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Coleman–Weinberg potential

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The Coleman–Weinberg model represents quantum electrodynamics of a scalar field in four-dimensions. The Lagrangian for the model is

L=−14(Fμν)2+|Dμϕ|2−m2|ϕ|2−λ6|ϕ|4

where the scalar field is complex, Fμν=∂μAν−∂νAμ is the electromagnetic field tensor, and Dμ=∂μ−i(e/ℏc)Aμ the covariant derivative containing the electric charge e of the electromagnetic field.

Assume that λ is nonnegative. Then if the mass term is tachyonic, m2<0 there is a spontaneous breaking of the gauge symmetry at low energies, a variant of the Higgs mechanism. On the other hand, if the squared mass is positive, m2>0 the vacuum expectation of the field ϕ is zero. At the classical level the latter is true also if m2=0. However, as was shown by Sidney Coleman and Erick Weinberg, even if the renormalized mass is zero, spontaneous symmetry breaking still happens due to the radiative corrections (this introduces a mass scale into a classically conformal theory - the model has a conformal anomaly).

The same can happen in other gauge theories. In the broken phase the fluctuations of the scalar field ϕ will manifest themselves as a naturally light Higgs boson, as a matter of fact even too light to explain the electroweak symmetry breaking in the minimal model - much lighter than vector bosons. There are non-minimal models that give a more realistic scenarios. Also the variations of this mechanism were proposed for the hypothetical spontaneously broken symmetries including supersymmetry.

Equivalently one may say that the model possesses a first-order phase transition as a function of m2. The model is the four-dimensional analog of the three-dimensional Ginzburg–Landau theory used to explain the properties of superconductors near the phase transition.

The three-dimensional version of the Coleman–Weinberg model governs the superconducting phase transition which can be both first- and second-order, depending on the ratio of the Ginzburg–Landau parameter κ≡λ/e2, with a tricritical point near κ=1/2 which separates type I from type II superconductivity. Historically, the order of the superconducting phase transition was debated for a long time since the temperature interval where fluctuations are large (Ginzburg interval) is extremely small. The question was finally settled in 1982.[1] If the Ginzburg–Landau parameter κ that distinguishes type-I and type-II superconductors (see also here) is large enough, vortex fluctuations becomes important which drive the transition to second order. The tricritical point lies at roughly κ=0.76/2, i.e., slightly below the value κ=1/2 where type-I goes over into type-II superconductor. The prediction was confirmed in 2002 by Monte Carlo computer simulations.[2]

Literature

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  • S. Coleman and E. Weinberg (1973). "Radiative Corrections as the Origin of Spontaneous Symmetry Breaking". Physical Review D. 7 (6): 1888–1910. arXiv:hep-th/0507214. Bibcode:1973PhRvD...7.1888C. doi:10.1103/PhysRevD.7.1888. S2CID 6898114.
  • L.D. Landau (1937). "On the theory of phase transitions. II". Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki. 7: 627.
  • V.L. Ginzburg and L.D. Landau (2009). "On the Theory of Superconductivity". On Superconductivity and Superfluidity. pp. 113–137. doi:10.1007/978-3-540-68008-6_4. ISBN 978-3-540-68004-8.
  • M.Tinkham (2004). Introduction to Superconductivity. Dover Books on Physics (2nd ed.). Dover. ISBN 0-486-43503-2.

See also

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References

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