2002
DOI: 10.1142/s0218271802001834
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Chaotic Inflation With Time-Variable Space Dimensions

Abstract: Assuming the space dimension is not constant but decreases during the expansion of the Universe, we study chaotic inflation with the potential m 2 φ 2 /2. Our investigations are based on a model Universe with variable space dimensions. We write down field equations in the slow-roll approximation, and define slow-roll parameters by assuming the number of space dimensions decreases continuously as the Universe expands. The dynamical character of the space dimension shifts the initial and final value of the infla… Show more

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Cited by 5 publications
(40 citation statements)
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“…The reader can find the answers of these questions in detail in Refs. [2,3]. It is worth mentioning that for generalization of Friedmann equations from three-space to variable space dimension, we cannot define a metric approach.…”
Section: Review Of Model Universe With Variable Space Dimensionmentioning
confidence: 99%
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“…The reader can find the answers of these questions in detail in Refs. [2,3]. It is worth mentioning that for generalization of Friedmann equations from three-space to variable space dimension, we cannot define a metric approach.…”
Section: Review Of Model Universe With Variable Space Dimensionmentioning
confidence: 99%
“…As shown in [2], for different values of C, corresponding to the space dimension at the Planck length D P = 4, 10, 25 and +∞, we calculated the e-folding number N ∼ 69, 98, 116 and 132, respectively. Using the number of e-foldings, we have also obtained the size of the Universe at the onset of inflation, a i , see Table 1.…”
Section: Review Of Model Universe With Variable Space Dimensionmentioning
confidence: 99%
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