Vaidya Solutions in General Covariant Hořava-Lifshitz Gravity without Projectability: Infrared Limit

Abstract

In this paper, we have studied nonstationary radiative spherically symmetric spacetime, in general covariant theory ($U(1)$ extension) of Hořava-Lifshitz gravity without the projectability condition and in the infrared limit. The Newtonian prepotential $\phi$ was assumed null. We have shown that there is not the analogue of the Vaidya's solution in the Hořava-Lifshitz Theory (HLT), as we know in the General Relativity Theory (GRT). Therefore, we conclude that the gauge field $A$ should interact with the null radiation field of the Vaidya's spacetime in the HLT.

9 pages. arXiv admin note: text overlap with arXiv:1208.2491 by other authors

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Cited by in corpus (2)

• Vaidya Solution in General Covariant Hořava-Lifshitz Gravity with the Minimum Coupling and without Projectability: Infrared Limit
• Shear-free Dust Solution in General Covariant Hořava-Lifshitz Gravity