中文

Planck 2015 结果. XXIV. 来自苏尼阿耶夫-泽尔多维奇星系团计数的宇宙学

宇宙学与河外天体物理 2018-02-20 v3

摘要

我们给出了来自 Planck 全任务数据集的星系团计数及相应的宇宙学约束。我们的星表包含 439 个通过其苏尼阿耶夫-泽尔多维奇(SZ)信号探测到的星系团,信噪比低至 6,比 2013 年 Planck 星系团宇宙学样本大两倍以上。计数与 2013 年的一致,并在相同建模假设下给出兼容的约束。利用更大的星表,我们将分析扩展到红移和信噪比的二维分布。我们使用来自最近两项关于 Planck 星系团对背景星系引力透镜研究的质量估计,为流体静力偏差参数 (1b)(1-b) 提供先验。此外,我们使用 Planck 星系团对宇宙微波背景(CMB)温度涨落的透镜效应作为对该参数的独立约束。这些不同的校准对当前物质涨落振幅给出了约束,与来自 Planck 对 CMB 原初涨落分析的约束存在不同程度张力;对于最低的 (1b)(1-b) 估计值,张力温和,仅略高于一个标准偏差,而对于最大的估计值张力仍然显著(3.7σ3.7\,\sigma)。我们还通过结合星系团和 CMB 约束检验了对基础平坦 Λ\LambdaCDM 模型扩展的约束。该组合似乎倾向于非最小中微子质量,但这一可能性对缓解整体张力作用甚微,因为它同时降低了隐含的哈勃参数值,从而加剧了与当前大多数天体物理估计的差异。将星系团质量校准精度从当前的 10% 水平提高到 1% 将显著加强这些组合分析,并为基准 Λ\LambdaCDM 模型提供严格检验。

关键词

引用

@article{arxiv.1502.01597,
  title  = {Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts},
  author = {Planck Collaboration and 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 J. G. Bartlett and N. Bartolo and E. Battaner and R. Battye and K. Benabed and A. Benoît and A. Benoit-Lévy and J. -P. Bernard and M. Bersanelli and P. Bielewicz and J. J. Bock and A. Bonaldi and L. Bonavera and J. R. Bond and J. Borrill and F. R. Bouchet and M. Bucher and C. Burigana and R. C. Butler and E. Calabrese and J. -F. Cardoso and A. Catalano and A. Challinor and A. Chamballu and R. -R. Chary and H. C. Chiang and P. R. Christensen and S. Church and D. L. Clements and S. Colombi and L. P. L. Colombo and C. Combet and B. Comis and F. Couchot and A. Coulais and B. P. Crill 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 F. -X. Désert and J. M. Diego and K. Dolag and H. Dole and S. Donzelli and O. Doré and M. Douspis and A. Ducout and X. Dupac and G. Efstathiou and F. Elsner and T. A. Enßlin and H. K. Eriksen and E. Falgarone and J. Fergusson and F. Finelli and O. Forni and M. Frailis and A. A. Fraisse and E. Franceschi and A. Frejsel and S. Galeotta and S. Galli and K. Ganga and M. Giard and Y. Giraud-Héraud and E. Gjerløw and J. González-Nuevo and K. M. Górski and S. Gratton and A. Gregorio and A. Gruppuso and J. E. Gudmundsson 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 G. Hurier and A. H. Jaffe and T. R. Jaffe and W. C. Jones and M. Juvela and E. Keihänen and R. Keskitalo and T. S. Kisner and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and G. Lagache and A. Lähteenmäki and J. -M. Lamarre and A. Lasenby and M. Lattanzi and C. R. Lawrence and R. Leonardi and J. Lesgourgues and F. Levrier 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 G. Maggio and D. Maino and N. Mandolesi and A. Mangilli and M. Maris and P. G. Martin and E. Martínez-González and S. Masi and S. Matarrese and P. McGehee and P. R. Meinhold and A. Melchiorri and J. -B. Melin and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. -A. Miville-Deschênes and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and C. B. Netterfield and H. U. Nørgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and C. A. Oxborrow and F. Paci and L. Pagano and F. Pajot and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and T. J. Pearson and O. Perdereau and L. Perotto and F. Perrotta and V. Pettorino and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and L. Popa and G. W. Pratt and G. Prézeau and S. Prunet and J. -L. Puget and J. P. Rachen and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and A. Renzi and I. Ristorcelli and G. Rocha and M. Roman and C. Rosset and M. Rossetti and G. Roudier and J. A. Rubiño-Martín and B. Rusholme and M. Sandri and D. Santos and M. Savelainen and G. Savini and D. Scott and M. D. Seiffert and E. P. S. Shellard and L. D. Spencer and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and D. Sutton and A. -S. Suur-Uski and J. -F. Sygnet and J. A. Tauber and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and J. Tuovinen and M. Türler and G. Umana and L. Valenziano and J. Valiviita and B. Van Tent and P. Vielva and F. Villa and L. A. Wade and B. D. Wandelt and I. K. Wehus and J. Weller and S. D. M. White and D. Yvon and A. Zacchei and A. Zonca},
  journal= {arXiv preprint arXiv:1502.01597},
  year   = {2018}
}

备注

19 pages, 18 figures ; now matches the version accepted in A&A