A principle to determine the number (3+1) of large spacetime dimensions

@article{Rama2007APT,
  title={A principle to determine the number (3+1) of large spacetime dimensions},
  author={S. Kalyana Rama},
  journal={Physics Letters B},
  year={2007},
  volume={645},
  pages={365-368}
}
  • S. Rama
  • Published 6 October 2006
  • Physics
  • Physics Letters B
View PDF on arXiv
13 Citations
Background Citations
4

13 Citations

Citation Type

Citation Type

Non singular, bouncing M theory universe
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Non singular M theory universe in loop quantum cosmology—inspired models
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  • Physics
    General Relativity and Gravitation
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A class of LQC-inspired models for homogeneous, anisotropic cosmology in higher dimensional early universe
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We argue that de Sitter universes with a small cosmological constant are entropically favored to have three spatial dimensions. The conclusion relies on the causal-patch description of de Sitter…
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The bouncing evolution of an universe in Loop Quantum Cosmology can be described very well by a set of effective equations, involving a function sin x. Recently, we have generalised these effective…
Study of Early Universe in an M Theoretic Model
In this thesis we study early universe in the frame work of M theory. In particular We assume that the early universe is homogeneous, anisotropic, and is dominated by the mutually BPS 22'55'…
Quantum graphity: A model of emergent locality
Quantum graphity is a background-independent model for emergent macroscopic locality, spatial geometry and matter. The states of the system correspond to dynamical graphs on N vertices. At high…
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