The uniform expansion of the Universe

Klimenko, Alexey; Klimenko, V. A.; Fridman, A. M.

doi:10.1134/s106377291010001x

Cited by 2 publications

(8 citation statements)

References 21 publications

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“…To describe them, the standard Einstein's equations must be generalized. The adjusted technique of introducing cosmological repulsion forces into the equations of Einstein's, previously described in [19], for the convenience of readers, placed in section III of present work. Five-dimensional space-time associated with the coordinate system K 4 , is flat.…”

Section: Dynamics Of Hot 3r-worldmentioning

confidence: 99%

“…Into the equations of general relativity, except for Einstein's repulsion forces associated with Λ-term, can be introduced others cosmological forces of repulsion [19].…”

Section: E Generalized Einstein's Equation For 3r-worldmentioning

confidence: 99%

“…Have long had an almost uniform expansion of the universe. So, apparently, is not by chance a good approximation to describe its dynamics is an S-model (model of a uniformly expanding universe), proposed in [19].…”

Section: Explanation Of Observational Datamentioning

confidence: 99%

“…l 0 = 10pc (see, eq, [19]). Figure 2 shows the function (m − M)(z), calculated by formula (109), and observational data for supernova type Ia, with, presumably, the same absolute luminosity at the peak of their brilliance.…”

Section: Explanation Of Observational Datamentioning

confidence: 99%

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Centrifugal cosmological repulsive force in a homogeneous universe

Klimenko,

Klimenko

2011

Preprint

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We study the dynamics of homogeneous isotropic three-dimensional worlds filled with radiation (3R-worlds). It is shown that the dynamics of these worlds with the additional fourth large-scale spatial dimension leads to an important effect. At 3R-worlds the forces of repulsion appear. The source of these forces is the thermal energy of the radiation that fills these worlds. In the four-dimensional space, these forces are centrifugal. They operate in an external for 3R-world spatial dimension and stretch it. In the three-dimensional comoving coordinate system the centrifugal forces shows themselves as forces of repulsion. Standard Einstein's equations do not describe these forces.Written generalized Einstein's equation describing the dynamics of a homogeneous isotropic universe, taking into consideration the centrifugal forces of repulsion. We propose a cosmological model of the universe, based on these equations. This model apply to explain the observation data.

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Section: Dynamics Of Hot 3r-worldmentioning

confidence: 99%

“…Into the equations of general relativity, except for Einstein's repulsion forces associated with Λ-term, can be introduced others cosmological forces of repulsion [19].…”

Section: E Generalized Einstein's Equation For 3r-worldmentioning

confidence: 99%

Section: Explanation Of Observational Datamentioning

confidence: 99%

Section: Explanation Of Observational Datamentioning

confidence: 99%

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Centrifugal cosmological repulsive force in a homogeneous universe

Klimenko,

Klimenko

2011

Preprint

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“…0 , l 0 = 10пс (for details, see, e.g., [1,20]). The photometric distance r(z) is calculated as follows:…”

Section: The Dependence Apparent Magnitude Redshift For Type Ia Super...mentioning

confidence: 99%

The geometric interpretation of the cosmological repulsion forces

Klimenko,

Klimenko

2012

Preprint

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It seems likely that the generalized Einstein equations are not complete and only partly account for the effect on the Universe dynamics of that part of the energy of the space environment the change of which is purely geometric. There are offered the generalized Einstein's equations, describing not only the gravity forces, but also the cosmological forces of repulsion, which are geometric in their nature.The generalized Einstein equations are used to derive the cosmological Friedman's equations describing the dynamics of a homogeneous isotropic universe with the influence of cosmological repulsion forces. We propose a cosmological model of the universe based on these equations. Application of the model for explanation of the observations is considered here.

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The uniform expansion of the Universe

Cited by 2 publications

References 21 publications

Centrifugal cosmological repulsive force in a homogeneous universe

Centrifugal cosmological repulsive force in a homogeneous universe

The geometric interpretation of the cosmological repulsion forces

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