论文标题
UHE宇宙颗粒检测的无线电实验概述
Overview of radio experiments for UHE cosmic particles detection
论文作者
论文摘要
无线电检测是一种成熟的技术，在过去的几十年中，它已经获得了巨大的动力。它的物理检测原理主要由淋浴的电磁部分驱动，因此不太敏感，而不是在Hadronic相互作用上进行不确定性。此外，由于天线的低成本，其技术检测原理允许100％的占空比和较大的表面覆盖率。现在，UHE颗粒的各种检测方法依赖于无线电信号作为主要可观察的。例如，基于地面的实验，例如Pierre螺旋钻天文台上的AERA或LOFAR，检测到大气中高能量颗粒引起的空调的无线电发射；诸如ARA，ICECUBE或ARIANNA之类的In In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-In-Icecube或Arianna受益于降低相互作用长度的较密集的检测。最后，诸如ANITA之类的气球实验只能使用几个天线进行非常敏感的UHE中微子检测。无线电检测现在集中于构建越来越大的无线电实验，以增强检测器的敏感性并解决UHE处的低通量。在此程序中，我们概述了使用空气中的无线电技术（Anita，Pueo）或其他媒体（Icecube-gen2，Beacon，Beacon，rno-g）在Balloon（Anita，pueo）中使用无线电技术（Aera，oper-Prime，Grand）检测UHE宇宙颗粒的概述。
Radio-detection is a mature technique that has gained large momentum over the past decades. Its physical detection principle is mainly driven by the electromagnetic part of the shower, and is therefore not too sensitive to uncertainties on hadronic interactions. Furthermore its technical detection principle allows for a 100% duty cycle, and large surface coverage thanks to the low cost of antennas. Various detection methods of UHE particles now rely on the radio signal as main observable. For instance, ground based experiments such as AERA on the Pierre Auger Observatory or LOFAR detect the radio emission from air-showers induced by high-energy particles in the atmosphere; in-ice experiment such as ARA, IceCube, or ARIANNA benefits from a detection in denser media which reduces the interaction lengths; finally, balloon experiments such as ANITA allow for very sensitive UHE neutrino detection with only a few antennas. Radio-detection is now focused on building increasingly large-scale radio experiments to enhance the detector sensitivity and address the low fluxes at UHE. In this proceeding we give an overview of the past, current and future experiments for the detection of UHE cosmic particles using the radio technique in air (AERA, Auger-Prime, GRAND), in balloon (ANITA, PUEO) or in other media (IceCube-Gen2, BEACON, RNO-G).
