| Issue |
EAS Publications Series
Volume 20, 2006
Mass Profiles and Shapes of Cosmological Structures
|
|
|---|---|---|
| Page(s) | 217 - 224 | |
| DOI | https://doi.org/10.1051/eas:2006074 | |
| Published online | 19 May 2006 | |
Mass Profiles and Shapes of Cosmological Structures
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 217-224
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 217-224
MOND as modified inertia
The Weizmann Institute Center for Astrophysics
I briefly highlight the salient properties of modified-inertia formulations of MOND, contrasting them with those of modified-gravity formulations, which describe practically all theories propounded to date. Future data (e.g. the establishment of the Pioneer anomaly as a new physics phenomenon) may prefer one of these broad classes of theories over the other. I also outline some possible starting ideas for modified inertia.
© EAS, EDP Sciences, 2006