Cosmological Constant as the Coefficient of Quantum Tunneling in the Universe Exterior
Vladan Pankovic, Miodrag krmar, Sima Ciganovic

TL;DR
This paper proposes a model where the cosmological constant arises from quantum tunneling of vacuum fluctuations at the universe's boundary, aligning with quantum theory and observational data.
Contribution
It introduces a novel interpretation of the cosmological constant as a tunneling coefficient of vacuum fluctuations at the universe's boundary.
Findings
Consistent with quantum mechanics and quantum field theory.
Aligns with WMAP observational data.
Supports the fine-tuning condition of the cosmological constant.
Abstract
In this work we suggest a simple model of the cosmological constant as the coefficient of the quantum tunneling of vacuum fluctuations (with wave length larger than Planck length) at tiny, boundary spherical shell of the universe (with thickness equivalent to Planck length and radius equivalent to scale factor). Roughly speaking, given fluctuations can, by quantum tunneling (i.e. scattering with a potential barrier with highness equivalent to Planck energy and width proportional to, approximately, three hundred Planck length) leave universe and arrive in its exterior, i.e. multi-universe (in sense of Linde chaotic inflation theory universe can be considered as a causally-luminally connected space domain while its exterior can be considered as a space domain without causal-luminal connections with universe). It is in full agreement with usual quantum mechanics and quantum field theory as…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Dark Matter and Cosmic Phenomena
