Spontaneous symmetry breaking is a process where a symmetric system transitions into an asymmetric ground state.Spontaneous symmetry breaking (SSB) occurs when the ground state (vacuum) of a system is less symmetric than the equations describing it. The classic model is the 'Mexican hat' potential: the energy minimum is not at the center but on a circle of equally possible states. By randomly choosing one, the system generates massless excitations (Goldstone bosons). In gauge theories such as the electroweak theory, these bosons are 'eaten' by fields, becoming their longitudinal components and giving them mass (the Higgs mechanism). In a ferromagnet, rotational symmetry is broken, and the Goldstone bosons are magnons—magnetization waves.
The idea of spontaneous symmetry breaking goes back to Werner Heisenberg's theory of ferromagnetism in the 1920s and Lev Landau's theory of phase transitions (1937). In 1961, Yoichiro Nambu and Giovanni Jona-Lasinio built a model of chiral symmetry breaking in hadrons. In 1964, Peter Higgs, as well as François Englert and Robert Brout, showed how to combine SSB with gauge invariance, solving the problem of gauge boson masses. Emmy Noether had earlier in 1918 proved the fundamental connection between symmetries and conservation laws, which formed the basis for understanding broken symmetries.
Consider the Lagrangian L = (∂_μ Φ)* (∂^μ Φ) - V(Φ) with the potential V(Φ) = -μ^2 |Φ|^2 + λ |Φ|^4. The minima lie on the circle |Φ| = v = √(μ^2/(2λ)). Choosing a specific direction for the vacuum expectation value ⟨Φ⟩ = v breaks the U(1) symmetry. Parameterizing Φ = (v + h) e^{iθ/v} reveals a massive field h (the Higgs particle) and a massless field θ (the Goldstone boson). In the presence of a gauge field A_μ, the covariant derivative D_μ Φ = ∂_μ Φ - i e A_μ Φ leads to the field θ being absorbed, becoming the longitudinal mode of A_μ, which acquires the mass m_A = e v. Thus, like a ball rolling into one of the valleys, the vacuum chooses a specific state, and this choice determines the properties of elementary particles.
Thanks to this mechanism, particles gain mass, magnets stick to refrigerators, and superconducting magnets work in tomographs.
In the expanding Universe, spontaneous symmetry breaking could have produced cosmic strings—filament-like defects as thin as a proton but millions of light-years long. The search for them continues through light distortions from distant galaxies.
| N | variable | number of particles — particle number |
| p | variable | momentum — momentum kilogram metre per second |
| C | variable | normalization constant |
| Γ | variable | spectral index |
| p_b | variable | break momentum — momentum kilogram metre per second |
| Γ_1 | variable | low-energy spectral index |
| Γ_2 | variable | high-energy spectral index |
| s | variable | smoothness parameter |
| d/dp | operator | derivative with respect to momentum — derivative |












