Pryce-Hoyle Tensor in a Combined Einstein-Cartan-Brans-Dicke Model

Details Pryce-Hoyle Tensor in a Combined Einstein-Cartan-Brans-Dicke Model Pryce-Hoyle Tensor in a Combined Einstein-Cartan-Brans-Dicke Model

2008-05-04

arxiv.org/abs/0805.0448v4

Int.J.Theor.Phys.48:836-846,2009

Physics

General Physics

16 pages including front cover. New version, accepted by International Journal of Theoretical Physics. To be published soon

Scientific paper

10.1007/s10773-008-9857-0

In addition to introducing matter injection through a scalar field determined by Pryce-Hoyle tensor, we also combine it with a BCDE (Brans-Dicke-Einstein-Cartan) theory with lambdaterm developed earlier by Berman(2008), for inflationary scenario. It involves a variable cosmological constant, which decreases with time, jointly with energy density, cosmic pressure, shear, vorticity, and Hubble's parameter, while the scale factor, total spin and scalar field increase exponentially. The post-inflationary fluid resembles a perfect one, though total spin grows, but not the angular speed (Berman, 2007d). The Pryce-Hoyle tensor, which can measured by the number of injected particles per unit proper volume and time, as well as shear and vorticity, can be neglected in the aftermath of inflation ("no-hair").

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