Angular fluctuations in the cosmological microwave background in a universe with a cosmological constant

Details Angular fluctuations in the cosmological microwave background in a universe with a cosmological constant Angular fluctuations in the cosmological microwave background in a universe with a cosmological constant

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132..359b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. 359, 360.

Astronomy and Astrophysics

Astrophysics

13

Background Radiation, Big Bang Cosmology, Constants, Microwaves, Relic Radiation, Universe, Light Beams, Mathematical Models, Quasars, Red Shift

Scientific paper

The author investigates the temperature fluctuations of the cosmological background in a universe with a positive cosmological constant. Because of the geometry of light rays the angular δT/T can be quite different than in the standard model. As a result, the adiabatic scenario may be consistent with the observed upper limit on the microwave background even if Ω0h2 ⪉ 0.1.

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