Conférences  >  Physique  >  Astronomie, astrophysique et cosmologie  >  Allemagne

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

The focus of the conference is the theory of the Standard Model and beyond at finite temperature and density and in and out of equilibrium, including applications to cosmology, astrophysics and relativistic heavy-ion collision experiments.

QCD in extreme conditions and dense nuclear matter, Heavy-ion collisions and the Quark-Gluon Plasma, Quantum fields in and out equilibrium and thermalisation, Baryogenesis and leptogenesis, Electroweak phase transition beyond the Standard Model, Early Universe physics and sources for gravitational waves, Quantum field dynamics and inflation, Compact stars

Nuclear Physics in Astrophysics is an exciting field with many highlights in recent years in observational astronomy, simulating astrophysics, experimental and theoretical nuclear physics. Therefore, training and interaction of young scientists, PhD students and postdocs, are important for further progress and expansion of this community. We are organizing a Summer School on "Nuclear Physics in Astrophysics" in connection to the International Conference on Nuclear Physics in Astrophysics XI. It will be held at Burghotel Stolpen, Germany, from September 8 (arrival) to 15 (departure or transit to the conference), 2024.

Topics will cover the different aspects of nuclear astrophysics: observational astronomy and gravitational waves, astrophysical modelling and simulations, and nuclear physics experiments and theory.

Cours et événements pour étudiants en physique,    Physique nucléaire

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

Wilhelm and Else Heraeus-Foundation

The goal of this physics school is to offer master and Ph.D. students from the field of experimental and theoretical physics as well as mathematics and philosophy, a coherent introduction to the subject of quantum gravity phenomenology from both theoretical and experimental perspectives. The participants should be interested in, or already work on, the search for quantum gravity from the theoretical or experimental side, and be motivated to learn from both sides to be able to get a more complete overview over the research field.

Wilhelm and Else Heraeus-Foundation

Géophysique et géologie,    Cours et événements pour étudiants en physique