ARA-Next: a new DAQ and trigger architecture for the Askaryan Radio Array

TL;DR

ARA-Next introduces a new RFSoC-based data acquisition and trigger system for the Askaryan Radio Array, aiming to improve detection sensitivity for ultra-high-energy cosmic neutrinos through advanced trigger strategies.

Contribution

The paper presents the development of ARA-Next, a novel DAQ and trigger architecture incorporating multi-trigger techniques and sophisticated event identification methods for the ARA experiment.

Findings

Design of innovative trigger algorithms for neutrino detection.

Implementation of multi-trigger approach similar to collider experiments.

Enhanced sensitivity and lower thresholds for ARA detection capabilities.

Abstract

The Askaryan Radio Array (ARA) experiment aims to detect ultra-high-energy cosmic neutrinos (>10 PeV) using radio detection techniques. To enhance ARA's capabilities, a new RFSoC-based DAQ, ARA-Next, is in the early stages of development. This advanced system will facilitate the creation of sophisticated triggers, including a novel multi-trigger approach, similar to those used in collider experiments. Our approach involves crafting and implementing innovative triggers for ARA's new DAQ, such as identifying double pulses from potential in-ice neutrino interactions, utilizing templates for atmospheric cosmic ray signals, optimizing triggers for astrophysical neutrino sources, correlating special events between ARA and IceCube, and discerning anthropogenic events using directional information. These trigger designs aim to lower thresholds and enhance ARA's detector sensitivity. Overall, this upgrade will not only enhance ARA's capabilities but also contribute to the technological advancements necessary for future experiments of this nature.