A tensor—vector—scalar framework for modified dynamics and cosmic dark matter

By R. Sanders. 2005

137 citations recorded by the source corpus.

I describe a tensor-vector-scalar theory that reconciles the galaxy-scale success of modified Newtonian dynamics (MOND) with the cosmological scale evidence for cold dark matter (CDM). The theory provides a cosmological basis for MOND in the sense that the predicted phenomenology only arises in a cosmological background. The theory contains an evolving effective potential, and scalar field oscillations in this potential comprise the CDM; the de Broglie wavelength of these soft bosons, however, is sufficiently large that they cannot accumulate in galaxies. The theory predicts, inevitably, a constant anomalous acceleration in the outer Solar system, which, depending upon the choice of parameters, can be consistent with that detected by the Pioneer spacecrafts.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/afc31cd5b3165bcaaefaf53955ec6522e4a35865

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In Astronomy and Astrophysics

  1. Pavel Kroupa
  2. M. Pawlowski
  3. S. McGaugh
  4. B. Famaey
  5. J. Brownstein
  6. H. Jerjen
  7. Joerg Dabringhausen
  8. J. W. Moffat

In Nuclear and High Energy Physics

  1. Pavel Kroupa
  2. J. W. Moffat
  3. M. Pawlowski
  4. S. McGaugh
  5. B. Famaey
  6. J. Brownstein
  7. Joerg Dabringhausen
  8. M. Metz

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