v 2 1 7 Se p 20 03 M . W . Kalinowski ( Higher Vocational State School in Che lm , Poland ) On some Cosmological Consequences
نویسنده
چکیده
In the paper we consider some consequences of the Nonsymmetric Kaluza–Klein (Jordan–Thiry) Theory. We calculate primordial fluctuation spectrum functions, spectral indices, and first derivatives of spectral indices. In this paper we develop some ideas from Ref. [1]. We will refer to Ref. [1] in all the details of our considerations. Let us consider Eq. (3.313) from Ref. [1]. Φ(t) = (5 + 3a) √ 5 + 4a 8αs(A1 ns2(u) +A2) + ( 1 + √ 5 + 4a ) 2αs (1)
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متن کامل2 00 3 M . W . Kalinowski ( Higher Vocational State School in Che lm , Poland )
We consider a dynamics of Higgs’ field in the framework of cosmological models involving a scalar field Ψ from Nonsymmetric Kaluza–Klein (Jordan–Thiry) Theory. The field Ψ plays here a rôle of a quintessence field. We consider phase transition in cosmological models of the second and of the first order due to evolution of Higgs’ field. We developed inflationary models including calculation of a...
متن کامل2 00 3 M . W . Kalinowski ( Higher Vocational State School in Che lm , Poland ) On some
In the paper we consider some consequences of the Nonsymmetric Kaluza–Klein (Jordan–Thiry) Theory. We calculate primordial fluctuation spectrum functions, spectral indices, and first derivatives of spectral indices. In this paper we develop some ideas from Ref. [1]. We will refer to Ref. [1] in all the details of our considerations. Let us consider Eq. (3.313) from Ref. [1]. Φ(t) = (5 + 3a) √ 5...
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