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Initial value constraints with tensor matter

delete2011-12-01
delete21
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OA
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J
Jacobson, Ted *
DOI:10.1088/0264-9381/28/24/245011delete
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摘要

摘要

En 中文
In generally covariant metric gravity theories with tensor matter fields, the initial value constraint equations, unlike in general relativity, are in general not just the 0 mu components of the metric field equation. This happens because higher derivatives can occur in the matter stress tensor. A universal form for these constraints is derived here from a generalized Bianchi identity that includes matter fields. As an application, the constraints for Einstein-aether theory are found.
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Classical and Quantum Gravity 封面图
Classical and Quantum Gravity
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3.7
论文数:
1.3W
被引数:
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