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Rozprawy doktorskie na temat „Atmospheric muon”

Autor: Grafiati

Data publikacji: 7 grudnia 2024

Data aktualizacji: 31 lipca 2025

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1

Bazzotti, Marco <1980&gt. "Studies of the atmospheric muon flux with the ANTARES detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1906/1/bazzotti_marco_tesi.pdf.

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The thesis main topic is the determination of the vertical component of the atmospheric muon flux as a function of the sea depth at the ANTARES site. ANTARES is a Cherenkov neutrino telescope placed at 2500m depth in the Mediterranean Sea at 40 km from the southern cost of France. In order to retrieve back the physical flux from the experimental data a deconvolution algorithm has been perform which takes into consideration the trigger inefficiensies and the reconstruction errors on the zenith angle. The obtained results are in good agreement with other ANTARES indipendent analysis.

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Bazzotti, Marco <1980&gt. "Studies of the atmospheric muon flux with the ANTARES detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1906/.

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The thesis main topic is the determination of the vertical component of the atmospheric muon flux as a function of the sea depth at the ANTARES site. ANTARES is a Cherenkov neutrino telescope placed at 2500m depth in the Mediterranean Sea at 40 km from the southern cost of France. In order to retrieve back the physical flux from the experimental data a deconvolution algorithm has been perform which takes into consideration the trigger inefficiensies and the reconstruction errors on the zenith angle. The obtained results are in good agreement with other ANTARES indipendent analysis.

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Pretz, John. "Detection of atmospheric muon neutrinos with the IceCube 9-String Detector." College Park, Md. : University of Maryland, 2006. http://hdl.handle.net/1903/4163.

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Thesis (Ph. D.) -- University of Maryland, College Park, 2006.<br>Thesis research directed by: Physics. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.

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Mauri, Nicoletta <1980&gt. "Measurement of the atmospheric muon charge ratio with the OPERA detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3932/1/Mauri_Nicoletta_Tesi.pdf.

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The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an interesting quantity for the study of high energy hadronic interactions in atmosphere and the nature of the primary cosmic rays. The measurement of the charge ratio in the TeV muon energy range allows to study the hadronic interactions in kinematic regions not yet explored at accelerators. The OPERA experiment is a hybrid electronic detector/emulsion apparatus, located in the underground Gran Sasso Laboratory, at an average depth of 3800 meters water equivalent (m.w.e.). OPERA is the first

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Mauri, Nicoletta <1980&gt. "Measurement of the atmospheric muon charge ratio with the OPERA detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3932/.

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The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an interesting quantity for the study of high energy hadronic interactions in atmosphere and the nature of the primary cosmic rays. The measurement of the charge ratio in the TeV muon energy range allows to study the hadronic interactions in kinematic regions not yet explored at accelerators. The OPERA experiment is a hybrid electronic detector/emulsion apparatus, located in the underground Gran Sasso Laboratory, at an average depth of 3800 meters water equivalent (m.w.e.). OPERA is the first

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6

Bailly-Salins, Louis. "Atmοspheric muοn studies and light sterile neutrinο search with ΚΜ3ΝeΤ/ΟRCA". Electronic Thesis or Diss., Normandie, 2024. http://www.theses.fr/2024NORMC228.

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La collaboration KM3NeT construit actuellement deux télescopes Cherenkov à neutrinos au fond de la mer Méditerranée, ORCA (Oscillation Research with Cosmics in the Abyss) pour mesurer les oscillations des neutrinos atmosphériques et ARCA (Astroparticle Research with Cosmics in the Abyss) pour détecter les neutrinos provenant de sources astrophysiques.Dans ce manuscrit, après avoir passé en revue l'état des mesures d'oscillation des neutrinos et des recherches de neutrinos stériles légers dans le premier chapitre, les détecteurs KM3NeT sont présentés dans le deuxième chapitre.Dans le chapitre 3

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7

Versari, Federico <1992&gt. "Measurement of the atmospheric electron and muon neutrino flux with the ANTARES neutrino telescope." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amsdottorato.unibo.it/9664/1/PhD_Thesis____.pdf.

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This thesis presents a combined measurement of the energy spectra of atmospheric electron and muon neutrinos in the energy range between around 100 GeV and 50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period from 2007 to 2017, and selects 1016 neutrino interacting in (or close to) the instrumented volume of the detector, yielding shower-like events and starting track events. The contamination by atmospheric muons is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree cla

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8

Haberland, Marcus. "A search for a prompt atmospheric muon neutrino flux in the northern hemisphere using data releases from IceCube." Thesis, Uppsala universitet, Högenergifysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-415984.

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The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above hundreds of GeV produced in Earth’s atmosphere as well as outside our solar system whenever particles are accelerated to ultra-relativistic energies. The prompt atmospheric contribution is a result of the creation of heavy mesons with charm components in the atmosphere. Past studies from IceCube using a maximum likelihood estimation over the whole neutrino energy spectrum always reported a best-fit zero prompt contribution so far [1–5], contrary to theory [6, 7]. In this analysis we tried to me

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9

Biron, von Curland Alexander. "Search for atmospheric muon neutrinos and extraterrestric neutrino point sources in the 1997 AMANDA-B10 data." [S.l.] : [s.n.], 2002. http://deposit.ddb.de/cgi-bin/dokserv?idn=964841223.

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10

Geyer, Klaus [Verfasser], and Gisela [Akademischer Betreuer] Anton. "Measurements of the atmospheric muon rate with the ANTARES neutrino telescope / Klaus Geyer. Gutachter: Gisela Anton." Erlangen : Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), 2015. http://d-nb.info/1076165915/34.

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11

Curland, Alexander Biron von. "Search for atmospheric muon-neutrinos and extraterrestric neutrino point sources in the 1997 AMANDA-B10 data." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2002. http://dx.doi.org/10.18452/14743.

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Deutsche Zusammenfassung Die vorliegende Dissertation beschäftigt sich einerseits mit der Suche nach atmosphärischen Myonneutrinos und andererseits mit der Suche nach extraterrestrischen Neutrinopunktquellen in dem Datensatz, welcher im Jahre 1997 durch den AMANDA-Detektor aufgenommenen wurde. In dieser Arbeit wird zunächst die kosmische Strahlung eingeführt. Die Suche nach den Quellen dieser Strahlung wurde bisher insbesondere mit Hilfe der geladenen kosmischen Strahlung selber, sowie mit Hilfe von Cherenkovteleskopen für Gammastrahlen durchgeführt. Die mit diesen Techniken ge

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12

Garza, Juan Pablo Yáñez. "Measurement of neutrino oscillations in atmospheric neutrinos with the IceCube DeepCore detector." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2014. http://dx.doi.org/10.18452/17016.

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Neutrinooszillationen sind ein sehr aktives Forschungsfeld. In den letzten Jahrzehnten haben viele Experimente das Phänomen untersucht und sind inzwischen zu Präazisionsmessungen vorangeschritten. Mit seiner Niederenergieerweiterung DeepCore kann das IceCube-Experiment zu diesem Forschungsfeld beitragen. IceCube ist ein 1 km^3 großes Tscherenkow-Neutrino-Teleskop, welches das tiefe, antarktische Eis des Südpols als optisches Medium nutzt. DeepCore ist eine Erweiterung mit dichterer Instrumentierung im unteren Teil des IceCube-Teleskops. Diese dichte Instrumentierung ermöglicht den Nachweis

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13

Jeschke, Dominik [Verfasser], Lothar [Akademischer Betreuer] Oberauer, Robert [Gutachter] Svoboda, Lothar [Gutachter] Oberauer, and Elisa [Gutachter] Resconi. "Modulations of the Cosmic Muon Flux & Identification of Atmospheric Neutrino Interactions in Borexino / Dominik Jeschke ; Gutachter: Robert Svoboda, Lothar Oberauer, Elisa Resconi ; Betreuer: Lothar Oberauer." München : Universitätsbibliothek der TU München, 2018. http://d-nb.info/1168798582/34.

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14

Jeschke, Dominik Verfasser], Lothar [Akademischer Betreuer] [Oberauer, Robert [Gutachter] Svoboda, Lothar [Gutachter] Oberauer, and Elisa [Gutachter] Resconi. "Modulations of the Cosmic Muon Flux & Identification of Atmospheric Neutrino Interactions in Borexino / Dominik Jeschke ; Gutachter: Robert Svoboda, Lothar Oberauer, Elisa Resconi ; Betreuer: Lothar Oberauer." München : Universitätsbibliothek der TU München, 2018. http://nbn-resolving.de/urn:nbn:de:bvb:91-diss-20180920-1440369-1-2.

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15

Ruhe, Tim [Verfasser], Wolfgang [Akademischer Betreuer] Rhode, and Claus [Gutachter] Gößling. "Data mining on the rocks : A measurement of the atmospheric muon neutrino flux using IceCube in the 59-string configuration and a novel data mining based approach to unfolding / Tim Ruhe. Betreuer: Wolfgang Rhode. Gutachter: Claus Gößling." Dortmund : Universitätsbibliothek Dortmund, 2013. http://d-nb.info/1106257421/34.

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16

Vernet, Kinson. "Imagerie densitométrique 3D des volcans par muographie." Electronic Thesis or Diss., Université Clermont Auvergne (2021-...), 2022. http://www.theses.fr/2022UCFAC112.

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La muographie est une technique d’imagerie en physique des particules où les muons atmosphériques traversant une cible sont utilisés pour déterminer des informations de l’intérieur de la cible : distribution de la densité ou composition chimique via le numéro atomique. En fonction de l’énergie des muons et de la quantité de matière à traverser, il y en a qui vont survivre et d’autres qui vont être arrêtés par la cible. Et, la diffusion des muons dépend, en première approximation, de leur impulsion et du numéro atomique moyen le long de leur parcours de vol. La muographie propose, à partir de l

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17

Idrissi, Ibnsalih Walid. "Selection of showering events and background suppression in ANTARES: comparison between the effects using two different Monte Carlo version." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amslaurea.unibo.it/18132/.

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Al momento ANTARES è il più grande telescopio di neutrini sottomarino ed è situato nel Mar Meditteraneo, circa 40 km a largo di Tolone, Francia, ad una profondità di 2450 m in fondo al mare. Lo scopo principale di ANTARES è quello di poter osservare neutrini di alta energia riconducibili a sorgenti astrofisiche. Un fondo irriducibile del rivelatore è rappresentato dai muoni atmosferici, prodotti dalle interazioni dei raggi cosmici con i nuclei dell’atmosfera. La collaborazione ANTARES fa largo uso di simulazioni Monte Carlo e recentemente è stata rilasciata una nuova versione della simulazi

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18

Béné, Samuel. "Imagerie tomograpbique d'un volcan à l'aide des muons atmosphériques." Thesis, Clermont-Ferrand 2, 2016. http://www.theses.fr/2016CLF22786/document.

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Les muons atmosphériques sont des particules élémentaires créées lors de l’interaction des rayons cosmiques de haute énergie avec les atomes de la haute atmosphère. Leur capacité à traverser de grandes quantités de matière et leur abondance au niveau du sol permet d’utiliser leur flux comme support à la radiographie de grands objets. Cette technique, la muographie, possède notamment comme sujet d’application possible l’étude de volcans. La collaboration Tomuvol, au sein de laquelle cette thèse s’est déroulée, vise à mettre au point un détecteur et les techniques d’analyse permettant la réalisa

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19

Bos, Fabian [Verfasser], Julia [Gutachter] Tjus, and Wolfgang [Gutachter] Rhode. "Studying moon and sun shadows by using atmospheric muons detected with IceCube / Fabian Bos ; Gutachter: Julia Tjus, Wolfgang Rhode." Bochum : Ruhr-Universität Bochum, 2017. http://d-nb.info/112945181X/34.

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20

Biron, von Curland Alexander [Verfasser]. "Search for atmospheric muon neutrinos and extraterrestric neutrino point sources in the 1997 AMANDA-B10 data / von Alexander Prinz Biron von Curland." 2002. http://d-nb.info/964841223/34.

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21

Ganugapati, Raghunath. "Measurements of atmospheric muons using AMANDA with emphasis on the prompt component." 2008. http://www.library.wisc.edu/databases/connect/dissertations.html.

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22

Hsiang, Hua-Chun, and 向化君. "To study the possibility of using a particle detector array to detect atmospheric muons from near horizon." Thesis, 2006. http://ndltd.ncl.edu.tw/handle/jpr6d9.

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碩士<br>國立中央大學<br>太空科學研究所<br>94<br>The goal of this project is to build a particle detector array and to study the possibility of using this array to detect atmospheric muons from near horizon. First, we assembled the detectors, and then measured some basic specifications of those 4 detectors. We then design and construct a detector array. By using this detector array, we measured horizontal muons for 80 hours. Data collected during this experiment were then analyzed. Two types of events are presented, one is near horizontal direction (86.2�a < �� < 93.8�a, �� is zenith angle) ; the other types

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23

Ebr, Jan. "Fenomenologicé modely inspirované QCD a jejich využití v analýze kosmického záření při ultravysokých energiích." Doctoral thesis, 2017. http://www.nusl.cz/ntk/nusl-367703.

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Cosmic rays of energies above 1014 eV are detected mostly indirectly, by observing the extensive air showers they create in the atmosphere. Multiple experiments suggest that the current models of high-energy interactions do not describe the cosmic ray data perfectly, in particular when it comes to the prediction for the number of muons at ground. We present two models aiming to improve the description of the muon component, one based on the addition of particles with small momenta in the local center-of-mass frame of the high-energy hadronic interactions in the shower, the other on the additio

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