Astroparticle Physics

Recommended Prerequisites

Basic knowledge in Quantum Mechanics and Modern Physics.

Teaching Methods

Lectures using blackboard and the presentation of slides and computer animations. The discussion of the subjects should always include reference and analysis of the most significant experimental observations, along  with their implications. The lessons should always be open to discussion, involving the students. Preparation of problems for application of the material taught, to be discussed by the students. Study of typical cases.

Development of projects with wider scope and greater depth than the sample problems. Discussion of issues and recent observations on the edge of present knowledge.

Learning Outcomes

Main learning outcomes:
A solid background in the area of astroparticles. It is intended to focus on the physics of cosmic rays, dark matter and neutrinos, as well as on the experimental methods applied in these areas.
Other learning outcomes:
Development of analytical and synthesis reasoning skills, problem-solving and critical analysis of data and results. Development of learning autonomy and creativity.

Work Placement(s)

No

Syllabus

1 - Basic concepts on elementary particles.
2 - Cosmic rays
2.1 Introduction. Cosmic ray sources
2.2 Direct measurements
2.3 Cosmic ray showers
2.4 Cosmic ray detetection methods
3 - Neutrino physics
3.1 Neutrino properties and the big open questions
3.2 Atmospheric neutrinos
3.3 Solar neutrinos
3.4 Double beta decay (with and without neutrino emission)
4. Dark matter
4.1 Astrophysical observations and evidences of dark matter existence.
4.2 Dark matter candidates
4.3 Experimental methods for dark matter detection (direct, indirect and production at accelerators).

Head Lecturer(s)

Nuno Filipe Fiuza de Barros

Assessment Methods

Assessment
Resolution Problems: 40.0%
Exam: 60.0%

Bibliography

- M. Thomson, Particle Physics , Cambridge University Press, 2013
- K. Zuber, Neutrino Physics , CRC Press, 2020
- G. Bertone (editor), Particle Dark Matter , Cambridge University Press, 2010