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Probing the $Z'$ sector of the minimal $B-L$ model at future Linear Colliders in the $e^+e^-\to \mu^+\mu^-$ process

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arxiv 0903.4777 v2 pith:WAWBDZW6 submitted 2009-03-27 hep-ph

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

We study the capabilities of future electron-positron Linear Colliders, with centre-of-mass energy at the TeV scale, in accessing the parameter space of a $Z'$ boson within the minimal $B-L$ model. In such a model, wherein the Standard Model gauge group is augmented by a broken $U(1)_{B-L}$ symmetry -- with $B(L)$ being the baryon(lepton) number -- the emerging $Z'$ mass is expected to be in the above energy range. We carry out a detailed comparison between the discovery regions mapped over a two-dimensional configuration space ($Z'$ mass and coupling) at the Large Hadron Collider and possible future Linear Colliders for the case of di-muon production. As known in the literature for other $Z'$ models, we confirm that leptonic machines, as compared to the CERN hadronic accelerator, display an additional potential in discovering a $B-L$ $Z'$ boson as well as in allowing one to study its properties at a level of precision well beyond that of any of the existing colliders.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Exploring $Z'$ and Right-Handed Neutrinos in the BLSM at the Large Hadron Collider

    hep-ph 2024-12 conditional novelty 5.0 of 10

    For a benchmark B-L extension with a 3 TeV Z' and 420 GeV right-handed neutrinos, the HL-LHC could reach discovery-level significance in three final states using BDT-based event selection.

  2. Testing the gauged $\mathrm{U(1)}_{B-L}$ model for loop induced neutrino mass with dark matter

    hep-ph 2024-12 conditional novelty 4.0 of 10

    A benchmark parameter point in the U(1)_{B-L} radiative seesaw model is claimed to satisfy current neutrino, dark matter, and collider constraints.

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