Effects of dark sectors' mutual interaction on the growth of structures
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Y. Jing | Bin Wang | Jian-hua He | Y. P. Jing
[1] R. Maartens,et al. The growth of structure in interacting dark energy models , 2009, 0905.0492.
[2] A. Berera,et al. On the large-scale instability in interacting dark energy and dark matter fluids , 2009, 0901.3272.
[3] V. Pettorino,et al. Hydrodynamical N-body simulations of coupled dark energy cosmologies , 2008, 0812.3901.
[4] B. Moraes,et al. The growth of matter perturbations in f(R) models , 2008, 0809.3374.
[5] Jiliang Jing,et al. Dynamics of an interacting dark energy model in Einstein and loop quantum cosmology , 2008, 0808.3482.
[6] Y. Gong. The growth factor parameterization and modified gravity , 2008 .
[7] Y. Gong. Growth factor parametrization and modified gravity , 2008, 0808.1316.
[8] Bin Wang,et al. Stability of the curvature perturbation in dark sectors' mutual interacting models , 2008, 0807.3471.
[9] A. Riotto,et al. Parameterizing the effect of dark energy perturbations on the growth of structures , 2008, 0807.3343.
[10] L. Amendola,et al. Quintessence cosmologies with a growing matter component , 2008 .
[11] D. Pavón,et al. Toward a solution of the coincidence problem , 2008, 0806.2116.
[12] W. M. Wood-Vasey,et al. Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets , 2008, 0804.4142.
[13] E. Majerotto,et al. Large-scale instability in interacting dark energy and dark matter fluids , 2008, 0804.0232.
[14] L. Colombo,et al. DARK MATTER–DARK ENERGY COUPLING BIASING PARAMETER ESTIMATES FROM COSMIC MICROWAVE BACKGROUND DATA , 2008, 0804.0285.
[15] C. Feng,et al. Observational constraints on the dark energy and dark matter mutual coupling , 2008, 0804.0110.
[16] Shuang-Nan Zhang,et al. How to distinguish dark energy and modified gravity , 2008, 0803.3292.
[17] D. Polarski,et al. The growth of matter perturbations in some scalar–tensor DE models , 2008, 0802.4196.
[18] Alexandre Refregier,et al. The Dark UNiverse Explorer (DUNE): proposal to ESA’s cosmic vision , 2008, 0802.2522.
[19] Bin Wang,et al. Effects of the interaction between dark energy and dark matter on cosmological parameters , 2008, 0801.4233.
[20] E. Bertschinger,et al. Distinguishing modified gravity from dark energy , 2008, 0801.2431.
[21] Roy Maartens,et al. Dynamics of dark energy with a coupling to dark matter , 2008, 0801.1565.
[22] P. A. R. Ade,et al. HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET , 2008, 0801.1491.
[23] D. Pavón,et al. Le Châtelier–Braun principle in cosmological physics , 2007, 0712.0565.
[24] Bin Wang,et al. Thermodynamical description of the interaction between holographic dark energy and dark matter , 2007, 0711.2214.
[25] D. Pavón,et al. Thermodynamical description of the interaction between dark energy and dark matter , 2007 .
[26] D. Polarski,et al. On the growth of linear perturbations , 2007, 0710.1510.
[27] L. Sodré,et al. Signature of the interaction between dark energy and dark matter in galaxy clusters , 2007, 0710.1198.
[28] B. Jain,et al. Observational Tests of Modified Gravity , 2007, 0709.2375.
[29] M. Trodden,et al. The adiabatic instability on cosmology's dark side , 2007, 0709.1124.
[30] Mark Trodden,et al. Adiabatic instability in coupled dark energy/dark matter models , 2007, 0709.1128.
[31] Bin Wang,et al. Transition of equation of state of effective dark energy in the Dvali-Gabadadze-Porrati model with bulk contents , 2007, 0708.0992.
[32] R. Nichol,et al. Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS , 2007, 0705.3323.
[33] O. Bertolami,et al. The Abell Cluster A586 and the Equivalence Principle , 2007 .
[34] Ole Eggers Bjælde,et al. Neutrino dark energy—revisiting the stability issue , 2007, 0705.2018.
[35] S. Tsujikawa. Matter density perturbations and effective gravitational constant in modified gravity models of dark energy , 2007, 0705.1032.
[36] N. Riazi,et al. String inspired explanation for the superacceleration of our Universe , 2007, 0704.0666.
[37] O. Bertolami,et al. Dark energy–dark matter interaction and putative violation of the equivalence principle from the Abell cluster A586 , 2007, astro-ph/0703462.
[38] Alexander S. Szalay,et al. The Shape of the Sloan Digital Sky Survey Data Release 5 Galaxy Power Spectrum , 2007 .
[39] N. Ohta,et al. Probing the coupling between dark components of the universe , 2007, astro-ph/0702015.
[40] C. Tao,et al. Probing for dynamics of dark energy and curvature of universe with latest cosmological observations , 2006, astro-ph/0612728.
[41] Stefano Casertano,et al. New Hubble Space Telescope Discoveries of Type Ia Supernovae at z ≥ 1: Narrowing Constraints on the Early Behavior of Dark Energy , 2006, astro-ph/0611572.
[42] J. Bond,et al. Improved Measurements of the CMB Power Spectrum with ACBAR , 2006, astro-ph/0611198.
[43] R. Nichol,et al. Cosmological constraints from the SDSS luminous red galaxies , 2006, astro-ph/0608632.
[44] F. Atrio-Barandela,et al. Matter density perturbations in interacting quintessence models , 2006, astro-ph/0607604.
[45] J. Zang,et al. Interacting Dark Energy and Dark Matter: Observational Constraints from Cosmological Parameters , 2006, astro-ph/0607126.
[46] Edward J. Wollack,et al. Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology , 2006, astro-ph/0603449.
[47] M. Kaplinghat,et al. Stable models of superacceleration , 2006, astro-ph/0601517.
[48] J. Khoury,et al. Superacceleration as the signature of a dark sector interaction , 2005, astro-ph/0510628.
[49] J. Neill,et al. The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda,and w from the First Year Data Set , 2005, astro-ph/0510447.
[50] P. Ferreira,et al. Implications of the Cosmic Background Imager Polarization Data , 2005, astro-ph/0509203.
[51] M. Zaldarriaga,et al. Instability of dark energy with mass-varying neutrinos , 2005, astro-ph/0506663.
[52] L. Amendola,et al. Phantom damping of matter perturbations , 2005, astro-ph/0506222.
[53] W. Zimdahl. INTERACTING DARK ENERGY AND COSMOLOGICAL EQUATIONS OF STATE , 2005, gr-qc/0505056.
[54] D. Pavón,et al. Holographic dark energy and cosmic coincidence , 2005, gr-qc/0505020.
[55] R. Ellis,et al. The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications , 2005, astro-ph/0501174.
[56] R. Nichol,et al. Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies , 2005, astro-ph/0501171.
[57] Stefano Casertano,et al. Type Ia Supernova Discoveries at z > 1 from the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution , 2004, astro-ph/0402512.
[58] S. Carroll,et al. Is Cosmic Speed-Up Due to New Gravitational Physics? , 2003, astro-ph/0306438.
[59] Peter Garnavich,et al. Cosmological Results from High-z Supernovae , 2003, astro-ph/0305008.
[60] L. Amendola,et al. Tracking and coupled dark energy as seen by the Wilkinson Microwave Anisotropy Probe , 2003 .
[61] D. Pavón,et al. Interacting quintessence solution to the coincidence problem , 2003, astro-ph/0303145.
[62] M. Halpern,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: ANGULAR POWER SPECTRA , 2008, The Astrophysical Journal Supplement Series.
[63] Edward J. Wollack,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters , 2003, astro-ph/0302209.
[64] W. Zimdahl,et al. Interacting Quintessence , 2001, astro-ph/0105479.
[65] L. Amendola,et al. Stationary dark energy: The Present universe as a global attractor , 2000, astro-ph/0011243.
[66] M. Porrati,et al. 4D Gravity on a Brane in 5D Minkowski Space , 2000, hep-th/0005016.
[67] L. Amendola. Coupled Quintessence , 1999, astro-ph/9908023.
[68] I. Hook,et al. Measurements of Ω and Λ from 42 High-Redshift Supernovae , 1998, astro-ph/9812133.
[69] A. Riess,et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.
[70] A. G. Alexei,et al. OBSERVATIONAL EVIDENCE FROM SUPERNOVAE FOR AN ACCELERATING UNIVERSE AND A COSMOLOGICAL CONSTANT , 1998 .
[71] R. Ellis,et al. Discovery of a supernova explosion at half the age of the Universe , 1997, Nature.
[72] S. Carroll,et al. DARK MATTER WITH TIME-DEPENDENT MASS , 1997, COSMO-97.
[73] H. Kodama,et al. Cosmological Perturbation Theory , 1984 .