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Waheed, Saira
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Advances in High Energy Physics
Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
Nuclear and High Energy Physics
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spelling Sharif, M. Waheed, Saira 1687-7357 1687-7365 Hindawi Limited Nuclear and High Energy Physics http://dx.doi.org/10.1155/2013/253985 <jats:p>The study of energy conditions has many significant applications in general relativistic and cosmological contexts. This paper explores the energy conditions in the framework of the most general scalar-tensor theory with field equations involving second-order derivatives. For this purpose, we use flat FRW universe model with perfect fluid matter contents. By taking power law ansatz for scalar field, we discuss the strong, weak, null, and dominant energy conditions in terms of deceleration, jerk, and snap parameters. Some particular cases of this theory like<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M1"><mml:mrow><mml:mi>k</mml:mi></mml:mrow></mml:math>-essence model, modified gravity theories and so forth. are analyzed with the help of the derived energy conditions, and the possible constraints on the free parameters of the presented models are determined.</jats:p> Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity Advances in High Energy Physics
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title Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_unstemmed Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_full Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_fullStr Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_full_unstemmed Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_short Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_sort energy conditions in a generalized second-order scalar-tensor gravity
topic Nuclear and High Energy Physics
url http://dx.doi.org/10.1155/2013/253985
publishDate 2013
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description <jats:p>The study of energy conditions has many significant applications in general relativistic and cosmological contexts. This paper explores the energy conditions in the framework of the most general scalar-tensor theory with field equations involving second-order derivatives. For this purpose, we use flat FRW universe model with perfect fluid matter contents. By taking power law ansatz for scalar field, we discuss the strong, weak, null, and dominant energy conditions in terms of deceleration, jerk, and snap parameters. Some particular cases of this theory like<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M1"><mml:mrow><mml:mi>k</mml:mi></mml:mrow></mml:math>-essence model, modified gravity theories and so forth. are analyzed with the help of the derived energy conditions, and the possible constraints on the free parameters of the presented models are determined.</jats:p>
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description <jats:p>The study of energy conditions has many significant applications in general relativistic and cosmological contexts. This paper explores the energy conditions in the framework of the most general scalar-tensor theory with field equations involving second-order derivatives. For this purpose, we use flat FRW universe model with perfect fluid matter contents. By taking power law ansatz for scalar field, we discuss the strong, weak, null, and dominant energy conditions in terms of deceleration, jerk, and snap parameters. Some particular cases of this theory like<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M1"><mml:mrow><mml:mi>k</mml:mi></mml:mrow></mml:math>-essence model, modified gravity theories and so forth. are analyzed with the help of the derived energy conditions, and the possible constraints on the free parameters of the presented models are determined.</jats:p>
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spelling Sharif, M. Waheed, Saira 1687-7357 1687-7365 Hindawi Limited Nuclear and High Energy Physics http://dx.doi.org/10.1155/2013/253985 <jats:p>The study of energy conditions has many significant applications in general relativistic and cosmological contexts. This paper explores the energy conditions in the framework of the most general scalar-tensor theory with field equations involving second-order derivatives. For this purpose, we use flat FRW universe model with perfect fluid matter contents. By taking power law ansatz for scalar field, we discuss the strong, weak, null, and dominant energy conditions in terms of deceleration, jerk, and snap parameters. Some particular cases of this theory like<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M1"><mml:mrow><mml:mi>k</mml:mi></mml:mrow></mml:math>-essence model, modified gravity theories and so forth. are analyzed with the help of the derived energy conditions, and the possible constraints on the free parameters of the presented models are determined.</jats:p> Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity Advances in High Energy Physics
spellingShingle Sharif, M., Waheed, Saira, Advances in High Energy Physics, Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity, Nuclear and High Energy Physics
title Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_full Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_fullStr Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_full_unstemmed Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_short Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
title_sort energy conditions in a generalized second-order scalar-tensor gravity
title_unstemmed Energy Conditions in a Generalized Second-Order Scalar-Tensor Gravity
topic Nuclear and High Energy Physics
url http://dx.doi.org/10.1155/2013/253985