Phase of Confined Electroweak Force in the Early Universe
PHYSICAL REVIEW D 100, 055005 (2019) Phase of confined electroweak force in the early Universe Joshua Berger,1 Andrew J. Long,2,3 and Jessica Turner4 1Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA 2Leinweber Center for Theoretical Physics, University of Michigan, Ann Arbor, Michigan 48109, USA 3Department of Physics and Astronomy, Rice University, Houston, Texas 77005, USA 4Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA (Received 18 June 2019; published 6 September 2019) We consider a modified cosmological history in which the presence of beyond-the-Standard-Model 2 physics causes the weak gauge sector, SUð ÞL, to confine before it is Higgsed. Under the assumption of chiral symmetry breaking, quark and lepton weak doublets form condensates that break the global symmetries of the Standard Model, including baryon and lepton number, down to a U(1) subgroup under which only the weak singlet fermions and Higgs boson transform. The weakly coupled gauge group 3 1 2 1 SUð Þc ×Uð ÞY is also broken to an SUð Þc ×Uð ÞQ gauge group. The light states include (pseudo-) Goldstone bosons of the global symmetry breaking, mostly elementary fermions primarily composed of the weak singlet quarks and leptons, and the gauge bosons of the weakly coupled gauge group. We discuss possible signatures from early Universe cosmology including gravitational wave radiation, topological defects, and baryogenesis. DOI: 10.1103/PhysRevD.100.055005 I. INTRODUCTION composite particles and that the predicted low-energy fermion spectrum agrees well with the measured quark Quarks and leptons can interact via the weak force, and lepton masses.
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