Super-nonradiative states in fractal quantum systems

Valeriy Abramov,S Arakelyan,A Evlyukhin,A Naumov,A Kalachev

doi:10.1051/epjconf/201922002001

Abstract

Theoretically the relationships of the main parameters of active nanoobjects with the Higgs boson and the Higgs field in a fractal quantum systems, super-nonradiative states of physical fields are investigated. The estimations of numbers, mass and rest energy of the neutrino (solar, electronic), the rest energy of Majorana neutrino, dark matter are obtained.

Highlights

Based on the hypothesis of the hierarchical structure of the Cosmos [1, 2], we can use experimental results in cosmology: for studying of anisotropic models of fractal cosmological objects; superradiance [1] of gravitational waves, relic photons from binary black holes, neutron stars; the nature of dark matter particles and dark energy [3], the chiral fractal structures of the Universe
Direct experiments (DAMA/LIBRA, CoGeNT, CRESST-II collaborations) [3] by observing the spectrum and the angular distribution γ radiation, the modulation spectrum from the galactic center show the following features: at the background of stochastic behavior the main local maximum near 2.4 keV and two local main minimums near 1.9 keV, 2.7 keV are observed
The calculated energy dm4 1.9053559 keV, d m4 2.6945803keV, which correspond to the local minima of the optical energy branches for dark matter with rest energy dm 1.7872164 keV, d m 2.5275057 keV, practically coincide with the position of the indicated local minima in the experimental modulation spectrum

Summary

Introduction

Based on the hypothesis of the hierarchical structure of the Cosmos [1, 2], we can use experimental results in cosmology: for studying of anisotropic models of fractal cosmological objects; superradiance [1] of gravitational waves, relic photons from binary black holes, neutron stars; the nature of dark matter particles and dark energy [3], the chiral fractal structures of the Universe. These states can be realized in two models. We assume a 0 a m , where a m (z A2 )1/2 ; a 02 a 2m zμ (zμ 2)/4 ; am2 z A2 ; Nra z A2 z , (2)

Results

Conclusion