Journal of High Energy Astrophysics最新文献

{"title":"Cosmology in R2-gravity: Effects of a higher derivative scalar condensate background","authors":"","doi":"10.1016/j.jheap.2024.07.011","DOIUrl":"10.1016/j.jheap.2024.07.011","url":null,"abstract":"<div><p>A well known extension of Einstein's General Relativity is the addition of an <span><math><msup><mrow><mi>R</mi></mrow><mrow><mn>2</mn></mrow></msup></math></span>-term, which is free of ghost excitations and in the linearized framework, reduces to the conventional spin-2 graviton and an additional higher derivative scalar. According to <span><span>Chakraborty and Ghosh (2022)</span></span>, the above scalar sector can sustain a Time Crystal-like minimum energy state, with non-trivial time dependence. Exploiting previous result that the scalar can sustain modes with periodic time dependence in its lowest energy, we consider this condensate as a source and study the Friedmann-Lemaître-Robertson-Walker (FLRW) cosmology in this background. The effect of the <span><math><msup><mrow><mi>R</mi></mrow><mrow><mn>2</mn></mrow></msup></math></span>-term is interpreted as a back reaction. A remarkable consequence of the condensate is that, irrespective of open or close geometry of the Universe, for an appropriate choice of parameter window, the condensate can induce a decelerating phase before the accelerated expansion starts and again, in some cases, it can help to avoid the singularity in the deceleration parameter (that is present in conventional FLRW Cosmology).</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141853927","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Model-independent parameterization of H(z) and its implications for cosmic evolution","authors":"","doi":"10.1016/j.jheap.2024.07.010","DOIUrl":"10.1016/j.jheap.2024.07.010","url":null,"abstract":"<div><p>We investigate the model-independent parameterization of <span><math><mi>H</mi><mo>(</mo><mi>z</mi><mo>)</mo></math></span> in spatially homogeneous and isotropic FLRW space-time using Cosmic Chronometers (31 data points) and Pantheon+SH0ES (1701 points) datasets. The best-fit values for the model parameters <span><math><mo>(</mo><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub><mo>,</mo><msub><mrow><mi>A</mi></mrow><mrow><mn>1</mn></mrow></msub><mo>,</mo><msub><mrow><mi>A</mi></mrow><mrow><mn>2</mn></mrow></msub><mo>,</mo><msub><mrow><mi>A</mi></mrow><mrow><mn>3</mn></mrow></msub><mo>)</mo></math></span> are obtained through MCMC analysis. Our results show that the EoS parameter <em>ω</em> transitions from a matter-dominated era through quintessence to <span><math><mi>ω</mi><mo>=</mo><mo>−</mo><mn>1</mn></math></span>, indicating convergence to ΛCDM at late times. The current <em>ω</em> values suggest an accelerating universe. Moreover, the model's squared sound speed <span><math><msubsup><mrow><mi>v</mi></mrow><mrow><mi>s</mi></mrow><mrow><mn>2</mn></mrow></msubsup></math></span> evolves from negative to positive, indicating increasing stability. The deceleration parameter <em>q</em> shows a smooth transition from deceleration to acceleration, with transition redshift <span><math><msub><mrow><mi>z</mi></mrow><mrow><mi>t</mi></mrow></msub></math></span> between 0.5 and 0.8. Further, the energy conditions are satisfied, and SEC violation at <span><math><mi>z</mi><mo>=</mo><mn>0</mn></math></span> supports current acceleration. The <span><math><mi>ω</mi><mo>−</mo><msup><mrow><mi>ω</mi></mrow><mrow><mo>′</mo></mrow></msup></math></span> plane lies in the freezing region, and the <span><math><mi>r</mi><mo>−</mo><mi>s</mi></math></span> plane approaches the ΛCDM limit at late times.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141850006","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Gravitational lensing of dark energy models and ΛCDM using observational data in loop quantum cosmology","authors":"","doi":"10.1016/j.jheap.2024.07.013","DOIUrl":"10.1016/j.jheap.2024.07.013","url":null,"abstract":"<div><p>This paper investigates the accelerated cosmic expansion in the late Universe by examining two dark energy models, viscous modified Chaplygin gas (VsMCG) and variable modified Chaplygin gas (VMCG), within loop quantum cosmology alongside the ΛCDM model. The objective is to constrain cosmic parameters using the ΛCDM model and 30 of the latest <span><math><mi>H</mi><mo>(</mo><mi>z</mi><mo>)</mo></math></span> measurements from cosmic chronometers (CC), including Type Ia Supernovae, Gamma-Ray Bursts (GRB), Quasars, and 24 uncorrelated baryon acoustic oscillations (BAO) measurements across a redshift range from 0.106 to 2.33. The latest Hubble constant measurement from Riess in 2022 is included to enhance constraints. In the ΛCDM, VsMCG, and VMCG frameworks, best-fit parameters for the Hubble parameter (<span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span>) and sound horizon (<span><math><msub><mrow><mi>r</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span>) are obtained. The results highlight significant disparities between <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> and <span><math><msub><mrow><mi>r</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span> values from late-time observational measurements, reflecting the known <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> and <span><math><msub><mrow><mi>r</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span> tensions. The gravitational lensing optical depth of the two dark energy models is studied by plotting <span><math><mi>log</mi><mo>⁡</mo><mo>(</mo><mi>τ</mi><mo>(</mo><msub><mrow><mi>z</mi></mrow><mrow><mi>l</mi></mrow></msub><mo>)</mo><mo>/</mo><msubsup><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow><mrow><mo>−</mo><mn>3</mn></mrow></msubsup><msub><mrow><mi>τ</mi></mrow><mrow><mi>N</mi></mrow></msub><mo>)</mo></math></span> vs <span><math><msub><mrow><mi>z</mi></mrow><mrow><mi>l</mi></mrow></msub></math></span>. The probability of finding gravitational lenses (optical depth) in both models increases with lens redshift <span><math><msub><mrow><mi>z</mi></mrow><mrow><mi>l</mi></mrow></msub></math></span>. The change in optical depth behavior for different parameter constraints is graphically analyzed. A joint analysis of VsMCG and VMCG with ΛCDM is conducted. While the models diverge in the early Universe, they are indistinguishable at low redshift. Using the Akaike information criteria, the analysis indicates that neither dark energy model can be dismissed based on the latest observations.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141948333","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Massive Dirac equation in static Bumblebee black hole space-times, detailed derivations and novel exact solutions","authors":"","doi":"10.1016/j.jheap.2024.08.004","DOIUrl":"10.1016/j.jheap.2024.08.004","url":null,"abstract":"<div><p>In this work, we construct and investigate the relativistic spin-<span><math><mfrac><mrow><mn>1</mn></mrow><mrow><mn>2</mn></mrow></mfrac></math></span> fermionic fields quantum dynamics in static spherically symmetric Bumblebee black hole background. The derivation of the Dirac equation in a general static spherically symmetric black hole space-time is carried out in detail via tetrad formalism. With the help of total angular momentum operator, the angular equation can be separated from the radial part where the solution is given in terms of the spinor harmonics. The radial Dirac equation has a well-known problem due to the presence of the square root terms appearing simultaneously with the rest mass that prevents us to find exact solutions. In this work, we present exact solutions of light mass fermion's wave function and energy levels bound in the static Bumblebee black hole. We discover the exact solutions of the massive Dirac's radial equation in terms of the Confluent Heun functions. Moreover, thanks to the well-known polynomial condition of the Confluent Heun functions, we also derive the energy quantization.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142084263","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Impact of electron spectra on morphology of pulsar halos at ultra-high energies","authors":"","doi":"10.1016/j.jheap.2024.07.006","DOIUrl":"10.1016/j.jheap.2024.07.006","url":null,"abstract":"<div><p>The extended <em>γ</em>-ray halos around pulsars are unique probe of transportation of high-energy electrons (and positrons) in vicinities of such pulsars. Observations of morphologies of several such halos indicate that particles diffuse very slowly around pulsars, compared with that in the Milky Way halo. The energy-dependent morphologies are expected to be very important in studying the energy-dependence of the diffusion coefficient. In this work we point out that the spectrum of high-energy electrons takes effect in shaping the <em>γ</em>-ray morphologies at the ultra-high-energy bands, and thus results in a degeneracy between the electron spectrum and the energy-dependence of the diffusion coefficient. The reasons for such a degeneracy include both the Klein-Nishina effect of the inverse Compton scattering and the curvature (if any) of the electron spectrum. It thus necessary to take into account the spectral shape of electrons when deriving the energy-dependence of diffusion coefficient using ultra-high-energy <em>γ</em>-ray measurements of extended pulsar halos.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141838519","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Probing the nova shock physics with future gamma-ray observations of the upcoming outburst from T Coronae Borealis","authors":"","doi":"10.1016/j.jheap.2024.07.007","DOIUrl":"10.1016/j.jheap.2024.07.007","url":null,"abstract":"<div><p>Nova shocks behave like scaled-down supernova remnant shocks with a lifetime of only a few weeks or months, thereby providing a unique opportunity to study the dynamics of non-relativistic shocks as well as the shock acceleration physics. Recently, GeV and TeV gamma-ray emissions from an outburst of the recurrent nova RS Ophiuchi have been observed. The light curves of the gamma-ray emissions suggest that they arise from an external shock, which is formed as the nova ejecta interacts with the ambient medium. The shock is thought to transition from an adiabatic shock to a radiative one at later times, but no such later observations are available for RS Ophiuchi. In addition, the spectral evolution of the gamma-ray outburst of RS Ophiuchi was not well measured, and hence the related particle acceleration mechanisms are not well understood. T Coronae Borealis (T CrB) is another recurrent nova in Milky Way and its last outburst was nearly ten times optically brighter than RS Ophiuchi. Recently the optical light curve of T CrB displayed a state transition behavior before the eruption, and it has been predicted that T CrB will undergo an outburst in the near future. By performing a theoretical investigation, we find that Fermi-LAT could probably capture the transition of the shock from the adiabatic phase to the radiative phase at the GeV band if the ambient wind medium is dense with <span><math><msub><mrow><mi>A</mi></mrow><mrow><mo>⋆</mo></mrow></msub><mo>≥</mo><mn>1</mn></math></span>, thanks to a longer detectable time than that of RS Ophiuchi. Due to its higher brightness, we also find that imaging atmospheric Cherenkov telescopes (IACTs) such as MAGIC and VERITAS, and extensive air shower experiments such as LHAASO could detect the nova outburst and measure the gamma-ray spectrum in the very-high-energy (VHE, <span><math><mo>&gt;</mo><mn>0.1</mn><mspace></mspace><mrow><mi>TeV</mi></mrow></math></span>) band more precisely. This can be used to constrain the high-energy cutoff index in the accelerated proton spectrum and the acceleration efficiency, which will shed light on the particle acceleration physics in nova shocks.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141950095","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Addressing the rd tension using late-time observational measurements in a novel deceleration parametrization","authors":"","doi":"10.1016/j.jheap.2024.08.003","DOIUrl":"10.1016/j.jheap.2024.08.003","url":null,"abstract":"<div><p>This paper introduces a novel cosmological model aimed at probing the accelerated expansion of the late Universe through a unique parametrization of the deceleration parameter. We aim to constrain key cosmic parameters by integrating recent measurements of the Hubble parameter obtained from various observational methods, including cosmic chronometers, Type Ia Supernovae, Gamma-Ray Bursts (GRB), Quasars, and Baryon Acoustic Oscillations (BAO) from recent galaxy surveys. With a redshift range spanning <span><math><mn>0.106</mn><mo>&lt;</mo><mi>z</mi><mo>&lt;</mo><mn>2.33</mn></math></span> and incorporating the latest Hubble constant measurement from Riess in 2022, our analysis yields optimal fit values for the Hubble parameter (<span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span>) and sound horizon (<span><math><msub><mrow><mi>r</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span>). Notably, we uncover an inconsistency in <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> values derived from late-time observational measurements, reflecting the well-known <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> tension. In terms of <span><math><msub><mrow><mi>r</mi></mrow><mrow><mi>d</mi></mrow></msub></math></span>, while there is close agreement between Joint analysis and Joint analysis with R22, discrepancies arise upon gradual inclusion of BAO and BAO with R22 datasets. Our model demonstrates excellent fit to observed data and aligns well with the standard ΛCDM paradigm at higher redshifts. However, its most intriguing aspect lies in predicting a super-accelerated expansion in the distant future, in contrast to the de Sitter phase predicted by ΛCDM. Additionally, unique behaviors in the jerk parameter hint at novel dynamics beyond traditional cosmological models. Statefinder and <span><math><msub><mrow><mi>O</mi></mrow><mrow><mi>m</mi></mrow></msub></math></span> Diagnostics tests were conducted, and comparison using the Akaike information criterion indicates neither model can be ruled out based on the latest observational measurements. These findings propose our cosmological model as a compelling alternative to ΛCDM, offering fresh insights into dark energy's nature and the cosmos' future.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141985695","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Observational constraints on extended Starobinsky and Weyl gravity model of inflation","authors":"","doi":"10.1016/j.jheap.2024.07.005","DOIUrl":"10.1016/j.jheap.2024.07.005","url":null,"abstract":"<div><p>We present constraints on the extended Starobinsky and Weyl gravity model of inflation using updated available observational data. The data includes cosmic microwave background (CMB) anisotropy measurements from <em>Planck</em> and BICEP/<em>Keck</em> 2018 (BK18), as well as large-scale structure data encompassing cosmic shear and galaxy autocorrelation and cross-correlation functions measurements from Dark Energy Survey (DES), baryonic acoustic oscillation (BAO) measurements from 6dF, MGS and BOSS, and distance measurements from supernovae type Ia from Pantheon+ samples. By introducing a single additional parameter, each model extends the Starobinsky model to encompass larger region of parameter space while remaining consistent with all observational data. Our findings demonstrate that the inclusion of higher-order terms loosen the constraint on the upper bound of <em>e</em>-folding number <span><math><msub><mrow><mi>N</mi></mrow><mrow><mtext>e</mtext></mrow></msub></math></span> due to the presence of small additional parameter. The maximum limit on <span><math><msub><mrow><mi>N</mi></mrow><mrow><mtext>e</mtext></mrow></msub></math></span> could be refined by considering the reheating process to <span><math><msub><mrow><mi>N</mi></mrow><mrow><mtext>e</mtext></mrow></msub><mo>&lt;</mo><mn>55</mn><mo>−</mo><mn>59</mn></math></span> for <span><math><msub><mrow><mi>k</mi></mrow><mrow><mo>⁎</mo></mrow></msub><mo>=</mo><mn>0.002</mn><mo>,</mo><mn>0.05</mn></math></span> Mpc⁻¹. These models extend viable range of tensor-to-scalar ratio (<em>r</em>) to very small value <span><math><mi>r</mi><mo>&lt;</mo><mn>0.002</mn></math></span> in contrast to the original <span><math><msup><mrow><mi>R</mi></mrow><mrow><mn>2</mn></mrow></msup></math></span> Starobinsky model. In addition, our results continue to emphasize the tension in <span><math><msub><mrow><mi>H</mi></mrow><mrow><mn>0</mn></mrow></msub></math></span> and <span><math><msub><mrow><mi>S</mi></mrow><mrow><mn>8</mn></mrow></msub></math></span> between early-time CMB measurements and late-time large-scale structure observations.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141950094","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Prospects for joint reconstruction of imaging air Cherenkov telescope array and extensive air shower array","authors":"","doi":"10.1016/j.jheap.2024.07.012","DOIUrl":"10.1016/j.jheap.2024.07.012","url":null,"abstract":"<div><p>In this paper, we proposed a joint reconstruction of <em>γ</em>-ray events using both extensive air array (EAS) and Imaging air Cherenkov Telescope array (IACT). We considered eight Cherenkov telescopes to be built on the LHAASO (Large High Altitude Air Shower Observatory) site and investigate the improvement in differential sensitivity when combining the information from both IACT and Moun detectors of LHAASO-KM2A. We found that due to the higher cosmic ray background rejection power and higher gamma ray retention ratio provided by muon detectors of LHAASO, such a joint reconstruction can significantly improve the sensitivity of IACTs, especially for extended sources and long exposure time. The sensitivity of the eight-telescopes array can be improved by <span><math><mn>25</mn><mtext>%</mtext><mo>−</mo><mn>60</mn><mtext>%</mtext></math></span> in different energy ranges using joint reconstructions with muon detectors.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142012009","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Cosmological constraints on f(Q) gravity models in the non-coincident formalism","authors":"","doi":"10.1016/j.jheap.2024.08.002","DOIUrl":"10.1016/j.jheap.2024.08.002","url":null,"abstract":"<div><p>The article investigates cosmological applications of <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> theories in a non-coincident formalism. We explore a new <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> theory dynamics utilizing a non-vanishing affine connection involving a non-constant function <span><math><mi>γ</mi><mo>(</mo><mi>t</mi><mo>)</mo><mo>=</mo><mo>−</mo><msup><mrow><mi>a</mi></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup><mover><mrow><mi>H</mi></mrow><mrow><mo>˙</mo></mrow></mover></math></span>, resulting in Friedmann equations that are entirely distinct from those of <span><math><mi>f</mi><mo>(</mo><mi>T</mi><mo>)</mo></math></span> theory. In addition, we propose a new parameterization of the Hubble function that can consistently depicts the present deceleration parameter value, transition redshift, and the late time de-Sitter limit. We evaluate the predictions of the assumed Hubble function by imposing constraints on the free parameters utilizing Bayesian statistical analysis to estimate the posterior probability by employing the CC, Pantheon+SH0ES, and the BAO samples. Moreover, we conduct the AIC and BIC statistical evaluations to determine the reliability of MCMC analysis. Further, we consider some well-known corrections to the STEGR case such as an exponentital <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> correction, logarithmic <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> correction, and a power-law <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> correction and then we find the constraints on the parameters of these models via energy conditions. Finally, to test the physical plausibility of the assumed <span><math><mi>f</mi><mo>(</mo><mi>Q</mi><mo>)</mo></math></span> models we conduct the thermodynamical stability analysis via the sound speed parameter.</p></div>","PeriodicalId":54265,"journal":{"name":"Journal of High Energy Astrophysics","volume":null,"pages":null},"PeriodicalIF":10.2,"publicationDate":"2024-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141985663","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}