Testing realistic SO(10) SUSY GUTs with proton decay and gravitational waves
Aug 10, 2023
16 pages
Published in:
- Phys.Rev.D 109 (2024) 5, 5
- Published: Mar 1, 2024
e-Print:
- 2308.05799 [hep-ph]
DOI:
- 10.1103/PhysRevD.109.055025 (publication)
Report number:
- IPPP/23/41
View in:
Citations per year
Abstract: (APS)
We present a comprehensive analysis of a supersymmetric SO(10) grand unified theory, which is broken to the Standard Model via the breaking of two intermediate symmetries. The spontaneous breaking of the first intermediate symmetry, , leads to the generation of cosmic strings and right-handed neutrino masses and further to an observable cosmological background of gravitational waves and generation of light neutrino masses via type-I seesaw mechanism. Supersymmetry breaking manifests as sparticle masses below the breaking but far above the electroweak scale due to proton decay limits. This naturally pushes the breaking scale close to the grand unified theory scale, leading to the formation of metastable cosmic strings, which can provide a gravitational wave spectrum consistent with the recent pulsar timing arrays observation. We perform a detailed analysis of this model using two-loop renormalization group equations, including threshold corrections, to determine the symmetry-breaking scale consistent with the recent pulsar timing arrays signals such as NANOGrav 15-year data and testable by the next-generation limits on proton decay from Hyper-K and JUNO. Simultaneously, we find the regions of the model parameter space that can predict the measured quark and lepton masses and mixing, baryon asymmetry of our Universe, a viable dark matter candidate and can be tested by a combination of neutrinoless double beta decay searches and limits on the sum of neutrinos masses.Note:
- 15 pages, 6 figures
- p: decay
- neutrino: mass
- neutrino: right-handed: mass
- baryon: asymmetry
- gravitational radiation: background
- gravitational radiation: spectrum
- sparticle: mass
- symmetry breaking: scale
- scale: electroweak interaction
- lepton: mass
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Figures(6)
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