Second-order Boltzmann equation: Gauge dependence and gauge invariance

Atsushi Naruko, Cyril Pitrou, Kazuya Koyama, Misao Sasaki

研究成果: Article査読

20 被引用数 (Scopus)

抄録

In the context of cosmological perturbation theory, we derive the second-order Boltzmann equation describing the evolution of the distribution function of radiation without a specific gauge choice. The essential steps in deriving the Boltzmann equation are revisited and extended given this more general framework: (i) the polarization of light is incorporated in this formalism by using a tensor-valued distribution function; (ii) the importance of a choice of the tetrad field to define the local inertial frame in the description of the distribution function is emphasized; (iii) we perform a separation between temperature and spectral distortion, both for the intensity and polarization for the first time; (iv) the gauge dependence of all perturbed quantities that enter the Boltzmann equation is derived, and this enables us to check the correctness of the perturbed Boltzmann equation by explicitly showing its gauge-invariance for both intensity and polarization. We finally discuss several implications of the gauge dependence for the observed temperature.

本文言語English
論文番号165008
ジャーナルClassical and Quantum Gravity
30
16
DOI
出版ステータスPublished - 2013 8月 21
外部発表はい

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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