Conférences  >  Physique  >  Astronomie, astrophysique et cosmologie  >  Allemagne

The Arnold Sommerfeld Center for Theoretical Physics at the LMU in Munich will host a school on “The Quantum Gravity Swampland and its consequences for the observable world” in the period October 9-13, 2023. We plan to have the school in presence, in accordance with the Corona rules then in force. The school is primarily aimed at PhD students, but master students or more senior researchers are very welcome to apply as well. It will cover introductory lectures to the swampland program as well as more advanced topics on formal developments and phenomenological applications to particle physics and cosmology.

Physique des hautes énergies, des particules et des champs,    Cours et événements pour étudiants en physique

Email.: https://www.munich-iapbp.de/magnetic-fields

The goal of the seminar is to bring together global experts from experiment and theory in the field working on various storage ring projects for a constructive discussion of the most promising paths to maximize the impact of the available facilities and exploit synergies among the groups.

Physique des hautes énergies, des particules et des champs,    Accélérateurs de particules

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

ADONIS is aimed at investigating the chemical enrichment of nearby galaxies by using theory and observations. We plan to join efforts from world-leading experts working on resolved and unresolved stellar populations, and on state-of-the-art theoretical modelling.In case you would like either to become more familiar with these issues or to discuss recent findings on metallicity distribution and gradients youare really welcome to join us!

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

The exchange of mass, energy, and metals between galaxies, their surrounding circum-galactic medium (CGM), and the gas permeating halos at larger scale represents a fundamental part of the modern astrophysics. Both components still elude our knowledge. Indeed, we are very far from having a census of the CGM properties in the bulk of the galaxy population. Furthermore, the halo gas is well known at large scale only in the most massive halos of our Universe, the galaxy clusters (intra-cluster medium, ICM), but it is still very elusive in the bulk of the virtualized halo population at the group mass scale (Intra-group medium IGrM).

With the advent of instrument such as eROSITA, XRISM and JWST, and the enormous variety of results collected by Alma, MUSE, KCWI and LOFAR, it is time to review the state of the art of this research field. The final goal of this workshop is to fill the knowledge gap and review in an unbiased way all the key aspects of the baryon cycle: from the hot IGrM enclosed in the bulk of the virtualized halo population, to the CGM at hundreds of kpc from the central galaxy, and down to the main mechanisms in act at the galaxy center able to trigger the baryonic exchange.

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

It is widely accepted that habitability and the capability of a planet to maintain its habitable conditions are deeply interwoven with its chemical composition and physical properties such as its atmospheric and geological/geophysical characteristics, orbital motion, dynamics, and its interactions with its host star. How these interactions originate and how they enable the planet to maintain its habitability are complex questions that can only be answered through collaborations between scientists of their respective fields. This workshop aims to bring together scientists from the fields of stellar astrophysics, planetary science, planetary dynamics, geology, and geophysics to discuss fundamental questions regarding the formation, characterization, and detection of habitable planets. Our plan is to facilitate interactions among participants through lectures, presentations and discussion sessions as well as to provide them with ample time to initiate collaborations and carry out their independent research. Our workshop is open to scientists of all levels, in particular junior and early-career researchers.

Cours et événements pour étudiants en physique,    Géophysique et géologie

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

How did quantum fluctuations of the inflaton field provide the seeds for structure on cosmological scales? Did other fields play a role during inflation? How did their quantum fluctuations imprint on cosmological observables (e.g., non-Gaussianity) or survive as cosmological relics today (e.g., dark matter, matter/antimatter asymmetry)? How can these degrees of freedom be embedded into a compelling UV theory? By bringing together experts on particle physics and cosmology, we hope to develop a deeper understanding of these tough questions over the course of this 4-week MIAPbP meeting.

Cours et événements pour étudiants en physique,    Physique des hautes énergies, des particules et des champs

Mathematisches Forschungsinstitut Oberwolfach (MFO, Oberwolfach Research Institute for Mathematics)

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

In recent years, spurred in large part by the development of first-principles numerical simulations, the plasma astrophysics community has made important strides in understanding the plasma processes relevant for astrophysical systems. The next step, which will be a key topic of the MIAPbP program, is to connect the rich plasma behavior to observed radiative phenomena. These phenomena include old puzzles, e.g. hard X-ray emission from accreting black holes, gamma-ray flares from blazars, cosmic ray acceleration, giant magnetar flares and GRBs. Plasma physics is also key to solving new puzzles such as the cosmological FRBs and gamma-rays from neutron star mergers. The role of plasma instabilities is especially prominent in transient phenomena and strong connections are emerging between plasma physics and time-domain astronomy, a quickly developing observational field. Plasma physics also plays an increasing role in multi-messenger astronomy where main targets are energetic compact objects capable of producing neutrinos, gravitational waves, and nonthermal radiation. The current efforts to understand plasma behavior lay the foundations for the future of high-energy astrophysics. Within a two-week MIAPbP program, we want to facilitate progress in this direction by bringing together both senior researchers as well as early-career scientists.

Cours et événements pour étudiants en physique,    Physique des plasmas, fusion nucléaire

Physique nucléaire,    Physique des hautes énergies, des particules et des champs