Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories

We examine the validity of energy conditions of built-in inflation models in f(T) gravitational theories. For this purpose, we formulate the inequalities of energy conditions by assuming the flat and nonflat Friedmann-Robertson-Walker (FRW) universe. We find the feasible constraints on the constants...

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Main Author: Gamal G. L. Nashed
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2015/687940
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author Gamal G. L. Nashed
author_facet Gamal G. L. Nashed
author_sort Gamal G. L. Nashed
collection DOAJ
description We examine the validity of energy conditions of built-in inflation models in f(T) gravitational theories. For this purpose, we formulate the inequalities of energy conditions by assuming the flat and nonflat Friedmann-Robertson-Walker (FRW) universe. We find the feasible constraints on the constants of integration and evaluate their possible ranges graphically for the consistency of these energy conditions for flat, closed, and open universes. We constrain the constants of integration for flat space-time from the inflation epoch while the closed and open universe constants are constrained from late universe.
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spelling doaj-art-8c19cd804d0843ddaf3eeb68759bedb92025-02-03T05:59:10ZengWileyAdvances in High Energy Physics1687-73571687-73652015-01-01201510.1155/2015/687940687940Energy Conditions of Built-In Inflation Models in f(T) Gravitational TheoriesGamal G. L. Nashed0Centre for Theoretical Physics, The British University in Egypt, P.O. Box 43, Sherouk City 11837, EgyptWe examine the validity of energy conditions of built-in inflation models in f(T) gravitational theories. For this purpose, we formulate the inequalities of energy conditions by assuming the flat and nonflat Friedmann-Robertson-Walker (FRW) universe. We find the feasible constraints on the constants of integration and evaluate their possible ranges graphically for the consistency of these energy conditions for flat, closed, and open universes. We constrain the constants of integration for flat space-time from the inflation epoch while the closed and open universe constants are constrained from late universe.http://dx.doi.org/10.1155/2015/687940
spellingShingle Gamal G. L. Nashed
Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
Advances in High Energy Physics
title Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
title_full Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
title_fullStr Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
title_full_unstemmed Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
title_short Energy Conditions of Built-In Inflation Models in f(T) Gravitational Theories
title_sort energy conditions of built in inflation models in f t gravitational theories
url http://dx.doi.org/10.1155/2015/687940
work_keys_str_mv AT gamalglnashed energyconditionsofbuiltininflationmodelsinftgravitationaltheories