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Scalar field solution : ウィキペディア英語版
Scalar field solution
In general relativity, a scalar field solution is an exact solution of the Einstein field equation in which the gravitational field is due entirely to the field energy and momentum of a scalar field. Such a field may or may not be ''massless'', and it may be taken to have ''minimal curvature coupling'', or some other choice, such as ''conformal coupling''.
==Mathematical definition==

In general relativity, the geometric setting for physical phenomena is a Lorentzian manifold, which is physically interpreted as a curved spacetime, and which is mathematically specified by defining a metric tensor g_ (or by defining a frame field). The curvature tensor R_
of this manifold and associated quantities such as the Einstein tensor G^, are well-defined even in the absence of any physical theory, but in general relativity they acquire a physical interpretation as geometric manifestations of the gravitational field.
In addition, we must specify a scalar field by giving a function \psi. This function is required to satisfy two following conditions:
# The function must satisfy the (curved spacetime) ''source-free'' wave equation g^ \psi_ = 0,
# The Einstein tensor must match the stress-energy tensor for the scalar field, which in the simplest case, a ''minimally coupled massless scalar field'', can be written
G^= 8 \pi \left( \psi^ \psi^ - \frac
\psi_ \psi^ g^ \right) .
Both conditions follow from varying the Lagrangian density for the scalar field, which in the case of a minimally coupled massless scalar field is
: L = -g^ \, \psi_ \, \psi_
Here,
:\frac = 0
gives the wave equation, while
:\frac{\delta g^{ab}} = 0
gives the Einstein equation (in the case where the field energy of the scalar field is the only source of the gravitational field).

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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