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We study how 21 cm intensity mapping can be used to measure gravitational lensing over a wide range of redshift.
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Hu, W., 2001, ApJ, 557, L79
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Linder, E. V., 2003, Phys. Rev. Lett., 90, 091301
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Copeland, E. J., Sami, M., Tsujikawa, S., 2006, Int.J.Mod.Phys., D15, 1753
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Furlanetto, S. R., Oh, S. P. & Briggs, F. H., 2006, Phys. Rep., 433, 181
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Zhang, P., & Pen, U. L., 2006, MNRAS, 367, 169
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Metcalf, R. B., & White, S. D. M., 2007, MNRAS, 381, 447
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2011
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Chen, X., 2012, Int. J. Mod. Phys., 12, 256
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Clifton, T., Ferreira, P. G., Padilla, A., Skordis, C., (2012), Phys.Rept., 513, 1
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Ade, P. et al. (Planck Collaboration), 2013, 1303.5076
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Battye, R. A., Browne, I. W. A., Dickinson, C., Heron, G., Maffei, B., Pourtsidou, A., 2013, MNRAS, 434, 1239
2013
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2010
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Masui, K. W., McDonald, P., Pen, U.-L., 2010, Phys. Rev. D, 81,103527
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Seo, H. J., Dodelson, S., Marriner, J., Mcginnis, D., Stebbins, A., Stoughton, C., Vallinoto, A., 2010, Astrophys. J., 721, 164
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Pober, J. C. et al., 2013, AJ, 145, 65
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Pourtsidou, A., Skordis, C., Copeland, E. J., 2013, 1307.0458 (to appear in Phys. Rev. D)
2013
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