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Strong CP problem

From Wikipedia, the free encyclopedia
Question of why quantum chromodynamics does seem to not break CP-symmetry

Thestrong CP problem is a question inparticle physics, which brings up the following quandary: why doesquantum chromodynamics (QCD) seem to preserveCP-symmetry?

In particle physics,CP stands for the combination ofC-symmetry (charge conjugation symmetry) andP-symmetry (parity symmetry). According to the current mathematical formulation of quantum chromodynamics, aviolation of CP-symmetry instrong interactions could occur. However, no violation of the CP-symmetry has ever been seen in any experiment involving only the strong interaction. As there is no known reason in QCD for it to necessarily be conserved, this is a "fine tuning" problem known as thestrong CP problem.

The strong CP problem is sometimes regarded as anunsolved problem in physics, and has been referred to as "the most underrated puzzle in all of physics."[1][2] There are several proposed solutions to solve the strong CP problem. The most well-known isPeccei–Quinn theory,[3] involving newpseudoscalar particles calledaxions.

Theory

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CP-symmetry states that physics should be unchanged if particles were swapped with their antiparticles and then left-handed and right-handed particles were also interchanged. This corresponds to performing a charge conjugation transformation and then a parity transformation. The symmetry is known to be broken in theStandard Model throughweak interactions, but it is also expected to be broken throughstrong interactions which governquantum chromodynamics (QCD), something that has not yet been observed.

To illustrate how the CP violation can come about in QCD, consider aYang–Mills theory with a single massivequark.[4] The most general mass term possible for the quark is a complex mass written asmeiθγ5{\displaystyle me^{i\theta '\gamma _{5}}} for some arbitrary phaseθ{\displaystyle \theta '}. In that case theLagrangian describing the theory consists of four terms:

L=14FμνFμν+θg232π2FμνF~μν+ψ¯(iγμDμmeiθγ5)ψ.{\displaystyle {\mathcal {L}}=-{\frac {1}{4}}F_{\mu \nu }F^{\mu \nu }+\theta {\frac {g^{2}}{32\pi ^{2}}}F_{\mu \nu }{\tilde {F}}^{\mu \nu }+{\bar {\psi }}(i\gamma ^{\mu }D_{\mu }-me^{i\theta '\gamma _{5}})\psi .}

The first and third terms are the CP-symmetrickinetic terms of thegauge and quark fields. The fourth term is the quark mass term which is CP violating for non-zero phasesθ0{\displaystyle \theta '\neq 0} while the second term is the so-calledθ-term or “vacuum angle”, which also violates CP-symmetry.

Quark fields can always be redefined by performing a chiral transformation by some angleα{\displaystyle \alpha } as

ψ=eiαγ5/2ψ,      ψ¯=ψ¯eiαγ5/2,{\displaystyle \psi '=e^{i\alpha \gamma _{5}/2}\psi ,\ \ \ \ \ \ {\bar {\psi }}'={\bar {\psi }}e^{i\alpha \gamma _{5}/2},}

which changes the complex mass phase byθθα{\displaystyle \theta '\rightarrow \theta '-\alpha } while leaving the kinetic terms unchanged. The transformation also changes the θ-term asθθ+α{\displaystyle \theta \rightarrow \theta +\alpha } due to a change in thepath integral measure, an effect closely connected to thechiral anomaly.

The theory would be CP invariant if one could eliminate both sources of CP violation through such a field redefinition. But this cannot be done unlessθ=θ{\displaystyle \theta =-\theta '}. This is because even under such field redefinitions, the combinationθ+θ(θα)+(θ+α)=θ+θ{\displaystyle \theta '+\theta \rightarrow (\theta '-\alpha )+(\theta +\alpha )=\theta '+\theta } remains unchanged. For example, the CP violation due to the mass term can be eliminated by pickingα=θ{\displaystyle \alpha =\theta '}, but then all the CP violation goes to the θ-term which is now proportional toθ¯{\displaystyle {\bar {\theta }}}. If instead the θ-term is eliminated through a chiral transformation, then there will be a CP violating complex mass with a phaseθ¯{\displaystyle {\bar {\theta }}}. Practically, it is usually useful to put all the CP violation into the θ-term and thus only deal with real masses.

In the Standard Model where one deals with six quarks whose masses are described by theYukawa matricesYu{\displaystyle Y_{u}} andYd{\displaystyle Y_{d}}, the physical CP violating angle isθ¯=θargdet(YuYd){\displaystyle {\bar {\theta }}=\theta -\arg \det(Y_{u}Y_{d})}. Since the θ-term has no contributions to perturbation theory, all effects from strong CP violation is entirely non-perturbative. Notably, it gives rise to aneutron electric dipole moment[5]

dN=(5.2×1016ecm)θ¯.{\displaystyle d_{N}=(5.2\times 10^{-16}{\text{e}}\cdot {\text{cm}}){\bar {\theta }}.}

Current experimental upper bounds on the dipole moment give an upper bound ofdN<1026e{\displaystyle d_{N}<10^{-26}{\text{e}}\cdot }cm,[6] which requiresθ¯<1010{\displaystyle {\bar {\theta }}<10^{-10}}. The angleθ¯{\displaystyle {\bar {\theta }}} can take any value between zero and2π{\displaystyle 2\pi }, so it taking on such a particularly small value is a fine-tuning problem called the strong CP problem.

Proposed solutions

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The strong CP problem is solved automatically if one of the quarks is massless.[7] In that case one can perform a set of chiral transformations on all the massive quark fields to get rid of their complex mass phases and then perform another chiral transformation on the massless quark field to eliminate the residual θ-term without also introducing a complex mass term for that field. This then gets rid of all CP violating terms in the theory. The problem with this solution is that all quarks are known to be massive from experimental matching withlattice calculations. Even if one of the quarks was essentially massless to solve the problem, this would in itself just be another fine-tuning problem since there is nothing requiring a quark mass to take on such a small value.

The most popular solution to the problem is through the Peccei–Quinn mechanism.[8] This introduces a new globalanomalous symmetry which is thenspontaneously broken at low energies, giving rise to apseudo-Goldstone boson called an axion. The axion ground state dynamically forces the theory to be CP-symmetric by settingθ¯=0{\displaystyle {\bar {\theta }}=0}. Axions are also considered viable candidates fordark matter and axion-like particles are also predicted bystring theory.

Other less popular proposed solutions exist such as Nelson–Barr models.[9][10] These setθ¯=0{\displaystyle {\bar {\theta }}=0} at some high energy scale where CP-symmetry is exact but the symmetry is then spontaneously broken. The Nelson–Barr mechanism is a way of explaining whyθ¯{\displaystyle {\bar {\theta }}} remains small at low energies while the CP breaking phase in theCKM matrix is large.

See also

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References

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  1. ^Mannel, T. (2–8 July 2006)."Theory and Phenomenology of CP Violation"(PDF).Nuclear Physics B. The 7th International Conference on Hyperons, Charm, and Beauty Hadrons (BEACH 2006). Vol. 167. Lancaster: Elsevier. pp. 170–174.Bibcode:2007NuPhS.167..170M.doi:10.1016/j.nuclphysbps.2006.12.083. Retrieved15 Aug 2015.
  2. ^"The 'Strong CP Problem' is the Most Underrated Puzzle in All of Physics".Forbes.
  3. ^Peccei, R.D.;Quinn, H.R. (1977)."CP conservation in the presence of pseudoparticles".Physical Review Letters.38 (25):1440–1443.Bibcode:1977PhRvL..38.1440P.doi:10.1103/PhysRevLett.38.1440.
  4. ^Wu, D. (1991).A Brief Introduction to the Strong CP Problem. Austin, Texas, United States. SSCL-548.
  5. ^Schwartz, M.D. (2014). "29".Quantum Field Theory and the Standard Model. Cambridge University Press. p. 612.ISBN 9781107034730.
  6. ^Baker, C.A.; Doyle, D.D.; Geltenbort, P.; Green, K.; van der Grinten, M.G.D.; Harris, P.G.; Iaydjiev, P.; Ivanov, S.N.; May, D.J.R. (27 September 2006). "Improved experimental limit on the electric dipole moment of the neutron".Physical Review Letters.97 (13): 131801.arXiv:hep-ex/0602020.Bibcode:2006PhRvL..97m1801B.doi:10.1103/PhysRevLett.97.131801.PMID 17026025.S2CID 119431442.
  7. ^Hook, A. (2019-07-22)."TASI Lectures on the Strong CP Problem and Axions".Proceedings of Science.333: 004.arXiv:1812.02669.doi:10.22323/1.333.0004.S2CID 119073163. Retrieved2021-12-02.
  8. ^Peccei, R. D. (2008). "The Strong CP Problem and Axions". In Kuster, M.; Raffelt, G.; Beltrán, B. (eds.).Axions: Theory, Cosmology, and Experimental Searches. Lecture Notes in Physics. Vol. 741. pp. 3–17.arXiv:hep-ph/0607268.doi:10.1007/978-3-540-73518-2_1.ISBN 978-3-540-73517-5.S2CID 119482294.
  9. ^Nelson, A. (1984-03-15)."Naturally weak CP violation".Physics Letters B.136 (5, 6):387–391.Bibcode:1984PhLB..136..387N.doi:10.1016/0370-2693(84)92025-2. Retrieved2021-12-02.
  10. ^Barr, S. M. (1984-04-18)."Solving the Strong CP Problem without the Peccei–Quinn Symmetry".Phys. Rev. Lett.53 (4):329–332.Bibcode:1984PhRvL..53..329B.doi:10.1103/PhysRevLett.53.329. Retrieved2021-12-02.
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