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Open AccessJournal ArticleDOI

Fantappiè's group as an extension of special relativity on ε (∞) Cantorian space-time

Gerardo Iovane, +2 more
- 01 Dec 2004 - 
- Vol. 22, Iss: 5, pp 975-983
TLDR
In this article, the authors analyze the Fantappie group and its properties in connection with Cantorian space-time, focusing on the possibility of extending special relativity and the cosmological consequences of such extension appear relevant, since the model of the Big Bang and that of stationary state become compatible.
Abstract
In this paper, we will analyze the Fantappie group and its properties in connection with Cantorian space–time. Our attention will be focused on the possibility of extending special relativity. The cosmological consequences of such extension appear relevant, since thanks to the Fantappie group, the model of the Big Bang and that of stationary state become compatible. In particular, if we abandon the idea of the existence of only one time gauge, since we do not see the whole Universe but only a projection, the two models become compatible. In the end we will see the effects of the projective fractal geometry also on the galactic and extra-galactic dynamics.

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Citations
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Gravitation and spacetime.

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TL;DR: In this article, the authors propose some cosmological reflections at the qualitative and conjectural level, suggested by the Fantappie-Arcidiacono projective relativity theory.
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Archaic Universe and Cosmological Model: “Big-Bang” as Nucleation by Vacuum

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Fractional dynamics, fractional weak bosons masses and physics beyond the standard model

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El Naschie Ε-Infinity Cantorian Space-time, Fantappie's Group and Applications in Cosmology

TL;DR: In this article, the cosmological consequences of such extension appear relevant, since thanks to the Fantappie group, the model of the Big Bang and that of stationary state become compatible, in particular if we abandon the idea of the existence of only one time gauge, since we do not see the whole Universe but only a projection.
References
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Journal ArticleDOI

A new type of isotropic cosmological models without singularity

TL;DR: In this paper, the Einstein equations with quantum one-loop contributions of conformally covariant matter fields are shown to admit a class of nonsingular isotropic homogeneous solutions that correspond to a picture of the universe being initially in the most symmetric (de Sitter) state.
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TL;DR: In this article, the Robertson-Walker Metric is used to measure the radius of the Planck Epoch in the expanding universe, which is a measure of the number of atoms in the universe.
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The Emperor's New Mind

Roger Penrose
TL;DR: Aixi et al. as mentioned in this paper describe a massa gelada d'aigua consisting of a cabellera and a cua, which is composed of elements from the massa.
Journal ArticleDOI

Relativity in space-times with short distance structure governed by an observer independent (Planckian) length scale

TL;DR: In this paper, it was shown that it is possible to formulate the Relativity postulates in a way that does not lead to inconsistencies in the case of spacetimes whose short-distance structure is governed by an observer-independent length scale.
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