Division Particle & Astroparticle Physics
 
 

Seminars, Colloquia and Events

Period from 26 April 2024 to 10 May 2024


Friday, 26 April 2024

  17:00 Physikalisches Kolloquium
Prof. Dr. Gregor Kasieczka
The road to AI-based discovery in particle physics
KIP, INF 227, Hörsaal 1
Modern machine learning and artificial intelligence are starting to fundamentally change how we analyze huge volumes of data in particle physics and adjacent scientific disciplines. These breakthroughs promise new insights into major scientific questions such as the nature of dark matter or the existence of physical phenomena beyond the standard model. This colloquium will provide an overview of recent, exciting developments with a focus on model agnostic discovery strategies — including first experimental results, fast simulations, and foundation models that simultaneously solve multiple tasks across multiple datasets.

Monday, 29 April 2024

  16:30 Particle and Astroparticle Theory Seminar
Prof. Qaisar Shafi (Delaware)
Monopoles, Strings and Gravitational Waves
Seminar room Lindner 339, Gentner lab, 2nd floor
A variety of interesting topological objects arise in spontaneously broken unified theories. They include monopoles and strings as well as more complex structures with cosmological implications. In this talk I will discuss primordial magnetic monopoles, cosmic strings and gravitational waves.

Tuesday, 30 April 2024

  11:15 Seminar Theoretische Quantendynamik
Dr. Pei-Lun He, MPIK
Photoelectron Polarization Vortexes in Strong-Field Ionization
Otto Hahn lecture hall, library building
Abstract: // The spin polarization of photoelectrons induced by an intense linearly polarized laser field is investigated using numerical solutions of the time-dependent Schrödinger equation in companion with our analytic treatment via the spin-resolved strong-field approximation and classical trajectory Monte Carlo simulations. We demonstrate that, even though the total polarization vanishes upon averaging over the photoelectron momentum, momentum-resolved spin polarization is significant, typically exhibiting a vortex structure relative to the laser polarization axis. The polarization arises from the transfer of spin-orbital coupling in the bound state to the spin-correlated quantum orbits in the continuum. The rescattering of photoelectrons at the atomic core plays an important role in forming the polarization vortex structure, while there is no significant effect of the spin-orbit coupling during the continuum dynamics. Furthermore, spin-polarized electron holography is demonstrated, feasible for extracting fine structural information about the atom.
  14:15 Kosmologie und Elementarteilchenphysik
Alexander Ganz
Exploring Minimally Modified Gravity
Institut für Theoretische Physik, Phil12, SR106
Minimally modified gravity models are a class of modified gravity theories with only two local degrees of freedom as in General Relativity. In this seminar I want to discuss their general properties such as the existence of a preferred foliation and then discuss phenomenological applications in the early Universe. While during inflation the modifications to the power spectra are slow-roll suppressed, for the bispectrum we can get new signatures deviating from standard single scalar field models. Further, I will discuss how these models can be used to construct stable and viable bouncing scenarios.
  16:30 Heidelberg Joint Astronomical Colloquium
Dr Mario Flock
Rim Worlds: Computational astrophysics of accretion disks
Philosophenweg 12, Main Lecture hall (gHS)
Understanding the formation of (exo)-planetary systems requires the combined effort of advanced computational models and high-resolution multi-wavelength observations. In my talk, I will review our current understanding of the dynamic evolution of protoplanetary disks. 3D multi-physics simulations and high-performance computing allow us to study the thermal and kinematical evolution of young circumstellar disks and planets' birthplaces in detail. I will also highlight why the inner disk regions, especially those close to the silicate sublimation, are crucial for forming terrestrial planets. Those unable to attend the colloquium in person are invited to participate online through Zoom (Meeting ID: 942 0262 2849, passcode 792771) using the link: https://eu02web.zoom-x.de/j/94202622849?pwd=dGlPQXBiUytzY1M2UE5oUDRhbzNOZz09
  17:00 Particle Colloquium
Giovanni Dal Maso
Latest Results from MEG2
Physikalisches Institut INF 226, Konferenzraum 1-3 (Room 00.101 bis 00.103)

Thursday, 2 May 2024

  11:15 Teekolloquium
Dr Christoph Wiesinger
Probing the neutrino mass with KATRIN and ultra-low background X-ray detectors for IAXO
Grosser Hoersaal/Big Lecture Hall (library)
Our understanding of fundamental particles is incomplete. The absolute neutrino mass remains unknown and strong interactions appear suspiciously symmetric, hinting at the existence of axions. KATRIN performs precision spectroscopy of tritium beta-decay electrons, probing the effective electron anti-neutrino mass with unprecedented sensitivity. IAXO is a next-generation helioscope aiming to detect solar axions, as they are converted into X-rays along a strong magnet pointing towards the sun. In my presentation, I will discuss the challenging analysis of the first five KATRIN neutrino mass campaigns and the potential of ultra-low background semiconductor detectors, based on the TRISTAN upgrade of KATRIN, to boost the search for solar axions with IAXO.
    ARI Institute Colloquium
Francesco Flammini Dotti
Massless objects dynamics in star clusters
ARI, Moenchhofstrasse 12-14, Seminarraum 1.OG
The dynamical evolution of massless objects in star clusters aims to explore their dynamics during the dynamical evolution of such structures, which is not easy observable in star clusters, and still not possible in dense star clusters such as globular clusters. In a star cluster, the main phenomenon we are going to focus on are the mass segregation and core collapse. I will first introduce previous works that looked into the motion of these objects, and then I will numerically explore the dynamical evolution of such objects, varying the number density of the hosting star cluster. As a final point, I will try to confute if the relative large abundance of free-floating planets in our galaxy is due to their ejected free-floating planets. I will use NBODY6++GPU-ML (a N-body code which performs simulations with a large number of particles and massless particles, i.e., star clusters with free-floating planets). The results pinpoint how the massless particles are not particularly affected by mass segregation, but only by the central gravitational evolution of the core of the star cluster, suggesting that those particles, in relatively dense star clusters, are ejected only at much larger timescales.
  16:15 Teilchen-Tee
Wilke van der Schee
Bayesian analysis of heavy ion collisions (Pre-talk 15:30)
Institut für Theoretische Physik, Phil12, SR106
TBA

Friday, 3 May 2024

  17:00 Physikalisches Kolloquium
Prof. Dr. Elena Hassinger
Odd ways to unconventional superconductivity
KIP, INF 227, Hörsaal 1

Superconductivity is a fascinating state of matter that transforms metals at very low temperature into perfect conductors and perfect diamagnets. This enables numerous technical applications for magnetic levitation, electric current transport without loss and for quantum information technology. A desired but rare type of unconventional superconductivity with possible uses in topological quantum computing is one where the superconducting condensate is odd under inversion symmetry, so-called odd-parity superconductivity. Only a handful of uranium-based materials have this property and it is usually explained by the presence of ferromagnetism enforcing a parallel alignment of the electrons forming the Cooper pair.

In the colloquium talk I will present our astonishing discovery that superconductivity in the material CeRh2As2 with a critical temperature of only 0.4 kelvin switches its state in a magnetic field and is then stable up to the extreme magnetic field of 16 tesla. The switching is understood as a unique phase transition from even-parity to odd-parity superconductivity that likely relies on a special crystallographic feature of the underlying material, CeRh2As2, and not on ferromagnetic interactions. I will show our experimental investigations into the question what stabilises such a transition that we address by tuning superconductivity and other coexisting orders with temperature, magnetic field and hydrostatic pressure. The resulting knowledge paves the way for the design of other odd-parity superconductors with higher transition temperatures useful for applications.


Tuesday, 7 May 2024

  11:15 Seminar Theoretische Quantendynamik
Dr. Michael Quin, MPIK
TBA
Otto Hahn lecture hall, library building
  14:15 Kosmologie und Elementarteilchenphysik
Subinoy Das
Possible role of new neutrino interaction in cosmological Hubble anomaly?
Institut für Theoretische Physik, Phil12, SR106
The 5 sigma mismatch between CMB and local distance ladder measurements of Hubble parameter is one of the greatest challenge to our well known Lambda CDM model of cosmology. I will discuss that one needs beyond standard model particle physics to appear before and close to CMB epoch if the anomaly persists. I will also present a scenario where secret BSM neutrino interaction can play a crucial role to relax the mismatch and also point to predictions of such new physics in cosmological observables.
  16:30 Heidelberg Joint Astronomical Colloquium
Dr Andreas Sander
Deciphering the properties and impact of hot and massive stars with detailed stellar atmosphere modelling
Philosophenweg 12, Main Lecture hall (gHS)
Abstract to be announced. Those unable to attend the colloquium in person are invited to participate online through Zoom (Meeting ID: 942 0262 2849, passcode 792771) using the link: https://eu02web.zoom-x.de/j/94202622849?pwd=dGlPQXBiUytzY1M2UE5oUDRhbzNOZz09
  17:00 Particle Colloquium
Dr. Tamasi Kar
The Triplet Track Trigger Concept for the FCC-hh\n\n
Physikalisches Institut INF 226, Konferenzraum 1-3 (Room 00.101 bis 00.103)

Wednesday, 8 May 2024

  09:30 Seminar Dynamik und Struktur von Atomen und Molekülen
Nick Lackmann, Highly charged ion dynamics
tba
Central Seminar Room, library building
  11:15 Bothe-Kolloquium
Prof. Marcus Dahlström, Department of Physics, Lund University
Playing with XUV-dressed atoms: Stabilization, entanglement, triplets, zero areas and other ideas from quantum optics
Central seminar room, library building
  14:00 Zentrum für Quantendynamik Kolloquium
Dr. Cesar Cabrera
Tracking the confinement-induced hybridization of the Higgs mode in a strongly interacting superfluid
 
 


Last modified: Thu 25. April 2024 at 15:21:22 , Impressum , Datenschutzhinweis