Programm für das Wintersemester 2025/2026
Wednesdays, 13:00 Uhr s.t.
Institut für Physik
Lorentz-Raum, 05-127, Staudingerweg 7
| 29.10.25 | Prof. Dr. Andreas Weiler, TU Munich | |
Neutron stars and white dwarfs do not just produce axions—they change how axions behave. At high baryon density, the axion potential shifts and nucleon properties are modified, which can alter compact-star structure and amplify axion–nucleon interactions. That means more axion emission in supernovae and stronger, model-independent bounds. I will also outline a simple in-medium axion EFT that exposes a previously missed tree-level production channel, further sharpening supernova constraints, and will connect these ideas to current searches across the stellar graveyard. | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 05.11.25 | Prof. Dr. Seshadri Nadathur, University of Portsmouth, UK | |
More than 25 years after the discovery of the accelerated expansion of the Universe, understanding dark energy remains the biggest open problem in cosmology. The Dark Energy Spectroscopic Instrument (DESI) is the first of a new generation of “Stage-IV” cosmology survey experiments aiming to improve this understanding. By precisely mapping the positions of over 50 million galaxies and quasars, DESI is measuring the expansion history of the Universe over the last 11 billion years. I will describe the experiment and discuss the cosmological results from the first 3 years of data, from baryon acoustic oscillations (BAO) and the full shape of the clustering power spectrum. These include exciting hints of an anomaly in the cosmological constant model of dark energy, and unprecedented constraints on the neutrino mass scale. I will describe the nature of the data constraints and comment on the implications for fundamental physics models. | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 12.11.25 | Prof. Dr. Andrea Knue, University Dortmund | |
The top quark is the heaviest elementary particle known to date. With this very large mass come interesting consequences, like its extremely short lifetime. Unlike other quarks, which can form bound states, the top quarks lifetime does not allow for a stable bond. If two top quarks are produced almost at rest however, they can briefly exchange gluons before they then decay individually. This pseudo-bound state was already predicted in 1987, before the top quark was even discovered. It was thought to be impossible to measure this state at the LHC, as it constitutes less than 1% of the total production rate and is difficult to see in the data. With improved analysis techniques and theoretical predictions however, the CMS and ATLAS experiments have recently observed an excess of data close to the production threshold. This presentation will discuss these new measurements and shed some light on the fleeting connection between the two top quarks. | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 19.11.25 | Prof. Dr. Maria Bergemann, University Heidelberg | |
One of the prime questions in modern astrophysics is the origin and evolution of chemical elements. Why is the chemical composition so vastly (as of today, ~8 orders of magnitude) different for various astronomical objects, such as the Sun, Galactic stars and their planetary companions? How can one explore the full history of the evolution of elements, from the Big Bang to the present?
I will review recent progress in studying the chemical enrichment of the Milky Way galaxy. I will focus on advances in determining solar and stellar chemical composition, driven by new observations and new theoretical models. These models rely on the physics of non-local thermodynamic equilibrium (NLTE) and 3D radiation-hydrodynamics simulations of stellar convection.
I will touch upon the key science topics:
- how 3D NLTE solar abundances have advanced our understanding of the structure of the Sun and its neutrino fluxes,
- how evidence for non-standard supernova Ia explosions has emerged from 3D NLTE abundances of iron-group elements,
- how constraints on the properties of neutron star mergers can be obtained from observations of the heavy neutron-capture elements in stellar spectra.
I will conclude with a brief summary of the prospects for studies of stars using 3D NLTE modelling and next-generation large astronomical surveys.
Slides: https://keeper.mpdl.mpg.de/f/290a8b617dae47218bf8/ | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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zukünftige Termine
| 26.11.25 | Prof. Dr. Enrique Rico Ortega, CERN, Switzerland | |
Understanding the confinement mechanism in gauge theories and the universality of effective string-like descriptions of gauge flux tubes remains a fundamental challenge in modern physics. We probe string modes of motion with dynamical matter in a digital quantum simulation of a (2+1) dimensional gauge theory using a superconducting quantum processor with up to 144 qubits, stretching the hardware capabilities with quantum-circuit depths comprising up to 192 two-qubit layers. We realize the Z_2-Higgs model (Z_2HM) through an optimized embedding into a heavy-hex superconducting qubit architecture, directly mapping matter and gauge fields to vertex and link superconducting qubits, respectively. Using the structure of local gauge symmetries, we implement a comprehensive suite of error suppression, mitigation, and correction strategies to enable real-time observation and manipulation of electric strings connecting dynamical charges. Our results resolve a dynamical hierarchy of longitudinal oscillations and transverse bending at the end points of the string, which are precursors to hadronization and rotational spectra of mesons. We further explore multi-string processes, observing the fragmentation and recombination of strings. The experimental design supports 300,000 measurement shots per circuit, totaling 600,000 shots per time step, enabling high-fidelity statistics. We employ extensive tensor network simulations using the basis update and Galerkin method to predict large-scale real-time dynamics and validate our error-aware protocols. This work establishes a milestone for probing non-perturbative gauge dynamics via superconducting quantum simulation and elucidates the real-time behavior of confining strings.
Ref: CERN-TH-2025-111
[arXiv:2507.08088] | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 03.12.25 | Prof. Dr. Ruth Pöttgen, Lund University, Sweden | |
The Light Dark Matter eXperiment - a new window into the dark Universe | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 10.12.25 | Prof. Dr. Laura Munteanu, CERN, Geneva, Switzerland | |
Prospects of nuSCOPE | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 17.12.25 | Prof. Dr. Martin Hirsch, University Valencia, Spain | |
Long-lived particles (LLPs) have attracted considerable attention in the past few years, in particular because several new "far"
detectors have been proposed at the LHC. In this talk, I will discuss heavy neutral leptons (a.k.a. right-handed neutrinos).
Due to their connection to neutrino mass generation HNLs are well-motivated LLPs. After introducing minimal HNLs and studying prospects for discovery at the LHC, I will turn to HNLs in effective field theory (EFT). EFTs are well suited to study non-minimal extension of the SM in the absence of new resonances at the LHC.
The effects of non-renormalizable operators on prospects for HNLs discovery will be presented in some detail. | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 07.01.26 | Dr. Melissa Mendes, TU Darmstadt | |
New Constraints on the Neutron Star Equation of State | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 14.01.26 | Prof. Dr. Florian Hug, JGU Mainz | |
Improving energy efficiency of MESA by superconducting cavities | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 21.01.26 | Prof. Dr. Belen Galeva, UAM, Spain | |
Higgs Criticality And The Metastability Bound | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 28.01.26 | Prof. Dr. Graham Kribs, University of Oregon, USA | |
Strongly-Coupled Dark Sectors For Dark Matter, Colliders, and Cosmology | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 04.02.26 | Prof. Dr. Clarence Wret, Imperial College London, UK | |
Indications of CP violation and mass ordering via the first T2K and SK joint oscillation analysis using beam and atmospheric neutrinos | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| 11.02.26 | Prof. Dr. Johannes Albrecht, University Dortmund | |
Prospects of the LHCb Experiment | ||
| 13:00 Uhr s.t., Lorentz-Raum, 05-127, Staudingerweg 7 | ||
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| Koordination: | Kontakt: |
Prof. Dr. Tobias Hurth | Ellen Lugert |