A possibility to useCi infrared absorption lines for determination of the background radiation temperature at earlier cosmological epochs

Astrophysics and Space Science - Tập 105 - Trang 215-226 - 1984
I. E. Waltz1, V. K. Khersonskij1,2
1Space Research Institute of the USSR Academy of Sciences, Moscow, U.S.S.R.
2Leningrad Department of the Special Astrophysical Observatory of the USSR Academy of Sciences, Leningrad, U.S.S.R.

Tóm tắt

A method for the determination of the background radiation temperature in earlier cosmological epochs at redshiftsz>2 is discussed in detail. The method is based on the fact that in the clouds situated at cosmological distances at redshiftz the background radiation temperature must be (1+z) times more than in the modern epoch (z=0). This shall affect the level populations of the atoms, ions and molecules and, consequently, the parameters of the absorption lines observed in quasar absorption spectra. It is proposed to use the transition3 P 0−3 P 1 ofCi (λ=610 μ) for the measurement of the background radiation temperature. Atz>2 this absorption line shifts to the millimeter radio region and can be observed by radioastronomical methods.

Tài liệu tham khảo

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