{"title":"Cosmological implications and stability of f(Q,T) gravity with pilgrim dark energy model","authors":"M. Sharif , Iqra Ibrar","doi":"10.1016/j.ascom.2025.100967","DOIUrl":null,"url":null,"abstract":"<div><div>This manuscript endeavors to construct a pilgrim dark energy framework within the <span><math><mrow><mi>f</mi><mi>(Q,T)</mi></mrow></math></span> gravity theory, employing a correspondence approach aligned with a non-interacting model that incorporates pressureless matter alongside a power-law scale factor. Here <span><math><mi>Q</mi></math></span> and <span><math><mi>T</mi></math></span> represent the non-metricity and trace of the energy–momentum tensor, respectively. This extended modified gravity framework accurately replicates various epochs in the cosmological history. The <span><math><mrow><mi>f</mi><mi>(Q,T)</mi></mrow></math></span> gravity models are utilized to derive the equation of state parameter, phase planes and squared speed of sound. The analysis reveals that the reconstructed model exhibits an increasing or decreasing trend with the pilgrim dark energy parameter. The equation of state parameter characterizes the phantom regime, while the squared speed of sound parameter provides a stable framework for examining the ongoing cosmic evolution. The <span><math><mrow><msub><mrow><mi>ω</mi></mrow><mrow><mi>D</mi><mi>E</mi></mrow></msub><mo>−</mo><msubsup><mrow><mi>ω</mi></mrow><mrow><mi>D</mi><mi>E</mi></mrow><mrow><mo>′</mo></mrow></msubsup></mrow></math></span> plane trajectories reveal the freezing region, while the <span><math><mrow><mi>r</mi><mo>−</mo><mi>s</mi></mrow></math></span> phase plane shows the Chaplygin gas model. It is important to highlight that our findings align with the most recent observational data.</div></div>","PeriodicalId":48757,"journal":{"name":"Astronomy and Computing","volume":"53 ","pages":"Article 100967"},"PeriodicalIF":1.9000,"publicationDate":"2025-05-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy and Computing","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S221313372500040X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This manuscript endeavors to construct a pilgrim dark energy framework within the gravity theory, employing a correspondence approach aligned with a non-interacting model that incorporates pressureless matter alongside a power-law scale factor. Here and represent the non-metricity and trace of the energy–momentum tensor, respectively. This extended modified gravity framework accurately replicates various epochs in the cosmological history. The gravity models are utilized to derive the equation of state parameter, phase planes and squared speed of sound. The analysis reveals that the reconstructed model exhibits an increasing or decreasing trend with the pilgrim dark energy parameter. The equation of state parameter characterizes the phantom regime, while the squared speed of sound parameter provides a stable framework for examining the ongoing cosmic evolution. The plane trajectories reveal the freezing region, while the phase plane shows the Chaplygin gas model. It is important to highlight that our findings align with the most recent observational data.
Astronomy and ComputingASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍:
Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.