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Volumn 79, Issue 8, 2009, Pages

Can the relativistic field theory version of modified Newtonian dynamics avoid dark matter on galactic scales?

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EID: 65549123934     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.79.081301     Document Type: Article
Times cited : (40)

References (18)
  • 1
    • 0000011795 scopus 로고
    • ASJOAB 0004-637X 10.1086/161130
    • M. Milgrom, Astrophys. J. 270, 365 (1983). ASJOAB 0004-637X 10.1086/161130
    • (1983) Astrophys. J. , vol.270 , pp. 365
    • Milgrom, M.1
  • 2
    • 84927699419 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.70.083509
    • J.D. Bekenstein, Phys. Rev. D PRVDAQ 1550-7998 70, 083509 (2004); 10.1103/PhysRevD.70.083509
    • (2004) Phys. Rev. D , vol.70 , pp. 083509
    • Bekenstein, J.D.1
  • 3
    • 21444439400 scopus 로고    scopus 로고
    • The Published Extended Rotation Curves of Spiral Galaxies: Confrontation with Modified Dynamics
    • DOI 10.1086/178131
    • R.H. Sanders, Astrophys. J. 473, 117 (1996). ASJOAB 0004-637X 10.1086/178131 (Pubitemid 127002255)
    • (1996) Astrophysical Journal , vol.473 , pp. 117-129
    • Sanders, R.H.1
  • 4
    • 34547657850 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2007.07.004
    • N.E. Mavromatos and M. Sakellariadou, Phys. Lett. B 652, 97 (2007). PYLBAJ 0370-2693 10.1016/j.physletb.2007.07.004
    • (2007) Phys. Lett. B , vol.652 , pp. 97
    • Mavromatos, N.E.1    Sakellariadou, M.2
  • 6
    • 34548095743 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2007.12073.x
    • R.H. Sanders, Mon. Not. R. Astron. Soc. 380, 331 (2007). MNRAA4 0035-8711 10.1111/j.1365-2966.2007.12073.x
    • (2007) Mon. Not. R. Astron. Soc. , vol.380 , pp. 331
    • Sanders, R.H.1
  • 7
    • 41449095014 scopus 로고    scopus 로고
    • AAEJAF 0004-6361 10.1051/0004-6361:20078224
    • M. Feix, C. Fedeli, and M. Bartelmann, Astron. Astrophys. 480, 313 (2008). AAEJAF 0004-6361 10.1051/0004-6361:20078224
    • (2008) Astron. Astrophys. , vol.480 , pp. 313
    • Feix, M.1    Fedeli, C.2    Bartelmann, M.3
  • 10
  • 11
    • 33644512377 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/500805
    • H. Zhao and B. Famaey, Astrophys. J. ASJOAB 0004-637X 638, L9 (2006). 10.1086/500805
    • (2006) Astrophys. J. , vol.638 , pp. 9
    • Zhao, H.1    Famaey, B.2
  • 13
    • 33747503913 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2006.10668.x
    • G.W. Angus, B. Famaey, and H. Zhao, Mon. Not. R. Astron. Soc. MNRAA4 0035-8711 371, 138 (2006). 10.1111/j.1365-2966.2006.10668.x
    • (2006) Mon. Not. R. Astron. Soc. , vol.371 , pp. 138
    • Angus, G.W.1    Famaey, B.2    Zhao, H.3
  • 14
  • 15
  • 16
  • 17
    • 32644472614 scopus 로고    scopus 로고
    • Large scale structure in bekenstein's theory of relativistic modified Newtonian dynamics
    • DOI 10.1103/PhysRevLett.96.011301
    • C. Skordis, D.F. Mota, P.G. Ferreira, and C. Boehm, Phys. Rev. Lett. 96, 011301 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.96.011301 (Pubitemid 43248326)
    • (2006) Physical Review Letters , vol.96 , Issue.1 , pp. 011301
    • Skordis, C.1    Mota, D.F.2    Ferreira, P.G.3    Boehm, C.4
  • 18
    • 33845369824 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.97.231301
    • S. Dodelson and M. Liguori, Phys. Rev. Lett. 97, 231301 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.97.231301
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 231301
    • Dodelson, S.1    Liguori, M.2


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