Horava (Horava-Lifshitz) Gravity  

In General > s.a. gravity theories; Lifshitz-Type Theories.
* Idea: A non-relativistic renormalisable theory of gravitation which reduces to Einstein's general relativity at large distances but violates Lorentz
invariance at small distances and introduces anisotropic spacetime scaling; Proposed as a candidate for a UV completion of Einstein's theory.
@ General references: Horava PRD(09)-a0901 [proposal]; Nikolic a0904 [and notion of particles]; Volovik JETPL(09)-a0904 [and emergent gravity, condensed-matter examples]; Charmousis et al JHEP(09)-a0905 [strong-coupling problems]; Li & Pang JHEP(09)-a0905 [canonical formulation problems]; Germani et al JHEP(09)-a0906 [as gauge-fixed vector-tensor theory of gravity]; Mukohyama JCAP(09)-a0906 [caustic avoidance]; Horava & Melby-Thompson a0909 [conformal infinity]; > s.a. quantum spacetime [dimension].
@ Extra scalar-graviton mode: Cai et al PRD(09)-a0905; Blas et al JHEP(09)-a0906 [and inconsistency]; Kobakhidze a0906; Afshordi PRD(09)-a0907 [low-energy limit is cuscuton model]; Park a0910 [decoupling and consistency]; Koyama & Arroja a0910.
@ Quantum theory: Orlando & Reffert CQG(09)-a0905 [renormalizability]; Shu & Wu a0906 [stochastic quantization]; > s.a. modified quantum gravity theories.
@ Related topics: Calcagni a0905 [+ scalar field, and detailed balance]; Bogdanos & Saridakis a0907 [ghost-like scalar instabilities]; Myung PLB(09)-a0907, PLB(09) [and generalized uncertainty principle].

Phenomenology In General > s.a. gravitational thermodynamics; graviton.
* In general: The post-Newtonian coefficients coincide with those of general relativity, so the deviations from general relativity can be tested only in strong-gravity regimes; In its original version, the theory has a non-zero cosmological constant of the wrong sign.
@ Solar-system phenomenology: Harko et al a0908; Iorio & Ruggiero a0909, a0909 [orbital motions].
@ Particle kinematics: Capasso & Polychronakos a0909; Sindoni a0910.
@ Other phenomenology: Harko et al PRD(09)-a0907 [thin accretion disk properties]; Kalyana Rama a0910 [particle dispersion relations]; Momeni PLB-a0910 [cosmic strings].

Black Holes and Other Solutions
@ Black holes: Cai et al PRD(09)-a0904 [topological]; Chen & Jing a0905 [quasinormal modes]; Konoplya PLB(09)-a0905 [lensing and quasinormal modes]; Park JHEP(09)-a0905 [and cosmological solutions]; Ghodsi & Hatefi a0906 [rotating]; Kiritsis & Kofinas a0910; Capasso & Polychronakos a0911 [static spherically symmetric].
@ Black-hole thermodynamics: Cai et al PLB(09)-a0905; Myung PLB(09)-a0905; Castillo & Larrañaga a0906 [entropy]; Peng & Wu a0906 [radiation].
@ Other solutions: Lü et al PRL(09)-a0904 + Nastase Phy(09); Nastase a0904 [large-scale]; Colgáin & Yavartanoo JHEP(09)-a0904 [dyonic]; Boehmer & Lobo a0909 [Einstein static universe, stability]; Setare & Momeni a0911 [plane-symmetric].

Cosmology > s.a. gravitational thermodynamics; graviton.
* In general: The post-Newtonian coefficients coincide with those of general relativity, so the deviations from general relativity can be tested only in strong-gravity regimes; In its original version, the theory has a non-zero cosmological constant of the wrong sign.
@ General references: Kiritsis & Kofinas NPB(09); Calcagni JHEP(09)-a0904; Mukohyama et al PLB(09)-a0905 [radiation energy density]; Saridakis a0905 [and scalar field, dark energy]; Mukohyama PRD-a0905 [dark matter]; Minamitsuji a0905 [classification of evolutions]; Wang & Wu JCAP(09)-a0905 [thermodynamics]; Park a0906 [dark energy]; Appignani et al a0907 [and cosmological constant]; Carloni et al a0909/JCAP [as dynamical system]; Leon & Saridakis a0909 [phase-space analysis]; Dutta & Saridakis a0911.
@ Cosmological perturbations: Brandenberger PRD(09)-a0904 [and matter bounce]; Gao a0904; Gao et al a0905; Mukohyama JCAP(09)-a0904 [scale-invariant]; Yamamoto et al PRD(09)-a0907 [primordial power spectrum]; Wang & Maartens a0907; Kobayashi et al a0908 [large-scale evolution]; Wang et al a0909 [scalar]; Chen et al a0910 [power spectra of scalar and tensor modes]; Piao PLB(09) [primordial]; Gao et al a0911.

Modified Versions
@ References: Sotiriou et al PRL(09)-a0904 [phenomenologically viable extension], JHEP(09)-a0905 [classical evolution equations, graviton propagators]; Kluson a0907, a0910 [f(R) gravity]; Blas et al a0909 [healthy extension].


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