Planck 中间结果 XXIV:基本常数变化的限制
宇宙学与河外天体物理
2016-08-11 v1
摘要
基本物理常数的任何变化,特别是精细结构常数 或电子质量 的变化,都会影响宇宙的复合历史,并在宇宙微波背景角功率谱上留下印记。我们表明,与 WMAP 数据相比,Planck 数据能够将红移 处精细结构常数随时间变化的限制提高约 5 倍,并打破其与哈勃常数 的简并。除了 之外,我们还可以对电子质量 的变化以及这两个常数的同时变化设定限制。我们详细考察了基本常数与宇宙学参数之间的简并性,以便比较从 Planck 和 WMAP 获得的限制,并确定包含其他宇宙学探针所获得的约束能力。我们得出结论,Planck 将精细结构常数和电子质量的独立时间变化限制在 68% 置信水平下的 和 。我们还研究了精细结构常数空间变化的可能性。 的偶极空间变化(对应于跨越我们哈勃体积的梯度)的相对振幅被限制为 。
引用
@article{arxiv.1406.7482,
title = {Planck intermediate results. XXIV. Constraints on variation of fundamental constants},
author = {P. A. R. Ade and N. Aghanim and M. Arnaud and M. Ashdown and J. Aumont and C. Baccigalupi and A. J. Banday and R. B. Barreiro and E. Battaner and K. Benabed and A. Benoit-Lévy and J. -P. Bernard and M. Bersanelli and P. Bielewicz and J. R. Bond and J. Borrill and F. R. Bouchet and C. Burigana and R. C. Butler and E. Calabrese and A. Chamballu and H. C. Chiang and P. R. Christensen and D. L. Clements and L. P. L. Colombo and F. Couchot and A. Curto and F. Cuttaia and L. Danese and R. D. Davies and R. J. Davis and P. de Bernardis and A. de Rosa and G. de Zotti and J. Delabrouille and J. M. Diego and H. Dole and O. Doré and X. Dupac and T. A. Enßlin and H. K. Eriksen and O. Fabre and F. Finelli and O. Forni and M. Frailis and E. Franceschi and S. Galeotta and S. Galli and K. Ganga and M. Giard and J. González-Nuevo and K. M. Górski and A. Gregorio and A. Gruppuso and F. K. Hansen and D. Hanson and D. L. Harrison and S. Henrot-Versillé and C. Hernández-Monteagudo and D. Herranz and S. R. Hildebrandt and E. Hivon and M. Hobson and W. A. Holmes and A. Hornstrup and W. Hovest and K. M. Huffenberger and A. H. Jaffe and W. C. Jones and E. Keihänen and R. Keskitalo and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and J. -M. Lamarre and A. Lasenby and C. R. Lawrence and R. Leonardi and J. Lesgourgues and M. Liguori and P. B. Lilje and M. Linden-Vørnle and M. López-Caniego and P. M. Lubin and J. F. Macías-Pérez and N. Mandolesi and M. Maris and P. G. Martin and E. Martínez-González and S. Masi and S. Matarrese and P. Mazzotta and P. R. Meinhold and A. Melchiorri and L. Mendes and E. Menegoni and A. Mennella and M. Migliaccio and M. -A. Miville-Deschênes and A. Moneti and L. Montier and G. Morgante and A. Moss and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and H. U. Nørgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and C. A. Oxborrow and L. Pagano and F. Pajot and D. Paoletti and F. Pasian and G. Patanchon and O. Perdereau and L. Perotto and F. Perrotta and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and G. W. Pratt and S. Prunet and J. P. Rachen and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and S. Ricciardi and I. Ristorcelli and G. Rocha and G. Roudier and B. Rusholme and M. Sandri and G. Savini and D. Scott and L. D. Spencer and V. Stolyarov and R. Sudiwala and D. Sutton and A. -S. Suur-Uski and J. -F. Sygnet and J. A. Tauber and D. Tavagnacco and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and J. -P. Uzan and L. Valenziano and J. Valiviita and B. Van Tent and P. Vielva and F. Villa and L. A. Wade and D. Yvon and A. Zacchei and A. Zonca},
journal= {arXiv preprint arXiv:1406.7482},
year = {2016}
}
备注
25 pages, 16 figures, 11 tables, submitted to A&A