Abstract We present Euclidean wormhole solutions describing possible bridges within the multiverse. The study is carried out in the framework of third quantisation. The matter content is modelled through a scalar field which supports the existence of a whole collection of universes. The instanton solutions describe Euclidean solutions that connect baby universes with asymptotically de Sitter universes. We compute the tunnelling probability of these processes. Considering the current bounds on the energy scale of inflation and assuming that all the baby universes are nucleated with the same probability, we draw some conclusions about which universes are more likely to tunnel and therefore undergo a standard inflationary era
A multidimensional cosmological model with space-time consisting of n (n>1) Einstein spaces M_i is i...
We present a few Euclidean wormhole configurations using both the analytic and numerical solutions o...
In this letter we obtain wormhole solutions from the Karmarkar condition in f(Q) gravity formalism, ...
We present Euclidean wormhole solutions describing possible bridges within the multiverse. The study...
9 pags., 4 figs., app. -- Open Access funded by Creative Commons Atribution Licence 4.0We present E...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
We study some gravitational instanton solutions that offer a natural realization of the spontaneous ...
© 2021 Elsevier B.V.We investigate Euclidean wormholes in Gauss–Bonnet-dilaton gravity to explain th...
We present some wormhole configurations using analytic and numerical solutions of the Euclidean fiel...
Abstract: We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormh...
Abstract: We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormh...
Axions play a central role in inflationary model building and other cosmological applications. This ...
A multidimensional cosmological model with space-time consisting of n (n>1) Einstein spaces M_i is i...
We present a few Euclidean wormhole configurations using both the analytic and numerical solutions o...
In this letter we obtain wormhole solutions from the Karmarkar condition in f(Q) gravity formalism, ...
We present Euclidean wormhole solutions describing possible bridges within the multiverse. The study...
9 pags., 4 figs., app. -- Open Access funded by Creative Commons Atribution Licence 4.0We present E...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
Within the framework of the third quantization, we consider the possibility that an initially recoll...
We study some gravitational instanton solutions that offer a natural realization of the spontaneous ...
© 2021 Elsevier B.V.We investigate Euclidean wormholes in Gauss–Bonnet-dilaton gravity to explain th...
We present some wormhole configurations using analytic and numerical solutions of the Euclidean fiel...
Abstract: We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormh...
Abstract: We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormh...
Axions play a central role in inflationary model building and other cosmological applications. This ...
A multidimensional cosmological model with space-time consisting of n (n>1) Einstein spaces M_i is i...
We present a few Euclidean wormhole configurations using both the analytic and numerical solutions o...
In this letter we obtain wormhole solutions from the Karmarkar condition in f(Q) gravity formalism, ...