An f ( R , T ) gravity based FLRW model and o
暂无分享,去创建一个
[1] A. Banerjee,et al. Charged quark stars in f(R,T) gravity , 2022, Chinese Physics C.
[2] A. Banerjee,et al. Quark stars in f(R,T) gravity with an interacting quark equation of state , 2022, Physics of the Dark Universe.
[3] M. Ivanov. Cosmological constraints from the power spectrum of eBOSS emission line galaxies , 2021, Physical Review D.
[4] A. Pradhan,et al. Evaluation of cosmological models in $f(R, T)$ gravity in different dark energy scenario , 2021, 2106.03177.
[5] A. Chudaykin,et al. Constraints on the curvature of the Universe and dynamical dark energy from the full-shape and BAO data , 2020, 2009.10106.
[6] R. B. Barreiro,et al. Planck2018 results , 2020, Astronomy & Astrophysics.
[7] B. Sherwin,et al. Determining the Hubble constant without the sound horizon: Measurements from galaxy surveys , 2020, Physical Review D.
[8] T. Harko,et al. Comment on "Reexamining $f\left(R,T\right)$ gravity", Phys. Rev. D 100, 064059 (2019) , 2020, 2003.08107.
[9] M. Zaldarriaga,et al. Combining full-shape and BAO analyses of galaxy power spectra: a 1.6% CMB-independent constraint on H0 , 2020, Journal of Cosmology and Astroparticle Physics.
[10] F. Beutler,et al. Efficient cosmological analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 2019, Journal of Cosmology and Astroparticle Physics.
[11] A. Yadav,et al. Bulk viscous Bianchi-V cosmological model within the formalism of $f(R,T)=f_{1}(R)+f_{2}(R)f_{3}(T) $ gravity , 2019, Astrophysics and Space Science.
[12] A. Yadav,et al. Viability of Bianchi type V universe in f(R,T) = f1(R) + f2(R)f3(T) gravity , 2019, International Journal of Geometric Methods in Modern Physics.
[13] A. Yadav,et al. Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity , 2019, Modern Physics Letters A.
[14] E. Carlson,et al. Reexamining f(R,T) gravity , 2019, Physical Review D.
[15] E. Carlson,et al. Limits on f(R,T) gravity from Earth’s atmosphere , 2019, Physical Review D.
[16] N. E. Sommer,et al. First cosmological results using Type Ia supernovae from the Dark Energy Survey: measurement of the Hubble constant , 2018, Monthly Notices of the Royal Astronomical Society.
[17] A. Yadav,et al. Non-minimal matter-geometry coupling in Bianchi I space-time , 2018, Results in Physics.
[18] M. Malheiro,et al. Stellar equilibrium configurations of white dwarfs in the f(R, T) gravity , 2017, The European Physical Journal C.
[19] V. Oikonomou,et al. Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution , 2017, 1705.11098.
[20] R. Nichol,et al. Age-dating luminous red galaxies observed with the Southern African Large Telescope , 2016, 1702.00418.
[21] W. M. Wood-Vasey,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample , 2016, 1607.03155.
[22] Daniel Thomas,et al. A 6% measurement of the Hubble parameter at z∼0.45: direct evidence of the epoch of cosmic re-acceleration , 2016, 1601.01701.
[23] Michele Moresco. Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ 2 , 2015, 1503.01116.
[24] M. Shamir. Bianchi type-I cosmology in f(R, T) gravity , 2014, 1506.08699.
[25] Adam D. Myers,et al. Baryon acoustic oscillations in the Lyα forest of BOSS DR11 quasars , 2014, 1404.1801.
[26] Adam D. Myers,et al. Quasar-Lyman α forest cross-correlation from BOSS DR11: Baryon Acoustic Oscillations , 2013, 1311.1767.
[27] G. C. Samanta,et al. Higher Dimensional Cosmological Models Filled with Perfect Fluid in f(R,T) Theory of Gravity , 2013 .
[28] G. C. Samanta. Universe Filled with Dark Energy (DE) from a Wet Dark Fluid (WDF) in f(R,T) Gravity , 2013 .
[29] A. Myers,et al. Baryon Acoustic Oscillations in the Ly-\alpha\ forest of BOSS quasars , 2012, 1211.2616.
[30] Yun Wang,et al. Modelling the anisotropic two-point galaxy correlation function on small scales and single-probe measurements of H(z), DA(z) and f(z)σ8(z) from the Sloan Digital Sky Survey DR7 luminous red galaxies , 2012, 1209.0210.
[31] Siqi Liu,et al. Four new observational H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven , 2012, 1207.4541.
[32] K. Adhav. LRS Bianchi type-I cosmological model in f(R,T) theory of gravity , 2012 .
[33] S. Capozziello,et al. Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests , 2012, 1205.3421.
[34] Scott Croom,et al. The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1 , 2012, 1204.3674.
[35] B. Garilli,et al. Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers , 2012, 1201.3609.
[36] S. Deustua,et al. THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE z > 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE , 2011, 1105.3470.
[37] Tiberiu Harko,et al. f(R, T) Gravity , 2011, Extensions of f(R) Gravity.
[38] J. Yokoyama,et al. f(R) Gravity and its Cosmological Implications , 2011, 1101.0716.
[39] Sergei D. Odintsov,et al. Unified cosmic history in modified gravity: From F ( R ) theory to Lorentz non-invariant models , 2010, 1011.0544.
[40] Miao Li,et al. Dark Energy , 2011, Dialogue: A Journal of Mormon Thought.
[41] L. Verde,et al. Cosmic chronometers: constraining the equation of state of dark energy. I: H(z) measurements , 2009, 0907.3149.
[42] E. Gaztañaga,et al. Clustering of luminous red galaxies – IV. Baryon acoustic peak in the line-of-sight direction and a direct measurement of H(z) , 2008, 0807.3551.
[43] T. Sotiriou,et al. f(R) Theories Of Gravity , 2008, 0805.1726.
[44] J. Frieman,et al. Dark Energy and the Accelerating Universe , 2008, 0803.0982.
[45] S. Capozziello,et al. Extended theories of gravity and their cosmological and astrophysical applications , 2007, 0706.1146.
[46] E. Copeland,et al. Dynamics of dark energy , 2006, hep-th/0603057.
[47] S. D. Odintsov,et al. INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY , 2006, hep-th/0601213.
[48] S. Nojiri,et al. Dark energy problem : from phantom theory to modified Gauss-Bonnet gravity , 2005, hep-th/0510183.
[49] J. Prieto,et al. Hubble Space Telescope and Ground-based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications , 2005, astro-ph/0510155.
[50] Nikolay,et al. The Fourth Data Release of the Sloan Digital Sky Survey , 2005, The Astrophysical Journal Supplement Series.
[51] Yuan-zhong Zhang,et al. Probing the curvature and dark energy , 2005, astro-ph/0502262.
[52] L. Verde,et al. Constraints on the redshift dependence of the dark energy potential , 2004, astro-ph/0412269.
[53] R. Nichol,et al. Cosmological parameter analysis including SDSS Lyα forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy , 2004, astro-ph/0407372.
[54] S. Allen,et al. Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters , 2004, astro-ph/0405340.
[55] R. Nichol,et al. Cosmological parameters from SDSS and WMAP , 2003, astro-ph/0310723.
[56] S. Carroll,et al. Is Cosmic Speed-Up Due to New Gravitational Physics? , 2003, astro-ph/0306438.
[57] G. Ellis,et al. Multiverses and physical cosmology , 2003, astro-ph/0305292.
[58] Peter Garnavich,et al. Cosmological Results from High-z Supernovae , 2003, astro-ph/0305008.
[59] Edward J. Wollack,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results , 2003, astro-ph/0302207.
[60] Edward J. Wollack,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters , 2003, astro-ph/0302209.
[61] P. Peebles,et al. The Cosmological Constant and Dark Energy , 2002, astro-ph/0207347.
[62] A. Starobinsky,et al. Statefinder—A new geometrical diagnostic of dark energy , 2002, astro-ph/0201498.
[63] V. B. Johri. Genesis of cosmological tracker fields , 2000, astro-ph/0005608.
[64] V. V. Hristov,et al. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10'-5° , 2000, astro-ph/0005123.
[65] A. Melchiorri,et al. A flat Universe from high-resolution maps of the cosmic microwave background radiation , 2000, Nature.
[66] P. Steinhardt,et al. Cosmological tracking solutions , 1998, astro-ph/9812313.
[67] I. Hook,et al. Measurements of Ω and Λ from 42 High-Redshift Supernovae , 1998, astro-ph/9812133.
[68] A. Riess,et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.
[69] R. Ellis,et al. Discovery of a supernova explosion at half the age of the Universe , 1997, Nature.
[70] C. A. Oxborrow,et al. Planck 2015 results Special feature Planck 2015 results XIV . Dark energy and modified gravity , 2016 .
[71] R. Chaubey,et al. A new class of Bianchi cosmological models in f(R,T) gravity , 2013 .
[72] Edward J. Wollack,et al. SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2011 .
[73] Steven Weinberg,et al. The Cosmological Constant Problem , 1989 .