2015
DOI: 10.1007/s10714-015-1852-1
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Emergent cosmology, inflation and dark energy

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Cited by 83 publications
(127 citation statements)
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“…as (7) and (25). Finally for the stress energy tensor, which comes from variation with respect to the metric we obtain…”
Section: Equation Of Motion and Solutions For Diffusive Energy Withoumentioning
confidence: 96%
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“…as (7) and (25). Finally for the stress energy tensor, which comes from variation with respect to the metric we obtain…”
Section: Equation Of Motion and Solutions For Diffusive Energy Withoumentioning
confidence: 96%
“…Therefore we develop from a generalization of two measure theories [17][18][19][20][21][22][23][24][25][26][27][28] a "diffusive energy theory" which can produce on one hand a non-conserved stress energy tensor (T μν (χ ) ), as in (1), and on the other hand the conserved stress energy tensor (T μν (G) ) that we know from the right hand side of Einstein's equation. As we will see, this suggested theory is asymptotically different from the φCDM model, and more close in this limit to the standard CDM.…”
Section: Introductionmentioning
confidence: 99%
“…Let us particularly stress that the method of non-Riemannian spacetime volumeforms is a very powerful one having profound impact in any (field theory) models with general coordinate reparametrization invariance, such as general relativity and its extensions [27]- [31], [32]- [36], [37]- [39]; strings and (higher-dimensional) membranes [40,41]; and supergravity [42,43]. Among its main features we should mention:…”
Section: Introductionmentioning
confidence: 99%
“…• Employing two independent non-Riemannian volume-forms produces effective scalar potential with two infinitely large flat regions [37,38] (one for large negative and another one for large positive values of the scalar field ϕ) with vastly different scales appropriate for a unified description of both the early and late universe' evolution. A remarkable feature is the existence of a stable initial phase of non-singular universe creation preceding the inflationary phase -stable "emergent universe" without "Big-Bang" [37].…”
Section: Introductionmentioning
confidence: 99%
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