Origin of FRW cosmology in slow-roll inflation from non-compact Kaluza-Klein theory

被引：6

作者：

Aguilar, EM

Bellini, M

机构：

[1] Univ Michoacana, Inst Fis & Matemat, Morelia 58040, Michoacan, Mexico

[2] Consejo Nacl Invest Cient & Tecn, RA-1033 Buenos Aires, DF, Argentina

[3] Univ Mar del Plata, Fac Ciencias Exactas & Nat, Dept Fis, RA-7600 Mar Del Plata, Argentina

来源：

EUROPEAN PHYSICAL JOURNAL C | 2004年 / 38卷 / 01期

关键词：

D O I：

10.1140/epjc/s2004-02024-y

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

Using a recently introduced formalism we discuss slow-roll inflation from Kaluza-Klein theory without the cylinder condition. In particular, some examples corresponding to polynomic and hyperbolic phi-potentials are studied. We find that the evolution of the fifth coordinate should be determinant for both the evolution of the early inflationary universe and the quantum fluctuations.

引用

页码：123 / 128

页数：6

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[21] The structure of the big bang from higher-dimensional embeddings [J].