Jetzer, P; Sereno, M (2009). Limits on dark matter and cosmological constant from solar system dynamics. In: Pécontal, E; Buchert, T; Di Stefano, P; Copin, Y. Dark energy and dark matter: Observations, experiments and theories. Les Ulis, FR, 127-132. ISBN 978-2-7598-0439-9.
Full text not available from this repository.
View at publisher
We discuss the influence of the cosmological constant on the solar system dynamics. Observational constraints are derived from measurements of the periastron advance of the planets. Moreover, we consider the change in the mean motion due to . Up to now, Earth and Mars data give the best constraint, . If properly accounting for the gravito-magnetic effect, this upper limit on could greatly improve in the near future thanks to new data from planned or already operating space-missions. Dark matter or modifications of the Newtonian inverse-square law in the solar system are discussed as well. Variations in the 1/r2 behavior are considered in the form of either a possible Yukawa-like interaction or a modification of gravity of MOND type.
|Item Type:||Book Section, not refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Deposited On:||27 Feb 2010 15:50|
|Last Modified:||27 Nov 2013 21:39|
|Series Name:||EAS Publications Series|
|Additional Information:||Conference on Dark Energy, Dark Matter - Observation, Experiments and Theories, Lyon, France, July 07-11, 2008|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page