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REALISTIC MODELS WITH A LIGHT U(1) GAUGE BOSON COUPLED TO BARYON NUMBER

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arxiv hep-ph/9501220 v1 pith:FTJQL5HH submitted 1995-01-06 hep-ph

classification hep-ph
keywords baryonelectroweakgaugemodelsnumbertermbosonmeasurements
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We recently showed that a new gauge boson $\gamma_B$ coupling only to baryon number is phenomenologically allowed, even if $m_B<m_Z$ and $\alpha_B \approx 0.2$. In our previous work we assumed that kinetic mixing between the baryon number and hypercharge gauge bosons (via an $F^{\mu\nu}_B F_{\mu\nu}^Y$ term) was small enough to evade constraints from precision electroweak measurements. In this paper we propose a class of models in which this term is naturally absent above the electroweak scale. We show that the generation of a mixing term through radiative corrections in the low-energy effective theory does not lead to conflict with precision electroweak measurements and may provide a leptonic signal for models of this type at an upgraded Tevatron.

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Forward citations

Cited by 5 Pith papers

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    In a quark-universal U(1)_B model, the scalar φ that breaks the symmetry can be discovered first through its diphoton decay, and its rate can explain the 95 GeV diphoton excess.

  3. Custodial Naturalness

    hep-ph 2025-02 conditional novelty 6.0 of 10

    Custodial Naturalness uses classical scale invariance plus a custodial SO(6) symmetry to make the Higgs a naturally light pseudo-Goldstone boson, with testable new particle predictions.

  4. Dark CP Violation and Gauged Lepton/Baryon Number for Electroweak Baryogenesis

    hep-ph 2019-08 conditional novelty 6.0 of 10

    An electroweak baryogenesis model where dark-sector CP violation is transferred to Standard Model leptons through an anomalous U(1)_ℓ Z' background can produce the observed baryon asymmetry while evading current EDM bounds.

  5. Probing Leptophobic Dark Sectors via Gravitational Wave Signatures

    hep-ph 2025-08 unverdicted novelty 4.0 of 10

    A gauged U(1)_B extension of the Standard Model is claimed to produce observable gravitational waves from a first-order phase transition, with dark matter around 8-12 TeV.

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