The Third Quantization: To Tunnel or Not to Tunnel?

Bouhmadi-López, Mariam; Krämer, Manuel; Morais, João; Robles-Pérez, Salvador

doi:10.3390/galaxies6010019

Cited by 2 publications

(1 citation statement)

References 32 publications

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“…The existence of this wormhole allows the transformation of a baby micro-universe into a new expanding universe, leading to inflation in a new region of the multiverse. By following [34,35], the probability of the tunnelling of a baby micro-universe can be computed as follows…”

Section: 𝜕𝑎mentioning

confidence: 99%

Bubbles Nucleation from a de Sitter-Planck background with Quantum Boltzmann Statistics

Licata¹,

Fiscaletti²,

Tamburini³

2022

Preprint

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– Every physical theory involving quantum fields does require a model of the quantum vacuum. The vacuum associated to quantum gravity must incorporate the prescriptions from both the theory of relativity and quantum physics. In this work, starting from the hypothesis of nucleation of sub-Planckian bubbles from a de Sitter vacuum, we study the necessary conditions to obtain baby universes, black holes and particles. The de Sitter-Planck background is described by an “infinite” Quantum Boltzmann statistics that generates fermions and bosons, and manifests itself as a deformation of the geometry that leads to a generalized uncertainty principle and a unified expression for the generalized Compton wavelength and event horizon size, drawing a connection between quantum black holes and elementary particles, the latter seen as a collective organization of the bubbles of the vacuum described by the generalized Compton wavelength. The quantum thermodynamics of black holes is then outlined and the physical history of each bubble is found to depend on the cosmological constant described in terms of thermodynamic pressure. Finally, a suggestive treatment of the Casimir effect is provided in the de Sitter-Planck background with Quantum-Boltzmann statistics and wormholes are explored as bubble coalescence processes.

show abstract

Section: 𝜕𝑎mentioning

confidence: 99%

Bubbles Nucleation from a de Sitter-Planck background with Quantum Boltzmann Statistics

Licata¹,

Fiscaletti²,

Tamburini³

2022

Preprint

View full text Add to dashboard Cite

show abstract

Bubble Nucleation from a de Sitter–Planck Background with Quantum Boltzmann Statistics

Fiscaletti

Licata²,

Tamburini³

2022

Symmetry

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Every physical theory involving quantum fields requires a model of quantum vacuum. The vacuum associated to quantum gravity must incorporate the prescriptions from both the theory of relativity and quantum physics. In this work, starting from the hypothesis of nucleation of sub-Planckian bubbles from a de Sitter vacuum, we study the necessary conditions to obtain baby universes, black holes and particles. The de Sitter-Planck background is described by an “infinite” Quantum Boltzmann statistics that generates fermions and bosons, and manifests itself as a deformation of the geometry that leads to a generalized uncertainty principle, a unified expression for the generalized Compton wavelength and event horizon size, drawing a connection between quantum black holes and elementary particles, seen as a collective organization of the bubbles of the vacuum described by the generalized Compton wavelength. The quantum thermodynamics of black holes is then outlined and the physical history of each bubble is found to depend on the cosmological constant described in terms of thermodynamic pressure. A treatment of the Casimir effect is provided in the de Sitter-Planck background, and finally wormholes are explored as bubble coalescence processes.

show abstract

The Third Quantization: To Tunnel or Not to Tunnel?

Cited by 2 publications

References 32 publications

Bubbles Nucleation from a de Sitter-Planck background with Quantum Boltzmann Statistics

Bubbles Nucleation from a de Sitter-Planck background with Quantum Boltzmann Statistics

Bubble Nucleation from a de Sitter–Planck Background with Quantum Boltzmann Statistics

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