Search results for "Strong CP problem"

showing 10 items of 20 documents

The strong CP problem and the solar neutrino puzzle: Are they related?

1991

We discuss the possibility that a solution of the strong CP problem via the introduction of a chiral U(1), a la Peccei-Quinn, may also provide a natural scenario for explaining the apparent depletion of the solar neutrino flux through matter enhanced neutrino oscillations. The smallness of the neutrino masses is related to the scale at which the U(1)PQ symmetry is spontaneously broken, without introducing right-handed neutrino fields and invoking the see-saw mechanism. The model is consistent with all present experimental results. In particular, the phenomenology associated to the presence of an “invisible” axion is the same as in the Dine-Fischler-Srednicki-Zhitnisky model with the excepti…

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSpontaneous symmetry breakingSolar neutrinoHigh Energy Physics::PhenomenologyElementary particleStrong CP problemNeutrinoNeutrino oscillationPhenomenology (particle physics)AxionNuclear Physics B
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Search for Hidden-Sector Bosons inB0→K*0μ+μ−Decays

2015

A search is presented for hidden-sector bosons, $\chi$, produced in the decay ${B^0\!\to K^*(892)^0\chi}$, with $K^*(892)^0\!\to K^{+}\pi^{-}$ and $\chi\!\to\mu^+\mu^-$. The search is performed using $pp$-collision data corresponding to 3.0 fb$^{-1}$ collected with the LHCb detector. No significant signal is observed in the accessible mass range $214 \leq m({\chi}) \leq 4350$ MeV, and upper limits are placed on the branching fraction product $\mathcal{B}(B^0\!\to K^*(892)^0\chi)\times\mathcal{B}(\chi\!\to\mu^+\mu^-)$ as a function of the mass and lifetime of the $\chi$ boson. These limits are of the order of $10^{-9}$ for $\chi$ lifetimes less than 100 ps over most of the $m(\chi)$ range, a…

PhysicsParticle physics010308 nuclear & particles physicsBranching fractionGeneral Physics and AstronomyOrder (ring theory)01 natural sciencesGradient functionHidden sectorProduct (mathematics)0103 physical sciencesStrong CP problem010306 general physicsAxionBosonPhysical Review Letters
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An invisible axion model with controlled FCNCs at tree level

2015

We derive the necessary conditions to build a class of invisible axion models with Flavor Changing Neutral Currents at tree-level controlled by the fermion mixing matrices and present an explicit model implementation. A horizontal Peccei-Quinn symmetry provides a solution to the strong CP problem via the Peccei-Quinn mechanism and predicts a cold dark mater candidate, the invisible axion or familon. The smallness of active neutrino masses can be explained via a type I seesaw mechanism, providing a dynamical origin for the heavy seesaw scale. The possibility to avoid the domain wall problem stands as one of the most interesting features of the type of models considered. Experimental limits r…

PhysicsParticle physicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsDark matterHigh Energy Physics::PhenomenologyFOS: Physical scienceslcsh:QC1-999Domain wall (string theory)High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryStrong CP problemNeutrinoAxionMixing (physics)lcsh:PhysicsPhysics Letters B
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On the corner elements of the CKM and PMNS matrices

2013

Recent experiments show that the top-right corner element (U-e3) of the PMNS matrix is small but nonzero, and suggest further via unitarity that it is smaller than the bottom-left corner element (U-tau 1). Here, it is shown that if to the assumption of a universal rank-one mass matrix, long favoured by phenomenologists, one adds that this matrix rotates with scale, then it follows that A) by inputting the mass ratios m(c)/m(t), m(s)/m(b), m(mu)/m(tau), and m(2)/m(3), i) the corner elements are small but nonzero, ii) V-ub < V-td, U-e3 < U-tau 1, iii) estimates result for the ratios V-ub/V-td and U-e3/U-tau 1, and B) by inputting further the experimental values of V-us, V-tb and U-e2, U-mu 3,…

PhysicsParticle physicsUnitarityCabibbo–Kobayashi–Maskawa matrixGeneral Physics and AstronomyMass matrixPartícules (Física nuclear)CombinatoricsStrong CP ProblemMatrix (mathematics)Rotating Mass MatrixStrong CP problemFísica nuclearHiggs Decay
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The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)

2015

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best …

QCD axionParticle physicsPhysics::Instrumentation and DetectorsDark matterPhysics and Astronomy(all)01 natural sciences7. Clean energymagnetic helioscopeHigh Energy Physics::TheoryQCD axionsAstroparticle PhysicsAxionObservatory0103 physical sciencesDark matterQCD axions; magnetic helioscope; dark matterDark Matterddc:530Detectors and Experimental Techniques010306 general physicsAxionAstroparticle physicsPhysicsHelioscope010308 nuclear & particles physicsAxion Dark Matter ExperimentHigh Energy Physics::PhenomenologyStrong CP problemIAXOStrong CP ProblemALPStrong CP problemAstroparticle physicsCERN Axion Solar TelescopeParticle Physics - ExperimentHelioscopesPhysics Procedia
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Mass Hierarchy, Mixing, CP-Violation and Higgs Decay---or Why Rotation is Good for Us

2011

The idea of a rank-one rotating mass matrix (R2M2) is reviewed detailing how it leads to ready explanations both for the fermion mass hierarchy and for the distinctive mixing patterns between up and down fermion states, which can be and have been tested against experiment and shown to be fully consistent with existing data. Further, R2M2 is seen to offer, as by-products: (i) a new solution of the strong CP problem in QCD by linking the theta-angle there to the Kobayashi-Maskawa CP-violating phase in the CKM matrix, and (ii) some novel predictions of possible anomalies in Higgs decay observable in principle at the LHC. A special effort is made to answer some questions raised.

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsCabibbo–Kobayashi–Maskawa matrixHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesAstronomy and AstrophysicsObservableMass matrixAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonCP violationStrong CP problemHigh Energy Physics::ExperimentMixing (physics)
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Developing the Framed Standard Model

2011

The framed standard model (FSM) suggested earlier, which incorporates the Higgs field and 3 fermion generations as part of the framed gauge theory structure, is here developed further to show that it gives both quarks and leptons hierarchical masses and mixing matrices akin to what is experimentally observed. Among its many distinguishing features which lead to the above results are (i) the vacuum is degenerate under a global $su(3)$ symmetry which plays the role of fermion generations, (ii) the fermion mass matrix is "universal", rank-one and rotates (changes its orientation in generation space) with changing scale $\mu$, (iii) the metric in generation space is scale-dependent too, and in …

Quantum chromodynamicsQuarkPhysicsNuclear and High Energy PhysicsParticle physicsCabibbo–Kobayashi–Maskawa matrixHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesAstronomy and AstrophysicsFermionAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyStandard Model (mathematical formulation)Higgs fieldTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Strong CP problemHigh Energy Physics::ExperimentGauge theory
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Radiative axion inflation

2019

Planck data robustly exclude the simple $\lambda\phi^4$ scenario for inflation. This is also the case for models of Axion Inflation in which the inflaton field is the radial part of the Peccei-Quinn complex scalar field. In this letter we show that for the KSVZ model it is possible to match the data taking into account radiative corrections to the tree level potential. After writing down the 1-loop Coleman-Weinberg potential, we show that a radiative plateau is easily generated thanks to the fact that the heavy quarks are charged under $SU(3)_c$ in order to solve the strong CP problem. We also give a numerical example for which the inflationary observables are computed and the heavy quarks …

QuarkNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciences01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRadiative transferPlanck010306 general physicsAxionInflation (cosmology)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyInflatonlcsh:QC1-999High Energy Physics - PhenomenologysymbolsStrong CP problemScalar fieldlcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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New Angle on the Strong CP and Chiral Symmetry Problems from a Rotating Mass Matrix

2007

It is shown that when the mass matrix changes in orientation (i.e. rotates) in generation space for a changing energy scale, the masses of the lower generations are not given just by its eigenvalues. In particular, these masses need not be zero even when the eigenvalues are zero. In that case, the strong CP problem can be avoided by removing the unwanted theta term by a chiral transformation not in contradiction with the nonvanishing quark masses experimentally observed. Similarly, a rotating mass matrix may shed new light on the problem of chhiral symmetry breaking. That the fermion mass matrix may so rotate with the scale has been suggested before as a possible explanation for up-down fer…

QuarkPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeFOS: Physical sciencesFísicaAstronomy and AstrophysicsFermionSpace (mathematics)Mass matrixAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsStrong CP problemChiral symmetry breakingEigenvalues and eigenvectorsMixing (physics)
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A solution to the strong CP problem transforming the theta angle to the KM CP-violating phase

2010

It is shown that in the scheme with a rotating fermion mass matrix (i.e. one with a scale-dependent orientation in generation space) suggested earlier for explaining fermion mixing and mass hierarchy, the theta angle term in the QCD action of topological origin can be eliminated by chiral transformations, while giving still nonzero masses to all quarks. Instead, the effects of such transformations get transmitted by the rotation to the CKM matrix as the KM phase giving, for theta of order unity, a Jarlskog invariant typically of order 10(-5), as experimentally observed. Strong and weak CP violations appear then as just two facets of the same phenomenon.

QuarkPhysicsQuantum chromodynamicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCabibbo–Kobayashi–Maskawa matrixHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaAstronomy and AstrophysicsFermionAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)CP violationStrong CP problemInvariant (mathematics)Mixing (physics)
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