FY535: Astrophysics and Introduction to Cosmology
Study Board of Science
Teaching language: Danish or English depending on the teacher, but English if international students are enrolled
EKA: N500019102
Assessment: Second examiner: Internal
Grading: 7-point grading scale
Offered in: Odense
Offered in: Autumn
Level: Bachelor
STADS ID (UVA): N500019101
ECTS value: 5
Date of Approval: 12-05-2020
Duration: 1 semester
Version: Archive
Entry requirements
The course cannot be chosen by students who have passed FY806 Astrophysics or FY817 Introduction to Astrophysics and Cosmology.
Academic preconditions
Course introduction
The aim of the course is to give an overview of the subatomic structure of matter (nuclei and elementary particles), and a basic understanding of star formation, stability and evolution. The course includes an introduction also to cosmology, the Big Bang theory and the evolution of the universe.
The course builds on the knowledge acquired in the courses Quantum mechanics I and II (FY544 and FY547) / (old curriculum: Introductory quantum mechanics I and II (FY521 and FY522)), and gives an academic basis for studying the topics of astrophysics and cosmology, that are part of the degree.
In relation to the competence profile of the degree it is the explicit focus of the course to:
- Give the competence to follow a general relativity course
- Give skills to do analytical and numerical calculations in astrophysics and cosmology
- Give knowledge and understanding of basic concepts in astrophysics and cosmology
Expected learning outcome
The learning objectives of the course are that the student demonstrates the ability to:
- give an overview on an elementary level of the forces of nature governing the Universe
- explain basic reactions on the subatomic level (nuclei and elementary particles)
- understand the basics of the evolution of the universe
- explain the mechanisms governing birth, development and death of the stars
Content
The following main topics are contained in the course:
- Introduction to elementary particles, fundamental forces, nuclei and nuclear models.
- Star classification, formation, stability, energy transport and evolution.
- Introduction to the Big Bang theory and evolution of the universe.
Literature
Halliday, Resnick, Krane: Physics Vol 2, Wiley 5th ed.
J. Christensen-Dalsgaard: Stellar Structure and Evolution, Lecture Notes, Aarhus Universitet.
B. Ryden: Introduction to Cosmology, Addison-Wesley, 2003.
See itslearning for syllabus lists and additional literature references.
See itslearning for syllabus lists and additional literature references.
Examination regulations
Exam element a)
Timing
January
Tests
Written exam
EKA
N500019102
Assessment
Second examiner: Internal
Grading
7-point grading scale
Identification
Student Identification Card
Language
Normally, the same as teaching language
Duration
4 hours
Examination aids
Not allowed, a closer description of the exam rules will be posted in itslearning.
ECTS value
5
Indicative number of lessons
Teaching Method
At the faculty of science, teaching is organized after the three-phase model ie. intro, training and study phase.
- Intro phase: 32 hours
- Skills training phase: 16 hours
Lectures and assignments which are related to the topics taught in the lectures.
Activities during the study phase: During the study phase, students are expected to work with self-study of the textbook and examples and tasks in this. In addition, written home assignments form part of the study phase, and students can expect feedback from a teacher.