Cosmology with an extremely light scalar field

Mathematics – Logic

Scientific paper

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Origin And Formation Of The Universe, Lagrangian And Hamiltonian Approach

Scientific paper

A theory with a vanishing cosmological constant can have a nonzero effective cosmological constant of cosmological significance if the theory has a scalar field with a mass m of the order of the inverse age of the Universe (τ~1033 eV-1) provided the field has a nonzero but evolving expectation value. We discuss the cosmological consequences of scalar fields with masses m<~10-28 eV. The effect on the age of the Universe and on the growth of density perturbations is discussed in detail. For small masses (m<~τ-1~10-33 eV) the Universe behaves precisely as if a cosmological constant were present. For masses several orders of magnitude greater than τ-1 for which φ has made several oscillations only density perturbations on scales greater than m-1 grow significantly.

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