Tag: International Schools

SoUP is an advanced school for PhD students, post-docs and young researchers willing to gain deeper knowledge in topics related to underground physics. The 2024 edition is organized by INFN-Bologna at the Bertinoro University Center (CEUB) in the MiddleAge village of Bertinoro (FC – Italy). Lectures start on Monday 14th October and end at noon on Friday 18th October. The school includes lectures and hands-on sessions on Physics Phenomenology, Detection Techniques, Instrumentation Technologies.

A Speed-talk event and a Poster session are also foreseen.

Here the list of Topics and Lecturers:

• Dark Matter Phenomenology. Lecturer: Marco Cirelli (LPTHE Paris)
• Neutrino Phenomenology. Lecturer: Marco Pallavicini (University & INFN Genova) Axion Phenomenology and Detection. Lecturer: Gianni Carugno (INFN Padova)
• Liquid Scintillators and Water Cherenkov Detectors. Lecturers: Barbara Caccianiga (INFN Milano), Giorgio Riccobene (INFN LNS)
• Noble Liquid Detectors. Lecturer: Giuliana Fiorillo (University & INFN Naples)
• Solid State Detectors. Lecturer: Marco Vignati (University & INFN Roma La Sapienza)
• Statistics (Principles and Hands-on session). Lecturer: Knut Mora (Columbia University)
• Novel Photodetectors. Lecturer: Alberto Gola (FBK Trento)
• Material Screening. Lecturer: Monica Sisti (INFN Milano Bicocca)

Final Registration and Fee Payment are now open:

• deadline for the Early registration fee of 650 euro: June 15
• deadline for the Standard registration fee of 700 euro: July 31.

The fee covers:

admission to all lectures;
lodging in a double room for 5 nights, from Sunday evening to Friday morning (+50 euro for single room, if available);
breakfast, lunch, and two coffee breaks per day (Mon-Fri);
the social dinner;
welcome party;
shuttle from/to the railway station in Forlì.

We invite all Undergrad, PhD students and PostDoc to register asap.

School Website

The aim of the 12th Aegean Summer School is to discuss the recent developments in theory in Gravity and Cosmology and in observations discussing the LIGO, VIRGO, LISA and BINGO experiments.

The 12th Aegean Summer School will take place in the town of Apollonia in the island of Sifnos, in the Cultural Centre “Marianthi Simou” and it is organized and sponsored by the National Technical University of Athens, Greece, the University Paris-Sud, Orsay, France, the University of Tuebingen, Germany, the University Nottingham, England, the University Sapienza, Rome, Italy, the University Pontificia Universidad Católica de Valparaiso, Chile, the University Sao Paulo, Brazil and the European Cooperation in Science and Technology (COST).

One of the most successful theory describing cosmic objects, their interactions and their time evolution, is the Einstein’s theory of Gravity. One of the main prediction of the Gravity theory is the existence of Gravitational Waves (GW), the ripples of space-time. The latest GW detections by ground-based interferometers and the discovery of a binary pulsar whose orbital period changes in accordance with the predicted GW emission, verified the predictions of the Einstein’s theory and opened up an intensive activity of understanding all aspects of the GWs and the implications of this discovery to alternative theories of Gravities and their Cosmological implications.

The modified gravity theories can give us important information on the structure and properties of the compact objects predicted by these theories and also the observational signatures which they can introduce. It is expected that future ground and space-borne detectors will improve our perception of gravitational interactions in particular will shed light into the existence of exotic compact objects, like hairy black holes and wormholes. These compact objects provide a window into the microscopic structure of spacetime in Quantum Gravity and the hope is to understand the nature of their interior, potential applications to Quantum Cosmology, and the development of further connections to quantum information and laboratory quantum simulation. The formation of these compact objects may also trigger possible holographic phase transitions to other compact objects.

School Website