发表机构
Nanjing Normal University; Nanjing Key Laboratory of Particle Physics and Astrophysics（南京师范大学; 南京粒子物理与天体物理重点实验室）
机构由 AI 辅助整理，请以论文原文为准。AI 中文总结
本文提出利用月球表面将暗光子暗物质转化为射电波，并通过现有及未来射电望远镜探测，以覆盖此前不可及的参数空间。
AI 中文摘要
月球介电表面为暗物质暗光子转换为射电波提供了高效界面。这项工作探索了一种新颖的探测策略，旨在利用标准射电望远镜天线捕获这种射电辐射。文中给出了详细的灵敏度预测，展示了该技术的潜力。研究发现，当前和未来的射电天文台，包括阿塔卡马大型毫米/亚毫米波阵列（ALMA）和平方千米阵列（SKA）等大型阵列，以及五百米口径球面射电望远镜（FAST）和绿岸望远镜（GBT）等大型单碟望远镜，都可以探索这些暗物质候选粒子的大量且此前无法触及的参数空间。
英文摘要
The dielectric surface of the Moon provides an efficient interface for the conversion of dark matter dark photons into radio waves. This work explores a novel detection strategy that aims to capture this radio emission using standard radio telescope antennas. Detailed sensitivity projections are presented that demonstrate the power of this technique. It is found that both current and future radio observatories, including large arrays such as the Atacama Large Millimeter/submillimeter Array (ALMA) and the Square Kilometer Array (SKA), as well as large single dishes like the Five-hundred-meter Aperture Spherical Telescope (FAST) and the Green Bank Telescope (GBT), can explore a substantial and previously inaccessible parameter space for these dark matter candidates.
Comments8 pages, 5 figures
