Internal Seminars WS 19/20
Tue 01.10.2019 14:00 (Glassbox MBP1)
Annika Reinert (Bonn University)
Dark photons and plasma effects
Mon 07.10.2019 10:00 (MBP1 015)
3 Master Thesis Presentations:
10:00: Jasmina Nasufi (RWTH)
Beam functions in transverse momentum factorisation
10:40: Marco Niggetiedt (RWTH)
Quark mass effects in Higgs boson processes
11:20: Marcel Wald (RWTH)
Top-quark pair production in electron-positron collisions
Tue 08.10.2019 10:15 (MBP1 026)
Master Thesis Presentation:
Markus Schmidt (RWTH)
The Fermi Bubbles within a Stochastic Differential Equation Approach
Wed 16.10.2019 11:00 (26C 402)
Master Thesis Presentation:
Lucius Bsuhnaq (RWTH)
Calculational methods in the Gradient Flow Formalism
Thu 17.10.2019 14:00 (26C 402)
Master Thesis Midterm Presentation:
Thorben Finke (RWTH)
Deep neural networks for new physics searches at the LHC
Thu 17.10.2019 14:45 (26C 402)
Master Thesis Presentation:
Fabian Esser (RWTH)
Effects of higher-dimensional operators to the Higgs sector in a split-SUSY model
Tue 29.10.2019 10:15 (MBP110)
Master Thesis Midterm Presentation:
Juliana Carrasco (RWTH)
Long-lived particles in strongly interacting dark sectors
Wed 30.10.2019 10:00 (26C 402)
Master Thesis Midterm Presentation:
Juliana Carrasco (RWTH)
Feynman Rules with massive and massless spinor-helicity variables
Tue 12.11.2019 11:00 (26C 402)
Master Thesis Presentation:
Pattara Angkinun (RWTH)
Reinterpretation of Supersymmetry Searches in a Simplified Flavor Violation Model
Thu 05.12.2019 10:00 (26C 401)
Master Thesis Midterm Presentation:
Jonas Rongen (RWTH)
Scalar QCD/QED in the gradient flow formalism
Wed 11.12.2019 11:00 (MBP1 026)
Master Thesis Presentation:
Marc Klinger (RWTH)
Blazar variability in the context of magnetic reconnection and the plasmoid instability
Tue 14.01.2020 9:15 (MBP1 026)
Master Thesis Midterm Presentation:
Parth Bhargava (RWTH)
Beyond the single-stream treatment of cosmological structure formation with the Schrödinger Method
Abstract:
The Schrödinger method (ScM) for large scale structure formation is a phase-space based description of collisionless Cold Dark Matter (CDM). It involves modelling the dynamics of dark matter with the Vlasov - Poisson equation. So far it has been only applied to CDM, i.e. with a single phase-space sheet where it is able to resolve the shell-crossing singularity. The topic of my mid-term talk is to discuss how one can also model cosmological initial conditions with a finite velocity dispersion within ScM. I shall motivate the necessary theory and show some results with warm initial conditions which can be used to model Warm Dark Matter (WDM) and neutrinos.