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Dissertation
Recherche de la composante d'émission X non-thermique d'un échantillon d'étoiles massives
Authors: ---
Year: 2001 Publisher: [S.l.]: [chez l'auteur],

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Dissertation
A multiwavelength observational study of the non-thermal emission from O-type stars
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Year: 2006 Publisher: [S.l.] : [chez l'auteur],

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Dissertation
Les systèmes binaires massifs accélérant des particules : perspectives pour de futures observations
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Year: 2013 Publisher: [S.l.] : [chez l'auteur],

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Dissertation
L'émission X de la binaire massive à collision de vents V444 Cyg
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Year: 2010 Publisher: [S.l.] : [chez l'auteur],

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Dissertation
Immobilisation des ions uranyles par des composites polypyrrole/polymères complexants

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Dissertation
Impact of unitarization schemes on high-energy cosmic rays
Authors: --- --- --- --- --- et al.
Year: 2016 Publisher: Liège Université de Liège (ULiège)

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The hadronic event generators SIBYLL, QGSJET and EPOS use an Eikonal unitarization scheme. We focus on SIBYLL and present the general theoretical concepts behind this event generator and concentrate on diffraction. After a presentation of Regge theory, we present different unitarization schemes. We show the equivalence between the Good-Walker models used in SIBYLL and the GLM model. We test the U-matrix scheme. We show that U matrix fits very well the total, the elastic, the inelastic and the single diffractive cross sections with soft interactions. We show the asymptotic behaviour of the different cross sections.


Dissertation
Investigation of non-thermal processes in supernova remnants with emphasis on synchrotron radio emission
Authors: --- --- --- --- --- et al.
Year: 2019 Publisher: Liège Université de Liège (ULiège)

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This master thesis is focused on the non-thermal emission of supernova remnants, and especially on their synchrotron radio emission. Several physical parameters of a carefully selected sample of supernova remnants are determined through a dedicated method and discussed. Subsequently, this same method is applied after a data processing in the radio domain for two supplementary ones, with physical parameters extracted thanks to the obtained radio image. Finally, one of them is analyzed in the high-energy domain, to see if non-thermal processes and especially synchrotron radiation extends up to this range of energies.


Dissertation
Etude des modèles de 4ème génération d'étoiles sous-naines chaudes et application au pulsateur PG 1336-018
Authors: --- --- --- --- --- et al.
Year: 2019 Publisher: Liège Université de Liège (ULiège)

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Nous avons étudié de façon théorique, à l'aide des modèles sismiques de troisième et quatrième génération propres aux étoiles sous-naines de type B, l'impact du changement successif d'un des paramètres structurels de ces modèles sur le spectre de pulsation des modes de pression et de gravité. Ensuite, nous avons procédé à une modélisation sismique de la sdB du système PG 1336-018 en premier lieu, pour contraindre les paramètres des modèles 3G et ensuite ceux des modèles 4G.


Dissertation
Neutrino physics and the puzzle of ANITA
Authors: --- --- --- ---
Year: 2019 Publisher: Liège Université de Liège (ULiège)

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This master thesis offers an introduction to the peculiarities of neutrino physics, presents the principles behind the methods for neutrino detection and some experiments focusing on (ultra-)high energy neutrinos. It then discusses the anomalous events detected by the ANITA experiment.


Dissertation
Scalar Dark Matter Interpretation of the Positron Flux Anomaly
Authors: --- --- --- ---
Year: 2020 Publisher: Liège Université de Liège (ULiège)

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AMS-02 is an astrophysical experiment embarked on the International Space Station since 2011, designed to measure the fluxes of cosmic rays arriving at the Earth. AMS-02 has detected a significant excess in the positron flux at Earth that is inconsistent with the production of positrons in collisions of cosmic rays in the Galaxy. This thesis addresses the viability of a scalar two-component dark matter in the context of the AMS-02 measurements of positrons and antiprotons. Astrophysical alternatives to dark matter are briefly discusses, namely pulsars.

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