Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity

被引:15
作者
Ettori, S. [1 ,2 ]
Ghirardini, V. [1 ,3 ]
Eckert, D. [4 ]
Dubath, F. [4 ]
Pointecouteau, E. [5 ,6 ]
机构
[1] INAF, Osservatorio Astron Bologna, Via Pietro Gobetti 93-3, I-40129 Bologna, Italy
[2] INAF, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[3] Univ Bologna, Dipartimento Fis & Astron, Via Pietro Gobetti 93-2, I-40129 Bologna, Italy
[4] Univ Geneva, Dept Astron, Ch Ec 16, CH-1290 Versoix, Switzerland
[5] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France
[6] Univ Toulouse, IRAP, UPS OMP, F-31028 Toulouse, France
基金
欧盟地平线“2020”;
关键词
galaxies: clusters: individual: Abell 2142; galaxies: clusters: individual: Abell 2319; galaxies: clusters: intracluster medium; dark matter; X-rays: galaxies: clusters; HYDROSTATIC EQUILIBRIUM; MASS PROFILES; SAMPLE; NEWTON; II;
D O I
10.1093/mnrasl/slx074
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the radial distribution of the dark matter in two massive, X-ray luminous galaxy clusters, Abell 2142 and Abell 2319, and compare it with the quantity predicted as apparent manifestation of the baryonic mass in the context of the 'Emergent Gravity' scenario, recently suggested from Verlinde. Thanks to the observational strategy of the XMM-Newton Cluster Outskirt Programme (X-COP), using the X-ray emission mapped with XMM-Newton and the Sunyaev-Zel'dovich signal in the Planck survey, we recover the gas density, temperature and thermal pressure profiles up to similar to R-200, allowing us to constrain at an unprecedented level the total mass through the hydrostatic equilibrium equation. We show that, also including systematic uncertainties related to the X-ray-based mass modelling, the apparent 'dark' matter shows a radial profile that has a shape different from the traditional dark matter distribution, with larger discrepancies (by a factor of 2-3) in the inner (r < 200 kpc) cluster's regions and a remarkable agreement only across R-500.
引用
收藏
页码:L29 / L33
页数:5
相关论文
共 37 条
  • [1] Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources
    Ade, P. A. R.
    Aghanim, N.
    Armitage-Caplan, C.
    Arnaud, M.
    Ashdown, M.
    Atrio-Barandela, F.
    Aumont, J.
    Aussel, H.
    Baccigalupi, C.
    Banday, A. J.
    Barreiro, R. B.
    Barrena, R.
    Bartelinann, M.
    Bartlett, J. G.
    Battaner, E.
    Benabed, K.
    Benoit, A.
    Benoit-Levy, A.
    Bernard, J. .
    Bersanelli, M.
    Bielewicz, P.
    Bikmaev, I.
    Bobin, J.
    Bock, J. J.
    Boehringer, H.
    Bonaldi, A.
    Bond, J. R.
    Borrill, J.
    Bouchet, F. R.
    Bridges, M.
    Bucher, M.
    Burenin, R.
    Burigana, C.
    Butier, R. C.
    Cardoso, J. -F.
    Carvalho, P.
    Catalano, A.
    Challinor, A.
    Chamballu, A.
    Chary, R. -R.
    Chen, X.
    Chiang, H. C.
    Chiang, L. -Y.
    Chon, G.
    Christensen, P. R.
    Churazov, E.
    Church, S.
    Clements, D. L.
    Colombi, S.
    Colombo, L. P. L.
    [J]. ASTRONOMY & ASTROPHYSICS, 2014, 571
  • [2] Planck early results. I. The Planck mission
    Ade, P. A. R.
    Aghanim, N.
    Arnaud, M.
    Ashdown, M.
    Aumont, J.
    Baccigalupi, C.
    Baker, M.
    Balbi, A.
    Banday, A. J.
    Barreiro, R. B.
    Bartlett, J. G.
    Battaner, E.
    Benabed, K.
    Bennett, K.
    Benoit, A.
    Bernard, J. -P.
    Bersanelli, M.
    Bhatia, R.
    Bock, J. J.
    Bonaldi, A.
    Bond, J. R.
    Borrill, J.
    Bouchet, F. R.
    Bradshaw, T.
    Bremer, M.
    Bucher, M.
    Burigana, C.
    Butler, R. C.
    Cabella, P.
    Cantalupo, C. M.
    Cappellini, B.
    Cardoso, J. -F.
    Carr, R.
    Casale, M.
    Catalano, A.
    Cayon, L.
    Challinor, A.
    Chamballu, A.
    Charra, J.
    Chary, R. -R.
    Chiang, L. -Y.
    Chiang, C.
    Christensen, P. R.
    Clements, D. L.
    Colombi, S.
    Couchot, F.
    Coulais, A.
    Crill, B. P.
    Crone, G.
    Crook, M.
    [J]. ASTRONOMY & ASTROPHYSICS, 2011, 536
  • [3] Planck intermediate results V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
    Ade, P. A. R.
    Aghanim, N.
    Arnaud, M.
    Ashdown, M.
    Atrio-Barandela, F.
    Aumont, J.
    Baccigalupi, C.
    Balbi, A.
    Banday, A. J.
    Barreiro, R. B.
    Bartlett, J. G.
    Battaner, E.
    Benabed, K.
    Benoit, A.
    Bernard, J. -P.
    Bersanelli, M.
    Bhatia, R.
    Bikmaev, I.
    Bobin, J.
    Boehringer, H.
    Bonaldi, A.
    Bond, J. R.
    Borgani, S.
    Borrill, J.
    Bouchet, F. R.
    Bourdin, H.
    Brown, M. L.
    Burenin, R.
    Burigana, C.
    Cabella, P.
    Cardoso, J. -F.
    Carvalho, P.
    Castex, G.
    Catalano, A.
    Cayon, L.
    Chamballu, A.
    Chiang, L. -Y
    Chon, G.
    Christensen, P. R.
    Churazov, E.
    Clements, D. L.
    Colafrancesco, S.
    Colombi, S.
    Colombo, L. P. L.
    Comis, B.
    Coulais, A.
    Crill, B. P.
    Cuttaia, F.
    Da Silva, A.
    Dahle, H.
    [J]. ASTRONOMY & ASTROPHYSICS, 2013, 550
  • [4] Cosmological Parameters from Observations of Galaxy Clusters
    Allen, Steven W.
    Evrard, August E.
    Mantz, Adam B.
    [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 49, 2011, 49 : 409 - 470
  • [5] Cosmology and astrophysics from relaxed galaxy clusters - IV. Robustly calibrating hydrostatic masses with weak lensing
    Applegate, D. E.
    Mantz, A.
    Allen, S. W.
    von der Linden, A.
    Morris, R. Glenn
    Hilbert, S.
    Kelly, Patrick L.
    Burke, D. L.
    Ebeling, H.
    Rapetti, D. A.
    Schmidt, R. W.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 457 (02) : 1522 - 1534
  • [6] The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the YSZ-M500 relation
    Arnaud, M.
    Pratt, G. W.
    Piffaretti, R.
    Boehringer, H.
    Croston, J. H.
    Pointecouteau, E.
    [J]. ASTRONOMY & ASTROPHYSICS, 2010, 517
  • [7] Self-similarity of temperature profiles in distant galaxy clusters: the quest for a universal law
    Baldi, A.
    Ettori, S.
    Molendi, S.
    Gastaldello, F.
    [J]. ASTRONOMY & ASTROPHYSICS, 2012, 545
  • [8] Brouwer M. M., 2016, MNRAS, V466, P2547
  • [9] CAVALIERE A, 1976, ASTRON ASTROPHYS, V49, P137
  • [10] Diez-Tejedor A., 2016, ARXIV161206282