Dark gauge-mediated supersymmetry breaking with a massless dark photon
Brian Batell (Pittsburgh Particle Physics, Astrophysics, and Cosmology Center, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA, 15217, USA)
; Yechan Kim (Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon, 34141, Korea)
; Hye-Sung Lee (Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon, 34141, Korea)
; Jiheon Lee (Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon, 34141, Korea, Theoretical Physics Department, CERN, 1 Esplanade des Particules, Geneva 23, CH-1211, Switzerland)
We study dark gauge-mediated supersymmetry breaking (dark GMSB) in a theory with a new unbroken U(1) local symmetry and massless dark photon. Messenger fields charged under both Standard Model and dark gauge symmetries produce new soft supersymmetry-breaking terms due to gauge kinetic mixing between U(1) hypercharge and U(1) . We show that large kinetic mixing induces significant distortions to the superpartner spectra relative to conventional GMSB. Notably, shifts in the Higgs soft masses impact the conditions for electroweak symmetry breaking, lowering the $\textit{μ}$ parameter and yielding a relatively light Higgsino that may be accessible at the LHC. Furthermore, for very simple messenger representations, a very light bino-dark photino mixed state is present in the spectrum, which may be probed through exotic Higgs boson decays at future Higgs factories. We also examine the cosmological and phenomenological consequences of the messengers, the lightest of which is absolutely stable and carries fractional electric charge.