PHYS-717 / 2 credits

Teacher(s): Invited lecturers (see below), Schober Jennifer Waltraud

Language: English


Frequency

Only this year

Summary

The course will cover some fundamentals of magnetohydrodynamics (MHD) theory with hands-on sessions to learn the basics of MHD simulations using the open-source Pencil Code (http://pencil-code.nordita.org/).

Content

This minicourse on "Numerical simulations of magnetohydrodynamics (MHD) in the early Universe" is offered during the fourth week of the program "Generation, evolution, and observations of cosmological magnetic fields" at the Bernoulli Center.
The course will cover some fundamentals of MHD theory as well as phenomena relevant to the highly relativistic plasma that fills the early Universe. These phenomena include decaying MHD turbulence, dynamo instabilities related to the chiral magnetic effect, and production of primordial gravitational waves from decaying MHD turbulence. A main part of the course are hands-on sessions to learn the basics of MHD simulations using the open-source Pencil Code (http://pencil-code.nordita.org/).
The course is open to EPFL students and young researchers participating in the program (PhD students and postdocs). Senior researchers from other fields who are interested in learning MHD simulations are also welcome.

Note

Dates: 21.05.24 to 24.05.24

Lecturers: Jennifer Schober, Alberto Roper Pol

Keywords

Magnetohydrodynamics, Numerical Simulations, Early Universe

Learning Prerequisites

Required courses

Basic Python knowledge, Electrodynamics, Fluid Dynamics, Cosmology/Astrophysics

Learning Outcomes

By the end of the course, the student must be able to:

  • to setup simulations of magnetohydrodynamics problems with the Pencil Code and to analyze the simulation data with python routines.

Resources

Bibliography

Pencil Code website: https://pencil-code.nordita.org/
Bernoulli program "Generation, evolution, and observations of cosmological magnetic fields": https://indico.cern.ch/event/1334236/

Moodle Link

In the programs

  • Number of places: 45
  • Exam form: Oral (session free)
  • Subject examined: Simulations of Early Universe Magnetohydrodynamics
  • Lecture: 16 Hour(s)
  • Exercises: 16 Hour(s)
  • Type: optional

Reference week

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