Abstract

Perhaps the most important aspect of symmetry in physics is the idea that a state does not need to have the same symmetries as the theory that describes it. This phenomenon is known as spontaneous symmetry breaking. In these lecture notes, starting from a careful definition of symmetry in physics, we introduce symmetry breaking and its consequences. Emphasis is placed on the physics of singular limits, showing the reality of symmetry breaking even in small-sized systems. Topics covered include Nambu-Goldstone modes, quantum corrections, phase transitions, topological defects and gauge fields. We provide many examples from both high energy and condensed matter physics. These notes are suitable for graduate students.

Highlights

  • We need to distinguish between, on the one hand, the symmetries of the laws of nature, equations of motion, and the action or Hamiltonian, and on the other hand, the symmetries of states, objects, and solutions to the equations of motion. This distinction lies at the core of spontaneous symmetry breaking, which is said to occur whenever a physical state or object has less symmetry than the laws of nature that govern it

  • You cannot measure the position of a crystal with respect to a uniform fluid permeating all of space, and it is not possible to measure a direction of magnetisation with a piece of plastic that cannot itself be magnetised. This might seem obvious for crystals and magnets, one could wonder what it implies for materials hosting less intuitive forms of broken symmetry, like the U(1) phase-rotation symmetry associated with conserved particle number, which we argued in Section 2.5.2 to be broken in superfluids? This question found a literal manifestation in the spontaneous tunnelling current that was predicted by Josephson in 1962 to occur between two separated pieces of superconducting material [29]

  • The small and local perturbation will not affect the average value of the order parameter, o, which is equal to the value we found in the uniform Landau theory, Eq (5.2)

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Summary

Definition

Before talking about the breaking of symmetry, we need to define and understand what is meant by symmetry itself. We need to distinguish between, on the one hand, the symmetries of the laws of nature, equations of motion, and the action or Hamiltonian, and on the other hand, the symmetries of states, objects, and solutions to the equations of motion. This distinction lies at the core of spontaneous symmetry breaking, which is said to occur whenever a physical state or object has less symmetry than the laws of nature that govern it

Symmetries of states
Symmetries of Hamiltonians
Noether’s theorem
Conserved quantities
Continuity equations
Proving Noether’s theorem
Noether charge
Schrödinger field
Relativistic complex scalar field
Spacetime translations
Types of symmetry transformations
Symmetry breaking
Nambu–Goldstone modes
Quantum corrections and thermal fluctuations
Y -model
Phase transitions
Topological defects
Topological solitons and skyrmions critical slowing down
Gauge fields
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