Results 71 to 80 of about 458,070 (185)
Generalized Einstein’s Equations from Wald Entropy [PDF]
We derive the gravitational equations of motion of general theories of gravity from thermodynamics applied to a local Rindler horizon through any point in spacetime.
Sarkar, Sudipta +3 more
core +1 more source
Quantum geometry and gravitational entropy [PDF]
Most quantum states have wavefunctions that are widely spread over the accessible Hilbert space and hence do not have a good description in terms of a single classical geometry. In order to understand when geometric descriptions are possible, we exploit the AdS/CFT correspondence in the half-BPS sector of asymptotically AdS_5 x S^5 universes.
Simon, Joan +4 more
openaire +3 more sources
On relativistic generalization of Perelman’s W-entropy and thermodynamic description of gravitational fields and cosmology [PDF]
Using double $$2+2$$ and $$3+1$$ nonholonomic fibrations on Lorentz manifolds, we extend the concept of W-entropy for gravitational fields in general relativity (GR). Such F- and W-functionals were introduced in the Ricci flow theory of three dimensional
Olivia Vacaru +5 more
core +2 more sources
Gravitational entropy is observer-dependent
In quantum gravity, it has been argued that a proper accounting of the role played by an observer promotes the von Neumann algebra of observables in a given spacetime subregion from Type III to Type II.
Julian De Vuyst +3 more
doaj +1 more source
ENTROPY OF GRAVITATIONAL WAVES
Gravitational waves (GWs), the propagating perturbations within the structure of spacetime, provide a unique window into the dynamics of massive celestial objects and their cataclysmic events such as binary black hole (BBH), black hole – neutron star, binary neutron star (BNS) merger.
Nurzhan Ussipov +5 more
openaire +1 more source
Time evolution of entropy in gravitational collapse [PDF]
9 pages, 6 ...
openaire +2 more sources
Gravitational entropy and thermodynamics away from the horizon [PDF]
We define, by an integral of geometric quantities over a spherical shell of arbitrary radius, an invariant gravitational entropy. This definition relies on defining a gravitational energy and pressure, and it reduces at the horizon of both black branes ...
Brustein, R, Medved, A J M
core +2 more sources
Hot and Heavy Matters in the Foundations of Statistical Mechanics [PDF]
Are the generalizations of classical equilibrium thermodynamics true of self-gravitating systems? This question has not been addressed from a foundational perspective, but here I tackle it through a study of the "paradoxes" commonly said to afflict such ...
Craig Callender, Callender, Craig
core +1 more source
Gravitational entropy and the flatness, homogeneity and isotropy puzzles
We suggest a new explanation for the observed large scale flatness, homogeneity and isotropy of the universe. The basic ingredients are Einstein's theory of gravity and Hawking's method of computing the gravitational entropy. The new twist is provided by
Neil Turok, Latham Boyle
doaj +1 more source
Replica wormholes and the entropy of Hawking radiation
The information paradox can be realized in anti-de Sitter spacetime joined to a Minkowski region. In this setting, we show that the large discrepancy between the von Neumann entropy as calculated by Hawking and the requirements of unitarity is fixed by ...
Ahmed Almheiri +4 more
doaj +1 more source

