Constraining MOND with Solar System dynamics

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Latex2e, 8 pages, 1 table, 2 figures, 14 references. Reference updated. To appear in JGP (Journal of Gravitational Physics)

Scientific paper

In this letter we investigate the deep Newtonian regime of the MOND paradigm from a purely phenomenological point of view by exploiting the least-square estimated corrections to the secular rates of the perihelia of the inner and of some of the outer planets of the Solar System by E.V. Pitjeva with the EPM2004 ephemerides. By using $\mu(x)\approx 1-k_0(1/x)^n$ for the interpolating MONDian function, and by assuming that $k_0$, considered body-independent so to avoid violations of the equivalence principle, experiences no spatial variations throughout the Solar System we tightly constrain $n$ with the ratios of the perihelion precessions for different pairs of planets. We find that the range $1\leq n\leq 2$ is neatly excluded at much more than $3-\sigma$ level. Such a test would greatly benefit from the use of extra-precessions of perihelia independently estimated by other groups as well.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Constraining MOND with Solar System dynamics does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Constraining MOND with Solar System dynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraining MOND with Solar System dynamics will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-297674

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.