On distortion of the background radiation spectrum by wormholes: kinematic Sunyaev-Zel'dovich effect
arXiv:1812.11082 · doi:10.1007/s10509-018-3489-5
Abstract
The problem of scattering of the background radiation on relic cosmological wormholes is considered. It is shown that static wormholes do not perturb the spectrum at all. The presence of peculiar velocities of wormholes results in a distortion of the CMB spectrum which is analogous to the kinematic Sunyaev-Zel'dovich effect. In the first order in the distortion of CMB cannot be separated from from the Compton scattering on electrons. In next orders the scattering on wormholes exhibits some difference from the Compton scattering. High-energy cosmic-ray particles spectrum does not change the form by KSZ, but undergoes a common Doppler shift. Such features may give a new tool to detect the presence of relic wormholes in our Universe.
accepted in Astrophysics and Space Science
References in corpus (5)
- Dark Matter Candidates from Particle Physics and Methods of Detection
- Fractal analysis of the galaxy distribution in the redshift range 0.45 < z < 5.0
- The Universal Rotation Curve of Spiral Galaxies
- Active Galactic Nuclei and Transformation of Dark Matter into Visible Matter
- Propagation of cosmic rays in the foam-like Universe
Cited by in corpus (7)
- Complexity for Dynamical Anisotropic Sphere in f(G,T) Gravity
- Identifying outliers in astronomical images with unsupervised machine learning
- Possible formation of ring galaxies by torus-shaped magnetic wormholes
- The Growth Rate of Supermassive Black Holes and Its Dependence on the Stellar Mass of Galaxies at the Present Epoch
- Peculiar Velocity Estimation from Kinetic SZ Effect using Deep Neural Networks
- Investigating the Behavior and Spatiotemporal Variations of Green Line Emission in the Solar Corona
- On The Spin Dynamics of Elongated Minor Bodies with Applications to a Possible Solar System Analogue Composition for `Oumuamua