PHY_3F007_EP - High Energy Physics (2024-2025)

Prerequisites: PHY204, PHY205
Recommended previous courses: PHY106, PHY301

The quest for finding the ultimate constituents of matter has revealed that matter has a nested structure at scales that differ by many orders of magnitudes: atoms contain electrons and nuclei; nuclei are made up of nucleons, which in turn are composed of quarks and gluons. Nowadays, particle physicists are more concerned with the fundamental laws that govern the interactions of elementary particles. The most emblematic question is “how do particles acquire mass”; and the discovery of the Higgs boson in 2012 is an important clue that we are on the right path to answering this question. The infinitely small is also intimately linked to the infinitely large: to cite just one example, the most energetic particles detected to date, called cosmic rays, come from processes whose origin remains a mystery, probably created in the heart of accretion disks surrounding black holes, located at the center of active galaxies.

This course will give a pedestrian introduction to the subatomic physics, with 4 courses dedicated to the special relativity, 5 courses about the nuclear and high energy physics and 4 courses about high energy astrophysics. All courses will be illustrated in a balanced theoretical underpinning, experimental activities and technological aspects of subatomic physics. The bases for this course will be PHY205 (introductory quantum physics) and PHY204 (theoretical electrodynamics).

In the special relativity section, the following subjects will be treated: Lorentz transformations, spacetime diagrams, covariant formalism, 4-vectors including the energy-momentum vector, illustrated by several examples such as the famous twin paradox.

The nuclear and subatomic part of the course will provide the big picture of the structure of matter with the great discoveries. The nuclear models (droplet model) and the nuclear binding energy will be discussed. The Standard Model components and interactions will be presented, through the particle evolution equations and an introduction to the Feynman’s diagrams including the different conservation laws of the Standard Model. This section will end with a course dedicated to the particle accelerators/colliders and detectors and a discussion about the latest measurements arguing for a theory beyond the Standard Model.

In the last 4 courses, we will dive into the high energy astrophysics, where we will review nuclear and particle physics in various astrophysical environments. We will start with an introduction with a first course about stellar mass compact objects, from white dwarfs to black holes; and a second course dedicated to the environments of supermassive black holes, at the heart of active galactic nuclei. The 2 last courses will cover the high energy processes in astrophysics with a first lecture dedicated to the accretion and ejection phenomena, super-luminal jets, thermal and non-thermal processes; while the second lecture will detail synchrotron radiation, Inverse Compton, leptonic and hadronic interactions, diffusion and collision.