CMS: Gaseous Detectors R&DMuon System of the CMS Detector at the CERN LHChttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/cms_poster1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
CMS: Expedition into the high-energy frontierThe Compact Muon Solenoid (CMS) Large Hadron Collider (LHC), powerful particle accelerator located at CERN, Geneva.https://www.ugent.be/we/physics-astronomy/en/thesis/posters/cms_poster2.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
IceCube Neutrino Observatory : Particle Physics at South PoleThe IceCube Neutrino Observatory is neutrino detector, located at the geographic South Pole, close to the Amundsen-Scott South Pole Station.https://www.ugent.be/we/physics-astronomy/en/thesis/posters/icecube.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
3D radiative transfer with SKIRThttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/comp1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
BriX: Probing Nuclear properties of Imbalanced Fermi Systems with Quasi-free Proton Knock-out ReactionsWe are developing a reaction model for quasi-free AX(p,pN)A−1Y reactions with unstable nuclei.https://www.ugent.be/we/physics-astronomy/en/thesis/posters/brix1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
BriX: MODELING NEUTRINO-NUCLEUS SCATTERING FOR ACCELERATOR-BASED EXPERIMENTSFor accelerator-based experiments, we need an incoming neutrino beam. This is done e.g. at the Tevatron accelerator at Fermi- lab.https://www.ugent.be/we/physics-astronomy/en/thesis/posters/brix2.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
BriX: OPPORTUNITIES FOR A MASTER’S THESIS IN NEUTRINO PHYSICS!https://www.ugent.be/we/physics-astronomy/en/thesis/posters/brix3.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Can string theory cure heart rhythm disorders?https://www.ugent.be/we/physics-astronomy/en/thesis/posters/math_poster1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Network applications in economic systemshttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/labm_poster.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
The dark side of the galaxyhttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/astro_poster1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Deriving fog and visibility diagnostics from operational high-resolution numerical weather prediction model simulationsDeriving fog and visibility diagnostics from operational high-resolution numerical weather prediction model simulationshttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/fog.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Centre for X-ray Tomography: thesis subjectsPoster thesis subjectshttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/ugct-thesis-poster1.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Centre for X-ray Tomography: thesis subjectshttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/ugct-thesis-poster2.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg
Centre for X-ray Tomography: thesis subjectshttps://www.ugent.be/we/physics-astronomy/en/thesis/posters/ugct-thesis-poster3.pdf/viewhttps://www.ugent.be/++resource++plone-logo.svg