Review of cosmic background radiation spectrum measurements: limits on distortions, energy release, and cosmological processes
Abstract
This paper reviews the three major cosmic microwave background radiation (CMBR) spectrum measurement programs conducted and published since the last (XVII) IAU General Assembly. The results are consistent with a Planckian spectrum with temperature 2.72 +- 0.03 K spanning a wavelength range of 0.1 to 12 cm. Limits on possible distortions and implications are outlined. Ongoing and future measurements are discussed.
- Authors:
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- U.S. Department of Energy (DOE)
- OSTI Identifier:
- 6061411
- Report Number(s):
- LBL-20942; CONF-8511151-2
ON: DE86007487
- DOE Contract Number:
- AC03-76SF00098
- Resource Type:
- Conference
- Resource Relation:
- Conference: International Astronomical Union meeting, New Delhi, India, 17 Nov 1985
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; RELICT RADIATION; SPECTRA; CYANIDES; EXPERIMENT PLANNING; PLANCK RADIATION FORMULA; ULTRALOW TEMPERATURE; ELECTROMAGNETIC RADIATION; MICROWAVE RADIATION; PLANNING; RADIATIONS; Astrophysics; Cosmology; Cosmic Radiation; 640101* - Astrophysics & Cosmology- Cosmic Radiation
Citation Formats
Smoot, G F. Review of cosmic background radiation spectrum measurements: limits on distortions, energy release, and cosmological processes. United States: N. p., 1986.
Web.
Smoot, G F. Review of cosmic background radiation spectrum measurements: limits on distortions, energy release, and cosmological processes. United States.
Smoot, G F. 1986.
"Review of cosmic background radiation spectrum measurements: limits on distortions, energy release, and cosmological processes". United States. https://www.osti.gov/servlets/purl/6061411.
@article{osti_6061411,
title = {Review of cosmic background radiation spectrum measurements: limits on distortions, energy release, and cosmological processes},
author = {Smoot, G F},
abstractNote = {This paper reviews the three major cosmic microwave background radiation (CMBR) spectrum measurement programs conducted and published since the last (XVII) IAU General Assembly. The results are consistent with a Planckian spectrum with temperature 2.72 +- 0.03 K spanning a wavelength range of 0.1 to 12 cm. Limits on possible distortions and implications are outlined. Ongoing and future measurements are discussed.},
doi = {},
url = {https://www.osti.gov/biblio/6061411},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Wed Jan 01 00:00:00 EST 1986},
month = {Wed Jan 01 00:00:00 EST 1986}
}
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