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.
Authors
- T. Ortmann
- F. Petricca (ORCID: https://orcid.org/0000-0002-6355-2545)
- L. Pattavina (ORCID: https://orcid.org/0000-0003-4192-849X)
- Veronika Palušová (ORCID: https://orcid.org/0000-0003-2467-1215)
- V. Mokina (ORCID: https://orcid.org/0000-0002-7744-1950)
- J. Schieck
- V. Zema (ORCID: https://orcid.org/0000-0003-3566-0407)
- M. Kaznacheeva (ORCID: https://orcid.org/0000-0002-2712-1326)
- S. Banik (ORCID: https://orcid.org/0000-0003-1925-0088)
- K. Schäffner (ORCID: https://orcid.org/0000-0002-7928-6923)
- G. Angloher
- F. Reindl (ORCID: https://orcid.org/0000-0003-0151-2174)
- P. Murali
- S. Schönert (ORCID: https://orcid.org/0000-0001-5276-2881)
- A. Langenkämper
- A. Erb
- D. Fuchs (ORCID: https://orcid.org/0009-0006-7841-9073)
- C. Moore (ORCID: https://orcid.org/0000-0002-8140-4183)
- C. Bucci (ORCID: https://orcid.org/0000-0002-4528-2924)
- S. Di Lorenzo (ORCID: https://orcid.org/0000-0003-1582-9711)
- R. Breier (ORCID: https://orcid.org/0000-0003-1124-4812)
- D. Hauff
- J. Burkhart (ORCID: https://orcid.org/0000-0002-1989-7845)
- L. Einfalt
- P. Gorla
- C. Strandhagen (ORCID: https://orcid.org/0009-0003-3250-9792)
- P. V. Guillaumon (ORCID: https://orcid.org/0000-0001-7772-5526)
- H. Kluck (ORCID: https://orcid.org/0000-0003-3061-3732)
- Louis C. Burmeister
- F. Pröbst
- L. Canonica (ORCID: https://orcid.org/0000-0001-8734-206X)
- M. Ješkovský
- A. Bertolini
- A. Bento (ORCID: https://orcid.org/0000-0002-3817-6015)
- M. Stahlberg (ORCID: https://orcid.org/0000-0003-4201-071X)
- L. Stodolsky (ORCID: https://orcid.org/0000-0002-4842-1889)
- M. Mancuso
- I. Usherov
- R. Strauß (ORCID: https://orcid.org/0000-0002-5589-9952)
- S. Fichtinger
- V. M. Ghete (ORCID: https://orcid.org/0000-0002-9595-6560)
- E. Fascione
- J. Jochum
- B. von Krosigk (ORCID: https://orcid.org/0000-0001-5223-3023)
- B. Mauri
- W. Potzel
- M. Macko
- Pavel P. Povinec (ORCID: https://orcid.org/0000-0003-0275-794X)
- J. Rothe (ORCID: https://orcid.org/0000-0001-5748-7428)
- F. von Feilitzsch
- M. Olmi
- F. Pucci
- H. Kraus
- C. Schwertner
- C. Pagliarone
- F. Dominsky (ORCID: https://orcid.org/0009-0005-7775-3654)
- E. Cipelli
- D. Valdenaire
- M. Zanirato
- F. Casadei
- J. Dohm (ORCID: https://orcid.org/0009-0007-8553-9812)
Institutions
- 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)
Publication Details
- 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
- Type
- article
- Field-Weighted Citation Impact
- 1.87