Conferences  >  Physics  >  High Energy Physics, Particles and Fields

Hausdorff Research Institute for Mathematics (HIM)

Mathematical Physics,    Courses and Events for Physics Students

Galileo Galilei Institute

In this workshop we will explore the opportunities unleashed by progress in muon-based experiments, with particular focus on a multi-TeV muon collider. We will discuss both Standard Model precision physics and the search for new phenomena at the highest possible accelerator energies.

Topics to be discussed include: the physics of Standard Model particles at multi-TeV energies, and in particular the phenomenology across the frontier of electroweak symmetry restoration at high energy; searches for new physics at the high-energy frontier; possible uses of muon beams and related technologies for further exploration of fundamental interactions at the high-intensity frontier; synergies with other experiments in flavor, dark matter, neutrino physics, and more

Centro de Ciencias de Benasque Pedro Pascual

Erwin Schrödinger International Institute for Mathematics and Physics (ESI)

Courses and Events for Physics Students,    Astronomy, Astrophysics and Cosmology

Centro de Ciencias de Benasque Pedro Pascual

Centro de Ciencias de Benasque Pedro Pascual

CONICET

The activities of the workshop will focus on an educational program based on lectures, formal and informal discussions aimed at introducing participants in general and students in particular to new trends in theoretical and experimental research on Matter, Astrophysics, Gravitation, Ions, and Cosmology, topics summarized in the acronym MAGIC.

Phone: [+5551983571902];     Email: cesaraugustozenvasconcellos@gmail.com

New phenomena and new states of matter in the Universe, General relativity, gravitation, modified gravity theories and cosmology, White dwarfs, neutron stars, pulsars and black holes, Gamma-ray emission in the Universe, high energy cosmic rays and gravitational waves, Strong magnetic fields in compact stars and in galaxies, Strange matter, strange stars, quark stars and magnetars, The cosmic microwave background and the stochastic gravitational wave background, Dark matter and dark energy, Matter and antimatter in the Universe, Heavy ion collisions and the quark-gluon plasma, High energy particle physics and astroparticles,

Astronomy, Astrophysics and Cosmology,    Nuclear Physics

University of Camerino

The conference ‘Astrophysics in Le Marche 2’ will convene leading experts to discuss the latest advancements in multimessenger astrophysics and precision cosmology, including both theoretical and observational aspects. This event aims to provide a comprehensive international overview of the most recent findings, fostering collaboration and inspiring new directions in the study of the entire universe.

Email: astromarche2@gmail.com

Cosmology, Astronomy, Particle physics, Astroparticles, Astrophysics, Dark Matter, Dark Energy, early universe, Black Holes, Cosmological tensions, Gravitation Theories, Quantum Cosmology, Thermodynamics, Accreation Disks

KMPB, Humboldt-Universität zu Berlin

The KMPB School 2025: D-branes in Physics & Mathematics is a one-week program which will offer introductory courses covering topics underlying the modern understanding of D-branes in string theory and their incarnations in mathematics. The school is organized by PhD students at Humboldt-Universität zu Berlin with the support of the KMPB (Kolleg Mathematik Physik Berlin), an interdisciplinary center at HU whose community of research groups shares a mutual interest in mathematics and physics. In the spirit of the KMPB, the school aims at generating synergies between mathematicians and physicists and welcomes early career researchers (PhDs/PostDocs) in both fields.

Organizers;     Email: kmpbschool2025@gmail.com

string theory, mirror symmetry, D-branes, mathematical physics

Mathematical Physics,    Courses and Events for Math Students and Early Career Researchers

EuNPC2025 is the sixth European Nuclear Physics Conference, organized by the Nuclear Physics Division of the European Physical Society, and jointly by GANIL-SPIRAL2, LPC Caen, IJCLab Orsay and IRFU Saclay. The conference will take place from September 22nd to 26th 2025, and will be held in Caen.

Institute of Physics Belgrade

This international conference brings together researchers and practitioners to explore the impact of space weather on Earth and its systems, including satellite operations, power grids, communication, navigation, aviation, and human health. Topics will cover solar radiation, solar wind, magnetic field variations, and their effects on Earth’s magnetosphere, ionosphere, atmosphere, and climate. Despite advances, predictive capabilities for solar-driven events remain limited. This inaugural event aims to bridge observational, theoretical, and operational efforts and promote integrated approaches to improve forecasting and preparedness.

Email: cosmicIPB@gmail.com

Space weather, Cosmic rays, Ionosphere, Solar-terrestrial coupling, Real-time monitoring and forecasting tools

Astronomy, Astrophysics and Cosmology,    Radiation Processing, Study of Radiation Effects, Radiation Protection

Masaryk University, Faculty of Science, Department of Theoretical Physics and Astrophysics

The Galactic Center (GC) plays a pivotal role in the evolution of the Milky Way. It is instrumental in mapping and understanding the central regions of quiescent galaxies since it is the closest galactic nucleus to us. It serves as a unique test bed for both stellar dynamics in an extremely dense environment as well as magnetohydrodynamics in the vicinity of the supermassive black hole Sagittarius A* (Sgr A*). It is fundamental for studying star formation, because the conditions of its interstellar medium (magnetic fields, temperature, turbulence) are unlike any other place in the Milky Way. Despite many detailed multiwavelength studies of the central regions of our Galaxy, we still have many open questions concerning its history and future evolution. This symposium will bring together experts working on both observational and theoretical studies of the Galactic Center so that they can “traverse” this exciting region from Sgr A* and the surrounding dense nuclear star cluster to the central molecular zone and back, covering about eight orders of magnitude in spatial length. Looking at the Galactic nucleus from this vantage point will uncover details of its past processes and potential future. We will explore the remarkable progress made since the last major meeting of the community—the Galactic Center Workshop in Granada (April 24–28, 2023). We will examine exciting new results, including those from JWST and GRAVITY/ERIS at the VLT, as well as insights from ALMA and MeerKAT.

Phone: [00420 549 49 8773];     Email: info.gc2026@muni.cz

Galactic Center, supermassive black hole, nuclear star cluster, nuclear stellar disk, central molecular zone

Astronomy, Astrophysics and Cosmology,    Computational Physics and Numerical Simulation