 范围内的轴子样粒子质量,在没有微调的情况下,QCD 轴子可以被压缩到(100,450)meV。未来的实验和大规模调查,特别是国际轴子观测站(IAXO)和 EUCLID,应该有能力直接检验这种情况。

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