Astron. Astrophys. 342, 15-33 (1999)

Acknowledgements

It is a pleasure to thanks S. Colombi for his useful suggestion to use a second order Lagrangian dynamics, B. Fort, P. Schneider, B. Jain and U. Seljak for fruitful discussions. We are very grateful to the referee S. Seitz for her extremely detailed report with very useful remarks and suggestions. This research has been conducted under the auspices of a European TMR network programme made possible via generous financial support from the European Commission. This work was also supported by the Programme National de Cosmologie and the "Sonderforschungsbereich 375-95 für Astro-Teilchenphysik" der Deutschen Forschungsgemeischaft. L.V.W. and F.B. thank IAP, where a fair fraction of this work has been done, for hospitality.

© European Southern Observatory (ESO) 1999

Online publication: December 22, 1998
helpdesk.link@springer.de