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Analysing Hubble Tension and Gravitational Waves for $f(Q,T)$ Gravity Theories

General Relativity and Quantum Cosmology · Submitted 27 Aug 2024

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We show that these models have the capability to alleviate the Hubble tension, by predicting the present value of the Hubble parameter close to $74$km/s/Mpc.

how it is stated · asserted 0.92 read the record →

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arXiv ID2408.14878 (version 1)
Pith ID7BLAK35Q, Pith's permanent record of this paper and its review
CitationAritrya Paul, Shreya Banerjee. "Analysing Hubble Tension and Gravitational Waves for $f(Q,T)$ Gravity Theories." arXiv:2408.14878 (2024). https://pith.science/paper/7BLAK35Q
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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,341 input tokens.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.40 · randomized assignment 0.01 · states quantitative result 0.97 · compares with prior results 0.75 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

In this work, we examine viable models of $f(Q,T)$ gravity theories against observational data with the aim to constrain the parameter space of these models. We have analysed five different models of $f(Q,T)$ gravity and tested them against Type Ia supernovae, Cosmic Chronometer data, Baryon Acoustic Oscillations data and Pantheon data. We put stringent constraints on the $f(Q,T)$ gravity models, $f(Q,T) = Q^{n} +\beta T$ $(n=1,2,3)$, $f(Q,T)=-\alpha Q-\beta T^{2}$ and $f(Q,T)=Q^{-2}T^{2}$ along with other cosmological parameters such as deceleration parameter, equation of state parameter and demonstrate their alignment with the $\Lambda CDM$ model and the observational data. We show that these models have the capability to alleviate the Hubble tension, by predicting the present value of the Hubble parameter close to $74$km/s/Mpc. $f(Q,T)$ gravity theory introduces alterations in the background evolution and imposes a friction term in the propagation of gravitational waves, this phenomenon has also been examined. We have shown their agreement with the Gravitational Wave (GW) luminosity distance with the Electromagnetic (EM) counter part data from Advanced LIGO and Advanced VIRGO across different observing runs capturing coalescence of Binary Neutron Stars (BNS), mergers of Binary Black Holes (BBHs), and Neutron Star-Black Hole (NSBH) binaries with EM counterparts.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 In this work, we examine viable models of $f(Q,T)$ gravity theories against observational data with the aim to constrain the parameter space of these models. contribution 0.98 0.85 0.04 asserted 0.57
s1 We have analysed five different models of $f(Q,T)$ gravity and tested them against Type Ia supernovae, Cosmic Chronometer data, Baryon Acoustic Oscillations data and Pantheon data. method 0.84 0.96 0.04 asserted 1.00
s2 We put stringent constraints on the $f(Q,T)$ gravity models, $f(Q,T) = Q^{n} +\beta T$ $(n=1,2,3)$, $f(Q,T)=-\alpha Q-\beta T^{2}$ and $f(Q,T)=Q^{-2}T^{2}$ along with other cosmological parameters such as deceleration parameter, equation of state parameter and demonstrate their alignment with the $\Lambda CDM$ model and the observational data. result 0.75 0.94 0.24 asserted 1.00
s3 We show that these models have the capability to alleviate the Hubble tension, by predicting the present value of the Hubble parameter close to $74$km/s/Mpc. result 0.85 0.93 0.41 asserted 0.92
s4 $f(Q,T)$ gravity theory introduces alterations in the background evolution and imposes a friction term in the propagation of gravitational waves, this phenomenon has also been examined. contribution 0.60 0.61 0.05 asserted 1.00
s5 We have shown their agreement with the Gravitational Wave (GW) luminosity distance with the Electromagnetic (EM) counter part data from Advanced LIGO and Advanced VIRGO across different observing runs capturing coalescence of Binary Neutron Stars (BNS), mergers of Binary Black Holes (BBHs), and Neutron Star-Black Hole (NSBH) binaries with EM counterparts. result 0.89 0.90 0.11 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.53 · evidence from analysis of existing data 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

In this work, we examine viable models of $f(Q,T)$ gravity theories against observational data with the aim to constrain the parameter space of these models. We have analysed five different models of $f(Q,T)$ gravity and tested them against Type Ia supernovae, Cosmic Chronometer data, Baryon Acoustic Oscillations data and Pantheon data. We put stringent constraints on the $f(Q,T)$ gravity models, $f(Q,T) = Q^{n} +\beta T$ $(n=1,2,3)$, $f(Q,T)=-\alpha Q-\beta T^{2}$ and $f(Q,T)=Q^{-2}T^{2}$ along with other cosmological parameters such as deceleration parameter, equation of state parameter and demonstrate their alignment with the $\Lambda CDM$ model and the observational data. We show that these models have the capability to alleviate the Hubble tension, by predicting the present value of the Hubble parameter close to $74$km/s/Mpc. $f(Q,T)$ gravity theory introduces alterations in the background evolution and imposes a friction term in the propagation of gravitational waves, this phenomenon has also been examined. We have shown their agreement with the Gravitational Wave (GW) luminosity distance with the Electromagnetic (EM) counter part data from Advanced LIGO and Advanced VIRGO across different observing runs capturing coalescence of Binary Neutron Stars (BNS), mergers of Binary Black Holes (BBHs), and Neutron Star-Black Hole (NSBH) binaries with EM counterparts.

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1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

What it cites · 3 sentences without a confident label

Uses data or values from 1 paper
Compares with 1 paper
Cites as background 8 papers
  • To address these challenges, alternative modified gravity theories have been proposed, including the $f(R,T)$ [ref] theory, which incorporates a non-minimal interaction between matter and geometry, and the $f(R,G)$ [ref] theory, which involves modifications based on the Gauss-Bonnet invariant.

    Thermodynamic interpretation of the generalized gravity models with geometry - matter coupling · Introduction · 0.88

  • The first involves modifying the energy-momentum tensor in Einstein's field equations, which includes theories involving scalar fields (like quintessence and phantom models) [ref] , exotic equations of state (such as the Chaplygin gas) [ref] , and effects like bulk viscosity [ref] .

    Quintessence: A Review · Introduction · 0.97

  • The first involves modifying the energy-momentum tensor in Einstein's field equations, which includes theories involving scalar fields (like quintessence and phantom models) [ref] , exotic equations of state (such as the Chaplygin gas) [ref] , and effects like bulk viscosity [ref] .

    An alternative to quintessence · Introduction · 0.97

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