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An analysis of recent measurements of the temperature of the cosmic microwave background radiation

1988; IOP Publishing; Volume: 331; Linguagem: Inglês

10.1086/166589

1538-4357

George F. Smoot, S. Levin, C. Witebsky, Giovanni De Amici, Yoel Rephaeli,

Cosmology and Gravitation Theories

view Abstract Citations (38) References (34) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS An Analysis of Recent Measurements of the Temperature of the Cosmic Microwave Background Radiation Smoot, George ; Levin, Steven M. ; Witebsky, Chris ; de Amici, Giovanni ; Rephaeli, Yoel Abstract This paper presents an analysis of the results of recent temperature measurements of the cosmic microwave background radiation (CMBR). The observations for wavelengths longer than 0.1 cm are well fitted by a blackbody spectrum at 2.74 +/- 0.02 K; however, including the new data of Matsumoto et al. the result is no longer consistent with a Planckian spectrum. The data are described by a Thomson-distortion parameter u = 0.020 +/- 0.002 and temperature 2.813 +/- 0.010 K at the 68% confidence level. Fitting the low-frequency data to a Bose-Einstein spectral distortion yields a 95% confidence level upper limit of 1.4 x 10^-2^ on the chemical potential μ_0_. These limits on spectral distortions place restrictions on a number of potentially interesting sources of energy release to the CMBR, including the hot intergalactic medium proposed as the source of the X-ray background. Publication: The Astrophysical Journal Pub Date: August 1988 DOI: 10.1086/166589 Bibcode: 1988ApJ...331..653S Keywords: Background Radiation; Black Body Radiation; Microwaves; Relic Radiation; Temperature Measurement; X Ray Sources; Distortion; Galactic Evolution; Intergalactic Media; Low Frequencies; Quantum Statistics; Thomson Scattering; Astrophysics; COSMIC BACKGROUND RADIATION; COSMOLOGY; X-RAYS: SOURCES full text sources ADS |