A SIMPLIFIED TREATMENT OF GRAVITATIONAL INTERACTION ON GALACTIC SCALES

被引:5
|
作者
Trippe, Sascha [1 ]
机构
[1] Seoul Natl Univ, Dept Phys & Astron, Seoul 151742, South Korea
基金
新加坡国家研究基金会;
关键词
Gravitation; Galaxies: kinematics and dynamics; NEWTONIAN DYNAMICS; MASS; GALAXIES; MATTER; CLUSTER; HALO;
D O I
10.5303/JKAS.2013.46.1.41
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I present a simple scheme for the treatment of gravitational interactions on galactic scales. In analogy with known mechanisms of quantum field theory, I assume ad hoc that gravitation is mediated by virtual exchange particles - gravitons - with very small but non-zero masses. The resulting density and mass profiles are proportional to the mass of the gravitating body. The mass profile scales with the centripetal acceleration experienced by a test particle orbiting the central mass, but this comes at the cost of postulating a universal characteristic acceleration ao approximate to 4.3 x 10(-12) m sec(-2) (or 8 pi a(0) approximate to 1.1 x 10(-10) m sec(-2)). The scheme predicts the asymptotic flattening of galactic rotation curves, the Tully-Fisher/Faber-Jackson relations, the mass discrepancy acceleration relation of galaxies, the surface brightness acceleration relation of galaxies, the kinematics of galaxy clusters, and "Renzo's rule" correctly; additional (dark) mass components are not required. Given that it is based on various ad-hoc assumptions and given further limitations, the scheme I present is not yet a consistent theory of gravitation; rather, it is a "toy model" providing a convenient scaling law that simplifies the description of gravity on galactic scales.
引用
收藏
页码:41 / 47
页数:7
相关论文
共 50 条
  • [31] GRAVITATIONAL MICROLENSING OF THE GALACTIC BULGE STARS
    PACZYNSKI, B
    ASTROPHYSICAL JOURNAL, 1991, 371 (02): : L63 - &
  • [32] FOCUSING OF GRAVITATIONAL RADIATION BY GALACTIC CORE
    LAWRENCE, JK
    PHYSICAL REVIEW D, 1971, 3 (12): : 3239 - &
  • [33] Galactic binaries as sources of gravitational waves
    Nelemans, G
    ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES, 2003, 686 : 263 - 272
  • [34] Radio source evolution on galactic scales
    Maciel, T.
    Alexander, P.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 442 (04) : 3469 - 3483
  • [35] Testing quantised inertia on galactic scales
    McCulloch, M. E.
    ASTROPHYSICS AND SPACE SCIENCE, 2012, 342 (02) : 575 - 578
  • [36] Towards cosmological concordance on galactic scales
    van den Bosch, FC
    Mo, HJ
    Yang, XH
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 345 (03) : 923 - 938
  • [37] The structure of Galactic hydrogen on the largest scales
    McClure-Griffiths, NM
    Dickey, JM
    Gaensler, BM
    Green, AJ
    HOW DOES THE GALAXY WORK?: A GALACTIC TERTULIA WITH DON COX AND RON REYNOLDS, 2004, 315 : 34 - 38
  • [38] Triggered star formation on galactic scales
    Palous, J
    Ehlerová, S
    Wünsch, R
    Tenorio-Tagle, G
    Silich, S
    Medina-Tanco, GA
    Muñoz-Tuñon, C
    DENSE INTERSTELLAR MEDIUM IN GALAXIES, 2004, 91 : 129 - 134
  • [39] Galaxies on Sub-Galactic Scales
    Jerjen, Helmut
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 2012, 29 (04): : 383 - 394
  • [40] Testing quantised inertia on galactic scales
    M. E. McCulloch
    Astrophysics and Space Science, 2012, 342 : 575 - 578