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Characteristic angular scales in cosmic microwave background radiation

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Characteristic angular scales in cosmic microwave background radiation. / Ghasemi, F.; Bahraminasab, A.; Sadegh Movahed, M. et al.
In: Journal of Statistical Mechanics: Theory and Experiment, No. P11008, 11.2006.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Ghasemi, F, Bahraminasab, A, Sadegh Movahed, M, Rahvar, S, Sreenivasan, KR & Reza Rahimi Tabar, M 2006, 'Characteristic angular scales in cosmic microwave background radiation', Journal of Statistical Mechanics: Theory and Experiment, no. P11008. https://doi.org/10.1088/1742-5468/2006/11/P11008

APA

Ghasemi, F., Bahraminasab, A., Sadegh Movahed, M., Rahvar, S., Sreenivasan, K. R., & Reza Rahimi Tabar, M. (2006). Characteristic angular scales in cosmic microwave background radiation. Journal of Statistical Mechanics: Theory and Experiment, (P11008). https://doi.org/10.1088/1742-5468/2006/11/P11008

Vancouver

Ghasemi F, Bahraminasab A, Sadegh Movahed M, Rahvar S, Sreenivasan KR, Reza Rahimi Tabar M. Characteristic angular scales in cosmic microwave background radiation. Journal of Statistical Mechanics: Theory and Experiment. 2006 Nov;(P11008). doi: 10.1088/1742-5468/2006/11/P11008

Author

Ghasemi, F. ; Bahraminasab, A. ; Sadegh Movahed, M. et al. / Characteristic angular scales in cosmic microwave background radiation. In: Journal of Statistical Mechanics: Theory and Experiment. 2006 ; No. P11008.

Bibtex

@article{d365f97edf8d46db84ad92a61985092b,
title = "Characteristic angular scales in cosmic microwave background radiation",
abstract = "We investigate the stochasticity in temperature fluctuations in the cosmic microwave background (CMB) radiation data from the Wilkinson Microwave Anisotropy Probe. We show that the angular fluctuation of the temperature is a Markov process with a Markov angular scale, ΘMarkov = 1.01-0.07+0.09. We characterize the complexity of the CMB fluctuations by means of a Fokker–Planck or Langevin equation and measure the associated Kramers–Moyal coefficients for the fluctuating temperature field T(\hat n) and its increment, \Delta T=T(\hat n_1)-T(\hat n_2) . Through this method we show that temperature fluctuations in the CMB have fat tails compared to a Gaussian distribution.",
author = "F. Ghasemi and A. Bahraminasab and {Sadegh Movahed}, M. and S. Rahvar and Sreenivasan, {K. R.} and {Reza Rahimi Tabar}, M.",
year = "2006",
month = nov,
doi = "10.1088/1742-5468/2006/11/P11008",
language = "English",
journal = "Journal of Statistical Mechanics: Theory and Experiment",
publisher = "IOP Publishing Ltd.",
number = "P11008",

}

RIS

TY - JOUR

T1 - Characteristic angular scales in cosmic microwave background radiation

AU - Ghasemi, F.

AU - Bahraminasab, A.

AU - Sadegh Movahed, M.

AU - Rahvar, S.

AU - Sreenivasan, K. R.

AU - Reza Rahimi Tabar, M.

PY - 2006/11

Y1 - 2006/11

N2 - We investigate the stochasticity in temperature fluctuations in the cosmic microwave background (CMB) radiation data from the Wilkinson Microwave Anisotropy Probe. We show that the angular fluctuation of the temperature is a Markov process with a Markov angular scale, ΘMarkov = 1.01-0.07+0.09. We characterize the complexity of the CMB fluctuations by means of a Fokker–Planck or Langevin equation and measure the associated Kramers–Moyal coefficients for the fluctuating temperature field T(\hat n) and its increment, \Delta T=T(\hat n_1)-T(\hat n_2) . Through this method we show that temperature fluctuations in the CMB have fat tails compared to a Gaussian distribution.

AB - We investigate the stochasticity in temperature fluctuations in the cosmic microwave background (CMB) radiation data from the Wilkinson Microwave Anisotropy Probe. We show that the angular fluctuation of the temperature is a Markov process with a Markov angular scale, ΘMarkov = 1.01-0.07+0.09. We characterize the complexity of the CMB fluctuations by means of a Fokker–Planck or Langevin equation and measure the associated Kramers–Moyal coefficients for the fluctuating temperature field T(\hat n) and its increment, \Delta T=T(\hat n_1)-T(\hat n_2) . Through this method we show that temperature fluctuations in the CMB have fat tails compared to a Gaussian distribution.

U2 - 10.1088/1742-5468/2006/11/P11008

DO - 10.1088/1742-5468/2006/11/P11008

M3 - Journal article

JO - Journal of Statistical Mechanics: Theory and Experiment

JF - Journal of Statistical Mechanics: Theory and Experiment

IS - P11008

ER -