Physikalisches Kolloquium

Programm für das Sommersemester 2025

Tuesdays, 16:15 Uhr s.t.

Institut für Physik

HS KPH
15.04.25Andrew Webb, Leiden University Medical Centre, NL
Magnetic resonance imaging is an inherently non-invasive technique with biological applications from the cellular to human size-scales. A major technological push has been towards stronger magnetic fields, which can be >20 Tesla for preclinical studies and >10 Tesla for humans, since these increase the signal strength and ultimate imaging resolution. Such systems, however, require advances in hardware design, acquisition sequences and image processing algorithms to achieve optimal performance. The first part of this talk will concentrate on technical challenges and practical approaches for human scanning at 7 Tesla and above. The challenges include B_1 and B_0 inhomogeneities, increased specific absorption rate, and high sensitivity to movement. Neurological and neuroscience applications discussed include ocular and neurological tumours, epilepsy, neuromuscular diseases, glymphatic clearance and mechanistic studies of lithium for bipolar disorders. The second part will discuss the opposite end of the MRI spectrum, ultra-low field systems at ~50 mT which have been designed to address the challenges of global healthcare accessibility. The challenges here are diametrically opposite to those at high field, and topics of system design, characterization and in vivo applications will be highlighted.
16:15 Uhr s.t., HS KPH

zukünftige Termine
29.04.25Frauke Gräter, Max Planck Institute for Polymer Research
Life is physics and chemistry in action. While molecular simulations of systems as complex as whole cells are now within reach, predicting chemical reactivity on relevant time and length scales remains a challenge. I will present our recent work towards bringing action – here: chemistry – to classical simulations and molecular design through machine learning. Among others, we substitute costly quantum mechanical calculations with a graph neural network-based emulator. Our framework can deal with the plethora of life’s chemistry amidst the ‘jiggling and wiggling’ of biomolecules. Importantly, we also uncover unexpected biomolecular processes that we in turn put to test in experiments. Finally, I will demonstrate how we harness a flow-matching model to predict biomolecular dynamics. Our method paves the way for generating novel flexible and functional proteins.
16:15 Uhr s.t., HS KPH

06.05.25Yafang Cheng, Max Planck Institute for Chemistry
Aerosol chemistry: from molecular dynamics to atmospheric vortices
16:15 Uhr s.t., HS KPH

13.05.25Anna Balazs, University of Pittsburgh, USA
Harnessing Chemo-Mechanical Interactions To Regulate Behavior Of Flexible Materials In Confined Fluids
16:15 Uhr s.t., HS KPH

20.05.25Libor Smejkal, JGU Mainz, INSPIRE Group
tba
16:15 Uhr s.t., HS KPH

27.05.25Subir Sarkar, University of Oxford
In the ΛCDM cosmological model the Universe is assumed to be isotropic and homogeneous when averaged on large scales. That the Cosmic Microwave Background has a dipole anisotropy is interpreted as due to our peculiar (non-Hubble) motion because of local inhomogeneity. There must then be a corresponding dipole in the sky distribution of sources at high redshift. Using catalogues of radio sources and quasars we find that this expectation is rejected at >5σ, i.e. the distribution of distant matter is not isotropic in the 'CMB frame’. This calls into question the standard practice of boosting to this frame to analyse cosmological data, in particular to infer acceleration of the Hubble expansion rate using Type Ia supernovae, which is then interpreted as due to a Cosmological Constant Λ. We find that the inferred acceleration is anisotropic (in the direction of the CMB hotspot) and likely illusory because of our being embedded in a coherent bulk flow, rather than due to dark energy.
16:15 Uhr s.t., HS KPH

03.06.25Christian Weinheimer, Universität Münster
tba
16:15 Uhr s.t., HS KPH

10.06.25Günter Reiss, Universität Bielefeld
Magnetic Heterostructures: From Sensors and Memories to Altermagnets
16:15 Uhr s.t., HS KPH

17.06.25Serge Haroche, Laboratoire Kastler Brossel, Collège de France
TBA
16:15 Uhr s.t., Staudinger Hörsaal

24.06.25Nir Barnea, The Hebrew University of Jerusalem
Behaviour of Correlated Nucleon Pairs Inside Nuclei
16:15 Uhr s.t., HS KPH

01.07.25Dennis Lehmkuhl, Universität Bonn
Philosophy of Physics
16:15 Uhr s.t., HS KPH

08.07.25Volker Springel, Max Planck-Institut für Astrophysik, Garching
Numerical calculations of cosmic structure formation have become a powerful tool in astrophysics. Starting right after the Big Bang, they are not only able to accurately predict the dark matter backbone of the cosmic web far into the non-linear regime, but are also capable of following baryonic physics with rapidly improving fidelity. In my talk, I will review the methodology and selected results of recent structure formation simulations that follow large parts of the observable universe. I will discuss some of the primary challenges in modelling strong, scale-dependent feedback processes that regulate star formation in galaxies, and highlight the important role played by supermassive black holes in galaxy formation. I will also discuss extremely large simulations and describe how they help to make reliable predictions for the impact of baryons and massive neutrinos on cosmological observables, effects that need to be understood to make full use of upcoming new survey data. The simulation results also shed light on cosmic reionization and magnetic field amplification during non-linear structure formation. Finally, I will highlight some of the methodological and technical challenges involved in obtaining future multi-physics, multi-scale simulations that aim for more accurate predictions.
16:15 Uhr s.t., HS KPH

Koordination: Kontakt:

Prof. Dr. Friederike Schmid
Institut für Physik
friederike.schmid@uni-mainz.de

Prof. Dr. Hartmut Wittig
Institut für Kernphysik
hartmut.wittig@uni-mainz.de

Daniela Reibel
Sekretariat Prof. Dr. Friederike Schmid
Institut für Physik
reibel@uni-mainz.de

Fulya Mank
Sekretariat Prof. Dr. Hartmut Wittig
Institut für Kernphysik
mank@uni-mainz.de