Journal
PHYSICAL REVIEW D
Volume 87, Issue 8, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.87.084041
Keywords
-
Funding
- DOE [DE-FG02-10ER41692]
- NSFC [11173021, 11075141, 11178018, 11075224]
- FAPESP [2012/08934-0]
Ask authors/readers for more resources
In this paper, we study static post-Newtonian limits in nonprojectable Horava-Lifshitz gravity with an extra U(1) symmetry. After obtaining all static spherical solutions in the infrared, we apply them to the Solar System tests, and obtain the Eddington-Robertson-Schiff parameters in terms of the coupling constants of the theory. These parameters are well consistent with observations for the physically viable coupling constants. In contrast to the projectable case, this consistence is achieved without taking the gauge field and Newtonian prepotential as part of the metric. DOI: 10.1103/PhysRevD.87.084041
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available