Coleman–Weinberg potential

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

$L=-{\frac {1}{4}}(F_{{\mu \nu }})^{2}+(D_{{\mu }}\phi )^{2}-m^{2}\phi ^{2}-{\frac {\lambda }{6}}\phi ^{4}$

where the scalar field is complex, $F_{{\mu \nu }}=\partial _{\mu }A_{\nu }-\partial _{\nu }A_{\mu }$ is the electromagnetic field tensor, and $D_{\mu }=\partial _{\mu }-\mathrm {i} (e/\hbar c)A_{\mu }$ the covariant derivative containing the electric charge $e$ of the electromagnetic field.

Assume that $\lambda$ is nonnegative. Then if the mass term is tachyonic, $m^{2}<0$ 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, $m^{2}>0$ the vacuum expectation of the field $\phi$ is zero. At the classical level the latter is true also if $m^{2}=0$ 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 - model have a conformal anomaly).

The same can happen in other gauge theories. In the broken phase the fluctuations of the scalar field $\phi$ 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 $m^{2}$ . 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 $\kappa \equiv \lambda /e^{2}$ , with a tricritical point near $\kappa =1/{\sqrt 2}$ 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 $\kappa$ 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 tricitical point lies at roughly $\kappa =0.76/{\sqrt {2}}$ , i.e., slightly below the value $\kappa =1/{\sqrt {2}}$ where type-I goes over into type-II superconductor. The prediction was confirmed in 2002 by Monte Carlo computer simulations.^[2]

Literature

S. Coleman and E. Weinberg (1973). "Radiative Corrections as the Origin of Spontaneous Symmetry Breaking". Physical Review D. 7: 1888. Bibcode:1973PhRvD...7.1888C. doi:10.1103/PhysRevD.7.1888.
L.D. Landau (1937). Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki. 7: 627. Missing or empty |title= (help)
V.L. Ginzburg and L.D. Landau (1950). Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki. 20: 1064. Missing or empty |title= (help)
M.Tinkham (2004). Introduction to Superconductivity. Dover Books on Physics (2nd ed.). Dover. ISBN 0-486-43503-2.

References

↑ H. Kleinert (1982). "Disorder Version of the Abelian Higgs Model and the Order of the Superconductive Phase Transition" (PDF). Lett. Nuovo Cimento. 35: 405–412. doi:10.1007/BF02754760.
↑ J. Hove; S. Mo; A. Sudbo (2002). "Vortex interactions and thermally induced crossover from type-I to type-II superconductivity" (PDF). Phys. Rev. B 66: 064524. arXiv:cond-mat/0202215. Bibcode:2002PhRvB..66f4524H. doi:10.1103/PhysRevB.66.064524.

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