scholarly journals No de Sitter Invariant Vacuum in Massive Gravity Theory with Ghost

2009 ◽  
Vol 121 (2) ◽  
pp. 419-426 ◽  
Author(s):  
K. Izumi ◽  
T. Tanaka
Keyword(s):  
Massive Gravity ◽  
Gravity Theory ◽  
De Sitter

scholarly journals De Sitter vacua in ghost-free massive gravity theory

2015 ◽  
Vol 751 ◽  
pp. 19-24 ◽  
Author(s):  
Charles Mazuet ◽  
Mikhail S. Volkov
Keyword(s):  
Massive Gravity ◽  
Gravity Theory ◽  
De Sitter ◽  
De Sitter Vacua

scholarly journals The third way to 3D gravity

2015 ◽  
Vol 24 (12) ◽  
pp. 1544015 ◽  
Author(s):  
Eric Bergshoeff ◽  
Wout Merbis ◽  
Alasdair J. Routh ◽  
Paul K. Townsend
Keyword(s):  
Equations Of Motion ◽  
Massive Gravity ◽  
De Sitter ◽  
Gravitational Field Equation ◽  
Third Way ◽  
Metric Tensor ◽  
The Third ◽  
Higher Dimensional ◽  
Conservation Condition ◽  
3D Gravity

Consistency of Einstein’s gravitational field equation [Formula: see text] imposes a “conservation condition” on the [Formula: see text]-tensor that is satisfied by (i) matter stress tensors, as a consequence of the matter equations of motion and (ii) identically by certain other tensors, such as the metric tensor. However, there is a third way, overlooked until now because it implies a “nongeometrical” action: one not constructed from the metric and its derivatives alone. The new possibility is exemplified by the 3D “minimal massive gravity” model, which resolves the “bulk versus boundary” unitarity problem of topologically massive gravity with Anti-de Sitter asymptotics. Although all known examples of the third way are in three spacetime dimensions, the idea is general and could, in principle, apply to higher dimensional theories.

scholarly journals Anisotropic deformations of spatially open cosmology in massive gravity theory

2017 ◽  
Vol 2017 (04) ◽  
pp. 039-039
Author(s):  
Charles Mazuet ◽  
Shinji Mukohyama ◽  
Mikhail S. Volkov
Keyword(s):  
Massive Gravity ◽  
Gravity Theory

Causality of 3D extended gravity theories

2019 ◽  
Vol 34 (16) ◽  
pp. 1950122
Author(s):  
Meguru Komada
Keyword(s):  
Shock Wave ◽  
Three Dimensional ◽  
Massive Gravity ◽  
Gravity Theory ◽  
Delay Effect ◽  
Fundamental Physics ◽  
Extended Gravity ◽  
3D Gravity ◽  
Gravity Theories ◽  
Time Delay Effect

Causality is one of the most important properties to understand gravity theories. It gives us not only a method to confirm that the gravity theories are really consistent, but also gives implications about the properties which unknown fundamental physics should obey. We investigate the causality of three-dimensional (3D) gravity theories, which are considered to be important, by using the Shapiro time delay effect in the Shock wave geometry. One of such gravity theories is the Zwei-Dreibein Gravity (ZDG) theory, which is a consistent 3D gravity theory. In ZDG theory, the serious problems can be removed that have appeared in another important gravity theory called New Massive Gravity (NMG). We study whether the ZDG theory could preserve the causality without losing the above good properties and how the causality structure is related to the structure of the NMG theory.

scholarly journals Bouncing cosmologies in massive gravity on de Sitter

2013 ◽  
Vol 30 (20) ◽  
pp. 205012 ◽  
Author(s):  
David Langlois ◽  
Atsushi Naruko
Keyword(s):  
Massive Gravity ◽  
De Sitter ◽  
Bouncing Cosmologies

scholarly journals Quantum topologically massive gravity in de Sitter space

2011 ◽  
Vol 2011 (8) ◽  
Author(s):  
Alejandra Castro ◽  
Nima Lashkari ◽  
Alexander Maloney
Keyword(s):  
De Sitter Space ◽  
Massive Gravity ◽  
De Sitter ◽  
Topologically Massive Gravity

scholarly journals On the black holes in alternative theories of gravity: The case of nonlinear massive gravity

2015 ◽  
Vol 24 (03) ◽  
pp. 1550022 ◽  
Author(s):  
Ivan Arraut
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Degrees Of Freedom ◽  
Massive Gravity ◽  
Alternative Theories Of Gravity ◽  
De Sitter ◽  
Theories Of Gravity ◽  
Bound Orbits ◽  
Black Hole Temperature ◽  
Alternative Theories

I derive general conditions in order to explain the origin of the Vainshtein radius inside dRGT. The set of equations, which I have called "Vainshtein" conditions are extremal conditions of the dynamical metric (gμν) containing all the degrees of freedom of the theory. The Vainshtein conditions are able to explain the coincidence between the Vainshtein radius in dRGT and the scale [Formula: see text], obtained naturally from the Schwarzschild de-Sitter (S-dS) space inside general relativity (GR). In GR, this scale was interpreted as the maximum distance in order to get bound orbits. The same scale corresponds to the static observer position if we want to define the black hole temperature in an asymptotically de-Sitter space. In dRGT, the scale marks a limit after which the extra degrees of freedom of the theory become relevant.

scholarly journals One-loop divergences in massive gravity theory

2012 ◽  
Vol 712 (1-2) ◽  
pp. 104-108 ◽  
Author(s):  
I.L. Buchbinder ◽  
D.D. Pereira ◽  
I.L. Shapiro
Keyword(s):  
Massive Gravity ◽  
Gravity Theory

Thermal corrections of Born–Infeld–anti-de Sitter black hole in massive gravity

2019 ◽  
Vol 34 (27) ◽  
pp. 1950222
Author(s):  
Abdul Jawad ◽  
Shahid Chaudhary
Keyword(s):  
Black Hole ◽  
Critical Points ◽  
Thermal Fluctuations ◽  
Massive Gravity ◽  
Vital Role ◽  
De Sitter ◽  
Logarithmic Corrections ◽  
The Impact

The impact of thermal fluctuations on the thermodynamics of Born–Infeld–anti-de Sitter black hole is being investigated. For this purpose, we analyze the consequences of logarithmic corrections on thermodynamics potentials like Helmholtz and Gibbs. We find out the relations for critical points and stability and observe that thermal corrections play a vital role in them.

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