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Space-Time Structure of a Static Spherically Symmetric Scalar Field

O. BergmannDepartment of Mathematical Physics, University of Adelaide, Adelaide, South AustraliaRoy B. LeipnikDepartment of Mathematical Physics, University of Adelaide, Adelaide, South Australia
1957en
ABI

Аннотация

The Einstein equations of the general theory of relativity are solved for an energy-momentum tensor derived from a linear scalar field theory specialized to a static spherically symmetric field of a point-like source. This is the scalar analog to the structure of the field about a point electron. However, the mathematics is more complicated. A two-parameter family of line elements and associated fields is discovered, of which the Schwarzschild solutions from a one-parameter subfamily. The ${g}_{\mathrm{ik}}$ and field variable $V$ can be only implicitly expressed as algebraic and logarithmic functions of $r$, except for special one-parameter subfamilies where explicit expressions are obtainable. However, asymptotic approximations for large and small radius are derived except for one of the one-parameter subfamilies.

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