Bianchi-type cosmological models in Lyra's geometry with constant deceleration parameter.

Details Bianchi-type cosmological models in Lyra's geometry with constant deceleration parameter. Bianchi-type cosmological models in Lyra's geometry with constant deceleration parameter.

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ncimb.108..541s&link_type=abstract

Nuovo Cimento B, Vol. 108, No. 5, p. 541 - 558

Mathematics

Logic

Cosmology: Bianchi Models, Cosmology: Deceleration Parameter

Scientific paper

The Bianchi-type cosmological models have been studied in Lyra's
geometry for a low variation of Hubble's parameter presented by Berman
(1983) that yields constant deceleration parameter models of the
universe. All the models have a singular origin (t = 0) and evolve with
time. The gauge function β(t) is an arbitrary function of time.

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