The Dark Matter Crisis: Falsification of the Current Standard Model of Cosmology

被引：183

作者：

Kroupa, P. ^{[1
]}

机构：

[1] Univ Bonn, Argelander Inst Astron, D-53121 Bonn, Germany

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2012年 / 29卷 / 04期

关键词：

cosmology: theory; dark energy; dark matter; Galaxy: evolution; galaxies: interactions; Local Group; MILKY-WAY SATELLITES; MODIFIED NEWTONIAN DYNAMICS; DWARF SPHEROIDAL GALAXIES; DISTANT GLOBULAR-CLUSTERS; TULLY-FISHER RELATION; COMMON MASS SCALE; LOCAL-GROUP; FORNAX CLUSTER; STAR-FORMATION; LAMBDA-CDM;

D O I：

10.1071/AS12005

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The current standard model of cosmology (SMoC) requires The Dual Dwarf Galaxy Theorem to be true according to which two types of dwarf galaxies must exist: primordial dark-matter (DM) dominated (type A) dwarf galaxies, and tidal-dwarf and ram-pressure-dwarf (type B) galaxies void of DM. Type A dwarfs surround the host approximately spherically, while type B dwarfs are typically correlated in phase-space. Type B dwarfs must exist in any cosmological theory in which galaxies interact. Only one type of dwarf galaxy is observed to exist on the baryonic Tully-Fisher plot and in the radius-mass plane. The Milky Way satellite system forms a vast phase-space-correlated structure that includes globular clusters and stellar and gaseous streams. Other galaxies also have phase-space correlated satellite systems. Therefore, The Dual Dwarf Galaxy Theorem is falsified by observation and dynamically relevant cold or warm DM cannot exist. It is shown that the SMoC is incompatible with a large set of other extragalactic observations. Other theoretical solutions to cosmological observations exist. In particular, alone the empirical mass-discrepancy-acceleration correlation constitutes convincing evidence that galactic-scale dynamics must be Milgromian. Major problems with inflationary big bang cosmologies remain unresolved.

引用

页码：395 / 433

页数：39

共 311 条

[1] N-BODY SIMULATIONS OF GALAXY CLUSTERING .1. INITIAL CONDITIONS AND GALAXY COLLAPSE TIMES [J].

AARSETH, SJ ;

GOTT, JR ;

TURNER, EL .

ASTROPHYSICAL JOURNAL, 1979, 228 (03) :664-683

[2] A limit on the variation of the speed of light arising from quantum gravity effects [J].

Abdo, A. A. ;

Ackermann, M. ;

Ajello, M. ;

Asano, K. ;

Atwood, W. B. ;

Axelsson, M. ;

Baldini, L. ;

Ballet, J. ;

Barbiellini, G. ;

Baring, M. G. ;

Bastieri, D. ;

Bechtol, K. ;

Bellazzini, R. ;

Berenji, B. ;

Bhat, P. N. ;

Bissaldi, E. ;

Bloom, E. D. ;

Bonamente, E. ;

Bonnell, J. ;

Borgland, A. W. ;

Bouvier, A. ;

Bregeon, J. ;

Brez, A. ;

Briggs, M. S. ;

Brigida, M. ;

Bruel, P. ;

Burgess, J. M. ;

Burnett, T. H. ;

Caliandro, G. A. ;

Cameron, R. A. ;

Caraveo, P. A. ;

Casandjian, J. M. ;

Cecchi, C. ;

Celik, Oe ;

Chaplin, V. ;

Charles, E. ;

Cheung, C. C. ;

Chiang, J. ;

Ciprini, S. ;

Claus, R. ;

Cohen-Tanugi, J. ;

Cominsky, L. R. ;

Connaughton, V. ;

Conrad, J. ;

Cutini, S. ;

Dermer, C. D. ;

de Angelis, A. ;

de Palma, F. ;

Digel, S. W. ;

Dingus, B. L. .

NATURE, 2009, 462 (7271) :331-334

[3] VERITAS deep observations of the dwarf spheroidal galaxy Segue 1 [J].

Aliu, E. ;

Archambault, S. ;

Arlen, T. ;

Aune, T. ;

Beilicke, M. ;

Benbow, W. ;

Bouvier, A. ;

Bradbury, S. M. ;

Buckley, J. H. ;

Bugaev, V. ;

Byrum, K. ;

Cannon, A. ;

Cesarini, A. ;

Christiansen, J. L. ;

Ciupik, L. ;

Collins-Hughes, E. ;

Connolly, M. P. ;

Cui, W. ;

Decerprit, G. ;

Dickherber, R. ;

Dumm, J. ;

Errando, M. ;

Falcone, A. ;

Feng, Q. ;

Ferrer, F. ;

Finley, J. P. ;

Finnegan, G. ;

Fortson, L. ;

Furniss, A. ;

Galante, N. ;

Gall, D. ;

Godambe, S. ;

Griffin, S. ;

Grube, J. ;

Gyuk, G. ;

Hanna, D. ;

Holder, J. ;

Huan, H. ;

Hughes, G. ;

Humensky, T. B. ;

Kaaret, P. ;

Karlsson, N. ;

Kertzman, M. ;

Khassen, Y. ;

Kieda, D. ;

Krawczynski, H. ;

Krennrich, F. ;

Lee, K. ;

Madhavan, A. S. ;

Maier, G. .

PHYSICAL REVIEW D, 2012, 85 (06)

[4]

Amendola L., 2010, Dark Energy: Theory and Observations, DOI 10.1017/CBO9780511750823

[5] DO HOT HALOS AROUND GALAXIES CONTAIN THE MISSING BARYONS? [J].

Anderson, Michael E. ;

Bregman, Joel N. .

ASTROPHYSICAL JOURNAL, 2010, 714 (01) :320-331

[6] Results from 730 kg days of the CRESST-II Dark Matter search [J].

Angloher, G. ;

Bauer, M. ;

Bavykina, I. ;

Bento, A. ;

Bucci, C. ;

Ciemniak, C. ;

Deuter, G. ;

von Feilitzsch, F. ;

Hauff, D. ;

Huff, P. ;

Isaila, C. ;

Jochum, J. ;

Kiefer, M. ;

Kimmerle, M. ;

Lanfranchi, J. -C. ;

Petricca, F. ;

Pfister, S. ;

Potzel, W. ;

Proebst, F. ;

Reindl, F. ;

Roth, S. ;

Rottler, K. ;

Sailer, C. ;

Schaffner, K. ;

Schmaler, J. ;

Scholl, S. ;

Seidel, W. ;

v. Sivers, M. ;

Stodolsky, L. ;

Strandhagen, C. ;

Strauss, R. ;

Tanzke, A. ;

Usherov, I. ;

Wawoczny, S. ;

Willers, M. ;

Zoeller, A. .

EUROPEAN PHYSICAL JOURNAL C, 2012, 72 (04) :1-22

[7]

Angus GW, 2008, MON NOT R ASTRON SOC, V387, P1481, DOI [10.1111/j.1365-2966.2008.13351.x, 10.1111/j.1365-2966.2008.13351]

[8] The collision velocity of the bullet cluster in conventional and modified dynamics [J].

Angus, G. W. ;

McGaugh, S. S. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2008, 383 (02) :417-423

[9] Can MOND take a bullet? Analytical comparisons of three versions of MOND beyond spherical symmetry [J].

Angus, G. W. ;

Famaey, B. ;

Zhao, H. S. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 371 (01) :138-146

[10] The abundance of galaxy clusters in modified Newtonian dynamics: cosmological simulations with massive neutrinos [J].

Angus, G. W. ;

Diaferio, Antonaldo .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 417 (02) :941-949

← 1 2 3 4 5 6 7 8 9 10 →