A 1D kinetic model for cosmic microwave background comptonization

Authors

  • A. Sandoval-Villalbazo U. Iberoamericana, Mexico City

DOI:

https://doi.org/10.31349/RevMexFis.66.352

Keywords:

Kinetic theory, CMB, Comptonization

Abstract

This work presents a novel derivation of the expressions that  describe the distortions of the CMB curve due to the interactions between photons and the electrons present in dilute ionized systems. In this approach, a simplified a one-dimensional evolution  equation for the photon number occupation is applied  in order to describe the aforemationed interaction. This methodology allows to emphasize the physical features ot the Sunyaev-Zeldovich effect and suggests the existence of links between basic statistical physics and complex applications involving radiative processes.

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References

Y.B. Zel’dovich and R.A. Sunyaev, "

The Interaction of Matter and Radiation in a Hot-Model Universe", Astrophys. Space Sci. 4, 301 (1969

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(2003).

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A. Sandoval-Villalbazo and L.S. García-Colín, "On a parity property in the thermal Sunyaev-Zel'dovich effect", AIP Conf. Proc. 758:170-175, 2005.

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Published

2020-05-01

How to Cite

[1]
A. Sandoval-Villalbazo, “A 1D kinetic model for cosmic microwave background comptonization”, Rev. Mex. Fís., vol. 66, no. 3 May-Jun, pp. 352–355, May 2020.

Issue

Vol. 66 No. 3 May-Jun (2020): Revista Mexicana de Fìsica

Section

17 Thermodynamics and Statistical Physics

License

Authors retain copyright and grant the Revista Mexicana de Física right of first publication with the work simultaneously licensed under a CC BY-NC-ND 4.0 that allows others to share the work with an acknowledgement of the work's authorship and initial publication in this journal.

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