Editorial: New Developments in Cosmology and Gravitation from Extended Theories of General Relativity
| Autor: | Mauricio Bellini, Kishor S. Adhav, José Edgar Madriz Aguilar, Dandala R. K. Reddy |
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| Jazyk: | angličtina |
| Rok vydání: | 2014 |
| Předmět: |
Physics
Nuclear and High Energy Physics Article Subject General relativity Ciencias Físicas Scalar theories of gravitation Non-standard cosmology GRAVITATION Astrophysics::Cosmology and Extragalactic Astrophysics Cosmological constant purl.org/becyt/ford/1.3 [https] Física de Partículas y Campos lcsh:QC1-999 Physical cosmology Gravitation purl.org/becyt/ford/1 [https] General Relativity and Quantum Cosmology Theoretical physics De Sitter universe COSMOLOGY Dark energy CIENCIAS NATURALES Y EXACTAS lcsh:Physics |
| Zdroj: | CONICET Digital (CONICET) Consejo Nacional de Investigaciones Científicas y Técnicas instacron:CONICET Advances in High Energy Physics, Vol 2014 (2014) Advances in High Energy Physics |
| Popis: | Extensions and modifications to the standard 4D theory of general relativity are topics that have an increasing impact in top original research on gravitation and cosmology. This issue compiles exciting papers that can be very interesting for researchers who could be interested in the study of extended theories of general relativity focused on cosmology and gravitation. An important topic for the present day cosmology consists in explaining why the universe is accelerated and how this acceleration is related to an unknown kind of energy called “dark energy.” In this issue it is considered a cosmic fluid as a quasi-static thermodynamic system. The status of the generalized second law of thermodynamics is investigated and the range of validity for the equation of state parameter is derived for a few important cosmological models. The physical origin of dark energy can be explored using a condensate of spinors which are free of interactions in a 5D relativistic vacuum defined in an extended de Sitter spacetime which is Riemann flat. This condensate of spinors could be an interesting candidate to explain the presence of dark energy in the early universe, during the inflationary stage. A new method for the study of general higher dimensional Kaluza-Klein theories based on the Riemannian adapted connection and on a theory of adapted tensor fields in the ambient space is also interesting to be studied. This topic can be explored in ac ovariant form and it is very |
| Databáze: | OpenAIRE |
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