Titlebook: ;

友好關(guān)系

Some New Results in Theoretical CosmologyAfter a general introduction to the standard Friedman models we discuss the topology of the big bang and the horizon structure of inflationary universes.

不容置疑

Developing the Cosmology of A Continuous State UniverseAlthough popular, Bigbang cosmology still contains untested assumptions and unresolved problems. Recent observational and theoretical work suggest it has become feasible to consider introducing a new standard model of cosmology. Parameters for developing a Continuous State Universe (CSU) are introduced in a primitive initial form.

尖酸一點(diǎn)

What is the Evans-Vigier Field?We explain connections of the Evans-Vigier model with theories proposed previously. The Comay’s criticism is proved to be irrelevant.

流逝

Whitehead Meets Feynman and the Big Bang carries none of the above conserved quantities. Dense “vacuonic” history, unobservable by the scientific method, nevertheless carries conserved magnetic charge, contacts material history and participates in magnetodynamic action at a distance. One outcome is . for most standard-model elementary par

doxazosin

The Problem of Observation in Cosmology and the Big Banglogy has been extrapolated to realms beyond its observational applicability and despite its impressive achievements, this methodology may go counter to the usual requirement of verification on which all science rests. We will present fundamentally different approaches that may be more in accord with

Lacunar-Stroke

Bohm & Vigier: Ideas as A Basis for A Fractal Universeent paper tries to find an answer to these questions in the framework of the universality of a fractal structure of spacetime and of stochastic acceleration. Some arguments in favour of a fractal structure of spacetime at small and large scales areas follows. (i) Fractal trajectories in space with H

Albinism

Connections Between Thermodynamics, Statostocal Mechanics, Quantum Mechanics, and Special Astrophysieasing inclination of scientists to attribute this expansion to “vacuum energy.” However, since the universe is not in a state of thermodynamic equilibrium, then the commonly accepted notion of “vacuum energy” or “zero-point” energy may not really be accurate. Altering this perspective may be helpfu

A簡潔的

New Developments in Electromagnetic Field Theorythese extended theories are manifold, including both time-dependent states with wave phenomena and timeindependent states with electromagnetic equilibria. The former states are discussed with emphasis on plane waves, axisymmetric models of the individual photon with its integrated parameters and uni

bizarre

梯田

https://doi.org/10.1007/978-3-642-87576-2logy has been extrapolated to realms beyond its observational applicability and despite its impressive achievements, this methodology may go counter to the usual requirement of verification on which all science rests. We will present fundamentally different approaches that may be more in accord with