Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'504'585
Articles rated: 2609

24 April 2024
 
  » arxiv » math.HO/0506395

 Article overview



Pseudospheres in geometry and physics: from Beltrami to De Sitter and beyond
B. Bertotti ; R. Catenacci ; C. Dappiaggi ;
Date 20 Jun 2005
Subject History and Overview; Mathematical Physics | math.HO gr-qc math-ph math.MP
AffiliationU. Pavia), R. Catenacci (U. Piemonte Orientale), C. Dappiaggi (U. Pavia and INFN - Sezione di Pavia
AbstractWe review the extraordinary fertility and proliferation in mathematics and physics of the concept of a surface with constant and negative Gaussian curvature. In his outstanding 1868 paper Beltrami discussed how non-Euclidean geometry is actually realized and displayed in a disk on the plane. This metric is intrinsically defined and definite but only if indefinite metrics are introduced it is possible to fully understand the structure of pseudospheres. In a 3D flat space R^3 the fundamental quadric is introduced, with the same signature as the metric of R^3; this leads to 3 kinds of surfaces with constant Gaussian curvature: the sphere, the single-sheet hyperboloid and the two-sheet hyperboloid; the last one is shown to be isomorphic to Beltrami’s disk. The spacetime corresponding to the single-sheet case is de Sitter cosmological model, which, due to its symmetry, has an important role in cosmology. When two of the three fundamental quadrics are combined, a simple, yet deep, solution of Einstein-Maxwell equations corresponding to a uniform electromagnetic field is obtained with many applications in mathematical physics. One of them is a "no go" theorem: when one tries to frame a Riemannian four-dimensional manifold in a Kahlerian structure, it is found that, while this is generically possible with a definite signature, in spacetime only BR fulfills the requirement. The BR metric plays an important role in the exploration of new principles in fundamental physical theories; we briefly mention some examples related to the horizon of a black hole and the dilaton in string theory.
Source arXiv, math.HO/0506395
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica