We present a new method for calculating loops in cosmological perturbation theory. This method is based on approximating a ACDM-like cosmology as a finite sum of complex power-law universes. The decomposition is naturally achieved using an FFTLog algorithm. For power-law cosmologies, all loop integrals are formally equivalent to loop integrals of massless quantum field theory. These integrals have analytic solutions in terms of generalized hypergeometric functions. We provide explicit formulae for the one-loop and the two-loop power spectrum and the one-loop bispectrum. A chief advantage of our approach is that the difficult part of the calculation is cosmology independent, need be done only once, and can be recycled for any relevant predictions. Evaluation of standard loop diagrams then boils down to a simple matrix multiplication. We demonstrate the promise of this method for applications to higher multiplicity/loop correlation functions.

Cosmological perturbation theory using the FFTLog: formalism and connection to QFT loop integrals / Marko Simonovic; Tobias Baldauf; Matias Zaldarriaga; John Joseph Carrasco; Juna A. Kollmeier. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - STAMPA. - 2018:(2018), pp. 030-030. [10.1088/1475-7516/2018/04/030]

Cosmological perturbation theory using the FFTLog: formalism and connection to QFT loop integrals

Marko Simonovic
;
2018

Abstract

We present a new method for calculating loops in cosmological perturbation theory. This method is based on approximating a ACDM-like cosmology as a finite sum of complex power-law universes. The decomposition is naturally achieved using an FFTLog algorithm. For power-law cosmologies, all loop integrals are formally equivalent to loop integrals of massless quantum field theory. These integrals have analytic solutions in terms of generalized hypergeometric functions. We provide explicit formulae for the one-loop and the two-loop power spectrum and the one-loop bispectrum. A chief advantage of our approach is that the difficult part of the calculation is cosmology independent, need be done only once, and can be recycled for any relevant predictions. Evaluation of standard loop diagrams then boils down to a simple matrix multiplication. We demonstrate the promise of this method for applications to higher multiplicity/loop correlation functions.
2018
2018
030
030
Marko Simonovic; Tobias Baldauf; Matias Zaldarriaga; John Joseph Carrasco; Juna A. Kollmeier
File in questo prodotto:
File Dimensione Formato  
Simonovi%C4%87_2018_J._Cosmol._Astropart._Phys._2018_030.pdf

accesso aperto

Tipologia: Pdf editoriale (Version of record)
Licenza: Open Access
Dimensione 1.53 MB
Formato Adobe PDF
1.53 MB Adobe PDF

I documenti in FLORE sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1344758
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 62
  • ???jsp.display-item.citation.isi??? 68
social impact