Observation of a low energy nuclear recoil peak in the neutron calibration data of an <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi>Al</mml:mi> <mml:mn>2</mml:mn> </mml:msub> <mml:msub> <mml:mi mathvari

The current generation of cryogenic solid state detectors used in direct dark matter and <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mi>CE</a:mi> <a:mi>ν</a:mi> <a:mi>NS</a:mi> </a:mrow> </a:math> searches typically reach energy thresholds of <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mrow> <c:mi mathvariant="script">O</c:mi> <c:mo stretchy="false">(</c:mo> <c:mn>10</c:mn> <c:mo stretchy="false">)</c:mo> <c:mtext> </c:mtext> <c:mtext> </c:mtext> <c:mi>eV</c:mi> </c:mrow> </c:math> for nuclear recoils. For a reliable calibration in this energy regime a method has been proposed, providing monoenergetic nuclear recoils at low energies <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:mrow> <h:mo>∼</h:mo> <h:mn>100</h:mn> <h:mtext> </h:mtext> <h:mi>eV</h:mi> <h:mi>–</h:mi> <h:mn>1</h:mn> <h:mtext> </h:mtext> <h:mtext> </h:mtext> <h:mi>keV</h:mi> </h:mrow> </h:math> . In this work we report on the observation of a peak at ( <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"> <j:msubsup> <j:mn>1113.6</j:mn> <j:mrow> <j:mo>−</j:mo> <j:mn>6.5</j:mn> </j:mrow> <j:mrow> <j:mo>+</j:mo> <j:mn>6.5</j:mn> </j:mrow> </j:msubsup> </j:math> ) <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"> <l:mi>eV</l:mi> </l:math> in the data of an <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"> <n:msub> <n:mtext>Al</n:mtext> <n:mn>2</n:mn> </n:msub> <n:msub> <n:mi mathvariant="normal">O</n:mi> <n:mn>3</n:mn> </n:msub> </n:math> crystal in CRESST-III, which was irradiated with neutrons from an AmBe calibration source. We attribute this monoenergetic peak to the radiative capture of thermal neutrons on <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"> <q:mrow> <q:mmultiscripts> <q:mrow> <q:mi>Al</q:mi> </q:mrow> <q:mprescripts/> <q:none/> <q:mrow> <q:mn>27</q:mn> </q:mrow> </q:mmultiscripts> </q:mrow> </q:math> and the subsequent deexcitation via single <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"> <s:mi>γ</s:mi> </s:math> emission. We compare the measured results with the outcome of Geant4 simulations and investigate the possibility to make use of this effect for the energy calibration of <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:msub> <u:mtext>Al</u:mtext> <u:mn>2</u:mn> </u:msub> <u:msub> <u:mi mathvariant="normal">O</u:mi> <u:mn>3</u:mn> </u:msub> </u:math> detectors at low energies. We further investigate the possibility of a shift in the expected energy scale of this effect caused by the creation of defects in the target crystal.

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Journal
Physical review. D/Physical review. D.
Published
2025-11-26
DOI
https://doi.org/10.1103/bb31-pgzg
Citations
1
Primary Topic
Dark Matter and Cosmic Phenomena
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article
Field-Weighted Citation Impact
1.87
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article

Observation of a low energy nuclear recoil peak in the neutron calibration data of an <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi>Al</mml:mi> <mml:mn>2</mml:mn> </mml:msub> <mml:msub> <mml:mi mathvari

T. Ortmann, F. Petricca, L. Pattavina, Veronika Palušová et al.
1 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
1.87
article

Observation of a low energy nuclear recoil peak in the neutron calibration data of an <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msub> <mml:mi>Al</mml:mi> <mml:mn>2</mml:mn> </mml:msub> <mml:msub> <mml:mi mathvari

T. Ortmann, F. Petricca, L. Pattavina, Veronika Palušová, V. Mokina, J. Schieck, V. Zema, M. Kaznacheeva, S. Banik, K. Schäffner, G. Angloher, F. Reindl, P. Murali, S. Schönert, A. Langenkämper, A. Erb, D. Fuchs, C. Moore, C. Bucci, S. Di Lorenzo, R. Breier, D. Hauff, J. Burkhart, L. Einfalt, P. Gorla, C. Strandhagen, P. V. Guillaumon, H. Kluck, Louis C. Burmeister, F. Pröbst, L. Canonica, M. Ješkovský, A. Bertolini, A. Bento, M. Stahlberg, L. Stodolsky, M. Mancuso, I. Usherov, R. Strauß, S. Fichtinger, V. M. Ghete, E. Fascione, J. Jochum, B. von Krosigk, B. Mauri, W. Potzel, M. Macko, Pavel P. Povinec, J. Rothe, F. von Feilitzsch, M. Olmi, F. Pucci, H. Kraus, C. Schwertner, C. Pagliarone, F. Dominsky, E. Cipelli, D. Valdenaire, M. Zanirato, F. Casadei, J. Dohm
article en
1 citations

Abstract

The current generation of cryogenic solid state detectors used in direct dark matter and <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mi>CE</a:mi> <a:mi>ν</a:mi> <a:mi>NS</a:mi> </a:mrow> </a:math> searches typically reach energy thresholds of <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mrow> <c:mi mathvariant="script">O</c:mi> <c:mo stretchy="false">(</c:mo> <c:mn>10</c:mn> <c:mo stretchy="false">)</c:mo> <c:mtext> </c:mtext> <c:mtext> </c:mtext> <c:mi>eV</c:mi> </c:mrow> </c:math> for nuclear recoils. For a reliable calibration in this energy regime a method has been proposed, providing monoenergetic nuclear recoils at low energies <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:mrow> <h:mo>∼</h:mo> <h:mn>100</h:mn> <h:mtext> </h:mtext> <h:mi>eV</h:mi> <h:mi>–</h:mi> <h:mn>1</h:mn> <h:mtext> </h:mtext> <h:mtext> </h:mtext> <h:mi>keV</h:mi> </h:mrow> </h:math> . In this work we report on the observation of a peak at ( <j:math xmlns:j="http://www.w3.org/1998/Math/MathML" display="inline"> <j:msubsup> <j:mn>1113.6</j:mn> <j:mrow> <j:mo>−</j:mo> <j:mn>6.5</j:mn> </j:mrow> <j:mrow> <j:mo>+</j:mo> <j:mn>6.5</j:mn> </j:mrow> </j:msubsup> </j:math> ) <l:math xmlns:l="http://www.w3.org/1998/Math/MathML" display="inline"> <l:mi>eV</l:mi> </l:math> in the data of an <n:math xmlns:n="http://www.w3.org/1998/Math/MathML" display="inline"> <n:msub> <n:mtext>Al</n:mtext> <n:mn>2</n:mn> </n:msub> <n:msub> <n:mi mathvariant="normal">O</n:mi> <n:mn>3</n:mn> </n:msub> </n:math> crystal in CRESST-III, which was irradiated with neutrons from an AmBe calibration source. We attribute this monoenergetic peak to the radiative capture of thermal neutrons on <q:math xmlns:q="http://www.w3.org/1998/Math/MathML" display="inline"> <q:mrow> <q:mmultiscripts> <q:mrow> <q:mi>Al</q:mi> </q:mrow> <q:mprescripts/> <q:none/> <q:mrow> <q:mn>27</q:mn> </q:mrow> </q:mmultiscripts> </q:mrow> </q:math> and the subsequent deexcitation via single <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"> <s:mi>γ</s:mi> </s:math> emission. We compare the measured results with the outcome of Geant4 simulations and investigate the possibility to make use of this effect for the energy calibration of <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:msub> <u:mtext>Al</u:mtext> <u:mn>2</u:mn> </u:msub> <u:msub> <u:mi mathvariant="normal">O</u:mi> <u:mn>3</u:mn> </u:msub> </u:math> detectors at low energies. We further investigate the possibility of a shift in the expected energy scale of this effect caused by the creation of defects in the target crystal.

Physical review. D/Physical review. D.Vol. 112(10)
Karlsruhe Institute of Technology (DE), TU Wien (AT), Universidade de São Paulo (BR), Università degli studi di Cassino e del Lazio Meridionale (IT), Johannes Gutenberg University Mainz (DE), Heidelberg University (DE), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso (IT), University of Oxford (GB), Max Planck Institute for Physics (DE), Institute of Particle Physics (CA), Kirchhoff (Germany) (DE), Czech Technical University in Prague (CZ), Technical University of Munich (DE), University of Milano-Bicocca (IT), Comenius University Bratislava (SK), University of Coimbra (PT), University of Tübingen (DE)
Openalex Percentile: Top 11%
Dark Matter and Cosmic Phenomena
1.87
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