Interaction position resolution simulations and in-beam measurements of the AGATA HPGe detectors
The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected γ ‐ ray spectra at two different target to...
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Published in | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Vol. 638; no. 1; pp. 96 - 109 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
2011
Elsevier |
Subjects | |
Online Access | Get full text |
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Abstract | The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected
γ
‐
ray
spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted
γ
‐
ray
. The
γ
‐
ray
tracking was used to determine the full energy of the
γ
‐
rays
and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of
<
1
mm
in the FWHM of the interaction position resolution for the
γ
‐
ray
energy range from 60
keV to 5
MeV. The method was tested with real data from an in-beam measurement using a
30Si beam at 64
MeV on a thin
12C target. Pulse-shape analysis of the digitized detector waveforms and
γ
‐
ray
tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the
γ
‐
ray
energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of
γ
‐
ray
energy from 8.5
mm at 250
keV to 4
mm at 1.5
MeV, and has an approximately constant value of about 4
mm in the
γ
‐
ray
energy range from 1.5 to 4
MeV. |
---|---|
AbstractList | The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected
γ
‐
ray
spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted
γ
‐
ray
. The
γ
‐
ray
tracking was used to determine the full energy of the
γ
‐
rays
and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of
<
1
mm
in the FWHM of the interaction position resolution for the
γ
‐
ray
energy range from 60
keV to 5
MeV. The method was tested with real data from an in-beam measurement using a
30Si beam at 64
MeV on a thin
12C target. Pulse-shape analysis of the digitized detector waveforms and
γ
‐
ray
tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the
γ
‐
ray
energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of
γ
‐
ray
energy from 8.5
mm at 250
keV to 4
mm at 1.5
MeV, and has an approximately constant value of about 4
mm in the
γ
‐
ray
energy range from 1.5 to 4
MeV. The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected gamma -ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted gamma -ray. The gamma -ray tracking was used to determine the full energy of the gamma -rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of [inline image] in the FWHM of the interaction position resolution for the gamma -ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a [super]30Si beam at 64 MeV on a thin [super]12C target. Pulse-shape analysis of the digitized detector waveforms and gamma -ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the gamma -ray energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of gamma -ray energy from 8.5 mm at 250 keV to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the gamma -ray energy range from 1.5 to 4 MeV. The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected γ ‐ ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted γ ‐ ray . The γ ‐ ray tracking was used to determine the full energy of the γ ‐ rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of &lt; 1 mm in the FWHM of the interaction position resolution for the γ ‐ ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a 30Si beam at 64 MeV on a thin 12C target. Pulse-shape analysis of the digitized detector waveforms and γ ‐ ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the γ ‐ ray energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of γ ‐ ray energy from 8.5 mm at 250 keV to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the γ ‐ ray energy range from 1.5 to 4 MeV. The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected γ -ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted γ -ray. The γ -ray tracking was used to determine the full energy of the γ -rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of in the FWHM of the interaction position resolution for the γ -ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a 30 Si beam at 64 MeV on a thin 12 C target. Pulse-shape analysis of the digitized detector waveforms and γ -ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the γ -ray energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of γ -ray energy from 8.5 mm at 250 keV to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the γ -ray energy range from 1.5 to 4 MeV. The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected gamma-ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted gamma-ray. The gamma-ray tracking was used to determine the full energy of the gamma-rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of <1 mm in the FVVHM of the interaction position resolution for the gamma-ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a (30)5i beam at 64 MeV on a thin C-12 target. Pulse-shape analysis of the digitized detector waveforms and gamma-ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the gamma-ray energy and on the energy, axial location and type of the first interaction point, are presented. The FVVHM of the interaction position resolution varies roughly linearly as a function of gamma-ray energy from 8.5 mm at 250 key to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the gamma-ray energy range from 1.5 to 4 MeV. The interaction position resolution of the segmented HPGe detectors of an AGATA triple cluster detector has been studied through Monte Carlo simulations and in an in-beam experiment. A new method based on measuring the energy resolution of Doppler-corrected γ-ray spectra at two different target to detector distances is described. This gives the two-dimensional position resolution in the plane perpendicular to the direction of the emitted γ-ray. The γ-ray tracking was used to determine the full energy of the γ-rays and the first interaction point, which is needed for the Doppler correction. Five different heavy-ion induced fusion-evaporation reactions and a reference reaction were selected for the simulations. The results of the simulations show that the method works very well and gives a systematic deviation of View the MathML source in the FWHM of the interaction position resolution for the γ-ray energy range from 60 keV to 5 MeV. The method was tested with real data from an in-beam measurement using a 30Si beam at 64 MeV on a thin 12C target. Pulse-shape analysis of the digitized detector waveforms and γ-ray tracking was performed to determine the position of the first interaction point, which was used for the Doppler corrections. Results of the dependency of the interaction position resolution on the γ-ray energy and on the energy, axial location and type of the first interaction point, are presented. The FWHM of the interaction position resolution varies roughly linearly as a function of γ-ray energy from 8.5 mm at 250 keV to 4 mm at 1.5 MeV, and has an approximately constant value of about 4 mm in the γ-ray energy range from 1.5 to 4 MeV. |
Author | Sahin, E. Filmer, F. Pascovici, G. Bortolato, D. Mengoni, D. Colosimo, S. Birkenbach, B. Judson, D.S. Khaplanov, A. Wiens, A. Joshi, P. Kempley, R. Bednarczyk, P. Boston, H.C. Eberth, J. Orlandi, R. Legay, E. Recchia, F. Nyberg, J. Napoli, D.R. Veyssiere, C. Dosme, N. Bucurescu, D. Crespi, F.C.L. Unsworth, C. Bazzacco, D. Gadea, A. Hess, H. Ur, C.A. Farnea, E. Pullia, A. Molini, P. Valiente-Dobón, J.J. Bruyneel, B. Meczynski, W. Söderström, P.-A. Griffiths, R. Grave, X. Calore, E. Reiter, P. Gulmini, M. Gottardo, A. Lersch, D. Lopez-Martens, A. Michelagnoli, C. Smith, J.F. Habermann, T. Al-Adili, A. Ataç, A. Aydin, S. Boston, A.J. Jones, P. Tonev, D. Grebosz, J. Ljungvall, J. Strachan, J. Jaworski, G. |
Author_xml | – sequence: 1 givenname: P.-A. surname: Söderström fullname: Söderström, P.-A. email: P-A.Soderstrom@physics.uu.se organization: Department of Physics and Astronomy,Uppsala University, SE-75121 Uppsala, Sweden – sequence: 2 givenname: F. surname: Recchia fullname: Recchia, F. organization: Dipartimento di Fisica dell’Università, Sezione di Padova, I-35122 Padova, Italy – sequence: 3 givenname: J. surname: Nyberg fullname: Nyberg, J. email: Johan.Nyberg@physics.uu.se organization: Department of Physics and Astronomy,Uppsala University, SE-75121 Uppsala, Sweden – sequence: 4 givenname: A. surname: Al-Adili fullname: Al-Adili, A. organization: Department of Physics and Astronomy,Uppsala University, SE-75121 Uppsala, Sweden – sequence: 5 givenname: A. surname: Ataç fullname: Ataç, A. organization: Department of Physics and Astronomy,Uppsala University, SE-75121 Uppsala, Sweden – sequence: 6 givenname: S. surname: Aydin fullname: Aydin, S. organization: INFN, Sezione di Padova, I-35122 Padova, Italy – sequence: 7 givenname: D. surname: Bazzacco fullname: Bazzacco, D. organization: INFN, Sezione di Padova, I-35122 Padova, Italy – sequence: 8 givenname: P. surname: Bednarczyk fullname: Bednarczyk, P. organization: The Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, 31-342 Krakow, Poland – sequence: 9 givenname: B. surname: Birkenbach fullname: Birkenbach, B. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 10 givenname: D. surname: Bortolato fullname: Bortolato, D. organization: Dipartimento di Fisica dell’Università, Sezione di Padova, I-35122 Padova, Italy – sequence: 11 givenname: A.J. surname: Boston fullname: Boston, A.J. organization: Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom – sequence: 12 givenname: H.C. surname: Boston fullname: Boston, H.C. organization: Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom – sequence: 13 givenname: B. surname: Bruyneel fullname: Bruyneel, B. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 14 givenname: D. surname: Bucurescu fullname: Bucurescu, D. organization: National Institute for Physics and Nuclear Engineering, RO-77125 Bucharest-Magurele, Romania – sequence: 15 givenname: E. surname: Calore fullname: Calore, E. organization: Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy – sequence: 16 givenname: S. surname: Colosimo fullname: Colosimo, S. organization: Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom – sequence: 17 givenname: F.C.L. surname: Crespi fullname: Crespi, F.C.L. organization: INFN Sezione di Milano, Università di Milano, I-20133 Milano, Italy – sequence: 18 givenname: N. surname: Dosme fullname: Dosme, N. organization: CSNSM, F-91405 Orsay Campus, France – sequence: 19 givenname: J. surname: Eberth fullname: Eberth, J. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 20 givenname: E. surname: Farnea fullname: Farnea, E. organization: INFN, Sezione di Padova, I-35122 Padova, Italy – sequence: 21 givenname: F. surname: Filmer fullname: Filmer, F. organization: Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom – sequence: 22 givenname: A. surname: Gadea fullname: Gadea, A. organization: IFIC, CSIC-Univ. Valencia, E-46071 Valencia, Spain – sequence: 23 givenname: A. surname: Gottardo fullname: Gottardo, A. organization: Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy – sequence: 24 givenname: X. surname: Grave fullname: Grave, X. organization: IPNO, IN2P3/CNRS et Université Paris-Sud, F-91405 Orsay, France – sequence: 25 givenname: J. surname: Grebosz fullname: Grebosz, J. organization: The Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, 31-342 Krakow, Poland – sequence: 26 givenname: R. surname: Griffiths fullname: Griffiths, R. organization: STFC Daresbury Laboratory, Daresbury, Warrington WA4 4AD, United Kingdom – sequence: 27 givenname: M. surname: Gulmini fullname: Gulmini, M. organization: Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy – sequence: 28 givenname: T. surname: Habermann fullname: Habermann, T. organization: GSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstrasse 1, D-64291 Darmstadt, Germany – sequence: 29 givenname: H. surname: Hess fullname: Hess, H. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 30 givenname: G. surname: Jaworski fullname: Jaworski, G. organization: Faculty of Physics, Warsaw University of Technology, Koszykowa 75, 00-662 Warsaw, Poland – sequence: 31 givenname: P. surname: Jones fullname: Jones, P. organization: Department of Physics, University of Jyväskylä, FIN-40014 Jyväskylä, Finland – sequence: 32 givenname: P. surname: Joshi fullname: Joshi, P. organization: Department of Physics, University of York, Heslington, York Y01 5DD, United Kingdom – sequence: 33 givenname: D.S. surname: Judson fullname: Judson, D.S. organization: Oliver Lodge Laboratory, University of Liverpool, Liverpool L69 7ZE, United Kingdom – sequence: 34 givenname: R. surname: Kempley fullname: Kempley, R. organization: Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom – sequence: 35 givenname: A. surname: Khaplanov fullname: Khaplanov, A. organization: Royal Institute of Technology, SE-10691 Stockholm, Sweden – sequence: 36 givenname: E. surname: Legay fullname: Legay, E. organization: CSNSM, F-91405 Orsay Campus, France – sequence: 37 givenname: D. surname: Lersch fullname: Lersch, D. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 38 givenname: J. surname: Ljungvall fullname: Ljungvall, J. organization: CSNSM, F-91405 Orsay Campus, France – sequence: 39 givenname: A. surname: Lopez-Martens fullname: Lopez-Martens, A. organization: CSNSM, F-91405 Orsay Campus, France – sequence: 40 givenname: W. surname: Meczynski fullname: Meczynski, W. organization: The Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, 31-342 Krakow, Poland – sequence: 41 givenname: D. surname: Mengoni fullname: Mengoni, D. organization: INFN, Sezione di Padova, I-35122 Padova, Italy – sequence: 42 givenname: C. surname: Michelagnoli fullname: Michelagnoli, C. organization: Dipartimento di Fisica dell’Università, Sezione di Padova, I-35122 Padova, Italy – sequence: 43 givenname: P. surname: Molini fullname: Molini, P. organization: Dipartimento di Fisica dell’Università, Sezione di Padova, I-35122 Padova, Italy – sequence: 44 givenname: D.R. surname: Napoli fullname: Napoli, D.R. organization: Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy – sequence: 45 givenname: R. surname: Orlandi fullname: Orlandi, R. organization: IEM, CSIC, E-28006 Madrid, Spain – sequence: 46 givenname: G. surname: Pascovici fullname: Pascovici, G. organization: Institut für Kernphysik, Universität zu Köln Zülpicher Straße 77, D-50937 Köln, Germany – sequence: 47 givenname: A. surname: Pullia fullname: Pullia, A. organization: INFN Sezione di Milano, Università di Milano, I-20133 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ContentType | Journal Article |
Copyright | 2011 Elsevier B.V. Distributed under a Creative Commons Attribution 4.0 International License |
Copyright_xml | – notice: 2011 Elsevier B.V. – notice: Distributed under a Creative Commons Attribution 4.0 International License |
CorporateAuthor | The AGATA Collaboration |
CorporateAuthor_xml | – name: The AGATA Collaboration |
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Keywords | γ ‐ ray tracking Monte Carlo simulations HPGe detectors AGATA Fusion-evaporation reactions g-ray tracking |
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SubjectTerms | [formula omitted] tracking AGATA Computer simulation Detectors Deviation Digitization Doppler Doppler effect Fusion-evaporation reactions Fysik gamma-ray tracking HPGe detectors Kärnfysik Monte Carlo methods Monte Carlo simulations NATURAL SCIENCES NATURVETENSKAP Nuclear Experiment Nuclear physics Physics Tracking γ ‐ ray tracking |
Title | Interaction position resolution simulations and in-beam measurements of the AGATA HPGe detectors |
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