Rotationally symmetric massless modes in closed Robertson-Walker universe.

Details Rotationally symmetric massless modes in closed Robertson-Walker universe. Rotationally symmetric massless modes in closed Robertson-Walker universe.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999fophl..12..267d&link_type=abstract

Found. Phys. Lett., Vol. 12, No. 3, p. 267 - 279

Physics

Cosmology: Robertson-Walker Metric

Scientific paper

The aim of the present paper is to investigate the minimally coupled rotationally symmetric scalar field configurations in spatially closed Friedmann-Robertson-Walker universe with incoherent dust. The authors have obtained the closed form solution of the Klein-Gordon equation in terms of two real-valued linearly independent hypergeometric functions. The orthonormal set of positive-frequency-like parity modes thereafter derived points out that each parity given state is conformally built up of three Einsteinian particle states and also leads to the explicit coordinate-representation of the field propagator.

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