%0 Generic %1 collaboration2013gravitational %A Collaboration, Polarbear %A Ade, P. A. R. %A Akiba, Y. %A Anthony, A. E. %A Arnold, K. %A Barron, D. %A Boettger, D. %A Borrill, J. %A Chapman, S. %A Chinone, Y. %A Dobbs, M. %A Elleflot, T. %A Errard, J. %A Fabbian, G. %A Feng, C. %A Flanigan, D. %A Gilbert, A. %A Grainger, W. %A Halverson, N. W. %A Hasegawa, M. %A Hattori, K. %A Hazumi, M. %A Holzapfel, W. L. %A Hori, Y. %A Howard, J. %A Hyland, P. %A Inoue, Y. %A Jaehnig, G. C. %A Jaffe, A. %A Keating, B. %A Kermish, Z. %A Keskitalo, R. %A Kisner, T. %A Jeune, M. Le %A Lee, A. T. %A Linder, E. %A Lungu, M. %A Matsuda, F. %A Matsumura, T. %A Meng, X. %A Miller, N. J. %A Morii, H. %A Moyerman, S. %A Myers, M. J. %A Navaroli, M. %A Nishino, H. %A Paar, H. %A Peloton, J. %A Quealy, E. %A Rebeiz, G. %A Reichardt, C. L. %A Richards, P. L. %A Ross, C. %A Schanning, I. %A Schenck, D. E. %A Sherwin, B. %A Shimizu, A. %A Shimmin, C. %A Shimon, M. %A Siritanasak, P. %A Smecher, G. %A Spieler, H. %A Stebor, N. %A Steinbach, B. %A Stompor, R. %A Suzuki, A. %A Takakura, S. %A Tomaru, T. %A Wilson, B. %A Yadav, A. %A Zahn, O. %D 2013 %K cmb lensing polarization %T Gravitational Lensing of Cosmic Microwave Background Polarization %U http://arxiv.org/abs/1312.6646 %X Primary fluctuations in both temperature and polarization of the Cosmic Microwave Background (CMB) reflect the properties of the Universe from the Big Bang until the photons decoupled from matter 380,000 years later. These primary fluctuations are then lensed by large-scale structures (such as clusters of galaxies and filaments of dark matter), with the result that the distribution and properties of dark matter, including the masses of neutrinos, can be determined more accurately by extracting the lensing information than through studying the primary fluctuations alone. Polarization lensing can give cleaner, higher resolution results than temperature lensing. The correlation of lensed CMB polarization with large-scale structure, traced through the Cosmic Infrared Background, was recently detected; however, this correlation does not trace all structure and depends on the relationship between the infrared flux from the galaxies and the underlying mass distribution. Here we report the detection of gravitational lensing directly from CMB polarization measurements. With these data, we have made a census of essentially all structure integrated along the line of sight through the full depth of the observable Universe on 30 square degrees of the sky, and we find good agreement with expectations from the standard Lambda cold-dark matter cosmology.

@misc{collaboration2013gravitational, abstract = {Primary fluctuations in both temperature and polarization of the Cosmic Microwave Background (CMB) reflect the properties of the Universe from the Big Bang until the photons decoupled from matter 380,000 years later. These primary fluctuations are then lensed by large-scale structures (such as clusters of galaxies and filaments of dark matter), with the result that the distribution and properties of dark matter, including the masses of neutrinos, can be determined more accurately by extracting the lensing information than through studying the primary fluctuations alone. Polarization lensing can give cleaner, higher resolution results than temperature lensing. The correlation of lensed CMB polarization with large-scale structure, traced through the Cosmic Infrared Background, was recently detected; however, this correlation does not trace all structure and depends on the relationship between the infrared flux from the galaxies and the underlying mass distribution. Here we report the detection of gravitational lensing directly from CMB polarization measurements. With these data, we have made a census of essentially all structure integrated along the line of sight through the full depth of the observable Universe on 30 square degrees of the sky, and we find good agreement with expectations from the standard Lambda cold-dark matter cosmology.}, added-at = {2013-12-24T09:03:00.000+0100}, author = {Collaboration, Polarbear and Ade, P. A. R. and Akiba, Y. and Anthony, A. E. and Arnold, K. and Barron, D. and Boettger, D. and Borrill, J. and Chapman, S. and Chinone, Y. and Dobbs, M. and Elleflot, T. and Errard, J. and Fabbian, G. and Feng, C. and Flanigan, D. and Gilbert, A. and Grainger, W. and Halverson, N. W. and Hasegawa, M. and Hattori, K. and Hazumi, M. and Holzapfel, W. L. and Hori, Y. and Howard, J. and Hyland, P. and Inoue, Y. and Jaehnig, G. C. and Jaffe, A. and Keating, B. and Kermish, Z. and Keskitalo, R. and Kisner, T. and Jeune, M. Le and Lee, A. T. and Linder, E. and Lungu, M. and Matsuda, F. and Matsumura, T. and Meng, X. and Miller, N. J. and Morii, H. and Moyerman, S. and Myers, M. J. and Navaroli, M. and Nishino, H. and Paar, H. and Peloton, J. and Quealy, E. and Rebeiz, G. and Reichardt, C. L. and Richards, P. L. and Ross, C. and Schanning, I. and Schenck, D. E. and Sherwin, B. and Shimizu, A. and Shimmin, C. and Shimon, M. and Siritanasak, P. and Smecher, G. and Spieler, H. and Stebor, N. and Steinbach, B. and Stompor, R. and Suzuki, A. and Takakura, S. and Tomaru, T. and Wilson, B. and Yadav, A. and Zahn, O.}, biburl = {https://www.bibsonomy.org/bibtex/2adecb755c2a9ea7b47e90e1c94e5a133/miki}, description = {[1312.6646] Gravitational Lensing of Cosmic Microwave Background Polarization}, interhash = {87800a968df62f4539e72da6e86b106e}, intrahash = {adecb755c2a9ea7b47e90e1c94e5a133}, keywords = {cmb lensing polarization}, note = {cite arxiv:1312.6646Comment: 8 pages, 4 figures. The companion paper describes a measurement of polarization lensing in cross-correlation}, timestamp = {2013-12-24T09:03:00.000+0100}, title = {Gravitational Lensing of Cosmic Microwave Background Polarization}, url = {http://arxiv.org/abs/1312.6646}, year = 2013 }