| Issue |
|
EAS Publications Series
Volume 20,
2006
Mass Profiles and Shapes of Cosmological Structures
|
|
Page(s)
|
|
217 - 224 |
| DOI |
|
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) 217-224DOI: 10.1051/eas:2006074
MOND as modified inertia
M. Milgrom The Weizmann Institute Center for Astrophysics
Abstract
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
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