A three-dimensional code for muon propagation through the rock: MUSIC
Identifieur interne : 000B44 ( Main/Exploration ); précédent : 000B43; suivant : 000B45A three-dimensional code for muon propagation through the rock: MUSIC
Auteurs : P. Antonioli [Italie] ; C. Ghetti [Italie] ; E. V. Korolkova [Russie] ; V. A. Kudryavtsev [Russie] ; G. Sartorelli [Italie]Source :
- Astroparticle Physics [ 0927-6505 ] ; 1997.
English descriptors
- Teeft :
- Angular deflection, Angular deviation, Angular deviations, Angular distributions, Antonioli, Basic assumptions, Bremsstrahlung, Continuous energy loss, Continuous process, Crosssection, Deflection, Deflection angle, Different depths, Different muon bremsstrahlung, Electron production, Energy loss, Energy losses, Experimental data, Inelastic, Initial energy, Iron nuclei, Lateral, Lateral displacement, Lateral distributions, Moliere theory, Multiple coulomb, Muon, Muon bremsstrahlung, Muon bundles, Muon energies, Muon energy, Muon flux, Muon intensities, Muon interaction, Muon multiplicity, Muon multiplicity distribution, Muon multiplicity distributions, Muon propagation, Muon transport, Other processes, Pair production, Pair production process, Power index, Power spectrum, Primary spectrum, Relative difference, Significant difference, Simulation, Single muons, Solid line, Standard rock, Stochastic, Stochastic processes, Survival probabilities, Ucut.
Abstract
Abstract: We present a new three-dimensional Monte-Carlo code MUSIC (MUon SImulation Code) for muon propagation through the rock. All processes of muon interaction with matter with high energy loss (including the knock-on electron production) are treated as stochastic processes. The angular deviation and lateral displacement of muons due to multiple scattering, as well as bremsstrahlung, pair production and inelastic scattering are taken into account. The code has been applied to obtain the energy distribution and angular and lateral deviations of single muons at different depths underground. The muon multiplicity distributions obtained with MUSIC and CORSIKA (Extensive Air Shower simulation code) are also presented. We discuss the systematic uncertainties of the results due to different muon bremsstrahlung cross-sections.
Url:
DOI: 10.1016/S0927-6505(97)00035-2
Affiliations:
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Korolkova</name><affiliation wicri:level="3"><country xml:lang="fr">Russie</country><wicri:regionArea>Institute for Nuclear Research of the Russian Academy of Science, Moscow</wicri:regionArea><placeName><settlement type="city">Moscou</settlement><region>District fédéral central</region></placeName></affiliation></author><author><name sortKey="Kudryavtsev, V A" sort="Kudryavtsev, V A" uniqKey="Kudryavtsev V" first="V. A." last="Kudryavtsev">V. A. Kudryavtsev</name><affiliation wicri:level="3"><country xml:lang="fr">Russie</country><wicri:regionArea>Institute for Nuclear Research of the Russian Academy of Science, Moscow</wicri:regionArea><placeName><settlement type="city">Moscou</settlement><region>District fédéral central</region></placeName></affiliation></author><author><name sortKey="Sartorelli, G" sort="Sartorelli, G" uniqKey="Sartorelli G" first="G." last="Sartorelli">G. Sartorelli</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>University of Bologna and INFN-Bologna, Bologna</wicri:regionArea><wicri:noRegion>Bologna</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Astroparticle Physics</title><title level="j" type="abbrev">ASTPHY</title><idno type="ISSN">0927-6505</idno><imprint><publisher>ELSEVIER</publisher><date type="published" when="1997">1997</date><biblScope unit="volume">7</biblScope><biblScope unit="issue">4</biblScope><biblScope unit="page" from="357">357</biblScope><biblScope unit="page" to="368">368</biblScope></imprint><idno type="ISSN">0927-6505</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0927-6505</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="Teeft" xml:lang="en"><term>Angular deflection</term><term>Angular deviation</term><term>Angular deviations</term><term>Angular distributions</term><term>Antonioli</term><term>Basic assumptions</term><term>Bremsstrahlung</term><term>Continuous energy loss</term><term>Continuous process</term><term>Crosssection</term><term>Deflection</term><term>Deflection angle</term><term>Different depths</term><term>Different muon bremsstrahlung</term><term>Electron production</term><term>Energy loss</term><term>Energy losses</term><term>Experimental data</term><term>Inelastic</term><term>Initial energy</term><term>Iron nuclei</term><term>Lateral</term><term>Lateral displacement</term><term>Lateral distributions</term><term>Moliere theory</term><term>Multiple coulomb</term><term>Muon</term><term>Muon bremsstrahlung</term><term>Muon bundles</term><term>Muon energies</term><term>Muon energy</term><term>Muon flux</term><term>Muon intensities</term><term>Muon interaction</term><term>Muon multiplicity</term><term>Muon multiplicity distribution</term><term>Muon multiplicity distributions</term><term>Muon propagation</term><term>Muon transport</term><term>Other processes</term><term>Pair production</term><term>Pair production process</term><term>Power index</term><term>Power spectrum</term><term>Primary spectrum</term><term>Relative difference</term><term>Significant difference</term><term>Simulation</term><term>Single muons</term><term>Solid line</term><term>Standard rock</term><term>Stochastic</term><term>Stochastic processes</term><term>Survival probabilities</term><term>Ucut</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Abstract: We present a new three-dimensional Monte-Carlo code MUSIC (MUon SImulation Code) for muon propagation through the rock. All processes of muon interaction with matter with high energy loss (including the knock-on electron production) are treated as stochastic processes. The angular deviation and lateral displacement of muons due to multiple scattering, as well as bremsstrahlung, pair production and inelastic scattering are taken into account. The code has been applied to obtain the energy distribution and angular and lateral deviations of single muons at different depths underground. The muon multiplicity distributions obtained with MUSIC and CORSIKA (Extensive Air Shower simulation code) are also presented. We discuss the systematic uncertainties of the results due to different muon bremsstrahlung cross-sections.</div></front></TEI><affiliations><list><country><li>Italie</li><li>Russie</li></country><region><li>District fédéral central</li></region><settlement><li>Moscou</li></settlement></list><tree><country name="Italie"><noRegion><name sortKey="Antonioli, P" sort="Antonioli, P" uniqKey="Antonioli P" first="P." last="Antonioli">P. Antonioli</name></noRegion><name sortKey="Antonioli, P" sort="Antonioli, P" uniqKey="Antonioli P" first="P." last="Antonioli">P. Antonioli</name><name sortKey="Ghetti, C" sort="Ghetti, C" uniqKey="Ghetti C" first="C." last="Ghetti">C. Ghetti</name><name sortKey="Sartorelli, G" sort="Sartorelli, G" uniqKey="Sartorelli G" first="G." last="Sartorelli">G. Sartorelli</name></country><country name="Russie"><region name="District fédéral central"><name sortKey="Korolkova, E V" sort="Korolkova, E V" uniqKey="Korolkova E" first="E. V." last="Korolkova">E. V. Korolkova</name></region><name sortKey="Kudryavtsev, V A" sort="Kudryavtsev, V A" uniqKey="Kudryavtsev V" first="V. A." last="Kudryavtsev">V. A. Kudryavtsev</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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