Proposal for a constant cosmological constant

Mar, 2000
12 pages
Published in:
  • Phys.Lett.B 492 (2000) 153-160
e-Print:
Report number:
  • NUB-3208-00-TH

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Abstract:
It is proposed that the apparent positive acceleration of the cosmological scale factor is due to the vacuum energy of an incomplete chiral phase transition in a hidden SU(2) sector. Constraints from primordial nucleosynthesis imply that the present metastable phase is in a substantially supercooled state. It is argued that massless chiral condensates can substantially enhance the possibility of supercooling, and a linear sigma model exhibiting scale invariance broken only at the quantum level is shown to accommodate the required supercooling with a reasonable choice of quartic couplings. The extensive supercooling can in principle be confirmed or rejected on the basis of interface tension measurements in lattice simulations with dynamical fermions.
  • cosmological constant
  • astrophysics: acceleration
  • vacuum state: energy
  • critical phenomena: chiral
  • gauge field theory: SU(2)
  • hidden symmetry
  • light nucleus: production
  • condensation: chiral
  • sigma model: linear
  • surface tension