Large-Scale Suppression from Stochastic Inflation

Kuhnel F, Schwarz D (2010)
Phys.Rev.Lett. 105(21): 211302.

Zeitschriftenaufsatz | Veröffentlicht | Englisch
 
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Autor*in
Kuhnel, Florian; Schwarz, DominikUniBi
Abstract / Bemerkung
We show that the power spectrum of a self-interacting scalar field in de Sitter space-time is strongly suppressed on large scales. The cut-off scale depends on the strength of the self-coupling, the number of e-folds of quasi-de Sitter evolution, and its expansion rate. As a consequence, the two-point correlation function of field fluctuations is free from infra-red divergencies.
Stichworte
Theory-HEP; power spectrum; infrared problem; space-time: de Sitter; Phenomenology-HEP; numerical calculations; inflation: stochastic; Gravitation and Cosmology; field theory: scalar; field theory: fluctuation; 98.80.Cq; 04.62.+v; 05.10.Gg; Astrophysics; correlation function; suppression
Erscheinungsjahr
2010
Zeitschriftentitel
Phys.Rev.Lett.
Band
105
Ausgabe
21
Art.-Nr.
211302
ISSN
0031-9007
eISSN
1079-7114
Page URI
https://pub.uni-bielefeld.de/record/1967069

Zitieren

Kuhnel F, Schwarz D. Large-Scale Suppression from Stochastic Inflation. Phys.Rev.Lett. 2010;105(21): 211302.
Kuhnel, F., & Schwarz, D. (2010). Large-Scale Suppression from Stochastic Inflation. Phys.Rev.Lett., 105(21), 211302. https://doi.org/10.1103/PhysRevLett.105.211302
Kuhnel, Florian, and Schwarz, Dominik. 2010. “Large-Scale Suppression from Stochastic Inflation”. Phys.Rev.Lett. 105 (21): 211302.
Kuhnel, F., and Schwarz, D. (2010). Large-Scale Suppression from Stochastic Inflation. Phys.Rev.Lett. 105:211302.
Kuhnel, F., & Schwarz, D., 2010. Large-Scale Suppression from Stochastic Inflation. Phys.Rev.Lett., 105(21): 211302.
F. Kuhnel and D. Schwarz, “Large-Scale Suppression from Stochastic Inflation”, Phys.Rev.Lett., vol. 105, 2010, : 211302.
Kuhnel, F., Schwarz, D.: Large-Scale Suppression from Stochastic Inflation. Phys.Rev.Lett. 105, : 211302 (2010).
Kuhnel, Florian, and Schwarz, Dominik. “Large-Scale Suppression from Stochastic Inflation”. Phys.Rev.Lett. 105.21 (2010): 211302.
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PMID: 21231284
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arXiv: 1003.3014

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