| Unit name | Nuclear and Particle Physics |
|---|---|
| Unit code | PHYS22040 |
| Credit points | 10 |
| Level of study | I/5 |
| Teaching block(s) |
Teaching Block 1 (weeks 1 - 12) |
| Unit director | Professor. Bremer |
| Open unit status | Not open |
| Pre-requisites | |
| Co-requisites |
None |
| School/department | School of Physics |
| Faculty | Faculty of Science |
The quantum world is non-intuitive but it correctly provides an explanation for many phenomena at the small scale. The quantum world of the atom and the nucleus are introduced, and the Standard Model of particle physics. The semi-empirical mass formula permits calculations of nuclear processes and an understanding of fission and fusion, as well as the explanation of nucleosynthesis of elements in stars and supernovae.
Aims:
To introduce the Standard Model of particle physics. To introduce nuclear physics and provide a systematic understanding of calculations of nuclear phenomena and particle interactions. To provide an understanding of the processes of nucleosynthesis.
Have an appreciation of the broad thrust of quantum physics and it wide applicability in explaining a wide range of observable phenomena. Understand the use of mass defects for nuclear decays and be able to calculate the energy released in fission and fusion processes. Understand and perform simple particle scattering calculations and be able to estimate the cross-section for simple systems. Understand the concept of conservation rules and be able to apply them in simple situations. Know the processes involved with nucleosynthesis, the significance of solar neutrinos and the production of heavy nuclei.
Lectures, problems classes.
Written examination.
