In theories of gravity with a positive cosmological constant, we consider product solutions with flux, of the form (A)dS_p x S^q. Most solutions are shown to be perturbatively unstable, including all uncharged dS_p x S^q spacetimes. For dimensions greater than four, the stable class includes universes whose entropy exceeds that of de Sitter space, in violation of the conjectured "N-bound". Hence, if quantum gravity theories with finite-dimensional Hilbert space exist, the specification of a positive cosmological constant will not suffice to characterize the class of spacetimes they describe.Comment: 25 pages; v2: references adde
We consider a 4D spherically-symmetric static spacetime region as a collection of quanta in the semi...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We study the time evolution of entanglement entropy in expanding universes with various matters. To ...
We argue that the flat spacetime with inexact quantum mechanics in it is dual to the de Sitter space...
The de Sitter (dS) entropy bound gives the maximal number of e-folds that non-eternal inflation can ...
There are at least two cosmological constants calling for explanation. The first one describes the q...
We consider the quantum gravity partition function that counts the dimension of the Hilbert space of...
We use a result of Hawking and Gilkey to define a Euclidean path integral of gravity and matter whic...
Abstract: The covariant entropy bound states that the entropy, S, of matter on a light-sheet cannot ...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We study the von Neumann algebra description of the inflationary quasi-de Sitter (dS) space. Unlike ...
It has been argued that the entropy of de Sitter space corresponds to the entanglement between disco...
The Planck scale has been believed to be an unpassable wall. Putting a cutoff there and thinking of ...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We consider a 4D spherically-symmetric static spacetime region as a collection of quanta in the semi...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We study the time evolution of entanglement entropy in expanding universes with various matters. To ...
We argue that the flat spacetime with inexact quantum mechanics in it is dual to the de Sitter space...
The de Sitter (dS) entropy bound gives the maximal number of e-folds that non-eternal inflation can ...
There are at least two cosmological constants calling for explanation. The first one describes the q...
We consider the quantum gravity partition function that counts the dimension of the Hilbert space of...
We use a result of Hawking and Gilkey to define a Euclidean path integral of gravity and matter whic...
Abstract: The covariant entropy bound states that the entropy, S, of matter on a light-sheet cannot ...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We study the von Neumann algebra description of the inflationary quasi-de Sitter (dS) space. Unlike ...
It has been argued that the entropy of de Sitter space corresponds to the entanglement between disco...
The Planck scale has been believed to be an unpassable wall. Putting a cutoff there and thinking of ...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We consider a 4D spherically-symmetric static spacetime region as a collection of quanta in the semi...
Semiclassical gravity predicts that de Sitter space has a finite entropy. We suggest a picture for E...
We study the time evolution of entanglement entropy in expanding universes with various matters. To ...