Explore advanced theoretical physics concepts in this comprehensive summer school program covering particle physics beyond the Standard Model. Delve into naturalness-motivated beyond Standard Model (BSM) theories through five detailed classes examining the theoretical foundations and experimental implications of natural solutions to hierarchy problems. Master cutting-edge computational tools and methodologies for BSM research, including amplitude calculations, future collider physics, and machine learning applications across ten specialized sessions. Investigate cosmological connections to particle physics through five classes exploring dark matter, early universe dynamics, and the intersection of cosmology with BSM theories. Examine frontiers in non-natural BSM approaches through four classes covering alternative theoretical frameworks that don't rely on naturalness assumptions. Study the light and feeble frontier of particle physics, focusing on light dark matter candidates and feebly interacting particles through five comprehensive sessions exploring detection methods and theoretical predictions. Gain expertise in modern analytical and computational techniques essential for contemporary BSM research, including advanced amplitude methods and machine learning applications in high-energy physics. Learn from leading experts in theoretical particle physics as they present the latest developments in BSM phenomenology, experimental searches, and theoretical frameworks that extend our understanding beyond the Standard Model of particle physics.

Syllabus

Csaba Csaki: Naturalness-motivated BSM - Class 1 of 5
Yael Shadmi: Tools at the Frontiers of BSM: amplitudes - Class 1 of 5
Jay M. Hubisz: Cosmology - Class 1 of 5
Yael Shadmi: Tools at the Frontiers of BSM: amplitudes - Class 2 of 5
Csaba Csaki: Naturalness-motivated BSM - Class 2 of 5
Jay M. Hubisz: Cosmology - Class 2 of 5
Yael Shadmi: Tools at the Frontiers of BSM: amplitudes - Class 3 of 5
Jay M. Hubisz: Cosmology - Class 3 of 5
Csaba Csaki: Naturalness-motivated BSM - Class 3 of 5
Jay M. Hubisz: Cosmology - Class 4 of 5
Yael Shadmi: Tools at the Frontiers of BSM: amplitudes - Class 4 of 5
Csaba Csaki: Naturalness-motivated BSM - Class 4 of 5
Yael Shadmi: Tools at the Frontiers of BSM: amplitudes - Class 5 of 5
Csaba Csaki: Naturalness-motivated BSM - Class 5 of 5
Jay M. Hubisz: Cosmology - Class 5 of 5
Gilad Perez: Frontiers in non-natural BSM - Class 1 of 4
Raffaele Tito d’Agnolo: The light and feeble frontier: light DM, Feebly Interacting...Class - 1 of 4
Tilman Plehn: Tools at the Frontiers of BSM: future colliders and machine learning - Class 1 of 5
Tilman Plehn: Tools at the Frontiers of BSM: future colliders and machine learning - Class 2 of 5
Raffaele Tito d’Agnolo: The light and feeble frontier: light DM, Feebly Interacting...Class - 2 of 5
Gilad Perez: Frontiers in non-natural BSM - Class 2 of 4
Raffaele Tito d’Agnolo: The light and feeble frontier: light DM, Feebly Interacting.. - Class 3 of 5
Gilad Perez: Frontiers in non-natural BSM - Class 3 of 4
Tilman Plehn: Tools at the Frontiers of BSM: future colliders and machine learning - Class 3 of 5
Gilad Perez: Frontiers in non-natural BSM - Class 4 of 4
Tilman Plehn: Tools at the Frontiers of BSM: future colliders and machine learning - Class 4 of 5
Raffaele Tito d’Agnolo: The light and feeble frontier: light DM, Feebly Interacting.. - Class 4 of 5
Tilman Plehn: Tools at the Frontiers of BSM: future colliders and machine learning - Class 5 of 5
Raffaele Tito d’Agnolo: The light and feeble frontier: light DM, Feebly Interacting.. - Class 5 of 5