Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths.

Details Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths. Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...302..635d&link_type=abstract

Astronomy and Astrophysics, v.302, p.635

Astronomy and Astrophysics

Astrophysics

20

Chaos, Radio Lines: General

Scientific paper

The formation of spectral disturbances of Cosmic Background Radiation (CBR) by hydrogen recombination at redshift z=1500 is considered. Special attention is paid here to the decimeter and meter wavelength bands. The most distinctive properties of spectral disturbances are an increase in amplitude with wavelength, followed by a decrease intensity of CBR and an increasing asymmetry of the contours of separate lines. It is shown, that it might be possible from their observations to determine the average density of barion and the average total density of matter in the Universe with great accuracy.

Affiliated with

Also associated with

No associations

Rating

Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths. 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 Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fossil radio lines of hydrogen in the cosmic background radiation at decimeter and meter wavelengths. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1351277