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arxiv: 1210.5900 · v1 · pith:3TPEJMK6new · submitted 2012-10-22 · ❄️ cond-mat.stat-mech · astro-ph.CO· hep-ph

Analysis of residual spectra and the monopole spectrum for 3 K blackbody radiation by means of non-extensive thermostatistics

classification ❄️ cond-mat.stat-mech astro-ph.COhep-ph
keywords blackbodylimitsmonopolenon-extensiveradiationresidualspectraspectrum
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We analyze residual spectra of 3 K blackbody radiation (CMB) using non-extensive thermostatistics with a parameter q-1. The limits of |q-1|<1.2x10^{-5} and the temperature fluctuation |delta T|<(1.6-4.3)x10^{-5} are smaller than those by Tsallis et al. Moreover, analyzing the monopole spectrum by a formula including the chemical potential mu, we obtain the limits |q-1|<2.3x10^{-5} and |mu|<1.6x10^{-4}. |q-1| is comparable with the Sunyaev-Zeldovich effect y.

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