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{{Mergeto|Linearized gravity|date=October 2006}}
{{Mergeto|Linearized gravity|date=October 2006}}


The [[weak-field approximation]] in [[general relativity]] is used to describe the gravitational field very far from the source of [[gravity]].
The '''weak-field approximation''' in [[general relativity]] is used to describe the gravitational field very far from the source of [[gravity]].


In this approximation, we assume the metric for [[spacetime]] (<math>g \ </math>) be written in coordinates as:
In this approximation, we assume the metric for [[spacetime]] (<math>g \ </math>) be written in coordinates as:
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* {{cite book | author=Stephani, Hans | title=General Relativity: An Introduction to the Theory of the Gravitational Field, | location=Cambridge | publisher=Cambridge University Press | year=1990 | id=ISBN 0-521-37941-5}}
* {{cite book | author=Stephani, Hans | title=General Relativity: An Introduction to the Theory of the Gravitational Field, | location=Cambridge | publisher=Cambridge University Press | year=1990 | id=ISBN 0-521-37941-5}}


* {{cite book | author=Adler, Ronald; Bazin, Maurice' & Schiffer, Menahem | title=Introduction to General Relativity | location=New York | publisher=McGraw-Hill | year=1965 | id=ISBN 0-070-00423-4}}
* {{cite book | author=Adler, Ronald; Bazin, Maurice' & Schiffer, Menahem | title=Introduction to General Relativity | location=New York | publisher=McGraw-Hill | year=1965 | id=ISBN 0-07-000423-4}}

{{relativity-stub}}


[[Category:Mathematical methods in general relativity]]
[[Category:Mathematical methods in general relativity]]


[[fr:Approximation des champs faibles]]
[[fr:Approximation des champs faibles]]


{{relativity-stub}}

Revision as of 15:28, 18 November 2006

The weak-field approximation in general relativity is used to describe the gravitational field very far from the source of gravity.

In this approximation, we assume the metric for spacetime () be written in coordinates as:

where is the Minkowski metric, is the deviation from the Minkowski metric and is taken to be a non-zero real constant.

A relation between the Newtonian gravitational potential and the deviation term above can be obtained by calculating the Christoffel symbols (upon ignoring terms of order higher than ):

from which follows:

()

The geodesic equation becomes

where is the Newtonian gravitational potential and is the speed of light. Thus:

As we know that

where is the gravitational constant, is the mass of the gravitating body and is the radial distance from the centre of this body, we find that:

The weak-field approximation is useful in finding the values of certain constants, for example in the Einstein field equations and in the Schwarzschild metric.

See also

References

  • Stephani, Hans (1990). General Relativity: An Introduction to the Theory of the Gravitational Field,. Cambridge: Cambridge University Press. ISBN 0-521-37941-5.
  • Adler, Ronald; Bazin, Maurice' & Schiffer, Menahem (1965). Introduction to General Relativity. New York: McGraw-Hill. ISBN 0-07-000423-4.{{cite book}}: CS1 maint: multiple names: authors list (link)