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Supersymmetric hybrid inflation and current-carrying metastable cosmic strings in SU(4)c×SU(2)L×U(1)R

Adeela Afzal1,*, Maria Mehmood1,†, Mansoor Ur Rehman2,‡, and Qaisar Shafi3

  • *Contact author: adeelaafzal555@gmail.com
  • †Contact author: mehmood.maria786@gmail.com
  • ‡Contact author: m.rehman@iu.edu.sa

Phys. Rev. D 112, 083545 – Published 23 October, 2025

DOI: https://doi.org/10.1103/d7zx-c7f7

Abstract

We construct a realistic supersymmetric model for superheavy metastable cosmic strings (CSs) that can be investigated in the current pulsar timing array (PTA) experiments. It is based on shifted μ-hybrid inflation in which the symmetry breaking SU(4)c×SU(2)L×U(1)R→SU(3)c×SU(2)L×U(1)B−L×U(1)R proceeds along an inflationary trajectory such that the topologically unstable primordial monopoles are inflated away. The breaking of U(1)B−L×U(1)R→U(1)Y after inflation ends yields the superheavy metastable CSs carrying the right handed neutrino zero modes that generate the stochastic gravitational wave background, which we show is consistent with the current PTA dataset and the LIGO O3 run. The scalar spectral index ns and the tensor-to-scalar ratio r are compatible with the Planck 2018 and Atacama Cosmology Telescope measurements. Both reheating and leptogenesis are briefly discussed.

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