Related items
Physical Origin of L = energy of quantum vacuum zero-point energy ?i (1/2 + ni) ?wi
The Cosmological Constant Problem (? ?wi/2)/V formally = ? cutoff at Planck energy KP = (?c/GN )1/2 [rL ]QFT = 10120 [rL ]obs
Bose-Einstein vs Fermi-Dirac statistics: Bosons (integer spin): photons, gravitons, etc. [rL ]boson ɬ Fermions (half-integer spin): electrons, quarks, etc. [rL ]fermion < 0 Mutual cancellation to 120 signif figures, and no more! Why?!
Inflationary epoch: also an exponential expansion Theory: During a phase transition associated with spontaneous symmetry breaking of particle interactions, the system (universe) is temporarily in a “false vacuum” with a large vacuum energy = Leff