The Robertson-Walker cosmological equation is generalized for the case of a flat world within the framework of the Kaluza-Klein theory in the absence of the cylindricity condition, which posits the hypothesis of a physical structure of the fifth dimension that can serve as a test object. The dependences of the Hubble parameter and the red shift parameter on the perturbation of the fifth dimension have been obtained here for the first time. A model of dark energy is proposed which treats it as the dynamic quintessence in the presence of a reactive potential, where the latter is the source of its effect upon gravitation. © 2014 Springer Science+Business Media New York
We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark ene...
[[abstract]]We present a new model of dark energy which could explain the observed accelerated expan...
A Friedman-Robertson-Walker cosmology arising from a five-dimensional Chern-Simons (CS) theory for t...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
The five-dimensional induced-matter theory is reformulated to describe matter and entropy creation i...
Kaluza-Klein theories are an elegant and highly predictive framework for unified theories. We relate...
32 pages. Corrected typos. Published as review article for IJMPD Special Issue on Modified Gravity a...
32 pages. Corrected typos. Published as review article for IJMPD Special Issue on Modified Gravity a...
We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark ene...
We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark ene...
[[abstract]]We present a new model of dark energy which could explain the observed accelerated expan...
A Friedman-Robertson-Walker cosmology arising from a five-dimensional Chern-Simons (CS) theory for t...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
The Robertson-Walker cosmological equation is generalized for the case of a flat world within the fr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
© 2017 Springer Science+Business Media, LLC On the basis of a scalar potential associated with Beltr...
The five-dimensional induced-matter theory is reformulated to describe matter and entropy creation i...
Kaluza-Klein theories are an elegant and highly predictive framework for unified theories. We relate...
32 pages. Corrected typos. Published as review article for IJMPD Special Issue on Modified Gravity a...
32 pages. Corrected typos. Published as review article for IJMPD Special Issue on Modified Gravity a...
We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark ene...
We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark ene...
[[abstract]]We present a new model of dark energy which could explain the observed accelerated expan...
A Friedman-Robertson-Walker cosmology arising from a five-dimensional Chern-Simons (CS) theory for t...