de.mpg.escidoc.pubman.appbase.FacesBean
Deutsch
 
Hilfe Wegweiser Impressum Kontakt Einloggen
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT

Freigegeben

Konferenzbeitrag

Future non-linear stability of the Einstein-Vlasov system with reflection Bianchi II and VI0 symmetry

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20695

Nungesser,  Ernesto
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Externe Ressourcen
Es sind keine Externen Ressourcen verfügbar
Volltexte (frei zugänglich)

AIP_ConfProc1458_499.pdf
(beliebiger Volltext), 794KB

Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

Nungesser, E. (2012). Future non-linear stability of the Einstein-Vlasov system with reflection Bianchi II and VI0 symmetry. In Towards New Paradigms: Proceedings of the Spanish Relativity Meeting 2011, AIP Conference Proceedings, Vol. 1458 (pp. 499-502).


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0010-0D26-5
Zusammenfassung
Assuming that the space-time is close to special solutions which will play the role of the ω-limit and that the maximal velocity of the particles is small, we have been able to show that for reflection symmetric Bianchi II and reflection symmetric Bianchi VI0 spacetimes with collisionless matter the asymptotic behaviour at late times is close to the special case of dust. The key was a bootstrap argument.