Abstract

Underwater acoustic detection of ultra-high-energy neutrinos was proposed already in 1950s: when a neutrino interacts with a nucleus in water, the resulting particle cascade produces a pressure pulse that has a bipolar temporal structure and propagates within a flat disk-like volume. A telescope that consists of thousands of acoustic sensors deployed in the deep sea can monitor hundreds of cubic kilometres of water looking for these signals and discriminating them from acoustic noise. To study the feasibility of the technique it is critical to have a calibrator able to mimic the neutrino “signature” that can be operated from a vessel. Due to the axial-symmetry of the signal, their very directive short bipolar shape and the constraints of operating at sea, the development of such a calibrator is very challenging. Once the possibility of using the acoustic parametric technique for this aim was validated with the first compact array calibrator prototype, in this paper we describe the new design for such a calibrator composed of an array of piezo ceramic tube transducers emitting in axial direction.

Highlights

  • The study of Ultra-High-Energy (UHE) neutrinos by means of the detection of the acoustic pulse generated by the energy deposition after interacting with a nucleus in water was proposed already in 1950s [1]

  • Underwater acoustic detection of ultra-high-energy neutrinos was proposed already in 1950s: when a neutrino interacts with a nucleus in water, the resulting particle cascade produces a pressure pulse that has a bipolar temporal structure and propagates within a flat disk-like volume

  • Once the possibility of using the acoustic parametric technique for this aim was validated with the first compact array calibrator prototype, in this paper we describe the new design for such a calibrator composed of an array of piezo ceramic tube transducers emitting in axial direction

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Summary

Introduction

The study of Ultra-High-Energy (UHE) neutrinos by means of the detection of the acoustic pulse generated by the energy deposition after interacting with a nucleus in water was proposed already in 1950s [1]. This phenomenon induces a local heating in a very short period of time leading to a submillisecond pressure pulse signal with bipolar shape and very directive flat disk-like pattern, with the bipolar pulse being emitted perpendicularly to the shower axis direction. Specific electronics adapted to the ceramics in order to feed them efficiently are required, as well as, to allow and control the different functionalities the calibrator has to provide

Compact array calibrator approach
Transducer characterization
Parametric bipolar pulse emission
Conclusions and future steps
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