The dark matter bispectrum from effective viscosity and one-particle irreducible vertices

Dark matter evolution during the process of cosmological structure formation can be described in terms of a one-particle irreducible effective action at a characteristic scale km and a loop expansion below this scale, based on the effective propagators and vertices. We calculate the form of the effe...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Flörchinger, Stefan (VerfasserIn) , Garny, Mathias (VerfasserIn) , Katsis, Aris (VerfasserIn) , Tetradis, Nikolaos (VerfasserIn) , Wiedemann, Urs Achim (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 24 July, 2019
In: Journal of cosmology and astroparticle physics
Year: 2019, Heft: 9
ISSN:1475-7516
DOI:10.1088/1475-7516/2019/09/047
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/1475-7516/2019/09/047
Volltext
Verfasserangaben:Stefan Floerchinger, Mathias Garny, Aris Katsis, Nikolaos Tetradis, Urs Achim Wiedemann
Beschreibung
Zusammenfassung:Dark matter evolution during the process of cosmological structure formation can be described in terms of a one-particle irreducible effective action at a characteristic scale km and a loop expansion below this scale, based on the effective propagators and vertices. We calculate the form of the effective vertices and compute the bispectrum of density perturbations within a one-loop approximation. We find that the effective vertices play a subdominant role as compared to the effective viscosity and sound velocity that modify the (inverse) propagators. For the bispectrum we reproduce the results of standard perturbation theory in the range where it is applicable, and find a slightly improved agreement with N-body simulations at larger wavenumbers.
Beschreibung:Gesehen am 12.03.2020
Beschreibung:Online Resource
ISSN:1475-7516
DOI:10.1088/1475-7516/2019/09/047