Other
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308l..37m&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 308, Sept. 15, 1986, p. L37-L41. Research supported
Other
41
Background Radiation, Cosmic Rays, Microwaves, Quasars, Temperature Distribution, Absorption Spectra, Astronomical Spectroscopy, Big Bang Cosmology, Brightness Temperature, Line Spectra, Red Shift
Scientific paper
The authors present observations of C I lines in the z = 1.776 absorption-line system toward the QSO 1331+170 which indicate a 2σ upper limit of 0.67 on the N(3P1)/N(3P0) fine-structure population ratio. Even in the presence of other excitation mechanisms in C0, this value provides an upper limit of 16K on the cosmic microwave background (CMB) temperature at 0.61 mm at z = 1.776. Based on the present-day 2.7K blackbody spectrum for the CMB, the CMB temperature at z = 1.776 should be 7.5K according to the standard Big Bang model prediction.
Black John Harry
Chaffee Frederic H. Jr.
Foltz Craig B.
Meyer David M.
York Don G.
No associations
LandOfFree
An upper limit on the microwave background temperature at Z = 1.776 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with An upper limit on the microwave background temperature at Z = 1.776, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An upper limit on the microwave background temperature at Z = 1.776 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1291083