nLab gauge coupling unification

Contents

Context

Physics

physics, mathematical physics, philosophy of physics

Surveys, textbooks and lecture notes


theory (physics), model (physics)

experiment, measurement, computable physics

Contents

Idea

The renormalization group flow of the coupling constants (“running coupling constants”) of the three gauge forces of the standard model of particle physics come close to all intersecting at a single point at some high energy. This observation has led to the speculation that there ought to be a refinement of the standard model such as GUT-theories and/or supersymmetry-extensions such as the MSSM in which the gauge coupling constants unify exactly at high energy. This idea is called gauge coupling unification.

Surveys include Uzan, section 5.3.1

From Ellis-Wells 15, p. 2:

Famously, the Standard Model (SM) does not unify under that rubric but the Minimal Supersymmetric Standard Model (MSSM) does according to many [1–7]. However, neither statement is true. The SM cannot be ruled out as the IR manifestation of a Grand Unified Theory (GUT), nor do the three gauge couplings meet at precisely one point in the MSSM. The key to understanding both claims is that high-scale thresholds are generically expected, which are the multiplets at the high scale that get masses by the same mechanism that breaks the GUT symmetry. High-scale threshold corrections kick the couplings further into exact unification if the underlying theory is gauge-coupling unified.

and further from Ellis-Wells 17, p. 23 to 26:

Thus, even the Standard Model up to the high scale is compatible with gauge coupling unification from this perspective, although the corrections becomes quite large in that case, and one has to ask whether nature would rather have large corrections at the GUT scale for a SM GUT or very small corrections for a low-scale SUSY GUT.

[...][...] the introduction of supersymmetry both reduces the needed threshold corrections at the high-scale and increases the GUT scale [...][...]. This latter element is helpful since one generally requires that the GUT scale be above about 10 1510^{15} GeV so that the XX,YY GUT gauge bosons do not induce too large dimension-six operators that cause the proton to decay faster than current limits allow.

Thus, exact gauge coupling unification is viable for intermediate values of supersymmetry breaking, which are also compatible with the Higgs boson mass constraint.

[...][...]

One important experimental prediction of minimal supersymmetry, even for superpartners at very high scales, is the existence of a relatively light Higgs boson. This has been seen by the LHC. We have shown in this paper that even arbitrary high scales of super-partners allow the light Higgs boson, due to the required matching of the SM effective theory Higgs self-interaction coupling to gauge couplings in the supersymmetric theory.

We have discussed how gauge coupling unification generally only improves in a supersymmetric theory, even at very high scales, with respect to the SM. Thus, we find that PeV scale [23–27] or intermediate scale supersymmetry [3, 5], two ideas that are prevalent in the literature for other reasons involving dark matter and neutrino physics, are compatible with the Higgs boson constraint and gauge coupling unification under the conditions described above.

References

Reviews include (roughly in increasing order of technical detail)

  • Savas Dimopoulos, Stuart Raby, Frank Wilczek, Unification of couplings, Physics Today, October 1991 pdf

  • Sander Mooij, section 1.3.4 of Supersymmetric Grand unification, 2008 (pdf)

  • Jean-Philippe Uzan, section 5.3.1 of Varying Constants, Gravitation and Cosmology, Living Reviews in Relativity (arXiv:1009.5514)

  • Sebastian A. R. Ellis, James Wells, Visualizing gauge unification with high-scale thresholds, Phys. Rev. D 91, 075016 (2015) (arXiv:1502.01362)

  • Sebastian A. R. Ellis, James Wells, High-scale Supersymmetry, the Higgs Mass and Gauge Unification, Phys. Rev. D 96, 055024 (2017) (arXiv:1706.00013)

Original articles:

Potential relation to flavour anomalies:

  • Purushottam Sahu, Aishwarya Bhatta, Rukmani Mohanta, Shivaramakrishna Singirala, Sudhanwa Patra, Flavour anomalies and dark matter assisted unification in SO(10)SO(10) GUT [arXiv:2204.06392]

Last revised on October 26, 2022 at 03:53:14. See the history of this page for a list of all contributions to it.