Quantum Generation of Dark Energy
A. de la Macorra, F. Briscese

TL;DR
This paper proposes a unified model where dark energy is generated through quantum transitions of a scalar field, which also unifies inflation and dark energy, explaining the cosmological coincidence problem.
Contribution
It introduces a novel quantum transition mechanism for dark energy generation and unifies inflation with dark energy using a single scalar field and potential.
Findings
Dark energy particles are produced at very low energies (~eV)
The model links inflation scale to dark energy and reheating processes
It provides a natural explanation for the timing of dark energy emergence
Abstract
We present a type of dark energy models where the particles of dark energy phi are dynamically produced via a quantum transition at very low energies. The scale where the transition takes places depends on the strength g of the interaction between phi and a relativistic field varphi. We show that a g \simeq 10^{-12} gives a generation scale E_gen simeq eV with a cross section sigma simeq 1 pb close to the WIMPs cross section sigma_w simeq pb at decoupling. The number density n_phi of the \phi particles are a source term in the eq. of motion of phi and it generates the scalar potential v(phi) responsible for the late time acceleration of our universe. Since the appearance of phi may be at very low scales, close to present time, the cosmological coincidence problem can be explained simply due to the size of the coupling constant. We unify dark energy with inflation in terms of a single…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
