|
Astrophysics |
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-10022 | Mechanics, Gravity and Relativity | C | M | 7.5 | 15 | |
| This level 1 module builds on A-level physics by taking the familiar subject of mechanics, but integrating it into calculus-based mathematics, thus laying the foundation for physics and astrophysics degrees. The module develops skills in applying physical principles and mathematical techniques to physical and astrophysical situations, and to laboratory based experiments. | ||||||
| PHY-10024 | Nature of matter | C | M | 7.5 | 15 | |
| This level 1 module is delivered in the first semester and provides an introduction to the subject material that bridges the gap between pre-university study and the first year of a university Physics/Astrophysics course. It explores the nature of solid and gaseous matter from the classical picture to the need for a quantum description. It sets the stage for more advanced study of quantum physics, thermodynamics and solid state physics in the second year. A mathematics component is included, in which the requisite material is taught in a Physics context. Also included is a laboratory component (which includes experiments on some of the subject matter delivered in lectures). | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-10020 | Oscillations and Waves | C | M | 7.5 | 15 | |
| This Level 1 module runs in the second semester. It explores the physical principles and mathematical description of oscillatory and wave phenomena, which find application in many areas of classical and modern physics and astrophysics. The module requires a firm grasp of material covered in Level 1 Mechanics, and it sets the stage for the treatment of more advanced topics in optics, quantum mechanics, and electromagnetism at Levels 2 and 3. A mathematics component is included, in which fundamental techniques routinely used in physics are taught and practised. There is also a laboratory component, which involves bench work, computing and communication exercises. | ||||||
| PHY-10023 | Electricity and Stellar Structure | C | M | 7.5 | 15 | |
| This level 1 module examines one of the fundamental forces of physics, electromagnetism, developing an understanding of how this applies to widespread physical processes. The course then turns to stars, showing that the physical laws studied in the course so far can be applied straightforwardly to stars, showing why stars behave and evolve as they do, thus developing an understanding of this most ubiquitous of astrophysical objects. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-20004 | Astrophysics - Study Abroad I | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20005 | Astrophysics - Study Abroad II | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20006 | Quantum Mechanics | C | M | 7.5 | 15 | |
| This module aims to introduce the students to quantum theory and its application to atomic physics and to give them the skills to solve the more straightforward problems and applications in these areas. | ||||||
| PHY-20027 | Optics and Thermodynamics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in geometrical optics, physical optics and thermodynamics. There is also a laboratory component, which is aimed at enhancing experimental and communication skills. | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-20002 | Stellar Astrophysics | C | M | 7.5 | 15 | |
| An understanding of the effect of physical processes on the structure and evolution of stars. Nuclear processes in stars and stellar evolution. The origin of elements in stars. 2 hour lecture & one general tutorial per week, plus astrophysics skills | ||||||
| PHY-20022 | Astrophysics - Study Abroad III | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20023 | Astrophysics - Study Abroad IV | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20026 | Statistical Mechanics and Solid State Physics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in statistical mechanics and solid-state physics. There is also a laboratory component aimed at enhancing experimental, team-working and communication skills. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-30012 | Electromagnetism | C | M | 7.5 | 15 | |
| Electromagnetism and its applications in Physics, the nature of electromagnetic waves in vacuum and various media, and of magnetism in solids. | ||||||
| PHY-30023 | Particles, Accelerators and Reactor Physics | O | M | 7.5 | 15 | |
| This module covers a range of topics in elementary particle physics, including the ingredients and the physical structure of the Standard Model; lepton phenomenology and neutrino physics; the quark model for the internal structures of baryons and mesons; experimental evidence for quarks; and aspects of quantum chromodynamics and electroweak unification. The module also gives an introduction to the physics and the operation of particle accelerators (both linear and circular) and nuclear reactors (especially thermal fission reactors). It builds upon some fundamentals of special relativity and quantum mechanics, and elements of nuclear physics and particle phenomenology, that all Physics and Astrophysics students will have in common from their core studies at Levels 1 and 2. | ||||||
| PHY-30023 | Particles, Accelerators and Reactor Physics | EP | M | 7.5 | 15 | |
| This module covers a range of topics in elementary particle physics, including the ingredients and the physical structure of the Standard Model; lepton phenomenology and neutrino physics; the quark model for the internal structures of baryons and mesons; experimental evidence for quarks; and aspects of quantum chromodynamics and electroweak unification. The module also gives an introduction to the physics and the operation of particle accelerators (both linear and circular) and nuclear reactors (especially thermal fission reactors). It builds upon some fundamentals of special relativity and quantum mechanics, and elements of nuclear physics and particle phenomenology, that all Physics and Astrophysics students will have in common from their core studies at Levels 1 and 2. | ||||||
| PHY-30028 | Physics of Galaxies | O | M | 7.5 | 15 | |
| This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. No prior knowledge of astronomy is assumed or required. The first half of the module builds on the study of mechanics and Newtonian gravity from Level 1, developing more advanced results that are applied to the structures and dynamics of galaxies, star clusters, and clusters of galaxies. Dark matter is a recurring theme. The second half of the module draws on further core physics from Levels 1 and 2 to calculate physical processes around supermassive black holes in the nuclei of active galaxies, and to analyze aspects of galaxy clusters, large-scale structure, and the first galaxies in the Universe. Contact is made throughout with the Level 3 study of electromagnetism. | ||||||
| PHY-30028 | Physics of Galaxies | EP | M | 7.5 | 15 | |
| This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. No prior knowledge of astronomy is assumed or required. The first half of the module builds on the study of mechanics and Newtonian gravity from Level 1, developing more advanced results that are applied to the structures and dynamics of galaxies, star clusters, and clusters of galaxies. Dark matter is a recurring theme. The second half of the module draws on further core physics from Levels 1 and 2 to calculate physical processes around supermassive black holes in the nuclei of active galaxies, and to analyze aspects of galaxy clusters, large-scale structure, and the first galaxies in the Universe. Contact is made throughout with the Level 3 study of electromagnetism. | ||||||
| Semester 1-2 | C/O | TYP | ECTS | CATS | ||
| # | PHY-30006 | Astrophysics Group Project and Science Communication - ISP | C | C | 7.5 | 15 |
| Students carry out a major project as part of a team activity. Projects are attached to research group and involve development of data analysis and reporting skills. 6 hours laboratory | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-30001 | Cosmology | O | M | 7.5 | 15 | |
| This module explores the key topics on expansion of the universe, cosmic microwave background, structure in the universe, dark matter, inflation and relevance of particle physics to cosmology. | ||||||
| PHY-30001 | Cosmology | EP | M | 7.5 | 15 | |
| This module explores the key topics on expansion of the universe, cosmic microwave background, structure in the universe, dark matter, inflation and relevance of particle physics to cosmology. | ||||||
| PHY-30003 | The Physics of Compact Objects | O | M | 7.5 | 15 | |
| Applications of statistical and quantum physics to stellar structure; white dwarf and neutron stars; pulsars (M15). | ||||||
| PHY-30003 | The Physics of Compact Objects | EP | M | 7.5 | 15 | |
| Applications of statistical and quantum physics to stellar structure; white dwarf and neutron stars; pulsars (M15). | ||||||
| PHY-30029 | Quantum Mechanics II | O | M | 7.5 | 15 | |
| This module will give the students an introduction to exciting applications of quantum mechanics at the cutting-edge of modern physics such as quantum computing and quantum cryptography. The module will also look at the quantum mechanics behind powerful investigative techniques used in laboratories and in astrophysics such as Raman spectroscopy. Fundamental results related to the interpretation of quantum mechanics such as the Aspect experiment will also be discussed. | ||||||
| PHY-30029 | Quantum Mechanics II | EP | M | 7.5 | 15 | |
| This module will give the students an introduction to exciting applications of quantum mechanics at the cutting-edge of modern physics such as quantum computing and quantum cryptography. The module will also look at the quantum mechanics behind powerful investigative techniques used in laboratories and in astrophysics such as Raman spectroscopy. Fundamental results related to the interpretation of quantum mechanics such as the Aspect experiment will also be discussed. | ||||||
| PHY-30030 | Physics of Fluids | O | M | 7.5 | 15 | |
| This module will introduce students to the physics of fluids, which treats objects under study as continuous bodies rather than point particles. Although the physics of fluids is based on very few basic principles (conservation of mass, momentum and energy), the field has immense practical applications in the real world. After introducing the main concepts and laws, these will be applied to selected topics relevant in nature and space (tsunamis, convection and charged plasmas). This module will also introduce the students to computational fluid dynamics, i.e. how to implement fluids dynamics theory into a computer programme in order to solve a problem. Students will then use computer programs to study basic flows. This will provide students with essential skills for their future career in research at post-graduate level or in the industry. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. Successful completion of level 2 in Physics or Astrophysics is the only entry requirement. | ||||||
| PHY-30030 | Physics of Fluids | EP | M | 7.5 | 15 | |
| This module will introduce students to the physics of fluids, which treats objects under study as continuous bodies rather than point particles. Although the physics of fluids is based on very few basic principles (conservation of mass, momentum and energy), the field has immense practical applications in the real world. After introducing the main concepts and laws, these will be applied to selected topics relevant in nature and space (tsunamis, convection and charged plasmas). This module will also introduce the students to computational fluid dynamics, i.e. how to implement fluids dynamics theory into a computer programme in order to solve a problem. Students will then use computer programs to study basic flows. This will provide students with essential skills for their future career in research at post-graduate level or in the industry. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. Successful completion of level 2 in Physics or Astrophysics is the only entry requirement. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-10022 | Mechanics, Gravity and Relativity | C | M | 7.5 | 15 | |
| This level 1 module builds on A-level physics by taking the familiar subject of mechanics, but integrating it into calculus-based mathematics, thus laying the foundation for physics and astrophysics degrees. The module develops skills in applying physical principles and mathematical techniques to physical and astrophysical situations, and to laboratory based experiments. | ||||||
| PHY-10024 | Nature of matter | C | M | 7.5 | 15 | |
| This level 1 module is delivered in the first semester and provides an introduction to the subject material that bridges the gap between pre-university study and the first year of a university Physics/Astrophysics course. It explores the nature of solid and gaseous matter from the classical picture to the need for a quantum description. It sets the stage for more advanced study of quantum physics, thermodynamics and solid state physics in the second year. A mathematics component is included, in which the requisite material is taught in a Physics context. Also included is a laboratory component (which includes experiments on some of the subject matter delivered in lectures). | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-10020 | Oscillations and Waves | C | M | 7.5 | 15 | |
| This Level 1 module runs in the second semester. It explores the physical principles and mathematical description of oscillatory and wave phenomena, which find application in many areas of classical and modern physics and astrophysics. The module requires a firm grasp of material covered in Level 1 Mechanics, and it sets the stage for the treatment of more advanced topics in optics, quantum mechanics, and electromagnetism at Levels 2 and 3. A mathematics component is included, in which fundamental techniques routinely used in physics are taught and practised. There is also a laboratory component, which involves bench work, computing and communication exercises. | ||||||
| PHY-10023 | Electricity and Stellar Structure | C | M | 7.5 | 15 | |
| This level 1 module examines one of the fundamental forces of physics, electromagnetism, developing an understanding of how this applies to widespread physical processes. The course then turns to stars, showing that the physical laws studied in the course so far can be applied straightforwardly to stars, showing why stars behave and evolve as they do, thus developing an understanding of this most ubiquitous of astrophysical objects. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-20004 | Astrophysics - Study Abroad I | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20005 | Astrophysics - Study Abroad II | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20006 | Quantum Mechanics | C | M | 7.5 | 15 | |
| This module aims to introduce the students to quantum theory and its application to atomic physics and to give them the skills to solve the more straightforward problems and applications in these areas. | ||||||
| PHY-20027 | Optics and Thermodynamics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in geometrical optics, physical optics and thermodynamics. There is also a laboratory component, which is aimed at enhancing experimental and communication skills. | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-20002 | Stellar Astrophysics | C | M | 7.5 | 15 | |
| An understanding of the effect of physical processes on the structure and evolution of stars. Nuclear processes in stars and stellar evolution. The origin of elements in stars. 2 hour lecture & one general tutorial per week, plus astrophysics skills | ||||||
| PHY-20022 | Astrophysics - Study Abroad III | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20023 | Astrophysics - Study Abroad IV | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20026 | Statistical Mechanics and Solid State Physics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in statistical mechanics and solid-state physics. There is also a laboratory component aimed at enhancing experimental, team-working and communication skills. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-30012 | Electromagnetism | C | M | 7.5 | 15 | |
| Electromagnetism and its applications in Physics, the nature of electromagnetic waves in vacuum and various media, and of magnetism in solids. | ||||||
| PHY-30023 | Particles, Accelerators and Reactor Physics | O | M | 7.5 | 15 | |
| This module covers a range of topics in elementary particle physics, including the ingredients and the physical structure of the Standard Model; lepton phenomenology and neutrino physics; the quark model for the internal structures of baryons and mesons; experimental evidence for quarks; and aspects of quantum chromodynamics and electroweak unification. The module also gives an introduction to the physics and the operation of particle accelerators (both linear and circular) and nuclear reactors (especially thermal fission reactors). It builds upon some fundamentals of special relativity and quantum mechanics, and elements of nuclear physics and particle phenomenology, that all Physics and Astrophysics students will have in common from their core studies at Levels 1 and 2. | ||||||
| PHY-30023 | Particles, Accelerators and Reactor Physics | EP | M | 7.5 | 15 | |
| This module covers a range of topics in elementary particle physics, including the ingredients and the physical structure of the Standard Model; lepton phenomenology and neutrino physics; the quark model for the internal structures of baryons and mesons; experimental evidence for quarks; and aspects of quantum chromodynamics and electroweak unification. The module also gives an introduction to the physics and the operation of particle accelerators (both linear and circular) and nuclear reactors (especially thermal fission reactors). It builds upon some fundamentals of special relativity and quantum mechanics, and elements of nuclear physics and particle phenomenology, that all Physics and Astrophysics students will have in common from their core studies at Levels 1 and 2. | ||||||
| PHY-30028 | Physics of Galaxies | O | M | 7.5 | 15 | |
| This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. No prior knowledge of astronomy is assumed or required. The first half of the module builds on the study of mechanics and Newtonian gravity from Level 1, developing more advanced results that are applied to the structures and dynamics of galaxies, star clusters, and clusters of galaxies. Dark matter is a recurring theme. The second half of the module draws on further core physics from Levels 1 and 2 to calculate physical processes around supermassive black holes in the nuclei of active galaxies, and to analyze aspects of galaxy clusters, large-scale structure, and the first galaxies in the Universe. Contact is made throughout with the Level 3 study of electromagnetism. | ||||||
| PHY-30028 | Physics of Galaxies | EP | M | 7.5 | 15 | |
| This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. No prior knowledge of astronomy is assumed or required. The first half of the module builds on the study of mechanics and Newtonian gravity from Level 1, developing more advanced results that are applied to the structures and dynamics of galaxies, star clusters, and clusters of galaxies. Dark matter is a recurring theme. The second half of the module draws on further core physics from Levels 1 and 2 to calculate physical processes around supermassive black holes in the nuclei of active galaxies, and to analyze aspects of galaxy clusters, large-scale structure, and the first galaxies in the Universe. Contact is made throughout with the Level 3 study of electromagnetism. | ||||||
| Semester 1-2 | C/O | TYP | ECTS | CATS | ||
| # | PHY-30006 | Astrophysics Group Project and Science Communication - ISP | C | C | 7.5 | 15 |
| Students carry out a major project as part of a team activity. Projects are attached to research group and involve development of data analysis and reporting skills. 6 hours laboratory | ||||||
| PHY-30017 | Dissertation | C | C | 7.5 | 15 | |
| A core module for Astrophysics majors. Use of a variety of library resources and the presentation of scientific information in the form of a paper, poster and talk. A 4,000 word dissertation is written on an approved astrophysics topic and poster and seminar presentations are made. | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-30001 | Cosmology | O | M | 7.5 | 15 | |
| This module explores the key topics on expansion of the universe, cosmic microwave background, structure in the universe, dark matter, inflation and relevance of particle physics to cosmology. | ||||||
| PHY-30001 | Cosmology | EP | M | 7.5 | 15 | |
| This module explores the key topics on expansion of the universe, cosmic microwave background, structure in the universe, dark matter, inflation and relevance of particle physics to cosmology. | ||||||
| PHY-30003 | The Physics of Compact Objects | O | M | 7.5 | 15 | |
| Applications of statistical and quantum physics to stellar structure; white dwarf and neutron stars; pulsars (M15). | ||||||
| PHY-30003 | The Physics of Compact Objects | EP | M | 7.5 | 15 | |
| Applications of statistical and quantum physics to stellar structure; white dwarf and neutron stars; pulsars (M15). | ||||||
| PHY-30029 | Quantum Mechanics II | O | M | 7.5 | 15 | |
| This module will give the students an introduction to exciting applications of quantum mechanics at the cutting-edge of modern physics such as quantum computing and quantum cryptography. The module will also look at the quantum mechanics behind powerful investigative techniques used in laboratories and in astrophysics such as Raman spectroscopy. Fundamental results related to the interpretation of quantum mechanics such as the Aspect experiment will also be discussed. | ||||||
| PHY-30029 | Quantum Mechanics II | EP | M | 7.5 | 15 | |
| This module will give the students an introduction to exciting applications of quantum mechanics at the cutting-edge of modern physics such as quantum computing and quantum cryptography. The module will also look at the quantum mechanics behind powerful investigative techniques used in laboratories and in astrophysics such as Raman spectroscopy. Fundamental results related to the interpretation of quantum mechanics such as the Aspect experiment will also be discussed. | ||||||
| PHY-30030 | Physics of Fluids | O | M | 7.5 | 15 | |
| This module will introduce students to the physics of fluids, which treats objects under study as continuous bodies rather than point particles. Although the physics of fluids is based on very few basic principles (conservation of mass, momentum and energy), the field has immense practical applications in the real world. After introducing the main concepts and laws, these will be applied to selected topics relevant in nature and space (tsunamis, convection and charged plasmas). This module will also introduce the students to computational fluid dynamics, i.e. how to implement fluids dynamics theory into a computer programme in order to solve a problem. Students will then use computer programs to study basic flows. This will provide students with essential skills for their future career in research at post-graduate level or in the industry. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. Successful completion of level 2 in Physics or Astrophysics is the only entry requirement. | ||||||
| PHY-30030 | Physics of Fluids | EP | M | 7.5 | 15 | |
| This module will introduce students to the physics of fluids, which treats objects under study as continuous bodies rather than point particles. Although the physics of fluids is based on very few basic principles (conservation of mass, momentum and energy), the field has immense practical applications in the real world. After introducing the main concepts and laws, these will be applied to selected topics relevant in nature and space (tsunamis, convection and charged plasmas). This module will also introduce the students to computational fluid dynamics, i.e. how to implement fluids dynamics theory into a computer programme in order to solve a problem. Students will then use computer programs to study basic flows. This will provide students with essential skills for their future career in research at post-graduate level or in the industry. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. Successful completion of level 2 in Physics or Astrophysics is the only entry requirement. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-10022 | Mechanics, Gravity and Relativity | C | M | 7.5 | 15 | |
| This level 1 module builds on A-level physics by taking the familiar subject of mechanics, but integrating it into calculus-based mathematics, thus laying the foundation for physics and astrophysics degrees. The module develops skills in applying physical principles and mathematical techniques to physical and astrophysical situations, and to laboratory based experiments. | ||||||
| PHY-10024 | Nature of matter | C | M | 7.5 | 15 | |
| This level 1 module is delivered in the first semester and provides an introduction to the subject material that bridges the gap between pre-university study and the first year of a university Physics/Astrophysics course. It explores the nature of solid and gaseous matter from the classical picture to the need for a quantum description. It sets the stage for more advanced study of quantum physics, thermodynamics and solid state physics in the second year. A mathematics component is included, in which the requisite material is taught in a Physics context. Also included is a laboratory component (which includes experiments on some of the subject matter delivered in lectures). | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-10020 | Oscillations and Waves | C | M | 7.5 | 15 | |
| This Level 1 module runs in the second semester. It explores the physical principles and mathematical description of oscillatory and wave phenomena, which find application in many areas of classical and modern physics and astrophysics. The module requires a firm grasp of material covered in Level 1 Mechanics, and it sets the stage for the treatment of more advanced topics in optics, quantum mechanics, and electromagnetism at Levels 2 and 3. A mathematics component is included, in which fundamental techniques routinely used in physics are taught and practised. There is also a laboratory component, which involves bench work, computing and communication exercises. | ||||||
| PHY-10023 | Electricity and Stellar Structure | C | M | 7.5 | 15 | |
| This level 1 module examines one of the fundamental forces of physics, electromagnetism, developing an understanding of how this applies to widespread physical processes. The course then turns to stars, showing that the physical laws studied in the course so far can be applied straightforwardly to stars, showing why stars behave and evolve as they do, thus developing an understanding of this most ubiquitous of astrophysical objects. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-20004 | Astrophysics - Study Abroad I | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20005 | Astrophysics - Study Abroad II | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20006 | Quantum Mechanics | C | M | 7.5 | 15 | |
| This module aims to introduce the students to quantum theory and its application to atomic physics and to give them the skills to solve the more straightforward problems and applications in these areas. | ||||||
| PHY-20027 | Optics and Thermodynamics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in geometrical optics, physical optics and thermodynamics. There is also a laboratory component, which is aimed at enhancing experimental and communication skills. | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-20002 | Stellar Astrophysics | C | M | 7.5 | 15 | |
| An understanding of the effect of physical processes on the structure and evolution of stars. Nuclear processes in stars and stellar evolution. The origin of elements in stars. 2 hour lecture & one general tutorial per week, plus astrophysics skills | ||||||
| PHY-20022 | Astrophysics - Study Abroad III | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20023 | Astrophysics - Study Abroad IV | EP | C | 7.5 | 15 | |
| This is a module that is automatically allocated to the records our Keele level II students who are going to Study Abroad at a partner University for a semester of their second year and cannot be selected by any other level II students. | ||||||
| PHY-20026 | Statistical Mechanics and Solid State Physics | C | M | 7.5 | 15 | |
| This module explores the theory and applications of the key topics in statistical mechanics and solid-state physics. There is also a laboratory component aimed at enhancing experimental, team-working and communication skills. | ||||||
| Semester 1 | C/O | TYP | ECTS | CATS | ||
| PHY-30023 | Particles, Accelerators and Reactor Physics | EP | M | 7.5 | 15 | |
| This module covers a range of topics in elementary particle physics, including the ingredients and the physical structure of the Standard Model; lepton phenomenology and neutrino physics; the quark model for the internal structures of baryons and mesons; experimental evidence for quarks; and aspects of quantum chromodynamics and electroweak unification. The module also gives an introduction to the physics and the operation of particle accelerators (both linear and circular) and nuclear reactors (especially thermal fission reactors). It builds upon some fundamentals of special relativity and quantum mechanics, and elements of nuclear physics and particle phenomenology, that all Physics and Astrophysics students will have in common from their core studies at Levels 1 and 2. | ||||||
| PHY-30028 | Physics of Galaxies | EP | M | 7.5 | 15 | |
| This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. No prior knowledge of astronomy is assumed or required. The first half of the module builds on the study of mechanics and Newtonian gravity from Level 1, developing more advanced results that are applied to the structures and dynamics of galaxies, star clusters, and clusters of galaxies. Dark matter is a recurring theme. The second half of the module draws on further core physics from Levels 1 and 2 to calculate physical processes around supermassive black holes in the nuclei of active galaxies, and to analyze aspects of galaxy clusters, large-scale structure, and the first galaxies in the Universe. Contact is made throughout with the Level 3 study of electromagnetism. | ||||||
| Semester 2 | C/O | TYP | ECTS | CATS | ||
| PHY-30001 | Cosmology | EP | M | 7.5 | 15 | |
| This module explores the key topics on expansion of the universe, cosmic microwave background, structure in the universe, dark matter, inflation and relevance of particle physics to cosmology. | ||||||
| PHY-30003 | The Physics of Compact Objects | EP | M | 7.5 | 15 | |
| Applications of statistical and quantum physics to stellar structure; white dwarf and neutron stars; pulsars (M15). | ||||||
| PHY-30029 | Quantum Mechanics II | EP | M | 7.5 | 15 | |
| This module will give the students an introduction to exciting applications of quantum mechanics at the cutting-edge of modern physics such as quantum computing and quantum cryptography. The module will also look at the quantum mechanics behind powerful investigative techniques used in laboratories and in astrophysics such as Raman spectroscopy. Fundamental results related to the interpretation of quantum mechanics such as the Aspect experiment will also be discussed. | ||||||
| PHY-30030 | Physics of Fluids | EP | M | 7.5 | 15 | |
| This module will introduce students to the physics of fluids, which treats objects under study as continuous bodies rather than point particles. Although the physics of fluids is based on very few basic principles (conservation of mass, momentum and energy), the field has immense practical applications in the real world. After introducing the main concepts and laws, these will be applied to selected topics relevant in nature and space (tsunamis, convection and charged plasmas). This module will also introduce the students to computational fluid dynamics, i.e. how to implement fluids dynamics theory into a computer programme in order to solve a problem. Students will then use computer programs to study basic flows. This will provide students with essential skills for their future career in research at post-graduate level or in the industry. This optional core module is open to students in Level 3 of any degree programme in Physics or Astrophysics. Successful completion of level 2 in Physics or Astrophysics is the only entry requirement. | ||||||