We proposed five $f(Q,T)$ models, which are an extension of symmetric teleparallel gravity, where $Q$ is the non-metricity and $T$ is the trace of the stress-energy tensor. By taking specific values of their parameters, these models have a $Λ$CDM limit.
Using cosmic chronometers and supernovae Ia data, we found that our models are consistent with $Λ$CDM at a 95\% confidence level. To see whether one of these models can challenge $Λ$CDM at a background perspective, we computed the Bayesian evidence for them and $Λ$CDM. According to it, the concordance model is preferred over four of them, showing a weak preference against $f(Q,T) = -Q/G_N + bT$ and $f(Q,T) = -(Q+2Λ)/G_N +bT$, a substantial preference against $f(Q,T) = -(Q+2 H_0^2 c (Q/(6H_0^2))^{n+1})/G_N + bT $, and a strong preference against $f(Q,T) = -(Q+2H_0^2c(Q/(6H_0^2))^{n+1} + 2Λ)/G_N + bT$. Interestingly, a model includying a $T^2$ dependence ($f(Q,T) = -(Q+2Λ)/G_N - ((16π)^2 G_N b)/(120 H_0^2) T^2$) showed a {substantial} preference against $Λ$CDM. {Therefore, we encourage further analyses of this model to test its viability outside the background perspective.}
Falsifying $Λ$CDM: Model-independent tests of the concordance model with eBOSS DR14Q and Pantheon
我们结合模型独立重建的膨胀历史,从最新的万神殿超新星距离模量汇编和测量重子声学振荡,以测试宇宙学的和谐模型,即FLRW度量和平坦度的空间曲率的一些重要方面。然后,我们使用重建的扩展历史,以适应红移空间失真的增长测量,并获得强约束$(Ω_\mathrm{m},γ,σ_8)$在一个模型无关的方式。我们的结果表明,与一个空间平坦的FLRW宇宙与广义相对论支配的扰动的结构形成和宇宙学常数作为暗能量的一致性。然而,我们也可以看到一些紧张的暗示,在不同的观测范围内的和谐模型相关的高红移观测($z > 1$)的膨胀历史。这支持了Sahni et al.(2014)和Zhao et al.(2017)的早期发现,并强调了精确测量膨胀历史和高红移结构增长的重要性。
Tightening Cosmological Constraints Within and Beyond $Λ$CDM Using Gamma-Ray Bursts Calibrated with Type Ia Supernovae
INAF - Osservatorio Astronomico di Capodimonte(意大利国家天体物理研究所卡波迪蒙特天文台);Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University(北京师范大学前沿天文与天体物理研究院);Department of Astronomy, Beijing Normal University(北京师范大学天文系);INAF - Osservatorio Astronomico di Padova(意大利国家天体物理研究所帕多瓦天文台);Università di Camerino(卡梅里诺大学);INAF - Osservatorio Astronomico di Brera(意大利国家天体物理研究所布雷拉天文台);Istituto Nazionale di Fisica Nucleare, Sezione di Perugia(意大利国家核物理研究所佩鲁贾分部);SUNY Polytechnic(纽约州立理工大学);Al-Farabi Kazakh National University(阿里-法拉比哈萨克国立大学);ICRANet(国际相对论天体物理中心网络)
Joint constraints on $R_h=ct$ cosmology from DESI DR2 BAO, CC, and SN\textit{Ia} Pantheon$^+$ sample
University Institute of Sciences, Chandigarh University(昌迪加尔大学科学研究所);Pacif Institute of Cosmology and Selfology (PICS)(Pacif宇宙学与自我学研究所);Research Center of Astrophysics and Cosmology, Khazar University(哈扎尔大学天体物理学与宇宙学研究中心);Programa de Pós-Graduação em Física, Instituto de Física, Universidade Federal de Mato Grosso(马托格罗索联邦大学物理学院物理研究生项目)
Probing departures from $Λ$CDM by late-time datasets
Babeș-Bolyai University(博巴伊-波约大学);Khazar University(哈萨尔大学);Indian Institute of Astrophysics(印度天体物理研究所);Università di Napoli “Federico II”(那不勒斯费德里科二世大学);Istituto Nazionale di Fisica Nucleare (INFN), sez. di Napoli(意大利国家核物理研究所那不勒斯分部);Scuola Superiore Meridionale(南方高等学院);Zhejiang Normal University(浙江师范大学)
Observational constraints on a modified-gravity model with an exponential function of the curvature using the expansion history, the RSD, and the Pantheon+SH0ES data
Probing late-time deviations from $Λ$CDM with a quadratic dark energy expansion
Plaksha University(普拉克斯哈大学);Universidade Federal do Paraná(巴拉那联邦大学);Federal University of Latin American Integration (UNILA)(拉丁美洲联邦大学);Universidade Federal do Rio Grande do Sul(南里奥格兰德联邦大学);Instituto Nacional de Pesquisas Espaciais(国家空间研究所)
Interacting dark energy after DESI DR2: a challenge for $Λ$CDM paradigm?
Presidency University(总统大学);Durban University of Technology(德班理工大学);National Observatory of Athens(雅典国家天文台);Universidad Católica del Norte(北天主教大学);University of Science and Technology of China(中国科学技术大学);Liaoning Normal University(辽宁师范大学)
Evidence of dynamical dark energy found via the DESI DR2 Lyman$α$ forest
Dipartimento di Fisica “E. Pancini”, Università degli Studi di Napoli “Federico II”(那不勒斯费德里科二世大学物理系);Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Napoli(意大利国家核物理研究所那不勒斯分部);Scuola Superiore Meridionale(南方高等学院);Research Center of Astrophysics and Cosmology, Khazar University(哈扎尔大学天体物理学与宇宙学研究中心);Department of Physics, Zhejiang Normal University(浙江师范大学物理系);Pacif Institute of Cosmology and Selfology (PICS)(帕西夫宇宙学与自我学研究所)
Testing $f(Q)$ Gravity with DESI DR2 and Strong-Lensing Time Delays
Henan Academy of Sciences(河南省科学院);GLA University(GLA大学);University of Delhi(德里大学);Symbiosis International (Deemed University)(西姆比奥西斯国际(认定)大学);Qingdao University of Science and Technology(青岛科技大学)
Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $Λ$CDM, XCDM, and $ϕ$CDM dark energy inflation cosmologies
Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB
Universidade Federal do Espírito Santo(埃斯皮里托圣托联邦大学);Aix Marseille Université, CNRS/IN2P3, CPPM(艾克斯-马赛大学);Centro Brasileiro de Pesquisas Físicas(巴西物理研究中心);Observatório do Valongo, Universidade Federal do Rio de Janeiro(瓦隆戈天文台,里约热内卢联邦大学);University of Arizona(亚利桑那大学)
No preference for generalized emergent dark energy from current cosmological data
Lovely Professional University(洛维专业大学);Babeș-Bolyai University(巴贝什-波约依大学);Khazar University(阿塞拜疆卡扎尔大学);Università di Napoli “Federico II”(那不勒斯费德里科二世大学);Istituto Nazionale di Fisica Nucleare (INFN)(意大利国家核物理研究所);Scuola Superiore Meridionale(南方高等学院);Madhabdev University(马德哈伯德夫大学);Zhejiang Normal University(浙江师范大学);Walailak University(瓦拉莱克大学)
Dark Energy within the Generalized Uncertainty Principle in Light of DESI DR2
Durban University of Technology(德班理工大学);North-West University(西北大学);National Institute for Theoretical and Computational Sciences (NITheCS)(南非理论与计算科学国家研究所)
Wilczek Quantum Center, Shanghai Institute for Advanced Studies(吴文俊量子中心,上海高等研究院);University of Science and Technology of China(中国科学技术大学);Institute of Space Sciences and Astronomy, University of Malta(马耳他大学空间科学与天文研究所);Department of Physics, University of Malta(马耳他大学物理系);Department of Mathematics, Birla Institute of Technology and Science, Pilani, Hyderabad Campus(比拉理工学院皮拉尼校区海得拉巴分校数学系)