FYS9525 – Advanced Nuclear Reactions and Applications in Astrophysics
Changes in the course due to coronavirus
Autumn 2020 we plan for teaching and examinations to be conducted as described in the course description and on semester pages. However, changes may occur due to the corona situation. You will receive notifications about any changes at the semester page and/or in Canvas.
Spring 2020: Teaching and examinations was digitilized. See changes and common guidelines for exams at the MN faculty spring 2020.
This course will provide the students with an understanding of the main astrophysical processes to produce elements in the cosmos. In particular, the connection of nuclear physics data to astrophysical relevant cross-sections will be covered, which includes hands-on experience with the state-of-the-art TALYS reaction code, to deepen the understanding of the interplay of nuclear physics and astrophysics.
After completing this course:
- You will have knowledge of how elements heavier than iron could be formed in astrophysical environments, especially the s-process, the r-process, and the p-process.
- you will have a detailed knowledge of the importance of nuclear structure physics and nuclear reactions underlying nuclear astrophysical processes.
- you will have a detailed knowledge of the nuclear reactions models, such as the Hauser-Feshbach formalism, relevant to nuclear astrophysics.
- you will be able to calculate nuclear cross-sections e.g. neutron capture cross-sections.
- you will have hands-on training in running the state-of-of-the-art reaction code TALYS using both experimental and theoretical level densities and gamma strength functions as inputs.
- you will have knowledge of experimental nuclear physics methods and techniques used for measuring nuclear properties for nuclear astrophysical processes.
- you will have completed a challenging project using the TALYS code and written a report on this.
Admission to the course
Send a short application to firstname.lastname@example.org. Only PhD candidates enrolled in the programme PhD at The Faculty of Mathematics and Natural Sciences (PhD) may apply. This course should be a part of your theoretical curriculum. Contact the Department of Physics if you are unsure if you are eligible.
Recommended previous knowledge
- 5 credits overlap with FYS4525 – Advanced Nuclear Reactions and Applications in Astrophysics.
The course will be given as an intensive course over two weeks with 30 hours of lectures and 30 hours of problem sessions and hands-on calculations using the TALYS code. There will be a mandatory report, with a deadline several weeks after the intensive course.
As the teaching involves laboratory and/or field work, you should consider taking out a separate travel and personal risk insurance. Read about your insurance cover as a student.
Cost of taking the course
The location of the intensive course may be in Oslo or abroad. If given abroad there will be travel and housing costs. Students can apply to have these costs covered, and selection of students for grants is based on the relevance of the course for their PhD or master thesis.
There will be a mandatory report on the TALYS calculations done during the course. Grading is based 100% on this report.
It will also be counted as one of the three attempts to sit the exam for this course, if you sit the exam for one of the following courses: FYS4525 – Advanced Nuclear Reactions and Applications in Astrophysics
Language of examination
The examination text is given in English, and you submit your response in English.
Grades are awarded on a pass/fail scale. Read more about the grading system.
Resit an examination
This course offers both postponed and resit of examination. Read more: