2011
DOI: 10.1103/physreve.83.046217
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Renormalized waves and thermalization of the Klein-Gordon equation

Abstract: We study the thermalization of the classical Klein-Gordon equation under a u 4 interaction. We numerically show that even in the presence of strong nonlinearities, the local thermodynamic equilibrium state exhibits a weakly nonlinear behavior in a renormalized wave basis. The renormalized basis is defined locally in time by a linear transformation and the requirement of vanishing wavewave correlations. We show that the renormalized waves oscillate around one frequency, and that the frequency dispersion relatio… Show more

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Cited by 39 publications
(95 citation statements)
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“…The upper limits of on the CMB anisotropies due to the secondary thermal and kinetic Sunyaev–Zel’dovich effects were estimated by Leuker et al (2010) and Shirokoff et al (2011). These are smaller than the amplitude of the anomaly we have reported here.…”
Section: Discussioncontrasting
confidence: 64%
“…The upper limits of on the CMB anisotropies due to the secondary thermal and kinetic Sunyaev–Zel’dovich effects were estimated by Leuker et al (2010) and Shirokoff et al (2011). These are smaller than the amplitude of the anomaly we have reported here.…”
Section: Discussioncontrasting
confidence: 64%
“…This was followed recently by the Balloon‐borne Large Aperture Submillimeter Telescope (BLAST), 2 which measured the clustering power near the energetic peak of the CIB at 600, 860 and 1200 GHz (500, 350 and 250 μm, respectively; Viero et al 2009). Hall et al (2010) reported the first detection of clustered CIB power at millimetre wavelengths, in South Pole Telescope (SPT) 3 data, soon followed by Dunkley et al (2011) in Atacama Cosmology Telescope (ACT) 4 data, and Shirokoff et al (2011) with additional SPT data. Most recently, measurements of the CIB fluctuation power, extending over a broad range in frequencies and angular scales, have been reported in Planck Collaboration (2011) and Amblard et al (2011), inferred from Planck and Herschel data, respectively 5 .…”
Section: Introductionmentioning
confidence: 99%
“…This has become possible recently using high‐resolution observations of the CMB by the Atacama Cosmology Telescope (ACT; Dunkley et al 2011) and by the South Pole Telescope (SPT; Lueker et al 2010; Shirokoff et al 2011). Both the ACT and SPT teams perform multiparameter fits to the temperature power spectra using ‘templates’ to model the secondary anisotropies.…”
Section: Introductionmentioning
confidence: 99%