We suggest that the (small but nonvanishing) cosmological constant, and the holographic properties of gravitational entropy, may both reflect unconventional quantum spin-statistics at a fundamental level. This conjecture is motivated by the nonlocality of quantum gravity and the fact that spin is an inherent property of spacetime. As an illustration we consider the `quon' model which interpolates between fermi and bose statistics, and show that this can naturally lead to an arbitrarily small cosmological constant. In addition to laboratory tests, we briefly discuss the possible observable imprint on cosmological fluctuations from inflation
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
Spacetime geometry is treated as a fluctuating, stochastic quantum system allowing an effective quan...
Bootstrapped Newtonian gravity was developed with the purpose of estimating the impact of quantum ph...
Many years ago Friedman and Sorkin [1] established the existence of certain topological solitonic ex...
Quantum gravity – as defined in the Feynman path integral approach by a gravitational action and a f...
The value of the cosmological constant is one of the major puzzles of modern cosmology: it is tiny b...
Recent astrophysical observations seem to indicate that the cosmological constant is small but nonze...
We point out that for a large class of universes, holography implies that the most probable value fo...
A nonlocal quantum gravity theory is presented which is finite and unitary to all orders of perturba...
Quantum gravity has been so elusive because we have tried to approach it by two paths which can neve...
The cosmological constant problem is turned around to argue for a new foundational physics postulate...
Gravitational holography is argued to render the cosmological constant stable against divergent quan...
Quantum gravity places entirely new challenges on the formulation of a consistent theory as well as ...
For almost a century, the cosmological constant has been a mysterious object, in relation to both it...
Under the assumption that the cosmological constant vanishes in the true ground state with lowest po...
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
Spacetime geometry is treated as a fluctuating, stochastic quantum system allowing an effective quan...
Bootstrapped Newtonian gravity was developed with the purpose of estimating the impact of quantum ph...
Many years ago Friedman and Sorkin [1] established the existence of certain topological solitonic ex...
Quantum gravity – as defined in the Feynman path integral approach by a gravitational action and a f...
The value of the cosmological constant is one of the major puzzles of modern cosmology: it is tiny b...
Recent astrophysical observations seem to indicate that the cosmological constant is small but nonze...
We point out that for a large class of universes, holography implies that the most probable value fo...
A nonlocal quantum gravity theory is presented which is finite and unitary to all orders of perturba...
Quantum gravity has been so elusive because we have tried to approach it by two paths which can neve...
The cosmological constant problem is turned around to argue for a new foundational physics postulate...
Gravitational holography is argued to render the cosmological constant stable against divergent quan...
Quantum gravity places entirely new challenges on the formulation of a consistent theory as well as ...
For almost a century, the cosmological constant has been a mysterious object, in relation to both it...
Under the assumption that the cosmological constant vanishes in the true ground state with lowest po...
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
Spacetime geometry is treated as a fluctuating, stochastic quantum system allowing an effective quan...
Bootstrapped Newtonian gravity was developed with the purpose of estimating the impact of quantum ph...