The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations

Calorimetric space experiments were employed for the direct measurements of cosmic-ray spectra above the TeV region. According to several theoretical models and recent measurements, relevant features in both electron and nucleus fluxes are expected. Unfortunately, sizable disagreements among the cur...

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Main Authors: Lorenzo Pacini, Oscar Adriani, Eugenio Berti, Pietro Betti, Gabriele Bigongiari, Lorenzo Bonechi, Massimo Bongi, Sergio Bottai, Paolo Brogi, Guido Castellini, Caterina Checchia, Raffaello D’Alessandro, Sebastiano Detti, Noemi Finetti, Paolo Maestro, Pier Simone Marrocchesi, Nicola Mori, Miriam Olmi, Paolo Papini, Claudia Poggiali, Sergio Ricciarini, Piero Spillantini, Oleksandr Starodubtsev, Francesco Stolzi, Alessio Tiberio, Elena Vannuccini
Format: Article
Language:English
Published: MDPI AG 2022-09-01
Series:Instruments
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Online Access:https://www.mdpi.com/2410-390X/6/4/53
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author Lorenzo Pacini
Oscar Adriani
Eugenio Berti
Pietro Betti
Gabriele Bigongiari
Lorenzo Bonechi
Massimo Bongi
Sergio Bottai
Paolo Brogi
Guido Castellini
Caterina Checchia
Raffaello D’Alessandro
Sebastiano Detti
Noemi Finetti
Paolo Maestro
Pier Simone Marrocchesi
Nicola Mori
Miriam Olmi
Paolo Papini
Claudia Poggiali
Sergio Ricciarini
Piero Spillantini
Oleksandr Starodubtsev
Francesco Stolzi
Alessio Tiberio
Elena Vannuccini
author_facet Lorenzo Pacini
Oscar Adriani
Eugenio Berti
Pietro Betti
Gabriele Bigongiari
Lorenzo Bonechi
Massimo Bongi
Sergio Bottai
Paolo Brogi
Guido Castellini
Caterina Checchia
Raffaello D’Alessandro
Sebastiano Detti
Noemi Finetti
Paolo Maestro
Pier Simone Marrocchesi
Nicola Mori
Miriam Olmi
Paolo Papini
Claudia Poggiali
Sergio Ricciarini
Piero Spillantini
Oleksandr Starodubtsev
Francesco Stolzi
Alessio Tiberio
Elena Vannuccini
author_sort Lorenzo Pacini
collection DOAJ
description Calorimetric space experiments were employed for the direct measurements of cosmic-ray spectra above the TeV region. According to several theoretical models and recent measurements, relevant features in both electron and nucleus fluxes are expected. Unfortunately, sizable disagreements among the current results of different space calorimeters exist. In order to improve the accuracy of future experiments, it is fundamental to understand the reasons of these discrepancies, especially since they are not compatible with the quoted experimental errors. A few articles of different collaborations suggest that a systematic error of a few percentage points related to the energy-scale calibration could explain these differences. In this work, we analyze the impact of the nonproportionality of the light yield of scintillating crystals on the energy scale of typical calorimeters. Space calorimeters are usually calibrated by employing minimal ionizing particles (MIPs), e.g., nonshowering proton or helium nuclei, which feature different ionization density distributions with respect to particles included in showers. By using the experimental data obtained by the CaloCube collaboration and a minimalist model of the light yield as a function of the ionization density, several scintillating crystals (BGO, CsI(Tl), LYSO, YAP, YAG and BaF2) are characterized. Then, the response of a few crystals is implemented inside the Monte Carlo simulation of a space calorimeter to check the energy deposited by electromagnetic and hadronic showers. The results of this work show that the energy scale obtained by MIP calibration could be affected by sizable systematic errors if the nonproportionality of scintillation light is not properly taken into account.
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spelling doaj.art-693837ba6d1f4bf5963e2e71d0ff92632023-11-24T15:40:40ZengMDPI AGInstruments2410-390X2022-09-01645310.3390/instruments6040053The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo SimulationsLorenzo Pacini0Oscar Adriani1Eugenio Berti2Pietro Betti3Gabriele Bigongiari4Lorenzo Bonechi5Massimo Bongi6Sergio Bottai7Paolo Brogi8Guido Castellini9Caterina Checchia10Raffaello D’Alessandro11Sebastiano Detti12Noemi Finetti13Paolo Maestro14Pier Simone Marrocchesi15Nicola Mori16Miriam Olmi17Paolo Papini18Claudia Poggiali19Sergio Ricciarini20Piero Spillantini21Oleksandr Starodubtsev22Francesco Stolzi23Alessio Tiberio24Elena Vannuccini25INFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyDepartment of Physics and Astronomy, University of Florence, Via G. Sansone 1, I-50019 Firenze, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyDepartment of Physical Sciences, Earth and Environment, University of Siena, I-53100 Siena, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyINFN Firenze, Via B. Rossi 1, I-50019 Firenze, ItalyCalorimetric space experiments were employed for the direct measurements of cosmic-ray spectra above the TeV region. According to several theoretical models and recent measurements, relevant features in both electron and nucleus fluxes are expected. Unfortunately, sizable disagreements among the current results of different space calorimeters exist. In order to improve the accuracy of future experiments, it is fundamental to understand the reasons of these discrepancies, especially since they are not compatible with the quoted experimental errors. A few articles of different collaborations suggest that a systematic error of a few percentage points related to the energy-scale calibration could explain these differences. In this work, we analyze the impact of the nonproportionality of the light yield of scintillating crystals on the energy scale of typical calorimeters. Space calorimeters are usually calibrated by employing minimal ionizing particles (MIPs), e.g., nonshowering proton or helium nuclei, which feature different ionization density distributions with respect to particles included in showers. By using the experimental data obtained by the CaloCube collaboration and a minimalist model of the light yield as a function of the ionization density, several scintillating crystals (BGO, CsI(Tl), LYSO, YAP, YAG and BaF2) are characterized. Then, the response of a few crystals is implemented inside the Monte Carlo simulation of a space calorimeter to check the energy deposited by electromagnetic and hadronic showers. The results of this work show that the energy scale obtained by MIP calibration could be affected by sizable systematic errors if the nonproportionality of scintillation light is not properly taken into account.https://www.mdpi.com/2410-390X/6/4/53cosmic rayscalorimetryscintillationlight yield
spellingShingle Lorenzo Pacini
Oscar Adriani
Eugenio Berti
Pietro Betti
Gabriele Bigongiari
Lorenzo Bonechi
Massimo Bongi
Sergio Bottai
Paolo Brogi
Guido Castellini
Caterina Checchia
Raffaello D’Alessandro
Sebastiano Detti
Noemi Finetti
Paolo Maestro
Pier Simone Marrocchesi
Nicola Mori
Miriam Olmi
Paolo Papini
Claudia Poggiali
Sergio Ricciarini
Piero Spillantini
Oleksandr Starodubtsev
Francesco Stolzi
Alessio Tiberio
Elena Vannuccini
The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
Instruments
cosmic rays
calorimetry
scintillation
light yield
title The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
title_full The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
title_fullStr The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
title_full_unstemmed The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
title_short The Impact of Crystal Light Yield Non-Proportionality on a Typical Calorimetric Space Experiment: Beam Test Measurements and Monte Carlo Simulations
title_sort impact of crystal light yield non proportionality on a typical calorimetric space experiment beam test measurements and monte carlo simulations
topic cosmic rays
calorimetry
scintillation
light yield
url https://www.mdpi.com/2410-390X/6/4/53
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