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A ] is an ] of ] in which the ] is ]. Physically speaking, this means that |
A ] is an ] of ] in which the ] is ]. The corresponding condition on the ] can be written | ||
<math>T_{ab} = \Phi k_{a} k_{b}</math> | |||
where <math>\Phi</math> is a scalar field and <math>k_{a}</math> is any ] vector field. | |||
Physically speaking, this means that a null dust describes either ], or some kind of nongravitational ] which is described by a ] ] (such as ]), or a combination of these two. Null dusts include ] as a special case. | |||
== References == | |||
{{Book reference | Author=Stephani, Hans; Kramer, Dietrich; Maccallum, Malcolm; Hoenselaers, Cornelius; & Herlt, Eduard | Title=Exact Solutions of Einstein's Field Equations| Publisher=Cambridge: Cambridge University Press | Year=2003 | ID=ISBN 0-521-46136-7}} |
Revision as of 04:00, 24 May 2005
A null dust solution is an exact solution of Einstein's field equation in which the Einstein tensor is null. The corresponding condition on the stress-energy tensor can be written
where is a scalar field and is any null vector field.
Physically speaking, this means that a null dust describes either gravitational radiation, or some kind of nongravitational radiation which is described by a relativistic classical field theory (such as electromagnetic radiation), or a combination of these two. Null dusts include vacuum solutions as a special case.
References
. ISBN 0-521-46136-7. {{cite book}}
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