Present limits to cosmic bubbles from the COBE-DMR three point correlation function

The existence of large scale voids in several galaxy surveys suggests the occurence of an inflationary first order phase transition. This process generates primordial bubbles that, before evolving into the present voids, leave at decoupling a non-Gaussian imprint on the CMB. I this paper we evaluate...

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Bibliographische Detailangaben
Hauptverfasser:	Corasaniti, Pier Stefano (VerfasserIn) , Amendola, Luca (VerfasserIn) , Occhionero, Franco (VerfasserIn)
Dokumenttyp:	Article (Journal) Kapitel/Artikel
Sprache:	Englisch
Veröffentlicht:	2000
In:	Arxiv
Online-Zugang:	Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/0005575
Verfasserangaben:	P.S. Corasaniti, L. Amendola, F. Occhionero

Present limits to cosmic bubbles from the COBE-DMR three-point correlation function von Corasaniti, Pier Stefano (VerfasserIn) , Amendola, Luca (VerfasserIn) , Occhionero, Franco (VerfasserIn) ,

in: Monthly notices of the Royal Astronomical Society, 323 (2001), 3, Seite 677-680

Article (Journal) Online Resource

Present limits to cosmic bubbles from the COBE-DMR three point correlation function

Present limits to cosmic bubbles from the COBE-DMR three-point correlation function von Corasaniti, Pier Stefano (VerfasserIn) , Amendola, Luca (VerfasserIn) , Occhionero, Franco (VerfasserIn) ,

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