Experiments on the CMB Spectrum, Big Jets Model and Their Implications for the Missing Half of the Universe

Abstract

Abstract. Based on the limiting continuation of Lorentz-Poincaré invariance, we propose an alternative formulation of the generalized Planck distribution for inertial and noninertial frames. The Lorentz invariant Planck distribution law leads to a new physical interpretation of the dipole anisotropy of the Cosmic Microwave Background. The Big Jets model predicts a distant 'antimatter blackbody,' whose radiations could make 50% of the sky very slightly warmer than the isotropic CMB temperature T CMB with a cosine function. The other 50% of the sky has the same isotropic temperature T CMB . Thus, we could have a pseudo-dipole anisotropy because the microwaves emitted from the antimatter blackbody are totally absorbed by our matter blackbody. We suggest that accurate data of satellite experiments might be used to search for the pseudo-dipole anisotropy and the missing half of the antimatter universe.

Big Jets model with CPT invariance and dynamics of expansion with quantum Yang–Mills gravity

“…After annihilations and decays, one fireball happened to be dominated by stable particles (baryons, electrons, antineutrinos) and formed matter half-universe, while the other was dominated by stable antiparticles (antibaryons, positrons, neutrinos) and formed antimatter half-universe. 8 From the vantage viewpoint of observers in each gigantic fireball, the evolution process is similar to that of a hot Big Bang model.…”

“…This prediction of a 'semi-dipole anisotropy' could be tested by satellite CMB data. 8 The usual Big Bang model would not result in such a 'semi-dipole asymmetry' of temperature in the CMB data.…”

“…This is related to the universal gravitational interaction of the T 4 tensor fields. The effective tensors G mhu µν and J µν in ( 2)-( 4), together with the replacement of S µν in (5) by T µν in (8), are postulated in the HHK model. b Thus, the dynamics b In the HHK model, one has T ν µ = (ρ, P, P, P ) and Tµν = T λ µ G mhu λν .…”

“…Such a distant antimatter half-universe (or blackbody) could be tested by a careful analysis of the satellite CMB data to see if there is a 'semi-dipole anisotropy' of ≈ 10 −5 or smaller. 8 The work was supported in part by the Jing Shin Research Fund of the UMassD Foundation.…”