
In the paper it is shown that the model with scalar ghost-field and other components of matter can explain the two main facts from modern cosmology that is the dark matter and accelerating expansion of the Universe. In such models the probability exists to obtain the representation of an inhomogeneous structure of a matter distribution forming in a nonlinear regime.
Universe, Majumadar-Papapetrou metric, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), dark matter, Relativistic cosmology
Universe, Majumadar-Papapetrou metric, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), dark matter, Relativistic cosmology
| citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 21 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 10% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
