Spherically symmetric, static solutions of the Brans-Dicke field equations in vacuum

Details Spherically symmetric, static solutions of the Brans-Dicke field equations in vacuum Spherically symmetric, static solutions of the Brans-Dicke field equations in vacuum

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261..229r&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 1, p. 229-232.

Physics

2

Celestial Mechanics, Field Theory (Physics), Galactic Rotation, Cosmology, Stellar Motions

Scientific paper

We present approximate solutions for the Brans-Dicke field equations in vacuum, assuming spherical symmetry and static fields. Apart from the trivial solution phi = constant, there exist solutions with phi vanishing at r = 0 and approaching a constant value as r tends to infinity. Finally, we show that these solutions produce flat rotation curves in the region r in the range between r(sh) and sq rt omega/2r(sh).

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