2004
DOI: 10.1134/1.1755396
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Cosmological production of vector bosons and cosmic microwave background radiation

Abstract: -The intensive cosmological creation of vector W, Z-bosons in the cosmological model with the relative units is considered. Field theoretical models are studied, which predict that the CMB radiation and the baryon matter in the universe can be products of decay and annihilation processes of these primordial bosons.

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Cited by 21 publications
(28 citation statements)
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“…We can see that this value surprisingly close to the observed temperature of the CMB radiation T c = T CMB = 2.73 K. The primordial mesons before their decays polarize the Dirac fermion vacuum and give the baryon asymmetry frozen by the CPviolation, so that n b /n γ ∼ X CP ∼ 10 −9 , Ω b ∼ α qed / sin 2 θ Weinberg ∼ 0.03, and Ω R ∼ 10 −5 ÷ 10 −4 [15].…”
Section: The Diffeomorphism-invariant Perturbation Theorymentioning
confidence: 62%
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“…We can see that this value surprisingly close to the observed temperature of the CMB radiation T c = T CMB = 2.73 K. The primordial mesons before their decays polarize the Dirac fermion vacuum and give the baryon asymmetry frozen by the CPviolation, so that n b /n γ ∼ X CP ∼ 10 −9 , Ω b ∼ α qed / sin 2 θ Weinberg ∼ 0.03, and Ω R ∼ 10 −5 ÷ 10 −4 [15].…”
Section: The Diffeomorphism-invariant Perturbation Theorymentioning
confidence: 62%
“…In the case of the stiff state: E ϕ = Q/ϕ, there is an exact solution of Bogoliubov's equation of a number of "universes" [16] These initial data ϕ I and H I are determined by parameters of matter cosmologically created from the Bogoliubov vacuum in beginning of a universe η ≃ 0. In the Standard Model (SM), W-, Z-vector bosons have maximal probability of this cosmological creation due to their mass singularity [15]. The uncertainty principle △E · △η ≥ 1 (where △E = 2M I , △η = 1/2H I ) shows us that at the moment of creation of vector bosons their Compton lengths defined by its inverse mass M …”
Section: The Diffeomorphism-invariant Perturbation Theorymentioning
confidence: 99%
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“…Therefore, (conformal) gravitons in quantum CCGR are obliged to have bilinear dynamics. Action (46) defined the cosmological dynamics of the model, while (48) the driving interaction between global (cosmological) and local physics.…”
Section: Quantum Features Of Ccgrmentioning
confidence: 99%
“…Thus, one can associate the plain wave solution (53) with a single graviton state, and the series (61) should be viewed as an expansion in single graviton states. Action (47) defines bilinear graviton dynamics, while the actions (46) and (48) define cosmological dynamics and gravity self-interaction correspondingly. Therefore, we obtain a new way to perform perturbative quantization of gravity with the use of new symmetry in the low energy regime.…”
Section: Quantum Features Of Ccgrmentioning
confidence: 99%