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Cosmic scenario of early universe in context of Euclidean wormhole in dilatonic Einstein–Gauss–Bonnet gravity.

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Title: Cosmic scenario of early universe in context of Euclidean wormhole in dilatonic Einstein–Gauss–Bonnet gravity.
Authors: Biswas, Gargi1 (AUTHOR) biswasgb@gmail.com, Modak, B.1 (AUTHOR) bijanmodak@yahoo.co.in
Source: Modern Physics Letters A. 5/10/2022, Vol. 37 Issue 14, p1-24. 24p.
Abstract: In this paper, we present some wormhole configurations using analytic and numerical solutions of the Euclidean field equations considering Einstein–Gauss–Bonnet dilaton coupled interaction in the Robertson–Walker metric. Analytic solutions invoking slow-roll type approximation for some potentials yield identical wormholes in the early era. Eventually, in later era, the universe enters to an expanding era much faster than usual inflation accompanied by oscillations with analytic continuation τ = i t. The numerical solutions of wormholes in terms of the scale factor a (τ) are almost identical for some standard potentials of the dilaton field, except for the evolution of potentials. The Hubble parameter and deceleration parameter obtained by curve fit of a (τ) of the numerical solution of wormhole yield an inflationary era away from the throat of the wormhole using τ = i t. A sharp decay of the potential is also observed. [ABSTRACT FROM AUTHOR]
Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Cosmic scenario of early universe in context of Euclidean wormhole in dilatonic Einstein–Gauss–Bonnet gravity.
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  Data: <searchLink fieldCode="AR" term="%22Biswas%2C+Gargi%22">Biswas, Gargi</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> biswasgb@gmail.com</i><br /><searchLink fieldCode="AR" term="%22Modak%2C+B%2E%22">Modak, B.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> bijanmodak@yahoo.co.in</i>
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  Data: <searchLink fieldCode="JN" term="%22Modern+Physics+Letters+A%22">Modern Physics Letters A</searchLink>. 5/10/2022, Vol. 37 Issue 14, p1-24. 24p.
– Name: Abstract
  Label: Abstract
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  Data: In this paper, we present some wormhole configurations using analytic and numerical solutions of the Euclidean field equations considering Einstein–Gauss–Bonnet dilaton coupled interaction in the Robertson–Walker metric. Analytic solutions invoking slow-roll type approximation for some potentials yield identical wormholes in the early era. Eventually, in later era, the universe enters to an expanding era much faster than usual inflation accompanied by oscillations with analytic continuation τ = i t. The numerical solutions of wormholes in terms of the scale factor a (τ) are almost identical for some standard potentials of the dilaton field, except for the evolution of potentials. The Hubble parameter and deceleration parameter obtained by curve fit of a (τ) of the numerical solution of wormhole yield an inflationary era away from the throat of the wormhole using τ = i t. A sharp decay of the potential is also observed. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1142/S0217732322500833
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        Text: English
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              Text: 5/10/2022
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              Y: 2022
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