DC ElementWertSprache
dc.contributor.advisorKasieczka, Gregor-
dc.contributor.authorBuhmann, Erik-
dc.date.accessioned2025-03-07T11:41:28Z-
dc.date.available2025-03-07T11:41:28Z-
dc.date.issued2024-
dc.identifier.urihttps://ediss.sub.uni-hamburg.de/handle/ediss/11539-
dc.description.abstractThe search for physics beyond the Standard Model is a central goal of particle physics. This research is conducted at collider experiments and requires a very large amount of simulated data. With the high-luminosity upgrade to the Large Hadron Collider (HL-LHC) the need for more and faster simulations is increasing. The CMS detector upgrade for the HL-LHC will feature high-granularity endcap calorimeters and highly granular calorimeters are also envisioned to be used at future collider detectors. Together, these factors heighten the demand for more precise fast simulations. In this thesis, generative machine learning is explored as a tool for high fidelity fast simulations. Several models for the fast simulation of calorimeter showers and jets are presented. The bounded information bottleneck autoencoder (BIB-AE) model generates calorimeter showers as 3-dimensional images. Its encoded latent space is analyzed and it is shown that only few variables encode most shower information. This motivates an improvement of the BIB-AE using a kernel density estimator to model the latent space. The resulting model is able to simulate highly granular photon showers with high fidelity at 10x faster than the traditional Monte Carlo simulation Geant4 on the same CPU hardware. To advance calorimeter shower generative models in terms of computational efficiency, the diffusion model CaloClouds, which models calorimeter shower as point clouds, is introduced. The representation as point clouds has several advantages over 3D images, including being more efficient and allowing for a geometry independent shower modeling. The CaloClouds II model improves the approach by applying continuous-time score matching to achieve a higher fidelity and faster generation. The model is further distilled into the consistency model CaloClouds II (CM) which not only greatly accelerates the model, it also increases the fidelity further. CaloClouds II (CM) is 46x faster than Geant4 on the same hardware. Finally, the equivariant point cloud (EPiC) layer structure is introduced to further improve point cloud generative models used in particle physics. The layer is utilized in three different point cloud generative models: in the generative adversarial network EPiC-GAN, in the score-based diffusion model EPiC-JeDi, and in the continuous normalizing flow EPiC-FM, trained with the flow matching objective. The models are evaluated on the common JetNet benchmark dataset for the generation of particle jets. The EPiC-GAN is the most efficient model being about 210x faster than the other two models and still reaches the performance of the more complex previous state-of-the art graph-based MP-GAN. However, EPiC-FM is the most accurate among all compared models. This underscores the flow matching approach and the EPiC layer structure as promising directions for future generative model for fast simulations in particle physics.en
dc.language.isoende_DE
dc.publisherStaats- und Universitätsbibliothek Hamburg Carl von Ossietzkyde
dc.rightshttp://purl.org/coar/access_right/c_abf2de_DE
dc.subjectParticle Physicsen
dc.subjectGenerative Machine Learningen
dc.subjectCalorimeter Simulationsen
dc.subjectJet Physicsen
dc.subjectNeural Networksen
dc.subject.ddc530: Physikde_DE
dc.titleGenerative Machine Learning for Fast Particle Physics Simulationsen
dc.typedoctoralThesisen
dcterms.dateAccepted2025-01-29-
dc.rights.cchttps://creativecommons.org/licenses/by/4.0/de_DE
dc.rights.rshttp://rightsstatements.org/vocab/InC/1.0/-
dc.subject.bcl33.56: Elementarteilchenphysikde_DE
dc.subject.gndElementarteilchenphysikde_DE
dc.subject.gndKünstliche Intelligenzde_DE
dc.type.casraiDissertation-
dc.type.dinidoctoralThesis-
dc.type.driverdoctoralThesis-
dc.type.statusinfo:eu-repo/semantics/publishedVersionde_DE
dc.type.thesisdoctoralThesisde_DE
tuhh.type.opusDissertation-
thesis.grantor.departmentPhysikde_DE
thesis.grantor.placeHamburg-
thesis.grantor.universityOrInstitutionUniversität Hamburgde_DE
dcterms.DCMITypeText-
dc.identifier.urnurn:nbn:de:gbv:18-ediss-126428-
item.creatorOrcidBuhmann, Erik-
item.creatorGNDBuhmann, Erik-
item.languageiso639-1other-
item.fulltextWith Fulltext-
item.advisorGNDKasieczka, Gregor-
item.grantfulltextopen-
Enthalten in den Sammlungen:Elektronische Dissertationen und Habilitationen
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