{"title":"Dynamics of some cosmological solutions in modified f(T, B) theory of gravity","authors":"Adnan Malik, Aimen Rauf, V. Venkatesha, Chaitra Chooda Chalavadi, Shahid Chaudhary","doi":"10.1140/epjp/s13360-024-05807-7","DOIUrl":null,"url":null,"abstract":"<div><p>The aim of this manuscript is to explore cosmological solutions using the modified <i>f</i>(<i>T</i>, <i>B</i>) theory of gravity, where <i>B</i> represents the boundary scalar term and <i>T</i> represents the torsion scalar. For our current work, we consider the Friedmann–Robertson–Walker spacetime to obtain solutions. We investigate the nature of the universe under various scenarios, including acceleration expansion of universe, ultra-relativistic universe, sub-relativistic universe, dust universe, radiation universe and stiff universes. Moreover, we choose power-law technique to study the expanding nature of the universe by taking two different <i>f</i>(<i>T</i>, <i>B</i>) gravity models. Additionally, we discuss the bouncing scenario of universe and observe the energy conditions, which must be satisfied for a successful bouncing model by selecting particular values for the model parameters. It can be concluded that some solutions in <i>f</i>(<i>T</i>, <i>B</i>) gravity models support the concept of exotic matter and accelerated expansion of the universe due to a large amount of negative pressure.</p></div>","PeriodicalId":792,"journal":{"name":"The European Physical Journal Plus","volume":"139 11","pages":""},"PeriodicalIF":2.8000,"publicationDate":"2024-11-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The European Physical Journal Plus","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1140/epjp/s13360-024-05807-7","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
Abstract
The aim of this manuscript is to explore cosmological solutions using the modified f(T, B) theory of gravity, where B represents the boundary scalar term and T represents the torsion scalar. For our current work, we consider the Friedmann–Robertson–Walker spacetime to obtain solutions. We investigate the nature of the universe under various scenarios, including acceleration expansion of universe, ultra-relativistic universe, sub-relativistic universe, dust universe, radiation universe and stiff universes. Moreover, we choose power-law technique to study the expanding nature of the universe by taking two different f(T, B) gravity models. Additionally, we discuss the bouncing scenario of universe and observe the energy conditions, which must be satisfied for a successful bouncing model by selecting particular values for the model parameters. It can be concluded that some solutions in f(T, B) gravity models support the concept of exotic matter and accelerated expansion of the universe due to a large amount of negative pressure.
本手稿的目的是利用修正的 f(T,B)引力理论探索宇宙学解法,其中 B 代表边界标量项,T 代表扭转标量。在我们目前的工作中,我们考虑在弗里德曼-罗伯逊-沃克时空(Friedmann-Robertson-Walker spacetime)中求解。我们研究了宇宙加速膨胀、超相对论宇宙、亚相对论宇宙、尘埃宇宙、辐射宇宙和僵化宇宙等各种情况下的宇宙性质。此外,我们选择了幂律技术,通过两种不同的 f(T, B) 引力模型来研究宇宙的膨胀性质。此外,我们还讨论了宇宙的反弹情况,并通过选择模型参数的特定值观察了成功的反弹模型必须满足的能量条件。可以得出的结论是,f(T,B)引力模型中的一些解支持奇异物质的概念,以及由于大量负压导致的宇宙加速膨胀。
期刊介绍:
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