cosmological constant problem parâse-ye pâyâ-ye keyhânšenâxti Fr.: problème de la constante cosmologique The impressive discrepancy of about 120 orders of magnitude between the theoretical
value of the → cosmological constant and its observed value.
→ Quantum field theory
interprets the cosmological constant as the density of the
→ vacuum energy. This density can be derived from
the maximum energy at which the theory is valid, i.e.
the → Planck energy scale (1018 GeV). See also: → cosmological; → constant; → problem. |