Application of Geant4 simulation in measurement of cosmic-ray muon flux and studies of muon-induced background

The low-level underground laboratory at the Institute of Physics Belgrade is a facility for gamma-ray spectroscopy measurements and for measurements of cosmic-ray muon intensity. Related to the two research subjects, studies of cosmic-ray muon-induced background in gamma spectroscopy are of particul...

Full description

Saved in:

Bibliographic Details
Published in	European physical journal plus Vol. 138; no. 11; p. 1006
Main Authors	Joković, Dejan, Maletić, Dimitrije, Dragić, Aleksandar, Veselinović, Nikola, Savić, Mihailo, Udovičić, Vladimir, Banjanac, Radomir, Knežević, David
Format	Journal Article
Language	English
Published	Berlin/Heidelberg Springer Berlin Heidelberg 10.11.2023 Springer Nature B.V
Subjects	Applied and Technical Physics Atomic Charged particles Complex Systems Condensed Matter Physics Cosmic rays Data acquisition systems Energy Focus Point on Physics in the Balkans: Perspectives and Challenges Gamma ray detectors Gamma rays Gamma spectroscopy Germanium Laboratories Mathematical and Computational Physics Molecular Monte Carlo simulation Muons Neutrons Optical and Plasma Physics Physics Physics and Astronomy Radiation Regular Article Sensors Simulation Spectrometers Spectroscopic analysis Spectrum analysis Theoretical
Online Access	Get full text
ISSN	2190-5444 2190-5444
DOI	10.1140/epjp/s13360-023-04639-1

Cover

Abstract	The low-level underground laboratory at the Institute of Physics Belgrade is a facility for gamma-ray spectroscopy measurements and for measurements of cosmic-ray muon intensity. Related to the two research subjects, studies of cosmic-ray muon-induced background in gamma spectroscopy are of particular interest. Continuous measurements of cosmic muon intensity at the ground level and underground sites have been carried out by means of plastic scintillation detectors. The detector response, interpretation of the experimental spectra and their calibration were obtained and verified using a Geant4-based simulation. The results of the simulation were used in measurement of muon flux at the surface and shallow underground (25 m w e)—the measured fluxes are (170 ± 6) m −2 s −1 and (44 ± 1) m −2 s −1 , respectively. An underground muon detector can operate in coincidence with a high-purity germanium gamma-ray detector, which allows investigations of muon-induced processes in germanium spectrometers. In low-level gamma spectroscopy, neutrons produced by muons in the lead shielding of a germanium detector contribute to the detector background. Simulation of prompt muon-induced background as well as simulation of neutron production by cosmic muons in lead were carried out. Estimated neutron yield in lead is (3.1 ± 0.4) × 10 –5 neutrons per g/cm 2 , per tagged muon. Also the average neutron multiplicity is calculated.
AbstractList	The low-level underground laboratory at the Institute of Physics Belgrade is a facility for gamma-ray spectroscopy measurements and for measurements of cosmic-ray muon intensity. Related to the two research subjects, studies of cosmic-ray muon-induced background in gamma spectroscopy are of particular interest. Continuous measurements of cosmic muon intensity at the ground level and underground sites have been carried out by means of plastic scintillation detectors. The detector response, interpretation of the experimental spectra and their calibration were obtained and verified using a Geant4-based simulation. The results of the simulation were used in measurement of muon flux at the surface and shallow underground (25 m w e)—the measured fluxes are (170 ± 6) m −2 s −1 and (44 ± 1) m −2 s −1 , respectively. An underground muon detector can operate in coincidence with a high-purity germanium gamma-ray detector, which allows investigations of muon-induced processes in germanium spectrometers. In low-level gamma spectroscopy, neutrons produced by muons in the lead shielding of a germanium detector contribute to the detector background. Simulation of prompt muon-induced background as well as simulation of neutron production by cosmic muons in lead were carried out. Estimated neutron yield in lead is (3.1 ± 0.4) × 10 –5 neutrons per g/cm 2 , per tagged muon. Also the average neutron multiplicity is calculated. The low-level underground laboratory at the Institute of Physics Belgrade is a facility for gamma-ray spectroscopy measurements and for measurements of cosmic-ray muon intensity. Related to the two research subjects, studies of cosmic-ray muon-induced background in gamma spectroscopy are of particular interest. Continuous measurements of cosmic muon intensity at the ground level and underground sites have been carried out by means of plastic scintillation detectors. The detector response, interpretation of the experimental spectra and their calibration were obtained and verified using a Geant4-based simulation. The results of the simulation were used in measurement of muon flux at the surface and shallow underground (25 m w e)—the measured fluxes are (170 ± 6) m−2 s−1 and (44 ± 1) m−2 s−1, respectively. An underground muon detector can operate in coincidence with a high-purity germanium gamma-ray detector, which allows investigations of muon-induced processes in germanium spectrometers. In low-level gamma spectroscopy, neutrons produced by muons in the lead shielding of a germanium detector contribute to the detector background. Simulation of prompt muon-induced background as well as simulation of neutron production by cosmic muons in lead were carried out. Estimated neutron yield in lead is (3.1 ± 0.4) × 10–5 neutrons per g/cm2, per tagged muon. Also the average neutron multiplicity is calculated.
ArticleNumber	1006
Author	Savić, Mihailo Maletić, Dimitrije Veselinović, Nikola Joković, Dejan Banjanac, Radomir Knežević, David Dragić, Aleksandar Udovičić, Vladimir
Author_xml	– sequence: 1 givenname: Dejan orcidid: 0000-0002-3404-2706 surname: Joković fullname: Joković, Dejan email: yokovic@ipb.ac.rs organization: Institute of Physics, University of Belgrade – sequence: 2 givenname: Dimitrije surname: Maletić fullname: Maletić, Dimitrije organization: Institute of Physics, University of Belgrade – sequence: 3 givenname: Aleksandar surname: Dragić fullname: Dragić, Aleksandar organization: Institute of Physics, University of Belgrade – sequence: 4 givenname: Nikola surname: Veselinović fullname: Veselinović, Nikola organization: Institute of Physics, University of Belgrade – sequence: 5 givenname: Mihailo surname: Savić fullname: Savić, Mihailo organization: Institute of Physics, University of Belgrade – sequence: 6 givenname: Vladimir surname: Udovičić fullname: Udovičić, Vladimir organization: Institute of Physics, University of Belgrade – sequence: 7 givenname: Radomir surname: Banjanac fullname: Banjanac, Radomir organization: Institute of Physics, University of Belgrade – sequence: 8 givenname: David surname: Knežević fullname: Knežević, David organization: Institute of Physics, University of Belgrade
BookMark	eNqNkE1LwzAYx4MoqHOfwYLnaN6argcPY-gUBl70HGJeRmab1ryA-_a2q6B40eSQkPx_eZ78zsGx77wB4BKja4wZujH9rr-JmFKOICIUIsZpDfEROCO4RrBkjB3_2J-CeYw7NAxWY1azM-CXfd84JZPrfNHZYm2kT6yIrs3NdOh80RoZczCt8WnMqC62TsEg90Wbh4Rt8kchvS5iytqZOGbGC-i8zsro4lWqt23ostcX4MTKJpr51zoDL_d3z6sHuHlaP66WG6goZQlqrBCVhNhhcky4LUuOLEfSEKmoLiViVYUNq7QhqiQVripVMs44plory-kMXE3v9qF7zyYmsety8ENJQWqC8IIgXg2p2ymlQhdjMFYolw6_TkG6RmAkRstitCwmy2KwLA6WBR746hffB9fKsP8HuZjIOBB-a8J3f3-hn7JkmAE
CitedBy_id	crossref_primary_10_1140_epjp_s13360_024_05083_5
Cites_doi	10.1088/1742-6596/409/1/012054 10.1016/j.apradiso.2016.12.039 10.1016/j.astropartphys.2022.102756 10.1016/j.nima.2008.02.053 10.2298/NTRP1103181D 10.1016/j.nima.2016.06.125 10.1016/j.apradiso.2016.12.047 10.1103/PhysRevD.86.054001 10.1140/epja/i2007-10539-6 10.1016/j.apradiso.2009.01.024 10.1016/j.astropartphys.2019.06.006 10.1016/j.astropartphys.2019.03.006 10.1016/S0168-9002(03)01368-8 10.1016/j.nima.2009.10.059 10.1140/epjd/s10053-021-00172-x 10.1016/0168-9002(92)90918-T 10.1016/j.astropartphys.2018.04.005 10.1007/s10967-023-08810-x 10.1016/j.astropartphys.2013.06.002 10.1016/j.nima.2022.166624 10.1016/j.nima.2005.08.065 10.1016/j.astropartphys.2019.01.006 10.1016/j.nima.2017.09.008 10.1093/ptep/ptaa104
ContentType	Journal Article
Copyright	The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
Copyright_xml	– notice: The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2023. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
DBID	AAYXX CITATION 8FE 8FG AEUYN AFKRA ARAPS BENPR BGLVJ BHPHI BKSAR CCPQU DWQXO HCIFZ P5Z P62 PCBAR PHGZM PHGZT PKEHL PQEST PQGLB PQQKQ PQUKI
DOI	10.1140/epjp/s13360-023-04639-1
DatabaseName	CrossRef ProQuest SciTech Collection ProQuest Technology Collection ProQuest One Sustainability ProQuest Central ProQuest Advanced Technologies & Aerospace Database ProQuest Central Technology Collection Natural Science Collection Earth, Atmospheric & Aquatic Science Collection ProQuest One ProQuest Central SciTech Premium Collection Advanced Technologies & Aerospace Collection ProQuest Advanced Technologies & Aerospace Collection Earth, Atmospheric & Aquatic Science Database ProQuest Central Premium ProQuest One Academic ProQuest One Academic Middle East (New) ProQuest One Academic Eastern Edition (DO NOT USE) ProQuest One Applied & Life Sciences ProQuest One Academic ProQuest One Academic UKI Edition
DatabaseTitle	CrossRef Advanced Technologies & Aerospace Collection Technology Collection ProQuest One Academic Middle East (New) ProQuest Advanced Technologies & Aerospace Collection ProQuest One Academic Eastern Edition Earth, Atmospheric & Aquatic Science Database SciTech Premium Collection ProQuest One Community College ProQuest Technology Collection ProQuest SciTech Collection Earth, Atmospheric & Aquatic Science Collection ProQuest Central Advanced Technologies & Aerospace Database ProQuest One Applied & Life Sciences ProQuest One Sustainability ProQuest One Academic UKI Edition Natural Science Collection ProQuest Central Korea ProQuest Central (New) ProQuest One Academic ProQuest One Academic (New)
DatabaseTitleList	Advanced Technologies & Aerospace Collection
Database_xml	– sequence: 1 dbid: 8FG name: ProQuest Technology Collection url: https://search.proquest.com/technologycollection1 sourceTypes: Aggregation Database
DeliveryMethod	fulltext_linktorsrc
Discipline	Physics
EISSN	2190-5444
ExternalDocumentID	10_1140_epjp_s13360_023_04639_1
GrantInformation_xml	– fundername: Institute of Physics Belgrade funderid: http://dx.doi.org/10.13039/100017592
GroupedDBID	-5F -5G -BR -EM -~C 06D 0R~ 203 29~ 2JN 2KG 30V 4.4 406 408 8UJ 95. 96X AABHQ AACDK AAHNG AAIAL AAJBT AAJKR AANZL AARTL AASML AATNV AATVU AAUYE AAWCG AAYIU AAYQN AAYTO AAYZH AAZMS ABAKF ABDZT ABECU ABFTV ABHLI ABJNI ABJOX ABKCH ABMQK ABQBU ABSXP ABTEG ABTHY ABTKH ABTMW ABXPI ACAOD ACDTI ACGFS ACHSB ACKNC ACMDZ ACMLO ACOKC ACPIV ACREN ACZOJ ADHHG ADINQ ADKNI ADKPE ADURQ ADYFF ADZKW AEFQL AEGNC AEJHL AEJRE AEMSY AENEX AEOHA AEPYU AESKC AETCA AEUYN AEVLU AEXYK AFBBN AFKRA AFQWF AFWTZ AFZKB AGAYW AGDGC AGMZJ AGQEE AGQMX AGRTI AGWZB AGYKE AHAVH AHBYD AHYZX AIAKS AIGIU AIIXL AILAN AITGF AJRNO AJZVZ ALFXC ALMA_UNASSIGNED_HOLDINGS AMKLP AMXSW AMYLF AMYQR ANMIH AOCGG ARAPS ARMRJ AXYYD AYJHY BENPR BGLVJ BGNMA BHPHI BKSAR CCPQU CSCUP DDRTE DNIVK DPUIP EBLON EBS EIOEI ESBYG FERAY FFXSO FIGPU FNLPD FRRFC GGCAI GGRSB GJIRD GNWQR GQ6 GQ7 HCIFZ HMJXF HRMNR HZ~ I0C IKXTQ IWAJR IXD J-C JBSCW JZLTJ KOV LLZTM M4Y NPVJJ NQJWS NU0 O93 O9J P9T PCBAR PT4 RID RLLFE ROL RSV S27 S3B SHX SISQX SJYHP SNE SNPRN SNX SOHCF SOJ SPH SPISZ SRMVM SSLCW STPWE SZN T13 TSG U2A UG4 UOJIU UTJUX UZXMN VC2 VFIZW W48 WK8 Z7S Z7Y ZMTXR ~A9 AAPKM AAYXX ABBRH ABDBE ABFSG ABRTQ ACSTC AEZWR AFDZB AFHIU AFOHR AHPBZ AHWEU AIXLP ATHPR AYFIA CITATION PHGZM PHGZT PQGLB PUEGO 8FE 8FG DWQXO P62 PKEHL PQEST PQQKQ PQUKI
ID	FETCH-LOGICAL-c334t-d1c03a22f2f26126f5560f60ae2ac3d5a04771e47de2c527177c5464613ddcf63
IEDL.DBID	BENPR
ISSN	2190-5444
IngestDate	Fri Jul 25 23:26:36 EDT 2025 Wed Oct 01 03:22:39 EDT 2025 Thu Apr 24 22:51:53 EDT 2025 Fri Feb 21 02:41:58 EST 2025
IsPeerReviewed	true
IsScholarly	true
Issue	11
Language	English
LinkModel	DirectLink
MergedId	FETCHMERGED-LOGICAL-c334t-d1c03a22f2f26126f5560f60ae2ac3d5a04771e47de2c527177c5464613ddcf63
Notes	ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14
ORCID	0000-0002-3404-2706
PQID	2920182067
PQPubID	2044220
ParticipantIDs	proquest_journals_2920182067 crossref_citationtrail_10_1140_epjp_s13360_023_04639_1 crossref_primary_10_1140_epjp_s13360_023_04639_1 springer_journals_10_1140_epjp_s13360_023_04639_1
ProviderPackageCode	CITATION AAYXX
PublicationCentury	2000
PublicationDate	2023-11-10
PublicationDateYYYYMMDD	2023-11-10
PublicationDate_xml	– month: 11 year: 2023 text: 2023-11-10 day: 10
PublicationDecade	2020
PublicationPlace	Berlin/Heidelberg
PublicationPlace_xml	– name: Berlin/Heidelberg – name: Heidelberg
PublicationTitle	European physical journal plus
PublicationTitleAbbrev	Eur. Phys. J. Plus
PublicationYear	2023
Publisher	Springer Berlin Heidelberg Springer Nature B.V
Publisher_xml	– name: Springer Berlin Heidelberg – name: Springer Nature B.V
References	AllisonJNucl. Instrum. Methods Phys. Res. A20168351862016NIMPA.835..186A10.1016/j.nima.2016.06.125 BaeHWJeonEJKimYDLeeSWAstropart. Phys.2020114602020APh...114...60B10.1016/j.astropartphys.2019.06.006 Geant4, https://geant4.web.cern.ch KneiβlRAstropart. Phys.2019111872019APh...111...87K10.1016/j.astropartphys.2019.03.006 GriederPKFCosmic Rays at Earth2001AmsterdamElsevier498 ŠkoroGNucl. Instrum. Methods Phys. Res. A19923163331992NIMPA.316..333S10.1016/0168-9002(92)90918-T HungNQHaiVHNomachiMAppl. Radiat. Isot.20171218710.1016/j.apradiso.2016.12.047 GuanMMuon Simulation at the Daya Bay Site2010Lawrence Berkeley National Laboratory SavićMAstropart. Phys.201910912019APh...109....1S10.1016/j.astropartphys.2019.01.006 BarkerDMeiD-MZhangCPhys. Rev. D2012862012PhRvD..86e4001B10.1103/PhysRevD.86.054001 EnquistTNucl. Instrum. Methods Phys. Res. A20055542862005NIMPA.554..286E10.1016/j.nima.2005.08.065 ZylaPAProg. Theor. Exp. Phys.20202020083C0110.1093/ptep/ptaa104 GriederPKFCosmic Rays at Earth2001AmsterdamElsevier372 ReichhartLAstropart. Phys.201347672013APh....47...67R10.1016/j.astropartphys.2013.06.002 DragićANucl. Instrum. Methods Phys. Res. A20085914702008NIMPA.591..470D10.1016/j.nima.2008.02.053 CORSIKA, https://www.iap.kit.edu/corsika D. Heck et al., CORSIKA: a Monte Carlo code to simulate extensive air showers, Report FZKA 6019. (Forschungszentrum Karlsruhe, 1998) AgostinelliSNucl. Instrum. Methods Phys. Res. A20035062502003NIMPA.506..250A10.1016/S0168-9002(03)01368-8 JovančevićNNucl. Instrum. Methods Phys. Res. A20106123032010NIMPA.612..303J10.1016/j.nima.2009.10.059 KnezevicJNucl. Instrum. Methods Phys. Res. A2022103210.1016/j.nima.2022.166624 VeselinovićNNucl. Instrum. Methods Phys. Res. A2017875102017NIMPA.875...10V10.1016/j.nima.2017.09.008 JokovićDRAppl. Radiat. Isot.20096771910.1016/j.apradiso.2009.01.024 TravarMJ. Radioanal. Nucl. Chem.202333281710.1007/s10967-023-08810-x KudryavtsevVAPandolaLTomaselloVEur. Phys. J. A2008361712008EPJA...36..171K10.1140/epja/i2007-10539-6 GriederPKFCosmic Rays at Earth2001AmsterdamElsevier467 VeselinovićNEur. Phys. J. D2021751732021EPJD...75..173V10.1140/epjd/s10053-021-00172-x DragićANucl. Technol. Radiat. Prot.20112618110.2298/NTRP1103181D BaginovaMVojtylaPPovinecPPAstropart. Phys.202214310.1016/j.astropartphys.2022.102756 DuQAstropart. Phys.2018102122018APh...102...12D10.1016/j.astropartphys.2018.04.005 GaisserTKCosmic Rays and Particle Physics1990CambridgeCambridge University Press71 DragićAJ. Phys. Conf. Ser.201340901205410.1088/1742-6596/409/1/012054 MitricaBAdv. High Energy Phys.20132013 BreierRLaubensteinMPovinecPPAppl. Radiat. Isot.201712618810.1016/j.apradiso.2016.12.039 R Breier (4639_CR26) 2017; 126 L Reichhart (4639_CR31) 2013; 47 PKF Grieder (4639_CR14) 2001 NQ Hung (4639_CR25) 2017; 121 4639_CR20 R Kneiβl (4639_CR33) 2019; 111 N Veselinović (4639_CR5) 2021; 75 HW Bae (4639_CR8) 2020; 114 M Baginova (4639_CR27) 2022; 143 A Dragić (4639_CR9) 2013; 409 G Škoro (4639_CR30) 1992; 316 N Veselinović (4639_CR3) 2017; 875 PKF Grieder (4639_CR18) 2001 J Knezevic (4639_CR28) 2022; 1032 D Barker (4639_CR7) 2012; 86 PKF Grieder (4639_CR15) 2001 TK Gaisser (4639_CR16) 1990 4639_CR10 J Allison (4639_CR12) 2016; 835 A Dragić (4639_CR2) 2008; 591 4639_CR19 M Travar (4639_CR29) 2023; 332 DR Joković (4639_CR13) 2009; 67 M Savić (4639_CR4) 2019; 109 S Agostinelli (4639_CR11) 2003; 506 T Enquist (4639_CR21) 2005; 554 N Jovančević (4639_CR24) 2010; 612 VA Kudryavtsev (4639_CR6) 2008; 36 M Guan (4639_CR17) 2010 PA Zyla (4639_CR22) 2020; 2020 B Mitrica (4639_CR23) 2013; 2013 Q Du (4639_CR32) 2018; 102 A Dragić (4639_CR1) 2011; 26
References_xml	– reference: BarkerDMeiD-MZhangCPhys. Rev. D2012862012PhRvD..86e4001B10.1103/PhysRevD.86.054001 – reference: JokovićDRAppl. Radiat. Isot.20096771910.1016/j.apradiso.2009.01.024 – reference: JovančevićNNucl. Instrum. Methods Phys. Res. A20106123032010NIMPA.612..303J10.1016/j.nima.2009.10.059 – reference: ReichhartLAstropart. Phys.201347672013APh....47...67R10.1016/j.astropartphys.2013.06.002 – reference: BaginovaMVojtylaPPovinecPPAstropart. Phys.202214310.1016/j.astropartphys.2022.102756 – reference: DragićAJ. Phys. Conf. Ser.201340901205410.1088/1742-6596/409/1/012054 – reference: SavićMAstropart. Phys.201910912019APh...109....1S10.1016/j.astropartphys.2019.01.006 – reference: CORSIKA, https://www.iap.kit.edu/corsika/ – reference: HungNQHaiVHNomachiMAppl. Radiat. Isot.20171218710.1016/j.apradiso.2016.12.047 – reference: DragićANucl. Technol. Radiat. Prot.20112618110.2298/NTRP1103181D – reference: KnezevicJNucl. Instrum. Methods Phys. Res. A2022103210.1016/j.nima.2022.166624 – reference: DuQAstropart. Phys.2018102122018APh...102...12D10.1016/j.astropartphys.2018.04.005 – reference: DragićANucl. Instrum. Methods Phys. Res. A20085914702008NIMPA.591..470D10.1016/j.nima.2008.02.053 – reference: BreierRLaubensteinMPovinecPPAppl. Radiat. Isot.201712618810.1016/j.apradiso.2016.12.039 – reference: EnquistTNucl. Instrum. Methods Phys. Res. A20055542862005NIMPA.554..286E10.1016/j.nima.2005.08.065 – reference: ZylaPAProg. Theor. Exp. Phys.20202020083C0110.1093/ptep/ptaa104 – reference: ŠkoroGNucl. Instrum. Methods Phys. Res. A19923163331992NIMPA.316..333S10.1016/0168-9002(92)90918-T – reference: GriederPKFCosmic Rays at Earth2001AmsterdamElsevier372 – reference: AllisonJNucl. Instrum. Methods Phys. Res. A20168351862016NIMPA.835..186A10.1016/j.nima.2016.06.125 – reference: GriederPKFCosmic Rays at Earth2001AmsterdamElsevier467 – reference: GuanMMuon Simulation at the Daya Bay Site2010Lawrence Berkeley National Laboratory – reference: AgostinelliSNucl. Instrum. Methods Phys. Res. A20035062502003NIMPA.506..250A10.1016/S0168-9002(03)01368-8 – reference: MitricaBAdv. High Energy Phys.20132013 – reference: VeselinovićNEur. Phys. J. D2021751732021EPJD...75..173V10.1140/epjd/s10053-021-00172-x – reference: GriederPKFCosmic Rays at Earth2001AmsterdamElsevier498 – reference: KneiβlRAstropart. Phys.2019111872019APh...111...87K10.1016/j.astropartphys.2019.03.006 – reference: VeselinovićNNucl. Instrum. Methods Phys. Res. A2017875102017NIMPA.875...10V10.1016/j.nima.2017.09.008 – reference: Geant4, https://geant4.web.cern.ch/ – reference: BaeHWJeonEJKimYDLeeSWAstropart. Phys.2020114602020APh...114...60B10.1016/j.astropartphys.2019.06.006 – reference: KudryavtsevVAPandolaLTomaselloVEur. Phys. J. A2008361712008EPJA...36..171K10.1140/epja/i2007-10539-6 – reference: GaisserTKCosmic Rays and Particle Physics1990CambridgeCambridge University Press71 – reference: TravarMJ. Radioanal. Nucl. Chem.202333281710.1007/s10967-023-08810-x – reference: D. Heck et al., CORSIKA: a Monte Carlo code to simulate extensive air showers, Report FZKA 6019. (Forschungszentrum Karlsruhe, 1998) – volume: 409 start-page: 012054 year: 2013 ident: 4639_CR9 publication-title: J. Phys. Conf. Ser. doi: 10.1088/1742-6596/409/1/012054 – volume: 126 start-page: 188 year: 2017 ident: 4639_CR26 publication-title: Appl. Radiat. Isot. doi: 10.1016/j.apradiso.2016.12.039 – volume: 143 year: 2022 ident: 4639_CR27 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2022.102756 – start-page: 467 volume-title: Cosmic Rays at Earth year: 2001 ident: 4639_CR18 – volume: 591 start-page: 470 year: 2008 ident: 4639_CR2 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2008.02.053 – start-page: 498 volume-title: Cosmic Rays at Earth year: 2001 ident: 4639_CR15 – volume: 26 start-page: 181 year: 2011 ident: 4639_CR1 publication-title: Nucl. Technol. Radiat. Prot. doi: 10.2298/NTRP1103181D – volume: 835 start-page: 186 year: 2016 ident: 4639_CR12 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2016.06.125 – volume: 121 start-page: 87 year: 2017 ident: 4639_CR25 publication-title: Appl. Radiat. Isot. doi: 10.1016/j.apradiso.2016.12.047 – volume: 86 year: 2012 ident: 4639_CR7 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.86.054001 – volume: 36 start-page: 171 year: 2008 ident: 4639_CR6 publication-title: Eur. Phys. J. A doi: 10.1140/epja/i2007-10539-6 – volume: 67 start-page: 719 year: 2009 ident: 4639_CR13 publication-title: Appl. Radiat. Isot. doi: 10.1016/j.apradiso.2009.01.024 – start-page: 71 volume-title: Cosmic Rays and Particle Physics year: 1990 ident: 4639_CR16 – volume: 114 start-page: 60 year: 2020 ident: 4639_CR8 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2019.06.006 – volume: 111 start-page: 87 year: 2019 ident: 4639_CR33 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2019.03.006 – volume: 506 start-page: 250 year: 2003 ident: 4639_CR11 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/S0168-9002(03)01368-8 – volume: 612 start-page: 303 year: 2010 ident: 4639_CR24 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2009.10.059 – ident: 4639_CR20 – volume: 75 start-page: 173 year: 2021 ident: 4639_CR5 publication-title: Eur. Phys. J. D doi: 10.1140/epjd/s10053-021-00172-x – ident: 4639_CR19 – volume: 316 start-page: 333 year: 1992 ident: 4639_CR30 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/0168-9002(92)90918-T – volume: 102 start-page: 12 year: 2018 ident: 4639_CR32 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2018.04.005 – start-page: 372 volume-title: Cosmic Rays at Earth year: 2001 ident: 4639_CR14 – volume: 332 start-page: 817 year: 2023 ident: 4639_CR29 publication-title: J. Radioanal. Nucl. Chem. doi: 10.1007/s10967-023-08810-x – volume-title: Muon Simulation at the Daya Bay Site year: 2010 ident: 4639_CR17 – ident: 4639_CR10 – volume: 2013 year: 2013 ident: 4639_CR23 publication-title: Adv. High Energy Phys. – volume: 47 start-page: 67 year: 2013 ident: 4639_CR31 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2013.06.002 – volume: 1032 year: 2022 ident: 4639_CR28 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2022.166624 – volume: 554 start-page: 286 year: 2005 ident: 4639_CR21 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2005.08.065 – volume: 109 start-page: 1 year: 2019 ident: 4639_CR4 publication-title: Astropart. Phys. doi: 10.1016/j.astropartphys.2019.01.006 – volume: 875 start-page: 10 year: 2017 ident: 4639_CR3 publication-title: Nucl. Instrum. Methods Phys. Res. A doi: 10.1016/j.nima.2017.09.008 – volume: 2020 start-page: 083C01 year: 2020 ident: 4639_CR22 publication-title: Prog. Theor. Exp. Phys. doi: 10.1093/ptep/ptaa104
SSID	ssj0000491494
Score	2.3044517
Snippet	The low-level underground laboratory at the Institute of Physics Belgrade is a facility for gamma-ray spectroscopy measurements and for measurements of...
SourceID	proquest crossref springer
SourceType	Aggregation Database Enrichment Source Index Database Publisher
StartPage	1006
SubjectTerms	Applied and Technical Physics Atomic Charged particles Complex Systems Condensed Matter Physics Cosmic rays Data acquisition systems Energy Focus Point on Physics in the Balkans: Perspectives and Challenges Gamma ray detectors Gamma rays Gamma spectroscopy Germanium Laboratories Mathematical and Computational Physics Molecular Monte Carlo simulation Muons Neutrons Optical and Plasma Physics Physics Physics and Astronomy Radiation Regular Article Sensors Simulation Spectrometers Spectroscopic analysis Spectrum analysis Theoretical
SummonAdditionalLinks	– databaseName: SpringerLink Journals (ICM) dbid: U2A link: http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV1LSwMxEA5SEbyIT6xWycFraHbz2PZYxFo8eLLQW8jmAdXutrgt6L93so-uerAgC3tJZg8zyc43mS8zCN0FVCA09USnaUq4hK045GJAUmqkpkZreAW2xbOcTPnTTMy-t_oKbPcmJVn-qat6trTvVq-rfgEhlaQEHE3gJLIhgcBnX4SaXrCUp_Foe7wCwBewP68ZXX_I__RHLcj8lRct3c34GB3VOBGPKsOeoD2Xn6KDkq9pijOUj9rEM156_OhAQxwX86xux4XnOc7a878wxyyLbG7Iu_7E2QZm-MXmA-vc4qLiEoY5YYBAmA4GtzjV5i3c-sjtOZqOH17uJ6RunUAMY3xNbGQo03Hs4QEMI70AZOMl1S7WhlmwDk-SyPHEutiIGGK6xAguOTh3a42X7AJ18mXuLhFmXFiXeGqlZdzTOBXMD4ZWxtw4r3XSRbJRoDJ1XfHQ3mKhqjvPVAXNq0rzCjSvSs2rqIvoVnBVldbYLdJrLKTqvVao0G-rKkPfRVFjtXZ4xyev_iFzjQ5D13lSsgF7qLN-37gbwCbr9LZchV8w893E priority: 102 providerName: Springer Nature
Title	Application of Geant4 simulation in measurement of cosmic-ray muon flux and studies of muon-induced background
URI	https://link.springer.com/article/10.1140/epjp/s13360-023-04639-1 https://www.proquest.com/docview/2920182067
Volume	138
hasFullText	1
inHoldings	1
isFullTextHit
isPrint
journalDatabaseRights	– providerCode: PRVLSH databaseName: SpringerLink Journals customDbUrl: mediaType: online eissn: 2190-5444 dateEnd: 99991231 omitProxy: false ssIdentifier: ssj0000491494 issn: 2190-5444 databaseCode: AFBBN dateStart: 20110107 isFulltext: true providerName: Library Specific Holdings – providerCode: PRVPQU databaseName: ProQuest Central customDbUrl: http://www.proquest.com/pqcentral?accountid=15518 eissn: 2190-5444 dateEnd: 20241102 omitProxy: true ssIdentifier: ssj0000491494 issn: 2190-5444 databaseCode: BENPR dateStart: 20110101 isFulltext: true titleUrlDefault: https://www.proquest.com/central providerName: ProQuest – providerCode: PRVAVX databaseName: SpringerLINK - Czech Republic Consortium customDbUrl: eissn: 2190-5444 dateEnd: 99991231 omitProxy: false ssIdentifier: ssj0000491494 issn: 2190-5444 databaseCode: AGYKE dateStart: 20110101 isFulltext: true titleUrlDefault: http://link.springer.com providerName: Springer Nature – providerCode: PRVAVX databaseName: SpringerLink Journals (ICM) customDbUrl: eissn: 2190-5444 dateEnd: 99991231 omitProxy: true ssIdentifier: ssj0000491494 issn: 2190-5444 databaseCode: U2A dateStart: 20110101 isFulltext: true titleUrlDefault: http://www.springerlink.com/journals/ providerName: Springer Nature
link	http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwhV1LaxsxEB4Sm0IvIW1T6iQ1OvQqrJW0WvtQilNshxZMKTUkJ6HVA9zGaydrQ_vvM9pHlvbQsKDD6nGYkTQz0qf5AD5EryA1LFCT5zmVCpfiRKZjmjOrDLPGYBHRFkt1vZJfbtKbI1i2b2EirLLdE6uN2m1tPCMfRValOtn4p909jaxR8Xa1pdAwDbWC-1ilGDuGPo-ZsXrQv5otv31_OnVBfxhDAtkAvTC4GPndz92oxEhNMYr2K0IdxYQmf5upzvf857q0skLzUzhp3EcyrfX9Co588RpeVDBOW76BYtrdR5NtIAuPgpOkXG8ali6yLsimOxaMbey23KwtfTB_yOaALcLd4TcxhSNlDTGMbWIFxegd54EjubG_4mOQwp3Baj778fmaNowK1Aoh99QllgnDecAPXRsVUnR4gmLGc2OFQ6XJLEu8zJznNuUY6mU2lUqizXfOBiXeQq_YFv4dECFT57PAnHJCBsbzVITxxCkurQ_GZANQrQC1bdKNR9aLO10_hWY6Sl7XktcoeV1JXicDYE8dd3XGjee7XLYa0s0SLHU3YQaQtFrrqp8Z8vz_Q17Ay8g7Tys84CX09g8H_x69k30-hOPxfDGE_nRx-3U2bCYg_l3x6SMoUubP
linkProvider	ProQuest
linkToHtml	http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwtV1Lb9QwEB6VVgguiKe6UMAHOFrr2I7TPVSoQMuWlhVCrdSbcfyQFrrZpdkV9M_1t3WcOI3gQE9VJF_8kDIz9szY38wAvIlWQW5YoKYsSyoVbsWRzLdpyawyzBqDTURbTNT4RH4-zU_X4LKLhYmwyu5MbA5qN7fxjnwYqyq1ycbfLX7RWDUqvq52JTRMKq3gdpoUYymw49Bf_EYXrt45-Ij8fsv5_t7xhzFNVQaoFUIuqcssE4bzgB-qexVyNAKCYsZzY4XDH5FFkXlZOM9tztH9KWwulUQ96JwNSuC6d2BDCjlC52_j_d7k67frWx60v9EFkQlYhs7M0C9-LIY1eoaKUdSXEVopRjT7Wy32tu4_z7ON1tt_CA-SuUp2W_l6BGu-egx3G9iorZ9Atdu_f5N5IJ88MkqSejpLVcHItCKz_hoyjrHzeja19NxckNkKR4Sz1R9iKkfqFtIYx8QOOq0cyp0jpbE_Y_BJ5Z7Cya3Q9hmsV_PKbwIRMne-CMwpJ2RgvMxF2B45xaX1wZhiAKojoLYpvXmssnGm29BrpiPldUt5jZTXDeV1NgB2PXHRZvi4ecpWxyGdtnytewEdQNZxre--Ycnn_1_yNdwbH3850kcHk8MXcJ9H0FJEXeZbsL48X_mXaBkty1dJ_Ah8v22JvwI3hR9W
linkToPdf	http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV1LTwIxEG4IRuPF-Iwoag9eG8q224UjURAfIR4k4dZ0-0hQWAgLif57p_uA6EESs0kv7exhps18034zg9CtRwWhoo6oOI4JF3AU2zxskZhqoahWCgbPthiI_pA_jcJRBXXLXJiM7V4-SeY5Db5KU7JszI0ratvShp2_zxsphFeCEnA6np_I2gSCoB3uqyXAth4GnfVVC4BgiAN4we76Q_6nb9oAzl9vpJnr6R2igwIz4k5u5CNUsckx2s24mzo9QUln8wiNZw4_WNAWx-l4WrTmwuMETzd3gX6NnqXTsSYL9YWnK1jhJqtPrBKD05xX6Nf4CQIhOxjf4FjpD58BkphTNOx13-76pGijQDRjfElMU1OmgsDBB3hGuBBQjhNU2UBpZsBSPIqalkfGBjoMIL6LdMgFB0dvjHaCnaFqMkvsOcKMh8ZGjhphGHc0iEPmWm0jAq6tUyqqIVEqUOqixrhvdTGRef4zlV7zMte8BM3LTPOyWUN0LTjPy2xsF6mXFpLFuUul772Vl6SvoWZptc30ll9e_EPmBu293vfky-Pg-RLt-2b0JCMJ1lF1uVjZK4Asy_g625Dfo0fk7A
openUrl	ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Application+of+Geant4+simulation+in+measurement+of+cosmic-ray+muon+flux+and+studies+of+muon-induced+background&rft.jtitle=European+physical+journal+plus&rft.au=Jokovi%C4%87%2C+Dejan&rft.au=Maleti%C4%87%2C+Dimitrije&rft.au=Dragi%C4%87%2C+Aleksandar&rft.au=Veselinovi%C4%87%2C+Nikola&rft.date=2023-11-10&rft.pub=Springer+Nature+B.V&rft.eissn=2190-5444&rft.volume=138&rft.issue=11&rft.spage=1006&rft_id=info:doi/10.1140%2Fepjp%2Fs13360-023-04639-1
thumbnail_l	http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=2190-5444&client=summon
thumbnail_m	http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=2190-5444&client=summon
thumbnail_s	http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=2190-5444&client=summon