Arijit Panda , Debashis Gangopadhyay , Goutam Manna
{"title":"NEC violation in f(R̄,T̄) gravity in the context of a non-canonical theory via modified Raychaudhuri equation","authors":"Arijit Panda , Debashis Gangopadhyay , Goutam Manna","doi":"10.1016/j.astropartphys.2024.103059","DOIUrl":null,"url":null,"abstract":"<div><div>In this work, we develop the Raychaudhuri equation in <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>,</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span> gravity in the setting of a non-canonical theory, namely K-essence theory. We solve the modified Raychaudhuri equation for the additive form of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>,</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span>, which is <span><math><mrow><msub><mrow><mi>f</mi></mrow><mrow><mn>1</mn></mrow></msub><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow><mo>+</mo><msub><mrow><mi>f</mi></mrow><mrow><mn>2</mn></mrow></msub><mrow><mo>(</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span>. For this solution, we employ two different scale factors to give two types of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>,</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span> solutions. The ongoing debate between Fisher et al. and Harko et al. in 2020 regarding the additive form of <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>,</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span> may provide a resolution within the modified <span><math><mrow><mi>f</mi><mrow><mo>(</mo><mover><mrow><mi>R</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>,</mo><mover><mrow><mi>T</mi></mrow><mrow><mo>̄</mo></mrow></mover><mo>)</mo></mrow></mrow></math></span> gravity theory. By conducting a viability test and analyzing energy conditions, we have determined that in the first scenario, the null energy condition (NEC) is violated between two regions where the NEC is satisfied. Additionally, we have observed that this violation of the NEC exhibits a symmetric property during the phase transition. These observations indicate that bouncing events may occur as a result of the symmetrical violation of the NEC during the expansion of the universe. Moreover, this model indicates that resonant-type quantum tunneling may take place during the period when the NEC is violated. The findings of NEC violation through the power law of scale factor may have empirical relevance in contemporary observations. In the second scenario, our model indicates that the strong energy condition is violated, but the NEC and weak energy conditions are satisfied. The effective energy density decreases and is positive, while the effective pressure and equation of state parameters are negative. This suggests that the universe is expanding with acceleration and is dominated by dark energy.</div></div>","PeriodicalId":55439,"journal":{"name":"Astroparticle Physics","volume":"165 ","pages":"Article 103059"},"PeriodicalIF":4.2000,"publicationDate":"2024-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astroparticle Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0927650524001361","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
In this work, we develop the Raychaudhuri equation in gravity in the setting of a non-canonical theory, namely K-essence theory. We solve the modified Raychaudhuri equation for the additive form of , which is . For this solution, we employ two different scale factors to give two types of solutions. The ongoing debate between Fisher et al. and Harko et al. in 2020 regarding the additive form of may provide a resolution within the modified gravity theory. By conducting a viability test and analyzing energy conditions, we have determined that in the first scenario, the null energy condition (NEC) is violated between two regions where the NEC is satisfied. Additionally, we have observed that this violation of the NEC exhibits a symmetric property during the phase transition. These observations indicate that bouncing events may occur as a result of the symmetrical violation of the NEC during the expansion of the universe. Moreover, this model indicates that resonant-type quantum tunneling may take place during the period when the NEC is violated. The findings of NEC violation through the power law of scale factor may have empirical relevance in contemporary observations. In the second scenario, our model indicates that the strong energy condition is violated, but the NEC and weak energy conditions are satisfied. The effective energy density decreases and is positive, while the effective pressure and equation of state parameters are negative. This suggests that the universe is expanding with acceleration and is dominated by dark energy.
在这项研究中,我们在非经典理论(即 K-essence 理论)的背景下发展了 f(R̄,T̄) 引力中的雷乔杜里方程。我们求解了 f(R̄,T̄)的加法形式的修正雷乔杜里方程,即 f1(R̄)+f2(T̄) 。对于这种解法,我们采用了两种不同的比例因子,给出了两种类型的 f(R̄,T̄) 解法。费舍尔等人和哈科等人在 2020 年就 f(R̄,T̄)的加法形式正在进行的争论,可能会为修正的 f(R̄,T̄) 引力理论提供一个解决方案。通过进行可行性测试和分析能量条件,我们确定在第一种情况下,在满足空能量条件(NEC)的两个区域之间违反了空能量条件。此外,我们还观察到,这种对 NEC 的违反在相变过程中表现出对称性。这些观测结果表明,在宇宙膨胀过程中,反弹事件可能是对称违反 NEC 的结果。此外,该模型还表明,共振型量子隧穿可能会在违反 NEC 期间发生。通过尺度因子幂律违反 NEC 的发现在当代观测中可能具有经验意义。在第二种情况下,我们的模型表明强能量条件被违反,但 NEC 和弱能量条件得到满足。有效能量密度减小并呈正值,而有效压力和状态方程参数呈负值。这表明宇宙正在加速膨胀,并由暗能量主导。
期刊介绍:
Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.