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Overview

Techniques and applications of classical mechanics: calculus of variations, Lagrangian and Hamiltonian formulations. The special theory of relativity with application in relativistic mechanics. Cosmology.

This paper presents the foundational theory for two major topics in physics. The classical mechanics section introduces the formal framework of classical mechanics and illustrates its application to two-body problems, oscillating systems and non-inertial frames, such as rotating systems. The special relativity and cosmology section covers the special theory of relativity with applications to relativistic mechanics as well as an introduction to cosmology. This paper is taught jointly by staff from the Department of Physics and the Department of Mathematics and Statistics.

About this paper

Paper title Mathematical Physics
Subject Physics
EFTS 0.15
Points 18 points
Teaching period Semester 2 (On campus)
Domestic Tuition Fees ( NZD ) $1,318.20
International Tuition Fees Tuition Fees for international students are elsewhere on this website.
Prerequisite
MATH 203 and 36 300-level PHSI or MATH points
Restriction
MATH 374
Recommended Preparation
(PHSI 221 and PHSI 222) and COMO 204
Schedule C
Science
Contact
terry.scott@otago.ac.nz
Teaching staff

Course Co-ordinator: Dr Terry Scott
Dr Florian Beyer
Dr Jörg Frauendiener

Textbooks
Classical Mechanics, John Taylor.
Graduate Attributes Emphasised
Global perspective, Interdisciplinary perspective, Lifelong learning, Scholarship, Communication, Critical thinking, Information literacy, Self-motivation, Teamwork.
View more information about Otago's graduate attributes.
Learning Outcomes

After completing this paper students will be able to:

  • Understand and use the calculus of variations, particularly in the derivation of the Lagrangian formulation of classical mechanics
  • Understand and use the Hamiltonian and Lagrangian formulations of classical mechanics and how they are related
  • Use the principles of classical mechanics to analyse standard systems, such as two-body central force problems and the rotation of rigid bodies
  • Understand the principles of special relativity and the representation of these principles in the Lorentz Transformation and covariant formalism
  • Solve problems in relativistic mechanics using these principles
  • Understand the introductory ideas of cosmology

Overview

Techniques and applications of classical mechanics: calculus of variations, Lagrangian and Hamiltonian formulations. The special theory of relativity with application in relativistic mechanics. Cosmology.

This paper presents the foundational theory for two major topics in physics. The classical mechanics section introduces the formal framework of classical mechanics and illustrates its application to two-body problems, oscillating systems and non-inertial frames, such as rotating systems. The special relativity and cosmology section covers the special theory of relativity with applications to relativistic mechanics as well as an introduction to cosmology. This paper is taught jointly by staff from the Department of Physics and the Department of Mathematics and Statistics.

About this paper

Paper title Mathematical Physics
Subject Physics
EFTS 0.15
Points 18 points
Teaching period Semester 2 (On campus)
Domestic Tuition Fees Tuition Fees for 2027 have not yet been set
International Tuition Fees Tuition Fees for international students are elsewhere on this website.
Prerequisite
MATH 203 and 36 300-level PHSI or MATH points
Restriction
MATH 374
Recommended Preparation
(PHSI 221 and PHSI 222) and COMO 204
Schedule C
Science
Contact
terry.scott@otago.ac.nz
Teaching staff

Course Co-ordinator: Dr Terry Scott
Associate Professor Florian Beyer
Professor Jörg Frauendiener

Textbooks
Classical Mechanics, John Taylor.
Graduate Attributes Emphasised
Global perspective, Interdisciplinary perspective, Lifelong learning, Scholarship, Communication, Critical thinking, Information literacy, Self-motivation, Teamwork.
View more information about Otago's graduate attributes.
Learning Outcomes

After completing this paper students will be able to:

  • Understand and use the calculus of variations, particularly in the derivation of the Lagrangian formulation of classical mechanics
  • Understand and use the Hamiltonian and Lagrangian formulations of classical mechanics and how they are related
  • Use the principles of classical mechanics to analyse standard systems, such as two-body central force problems and the rotation of rigid bodies
  • Understand the principles of special relativity and the representation of these principles in the Lorentz Transformation and covariant formalism
  • Solve problems in relativistic mechanics using these principles
  • Understand the introductory ideas of cosmology
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