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Dark <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Z</mml:mi></mml:math> at the International Linear Collider

Yik Chuen San, Maxim Perelstein, Philip Tañedo

2022Physical review. D/Physical review. D.15 citationsDOIOpen Access PDF

Abstract

A dark $Z$ is a massive Abelian gauge boson which is coupled to the Standard Model through both kinetic and mass mixing with the electroweak sector. We study the phenomenology of the dark $Z$ at an energy-frontier ${e}^{+}{e}^{\ensuremath{-}}$ collider, such as the proposed International Linear Collider (ILC). We show that precision electroweak constraints and the current bounds from the hadron colliders allow a dark $Z$ that is kinematically accessible at the ILC with 250 or 500 GeV center-of-mass energy. Further, the reach of the ILC searches for a dark $Z$ significantly exceeds the expected reach of the high luminosity LHC. If a signal consistent with a dark-$Z$ is discovered, it would motivate a dedicated run of the ILC at the center-of-mass energy matching the dark-$Z$ mass. We demonstrate that a short one month run at design luminosity could measure the dark-$Z$ chiral couplings to fermions with percent precision. This measurement can be used to discriminate between competing theoretical models of the resonance: for example, the dark $Z$ can be distinguished from a dark photon with purely kinetic mixing.

Topics & Concepts

PhysicsParticle physicsInternational Linear ColliderElectroweak interactionDark matterDark energyHiggs bosonColliderDark photonPhenomenology (philosophy)Physics beyond the Standard ModelLarge Hadron ColliderLuminosityNuclear physicsQuantum mechanicsCosmologyEpistemologyPhilosophyOpticsGalaxyDetectorParticle physics theoretical and experimental studiesDark Matter and Cosmic PhenomenaCosmology and Gravitation Theories
Dark <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>Z</mml:mi></mml:math> at the International Linear Collider | Litcius