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P and CP solution of the strong CP puzzle
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abstract
We use parity (P) to set $\theta_{QCD}$ to zero in the minimal left-right symmetric model with a bi-doublet Higgs, add a heavy vectorlike quark family, and obtain in a novel manner the Nelson Barr (NB) form associated so far only with spontaneous CP solution to the strong CP Puzzle. Our solution does not have the `coincidence of scales problem', that typically plagues NB models. P protects $\bar{\theta}$, if it breaks at a scale $v_R$ below the mass $M$ of the heavy quarks, and $\bar{\theta} \sim 10^{-9} (v_R/M)^2$ is radiatively generated, which can be acceptably small. On the other hand, if $M < v_R$, the $\bar{\theta} \sim 10^{-9}$ generated by the NB mechanism is too large, but if $\delta_{CKM}$ is obtained without the NB form, surprisingly a lower irreducible $\bar{\theta} \sim (10^{-13}~to~10^{-10}) ln( {v_R/M)}$, testable by neutron EDM experiments is generated. No leptonic CP violation is generated (Dirac phase $\delta_{CP} = 0~or~\pi$ in PMNS matrix) which makes the minimal model testable by neutrino experiments. We also discuss some challenges in a non-minimal model that generates leptonic CP violation. Lastly but importantly, we find with doublet rather than bi-doublet Higgses, that there is an automatic NB solution on imposing CP (the NB form is accidental due to $SU(2)_R$), which does not require generalized parity and needs just one mirror generation.
Forward citations
Cited by 4 Pith papers
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Vector-like quark doublets, weak-basis invariants and CP violation
Vector-like quark doublets allow CP violation in weak-basis invariants of mass dimension six; the resulting framework organizes the model's parameters, gives the complete CP-odd invariant set for one doublet, and link...
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Accidentally Stable Dark Matter in a Parity Solution to the Strong CP Problem
SU(2)_L×SU(2)_R bi-triplet fermions are accidentally stable dark matter in a parity solution to strong CP, with relic abundance forcing v_R ≲ 150 TeV.
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Universal Seesaw Pati-Salam Model with P for Strong CP
A parity-symmetric Pati-Salam model with universal seesaw masses gives an axionless strong-CP solution and radiatively induced neutrino masses.
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Upper Bound on Parity Breaking Scale for Doublet WIMP Dark Matter
In a Parity-symmetric extension of the Standard Model with doublet-pair WIMP dark matter, thermal relic abundance requires the Parity breaking scale to be below 25-60 TeV.
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