Quasi-linear formulation of MOND

By Mordehai Milgrom. 2009

190 citations recorded by the source corpus.

A new formulation of modified Newtonian dynamics (MOND) as a modified-potential theory of gravity is propounded. In effect, the theory dictates that the MOND potential φ produced by a mass distribution ρ is a solution of the Poisson equation for the modified source density ˆ ρ =− (4πG) −1 ∇· g, where g = ν(|g N |/a0)g N , and g N is the Newtonian acceleration field of ρ. This makes φ simply the scalar potential of the algebraic acceleration field g. The theory thus involves solving only linear-differential equations, with one non-linear, algebraic step. It is derivable from an action, satisfies all the usual conservation laws, and gives the correct centre-of-mass acceleration to composite bodies. The theory is akin in some respects to the non-linear Poisson formulation of Bekenstein and Milgrom, but it is different from it, and is obviously easier to apply. The two theories are shown to emerge as natural modifications of a Palatini-type formulation of Newtonian gravity, and are members in a larger class of bi-potential theories.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/2c30e810de868247ddf32488b205dd79aea3b69b

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In Astronomy and Astrophysics

  1. Pavel Kroupa
  2. M. Pawlowski
  3. S. McGaugh
  4. B. Famaey
  5. F. Lelli
  6. J. Schombert
  7. H. Jerjen
  8. Joerg Dabringhausen

In Nuclear and High Energy Physics

  1. Pavel Kroupa
  2. J. Schombert
  3. M. Pawlowski
  4. F. Lelli
  5. S. McGaugh
  6. B. Famaey
  7. Joerg Dabringhausen
  8. M. Metz

In Statistical and Nonlinear Physics

  1. F. Lelli
  2. Pavel Kroupa
  3. J. Schombert
  4. B. Famaey
  5. H. Jerjen
  6. S. McGaugh
  7. M. Pawlowski
  8. Joerg Dabringhausen

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