Distance-redshift and growth-redshift relations as two windows on acceleration and gravitation: Dark energy or new gravity?
暂无分享,去创建一个
[1] Neutrino mass and dark energy from weak lensing. , 2002, Physical review letters.
[2] 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.
[3] D. Wittman. Spurious Shear from the Atmosphere in Ground-based Weak-lensing Observations , 2005, astro-ph/0509003.
[4] M. White. Baryons and weak lensing power spectra , 2004, astro-ph/0405593.
[5] 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.
[6] Dependence of the non-linear mass power spectrum on the equation of state of dark energy , 2005, astro-ph/0505565.
[7] R. Ellis,et al. Measurements of $\Omega$ and $\Lambda$ from 42 high redshift supernovae , 1998, astro-ph/9812133.
[8] J. Miralda-Escudé. The correlation function of galaxy ellipticities produced by gravitational lensing , 1991 .
[9] Asantha Cooray,et al. Measuring Angular Diameter Distances through Halo Clustering , 2001, astro-ph/0105061.
[10] A. Evrard,et al. The baryon content of galaxy clusters: a challenge to cosmological orthodoxy , 1993, Nature.
[11] Illuminating dark energy with cosmic shear , 2004, astro-ph/0411673.
[12] Weak lensing in generalized gravity theories , 2004, astro-ph/0403654.
[13] S. J. Dodds,et al. Non-linear evolution of cosmological power spectra , 1996 .
[14] Yong Song. Looking for an extra dimension with tomographic cosmic shear , 2004, astro-ph/0407489.
[15] S. Dodelson,et al. Dark energy and the cosmic microwave background radiation. , 2000, Physical review letters.
[16] Glenn Starkman,et al. Differentiating between modified gravity and dark energy , 2004 .
[17] How Cold Dark Matter Theory Explains Milgrom's Law , 2001, astro-ph/0107284.
[18] A. Lue,et al. The phenomenology of Dvali–Gabadadze–Porrati cosmologies , 2005, astro-ph/0510068.
[19] Edward J. Wollack,et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters , 2003, astro-ph/0302209.
[20] Precision measurement of the mean curvature , 2005, astro-ph/0503405.
[21] Yong-Seon Song,et al. Determination of cosmological parameters from cosmic shear data , 2004 .
[22] M. Bartelmann,et al. Weak gravitational lensing , 2016, Scholarpedia.
[23] S. Dodelson,et al. Nonlinear cosmological matter power spectrum with massive neutrinos: The halo model , 2004, astro-ph/0411552.
[24] Wayne Hu,et al. � 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A. POWER SPECTRUM TOMOGRAPHY WITH WEAK LENSING , 1999 .
[25] M. Phillips,et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.
[26] Jun Zhang,et al. Isolating Geometry in Weak-Lensing Measurements , 2003, astro-ph/0312348.
[27] L. Knox,et al. Effect of Hot Baryons on the Weak-Lensing Shear Power Spectrum , 2004, astro-ph/0409198.
[28] Probing Newton's constant on vast scales: Dvali-Gabadadze-Porrati gravity, cosmic acceleration, and large scale structure , 2004, astro-ph/0401515.
[29] Calibrating the nonlinear matter power spectrum: Requirements for future weak lensing surveys , 2004, astro-ph/0412142.