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

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Publication:373155
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DOI10.1016/j.physletb.2006.11.077zbMath1273.83196arXivhep-th/0610071OpenAlexW1988497233MaRDI QIDQ373155

S. Kalyana Rama

Publication date: 21 October 2013

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0610071

zbMATH Keywords

entropic principlefluctuations of spacetime geometry


Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) String and superstring theories; other extended objects (e.g., branes) in quantum field theory (81T30)


Related Items

A class of LQC-inspired models for homogeneous, anisotropic cosmology in higher dimensional early universe, Entropy of anisotropic universe and fractional branes, Non singular M theory universe in loop quantum cosmology-inspired models, Variety of \((d + 1)\) dimensional cosmological evolutions with and without bounce in a class of LQC-inspired models



Cites Work

  • Dimensionality in the Freund-Rubin cosmology
  • A stringy correspondence principle in cosmology
  • Self-gravitating fundamental strings and black holes
  • String gas cosmology
  • The holographic principle
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