Undergraduate Course: Nuclear Physics (PHYS11041)
Course Outline
| School | School of Physics and Astronomy |
College | College of Science and Engineering |
| Course type | Standard |
Availability | Available to all students |
| Credit level (Normal year taken) | SCQF Level 11 (Year 4 Undergraduate) |
Credits | 10 |
| Home subject area | Undergraduate (School of Physics and Astronomy) |
Other subject area | None |
| Course website |
Course material will be made available in Learn |
Taught in Gaelic? | No |
| Course description | The course will build on the Subatomic Physics course by further exploring the fundamentals of nuclear matter as well as considering some of the most important applications of nuclear physics. Topics to be studied will include decay modes, nuclear reactions, and nuclear astrophysics. The lecture course will be integrated with problem solving classes. |
Information for Visiting Students
| Pre-requisites | None |
| Displayed in Visiting Students Prospectus? | Yes |
Course Delivery Information
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| Delivery period: 2013/14 Semester 2, Available to all students (SV1)
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Learn enabled: Yes |
Quota: None |
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Web Timetable |
Web Timetable |
| Class Delivery Information |
Workshop/tutorial sessions, as arranged. |
| Course Start Date |
13/01/2014 |
| Breakdown of Learning and Teaching activities (Further Info) |
Total Hours:
100
(
Lecture Hours 22,
Supervised Practical/Workshop/Studio Hours 22,
Formative Assessment Hours 10,
Summative Assessment Hours 2,
Programme Level Learning and Teaching Hours 2,
Directed Learning and Independent Learning Hours
42 )
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| Additional Notes |
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| Breakdown of Assessment Methods (Further Info) |
Written Exam
100 %,
Coursework
0 %,
Practical Exam
0 %
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| Exam Information |
| Exam Diet |
Paper Name |
Hours & Minutes |
|
| Main Exam Diet S2 (April/May) | Nuclear Physics | 2:00 | |
Summary of Intended Learning Outcomes
Upon completion of this course, the student should be able to:
1)identify basic nuclear properties and outline their theoretical descriptions
2)understand the differences between various decay modes, state selection rules, and determine wether a given decay can take place
3)calculate Q-values for alpha and beta decays and for nuclear reactions
4)apply conservation laws to nuclear reactions and transform quantities between laboratory and centre-of-mass frames
5)compare and constrast different reaction mechanisms in relation to cross-sections, excitation functions, and angular distributions
6)summarise and account for the main aspects of at least one application of nuclear physics (e.g. Nuclear Astrophysics)
7)manage to solve problems similar to those discussed in the afternoon sessions
8)develop critical thinking and independent learning, work effectively within a team
9)produce clear and informative written and oral presentations
10)develop judgement capabilities through assessment of their own work and that of others |
Assessment Information
| Degree Examination, 100% |
Special Arrangements
| None |
Additional Information
| Academic description |
Not entered |
| Syllabus |
Alpha decay:
Energetics. Tunneling effect and probability. Geiger-Nuttall plot. Transition rates and selection rules.
Beta decay:
Electron and positron spectra. (Neutrino mass). Kurie plot. Fermi theory of beta decay. Fermi and Gamow-Teller interactions. Transition rates and selection rules. Electron capture. Neutrinos. Parity violation in beta decay.
Gamma decay:
Energetics. Weisskopf units. Transition rates and selection rules. Angular distribution measurements. Internal conversion.
Nuclear reactions:
Nomenclature and general features. Conservation laws. Reference frames and transformation laws. Cross section. Energy spectra. Angular distributions. Elastic scattering. Direct reactions. Compound nucleus reactions. (Heavy-ion reactions).
Nuclear astrophysics:
General features of the universe. Abundance curve. HR diagram. Principles of star formation and evolution. Energy production and nucleosynthesis. Reaction rates. Gamow peak. Astrophysical S-factor.
Solar reactions and solar neutrinos.
Hydrogen burning. Proton-proton chain. CNO cycles.
Helium burning. Three-alpha process. 12C(¿,¿)16O reaction.
Advanced and explosive burning stages. Cataclysmic and catastrophic scenarios. Nucleosynthesis beyond iron. Neutron captures: s- and r-processes
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| Transferable skills |
Not entered |
| Reading list |
Course material will be made available in Learn |
| Study Abroad |
Not entered |
| Study Pattern |
Not entered |
| Keywords | NucPh |
Contacts
| Course organiser | Dr Marialuisa Aliotta
Tel: (0131 6)50 5288
Email: m.aliotta@ed.ac.uk |
Course secretary | Miss Paula Wilkie
Tel: (0131) 668 8403
Email: Paula.Wilkie@ed.ac.uk |
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