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相关论文: Updating constraints on phantom crossing $f(T)$ gr…

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In this paper, we propose two new models in $f(T)$ gravity to realize the crossing of the phantom divide line for the effective equation of state, and we then study the observational constraints on the model parameters. The best fit results…

广义相对论与量子宇宙学 · 物理学 2011-03-03 Puxun Wu , Hongwei Yu

$f(T)$ cosmology has shown promise in explaining aspects of cosmic evolution. In this work, we analyze constraints on leading models of $f(T)$ gravity in the context of the recently released Pantheon+ data set, together with comparisons…

广义相对论与量子宇宙学 · 物理学 2023-05-22 Rebecca Briffa , Celia Escamilla-Rivera , Jackson Levi Said , Jurgen Mifsud

In recent years, modifications to General Relativity (GR) have been explored to address cosmological observations, particularly in the context of late-time cosmic acceleration. Among these, modifications based on the Teleparallel Equivalent…

宇宙学与河外天体物理 · 物理学 2025-08-29 Saurabh Verma , Archana Dixit , Anirudh Pradhan , M. S. Barak

We study observational constraints on the modified symmetric teleparallel gravity, the non-metricity $f(Q)$ gravity, which reproduces background expansion of the universe. For this purpose, we use Hubble measurements, Baryonic Acoustic…

广义相对论与量子宇宙学 · 物理学 2021-11-25 Sanjay Mandal , P. K. Sahoo

In this paper, we propose two new models in $f(T)$ gravity to realize universe acceleration and phantom crossing due to dark torsion in the formalism. The model parameters are constrained and the observational test are discussed. The best…

综合物理 · 物理学 2015-06-03 H. Farajollahi , A. Ravanpak , P. Wu

We investigate two new observational perspectives in the context of torsional gravitational modification of general relativity, i.e., the $f(T)$ gravity: i) We use Pantheon data of type Ia supernovae motivated by a time variation of the…

宇宙学与河外天体物理 · 物理学 2023-03-21 Suresh Kumar , Rafael C. Nunes , Priya Yadav

We study the equation of state for dark energy and explicitly demonstrate that the future crossings of the phantom divide line $w_{\mathrm{DE}}=-1$ are the generic feature in the existing viable $f(R)$ gravity models. We also explore the…

宇宙学与河外天体物理 · 物理学 2015-05-19 Kazuharu Bamba , Chao-Qiang Geng , Chung-Chi Lee

We use the local value of the Hubble constant recently measured with 2.4% precision, as well as the latest compilation of cosmic chronometers data, together with standard probes such as Supernovae Type Ia and Baryon Acoustic Oscillation…

广义相对论与量子宇宙学 · 物理学 2016-08-10 Rafael C. Nunes , Supriya Pan , Emmanuel N. Saridakis

We extract observational constraints on $f(T)$ gravity, using the recently proposed statistical method which is not affected by the value of $H_0$ and thus it bypasses the problem of the disagreement in its exact numerical value between…

宇宙学与河外天体物理 · 物理学 2018-08-15 S. Basilakos , S. Nesseris , F. K. Anagnostopoulos , E. N. Saridakis

We identify the class of f(R) dark energy models which have a viable cosmology, i.e. a matter dominated epoch followed by a late-time acceleration. The deviation from a LambdaCDM model (f=R-Lambda) is quantified by the function…

天体物理学 · 物理学 2010-04-28 Luca Amendola , Shinji Tsujikawa

In the current era of precision cosmology, the persistence of cosmological tensions, most notably the Hubble tension and the $S_8$ tension, challenges the standard $\Lambda$CDM model. To reconcile these tensions via late-time modifications…

宇宙学与河外天体物理 · 物理学 2025-02-18 Yashi Tiwari , Ujjwal Upadhyay , Rajeev Kumar Jain

The late-time acceleration of the universe remains one of the most significant open problems in modern cosmology. Modified gravity frameworks such as $f(T)$ gravity provide a geometric alternative to dark energy by attributing cosmic…

广义相对论与量子宇宙学 · 物理学 2026-05-07 Anirudh Pradhan , S. A. Salve , V. B. Raut , S. H. Shekh

We explore the cosmological dynamics of a teleparallel Gauss-Bonnet gravity model defined by the torsion scalar $T$ and the torsion-based Gauss-Bonnet invariant $T_{\mathcal{G}}$, deriving modified Friedmann equations for a flat FLRW…

广义相对论与量子宇宙学 · 物理学 2026-01-16 Santosh V. Lohakare , S. K. Maurya , Aaisha Al Qassabi , B. Mishra

We establish new constraints on $f(T)$ gravity models by using cosmological data. In particular, we investigate the restrictions given by the gas mass fraction measurements of galaxy clusters and transversal BAO data. Both data sets are…

宇宙学与河外天体物理 · 物理学 2022-09-28 F. B. M. dos Santos , J. E. Gonzalez , R. Silva

The $f(T)$ theory, which is an extension of teleparallel, or torsion scalar $T$, gravity, is recently proposed to explain the present cosmic accelerating expansion with no need of dark energy. In this Letter, we first perform the…

广义相对论与量子宇宙学 · 物理学 2010-10-12 Puxun Wu , Hongwei Yu

In this paper we place observational constraints on the well-known $\gamma$-gravity $f(R)$ model using the latest cosmological data, namely we use the latest growth rate, Cosmic Microwave Background, Baryon Acoustic Oscillations, Supernovae…

宇宙学与河外天体物理 · 物理学 2018-07-17 Clara Álvarez Luna , Spyros Basilakos , Savvas Nesseris

In this work, we investigate new constraints on $f(T)$ gravity using the recent Baryon Acoustic Oscillation (BAO) data released by the Dark Energy Spectroscopic Instrument (DESI) and the Type Ia supernovae (SNIa) catalog from the full…

宇宙学与河外天体物理 · 物理学 2024-05-16 Celia Escamilla-Rivera , Rodrigo Sandoval-Orozco

Recent cosmological data, including DESI DR2, highlight significant tensions within the $\Lambda$CDM paradigm. When analyzed in the context of General Relativity (GR), the latest DESI data favor a dynamical dark energy (DDE) equation of…

宇宙学与河外天体物理 · 物理学 2025-11-19 Dimitrios Efstratiou , Evangelos Achilleas Paraskevas , Leandros Perivolaropoulos

We investigate the possibility of crossing a phantom divide line in the extension of symmetric teleparallel gravity or the $f(Q)$ gravity, where $Q$ is the non-metricity. We study the cosmic evolution of the effective equation of state…

广义相对论与量子宇宙学 · 物理学 2022-08-10 Simran Arora , P. K. Sahoo

In this paper, a cosmological model of the Universe is presented in $f(Q,T)$ gravity and the parameters are constrained by cosmological data sets. Initially, a generalised form of $f(Q,T)$ model is used as $f(Q,T)=-\lambda_{1}…

广义相对论与量子宇宙学 · 物理学 2024-03-21 A. S. Agrawal , B. Mishra , S. K. Tripathy
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