摘要: Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the nature of the earliest moments of time. The next gener... 展开
作者 | Abazajian, K. N. Arnold, K. Calabrese, E. Carlstrom, J. E. Carvalho, C. S. Chang, C. L. Chiang, H. C. Church, S. Cooray, A. Crawford, T. M. Crill, B. P. Dawson, K. S. Austermann, J. Das, S. Devline, M. J. Dobbs, M. Dodelson, S. Dore, O. Dunkley, J. Feng, J. L. Fraisse, A. Gallicchio, J. Giddings, S. B. Benson, B. A. Green, D. Halverson, N. W. Hannany, S. Hanson, D. Wollack, E. J. Bischoff, C. Bock, J. Bond, J. R. Borrill, J. Buder, I. Burke, D. L. | ||
---|---|---|---|
原报告号 | N150020915 | 总页数 | 11 |
主办者 | National Aeronautics and Space Administration | ||
报告分类号 | [ 54C - Astrophysics] | ||
报告类别/文献类型 | DE / NTIS科技报告 | ||
关键词 | Inflating Cosmic microwave background radiation Large-scale structure of the universe Cosmology Gravitational lenses Dark energy Spectroscopy Dark matter |