期刊
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
卷 50, 期 3, 页码 939-951出版社
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-010-0639-0
关键词
General relativity; Dark energy; Variable Lambda
Among various phenomenological Lambda models, a time-dependent model angstrom similar to H-3 is selected here to investigate the Lambda-CDM cosmology. The model can follow from dynamics, underlying the origin of Lambda. Using this model the expressions for the time-dependent equation of state parameter omega and other physical parameters are derived. It is shown that in H-3 model accelerated expansion of the Universe takes place at negative energy density, but with a positive pressure. It has also been possible to obtain the change of sign of the deceleration parameter q during cosmic evolution.
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