Abstract
Significant progress in the development of observational techniques gives us the hope to directly observe cosmological wormholes. We have collected basic effects produced by the scattering of radiation on wormholes, which can be used in observations. These are the additional topological damping of cosmic rays, the generation of a diffuse background around any discrete source, the generation of an interference picture, and distortion of the cosmic microwave background (CMB) spectrum. It turns out that wormholes in the leading order mimic perfectly analogous effects of the scattering of radiation on the standard matter (dust, hot electron gas, etc.). However, in higher orders, a small difference appears, which allows for disentangling effects of wormholes and ordinary matter.
Highlights
The greatest development of observational techniques that we observe in modern astrophysics allows us to challenge one of the most intriguing astrophysical problem, which is the direct observation of primordial wormholes
M(Ropt )/L & 1, which means that there is a small amount of DM, in low-surface-brightness (LSB). Galaxies, such a ratio may reach M(Ropt )/L ∼ 103. Such a correlation between the surface brightness and the amount of DM in galaxies could give indirect evidence for the topological nature of DM; in accordance with Equation (14), the number of wormholes determines the damping of cosmic rays, and analogously the number of wormholes determines the amount of dark matter in galaxies [10]
We have shown that wormholes produce a number of effects that can be disentangled from effects produced by ordinary matter
Summary
The greatest development of observational techniques that we observe in modern astrophysics allows us to challenge one of the most intriguing astrophysical problem, which is the direct observation of primordial wormholes. The rate of the expansion overruns the increase in the horizon size, and, regions that were causally connected lose such a connection very rapidly Such a rapid increase in the scale factor plays the role of the external field, which is capable of creating particles from zero-point fluctuations and real wormholes from virtual wormholes. Such a process (the creation of wormholes during of the inflationary stage) is not described rigorously yet, but there are no doubts that some. The widening of the background spectrum depends in a specific way on peculiar motions of wormholes This leads to a scale-dependent renormalization of all discrete sources of radiation, while the diffuse halo should correlate with the dark matter distribution around the source.
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