Testing the tensor-vector-scalar theory with the latest cosmological observations

被引：3

作者：

Xu, Xiao-dong ^{[1
]}

Wang, Bin ^{[1
]}

Zhang, Pengjie ^{[1
]}

机构：

[1] Shanghai Jiao Tong Univ, Dept Phys & Astron, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China

来源：

PHYSICAL REVIEW D | 2015年 / 92卷 / 08期

基金：

中国国家自然科学基金;

关键词：

MODIFIED NEWTONIAN DYNAMICS; EXTENDED ROTATION CURVES; CLUSTER PECULIAR VELOCITIES; SURFACE BRIGHTNESS GALAXIES; SPECTROSCOPIC SURVEY; MODIFIED GRAVITY; SPIRAL GALAXIES; DARK-MATTER; POWER; MASS;

D O I：

10.1103/PhysRevD.92.083505

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The tensor-vector-scalar (TeVeS) model is considered a viable theory of gravity. It produces the Milgrom's modified Newtonian dynamics in the nonrelativistic weak field limit and is free from ghosts. This model has been tested against various cosmological observations. Here, we investigate whether new observations such as the galaxy velocity power spectrum measured by 6dF and the kinetic Sunyaev Zel'dovich effect power spectrum measured by ACT/SPT can put further constraints on the TeVeS model. Furthermore, we perform the test of TeVeS cosmology with a sterile neutrino by confronting to Planck data, and find that it is ruled out by cosmic microwave background measurements from the Planck mission.

引用

页数：15

共 111 条

[1] Planck 2013 results. XV. CMB power spectra and likelihood [J].

Ade, P. A. R. ;

Aghanim, N. ;

Armitage-Caplan, C. ;

Arnaud, M. ;

Ashdown, M. ;

Atrio-Barandela, F. ;

Aumont, J. ;

Baccigalupi, C. ;

Banday, A. J. ;

Barreiro, R. B. ;

Bartlett, J. G. ;

Battaner, E. ;

Benabed, K. ;

Benoit, A. ;

Benoit-Levy, A. ;

Bemard, J. -P. ;

Bersanelli, M. ;

Bielewicz, P. ;

Bobin, J. ;

Bock, J. J. ;

Bonaldi, A. ;

Bonavera, L. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bridges, M. ;

Bucher, M. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

Cardoso, J. -F. ;

Catalano, A. ;

Challinor, A. ;

Chamballu, A. ;

Chiang, H. C. ;

Chiang, L. -Y ;

Christensen, P. R. ;

Church, S. ;

Clements, D. L. ;

Colombi, S. ;

Colombo, L. P. L. ;

Combet, C. ;

Couchot, F. ;

Coulais, A. ;

Crill, B. P. ;

Curto, A. ;

Cuttaia, F. ;

Danese, L. ;

Davies, R. D. .

ASTRONOMY & ASTROPHYSICS, 2014, 571

[2] Planck 2013 results. XVI. Cosmological parameters [J].

Ade, P. A. R. ;

Aghanim, N. ;

Armitage-Caplan, C. ;

Arnaud, M. ;

Ashdown, M. ;

Atrio-Barandela, F. ;

Aumont, J. ;

Baccigalupi, C. ;

Banday, A. J. ;

Barreiro, R. B. ;

Bartlett, J. G. ;

Battaner, E. ;

Benabed, K. ;

Benoit, A. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bielewicz, P. ;

Bobin, J. ;

Bock, J. J. ;

Bonaldi, A. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Bridges, M. ;

Bucher, M. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

Cappellini, B. ;

Cardoso, J. -F. ;

Catalano, A. ;

Challinor, A. ;

Chamballu, A. ;

Chary, R. -R. ;

Chen, X. ;

Chiang, H. C. ;

Chiang, L. -Y ;

Christensen, P. R. ;

Church, S. ;

Clements, D. L. ;

Colombi, S. ;

Colombo, L. P. L. ;

Couchot, F. ;

Coulais, A. ;

Crill, B. P. ;

Curto, A. ;

Cuttaia, F. ;

Danese, L. ;

Davies, R. D. .

ASTRONOMY & ASTROPHYSICS, 2014, 571

[3] Planck intermediate results XIII. Constraints on peculiar velocities [J].

Ade, P. A. R. ;

Aghanim, N. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Baccigalupi, C. ;

Balbi, A. ;

Banday, A. J. ;

Barreiro, R. B. ;

Battaner, E. ;

Benabed, K. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bielewicz, P. ;

Bikmaev, I. ;

Bobin, J. ;

Bock, J. J. ;

Bonaldi, A. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Burigana, C. ;

Butler, R. C. ;

Cabella, P. ;

Cardoso, J. -F. ;

Catalano, A. ;

Chamballu, A. ;

Chiang, L. -Y ;

Chon, G. ;

Christensen, P. R. ;

Clements, D. L. ;

Colombi, S. ;

Colombo, L. P. L. ;

Crill, B. P. ;

Cuttaia, F. ;

Da Silva, A. ;

Dahle, H. ;

Davies, R. D. ;

Davis, R. J. ;

de Bernardis, P. ;

de Gasperis, G. ;

de Zotti, G. ;

Delabrouille, J. ;

Democles, J. ;

Diego, J. M. ;

Dolag, K. ;

Dole, H. ;

Donzelli, S. ;

Dore, O. .

ASTRONOMY & ASTROPHYSICS, 2014, 561

[4] Trouble for cluster parameter estimation from blind SZ surveys? [J].

Aghanim, N ;

Hansen, SH ;

Lagache, G .

ASTRONOMY & ASTROPHYSICS, 2005, 439 (03) :901-912

[5] How accurately can the SZ effect measure peculiar cluster velocities and bulk flows? [J].

Aghanim, N ;

Górski, KM ;

Puget, JL .

ASTRONOMY & ASTROPHYSICS, 2001, 374 (01) :1-12

[6] 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

[7] Is an 11 eV sterile neutrino consistent with clusters, the cosmic microwave background and modified Newtonian dynamics? [J].

Angus, G. W. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 394 (01) :527-532

[8]

[Anonymous], EXPL SUPPL PLANCK 20

[9]

[Anonymous], 1932, Astron. Inst. Netherlands

[10] Measuring the Mach number of the universe via the Sunyaev-Zeldovich effect [J].

Atrio-Barandela, F ;

Kashlinsky, A ;

Mücket, JP .

ASTROPHYSICAL JOURNAL, 2004, 601 (02) :L111-L114

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