MINI REVIEW article
Front. Sens.
Sec. Sensor Devices
This article is part of the Research TopicParticle and radiation sensors developed at INFN-CSN5View all 10 articles
High-performance Electromagnetic Calorimeter with oriented crystals to open new pathways in particle and astroparticle physics
Provisionally accepted- 1Istituto Nazionale di Fisica Nucleare Sezione di Ferrara, Ferrara, Italy
- 2Universita degli Studi di Ferrara Dipartimento di Fisica e Scienze della Terra, Ferrara, Italy
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Progress in high-energy physics has long relied on electromagnetic calorimeters—total absorption devices used to measure the energy of electrons and photons. Recently, it has been shown that electromagnetic showers can develop more rapidly inside scintillating crystals when the incoming beam is aligned with a crystal axis within a few tenths of a degree. Building on this, we are developing and testing a novel type of calorimeter based on oriented crystals, which enables a significantly reduced depth for containing high-energy showers compared to conventional designs. We report here the full R&D path, from single-crystal studies across various materials to the construction of the first 3×3 matrix of PWO crystals. The angular acceptance for shower acceleration is largely energy-independent, while the shower-length reduction becomes more pronounced at higher energies. This makes oriented-crystal calorimetry a promising solution for next-generation high-performance detectors. In addition to improving particle identification through reduced hadronic sensitivity, this technology is well-suited for forward calorimetry at colliders, fixed-target setups, and beam dumps for light dark matter searches. Furthermore, in γ-ray astrophysics, such compact calorimeters could enhance sensitivity above 1 GeV by increasing effective area without adding weight—ideal for space-based telescopes targeting high-energy transients and multi-messenger events.
Keywords: Crystals, Electromagnetic calorimeter, Inorganic scintillator, Strong field, high-energy physics
Received: 04 Jul 2025; Accepted: 05 Nov 2025.
Copyright: © 2025 Bandiera and Fedeli. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
* Correspondence:
Laura Bandiera, bandiera@fe.infn.it
Pierluigi Fedeli, pierluigi.fedeli@fe.infn.it
Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.
