Superfluidity (like its cousin, superconductivity) is a particularly striking and concrete manifestation of the wavelike nature of matter. In electromagnetism, it is often fruitful to use Maxwell’s equations, forgetting about the existence of photons. Similarly, we will describe matter by a classical (complex-valued) field, forgetting about the existence of particles. This unconventional approach greatly helps to understand and derive the fundamental concepts and relations of superfluidity, under very general conditions (for any temperature below the transition temperature, including in 2 dimensions —where there is no condensate— and in presence of disorder —where there is no Galilean invariance). Superfluidity appears to be the natural state of the classical field, which can only be destroyed by topological defects (vortices). More formally, superfluidity is associated to a topological order, characterized by an emergent constant of motion. This will allow us to derive key equations of two-fluid hydrodynamics, which will enable us to explain key phenoma such as the fountain effect, the Josephson effect, or supertransport of heat.

 

 

The goal of this course is to introduce somewhat "advanced" topics in quantum matter, tackle truly quantum-entangled, strongly interacting, phases of matter and materials, and present how quantum matter is a particularly rich field, with many open theoretical problems.

In this course, we introduce the major concepts of soft condensed matter, with a focus on fluid interfaces. Soft condensed matter can be defined as the wide class of complex fluids that exhibit multi-hierarchical structural organization spanning the molecular scale up to the macroscopic scale. These complex fluids present unconventional (even paradoxical) physical properties that emerges due to coupling processes between these different length scales. For instance, mixing air and water (with surfactants) produces an aqueous foams which, although it is solely constituted of fluid phases, behaves as a solid phase that can “melt” under a small mechanical load.

 

 

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cosmoloy picture

ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi, CC BY-SA 3.0 IGO

The M1 cosmology lecture gives an introduction to cosmology: a branch of (astro)physics which deals with the universe at the largest observable scales as well as its history. It lasts a total of 32 hours (lectures and exercises included) and uses elements of General Relativity which will be reminded but not introduced in detail. It is taught in english. 

Ce parcours s'adresse aux élèves intéressés par l'optique, la physique des lasers, la physique quantique, la physique atomique et moléculaire, la physique des plasmas et la physique des systèmes de production d'énergie.

This course provides an introduction to probability theory and its applications adapted for physicists.
 

 

The supervised research project offers the possibility to pursue an experimental research project within a team of the ENS Physics department or neighbor institutes.

The course will introduce a number of concepts and techniques in current quantum physics experiments : entanglement, teleportation, Wigner function, non-gaussian quantum states, decoherence, squeezing... 

La physique expérimentale est une composante essentielle des études de physique à l’ENS. 

Les étudiants qui le souhaitent peuvent remplacer les projets expérimentaux par la préparation du French Physicists’ Tournament (FPT).