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All axion dark matter from supersymmetric models (2502.06955v2)

Published 10 Feb 2025 in hep-ph and hep-th

Abstract: Supersymmetric models accompanied by certain anomaly-free discrete R-symmetries Z_nR are attractive in that 1. the R-symmetry (which can arise from compactified string theory as a remnant of the broken 10-d Lorentz symmetry) forbids unwanted superpotential terms while allowing for the generation of an accidental, approximate global U(1){PQ} symmetry needed to solve the strong CP problem and 2. they provide a raison d'etre for an otherwise ad-hoc R-parity conservation. We augment the minimal supersymmetric Standard Model (MSSM) by two additional Z_nR- and PQ-charged fields X and Y wherein SUSY breaking at an intermediate scale m{hidden} leads to PQ breaking at a scale f_a\sim 10{11} GeV leading to a SUSY DFSZ axion. The same SUSY breaking can trigger R-parity breaking via higher-dimensional operators leading to tiny R-violating couplings of order (f_a/m_P)N and a WIMP quality problem. For Z_4R and Z_8R, we find only an N=1 suppression. Then the lightest SUSY particle (LSP) of the MSSM becomes unstable with a lifetime of order ~ 10{-3}-10 seconds so the LSPs all decay away before the present epoch. That leaves a universe with all axion cold dark matter and no WIMPs in accord with recent LZ-2024 WIMP search results.

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