Caustic avoidance in Hořava-Lifshitz gravity
نویسنده
چکیده
There are at least four versions of Hořava-Lishitz gravity in the literature. We consider the version without the detailed balance condition with the projectability condition and address one aspect of the theory: avoidance of caustics for constant time hypersurfaces. We show that caustics cannot form with codimension one in the absence of matter source if λ deviates from 1 near would-be caustics via RG flow. We argue that inclusion of matter source will not change the conclusion. We also argue that caustics with codimension higher than one will not form because of repulsive gravity generated by nonlinear higher curvature terms. Finally, we discuss implications to the recently proposed scenario of “dark matter as integration constant”.
منابع مشابه
Galaxy Rotation Curves in Covariant Hořava-Lifshitz Gravity
Using the multiplicity of solutions for the projectable case of the covariant extension of Hořava-Lifshitz gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This description is based on static and spherically symmetric solutions of covariant Hořava-Lifshitz gravity and does not require Dark Matter.
متن کاملSurplus Solid Angle: Toward Astrophysical Test of Hořava-Lifshitz Gravity
We consider electrostatic field of a point charge coupled to Hořava-Lifshitz gravity and find an exact solution describing the space with a surplus (or deficit) solid angle. Although, theoretically in general relativity, a surplus angle is hardly to be obtained in the presence of ordinary matter with positive energy distribution, it seems natural in Hořava-Lifshitz gravity. We present sudden di...
متن کاملDark matter as integration constant in Hořava-Lifshitz gravity
In the non-relativistic theory of gravitation recently proposed by Hořava, the Hamiltonian constraint is not a local equation satisfied at each spatial point but an equation integrated over a whole space. The global Hamiltonian constraint is less restrictive than its local version, and allows a richer set of solutions than in general relativity. We show that a component which behaves like press...
متن کاملThermodynamics of Black Holes in Hořava-Lifshitz Gravity
By using the canonical Hamiltonian method, we obtain the mass and entropy of the black holes with general dynamical coupling constant λ in Hořava-Lifshitz Gravity. Regardless of whether the horizon is sphere, plane or hyperboloid, we find these black holes are thermodynamically stable in some parameter space and unstable phase also exists in other parameter space. The relation between the entro...
متن کاملPrimordial non-Gaussianities in Hořava-Lifshitz Gravity
We address the issue of the origins of the primordial fluctuations is the Cosmic Microwave Background spectrum, the “seeds” of the Universe. We review the history of the discovery and the origins of the CMB and explain the questions surrounding it. We move on to consider famous cosmological “puzzles”, which served as an inspiration for the theory of Inflation, reviewed subsequently. We discuss ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2009