Logo

The Shape of the Universe by Gerd Pommerenke

Small book cover: The Shape of the Universe

The Shape of the Universe
by

Publisher: viXra
Number of pages: 321

Description:
A special solution of the Maxwell equations is presented, which disposes of the properties the recently postulated Higgs-field must have, if it should not violate already secured perceptions and observations. If both fields are identical remains to be seen at this time. An alternative vacuum propagation function for EM-waves is presented too, describing effects like the cosmologic red-shift and the unexpected results of the SN-cosmology-experiment, completely without dark matter etc.

Home page url

Download or read it online for free here:
Download link
(29MB, PDF)

Similar books

Book cover: Introductory Lectures on Quantum CosmologyIntroductory Lectures on Quantum Cosmology
by - arXiv
The modern approach to quantum cosmology, as initiated by Hartle and Hawking, Linde, Vilenkin and others. We explain how one determines the consequences for the late universe of a given quantum theory of cosmological initial or boundary conditions.
(17709 views)
Book cover: Introduction to Early Universe CosmologyIntroduction to Early Universe Cosmology
by - arXiv
This text covers the theory of cosmological perturbations, which describes the generation of inhomogeneities in the early universe and their evolution until the current time. The theory is applied to three classes of models of the early universe.
(13519 views)
Book cover: The Cosmic Web: Geometric AnalysisThe Cosmic Web: Geometric Analysis
by - arXiv
The lecture notes describe the Delaunay Tessellation Field Estimator for Cosmic Web analysis. The high sensitivity of Voronoi/Delaunay tessellations to the local point distribution is used to obtain estimates of density and related quantities.
(14081 views)
Book cover: Cosmic Microwave Background Anisotropies up to Second OrderCosmic Microwave Background Anisotropies up to Second Order
by - arXiv
These notes present the computation of the system of Boltzmann equations describing the evolution of the photon, baryon and cold dark matter fluids up to second order in perturbation theory. They follow the time evolution of the CMB anisotropies.
(12092 views)