Proposal for a constant cosmological constant
Mar, 200012 pages
Published in:
- Phys.Lett.B 492 (2000) 153-160
e-Print:
- hep-ph/0003197 [hep-ph]
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
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