• Corpus ID: 45133544

# Einstein ’ s Static Universe : An Idea Whose Time Has Come Back ?

@inproceedings{Segal2000EinsteinS,
title={Einstein ’ s Static Universe : An Idea Whose Time Has Come Back ?},
author={Irving Ezra Segal},
year={2000}
}
W hat is the shape of space? Is the universe finite or infinite? Did the world have a beginning, or has it always existed? These fundamental questions have intrigued and baffled humans since the most ancient times. But it was only in the twentieth century, with the development of powerful tools for probing the immensity of the skies, that it became possible to explore the cosmos beyond our galaxy’s neighborhood. Concurrently, advances in physics and mathematics provided the conceptual framework…
3 Citations
• Omid Makhmali
• Mathematics
Symmetry, Integrability and Geometry: Methods and Applications
• 2018
This article is concerned with causal structures, which are defined as a field of tangentially non-degenerate projective hypersurfaces in the projectivized tangent bundle of a manifold. The local
A solution to the more than 300-years old problem of geometric and physical interpretation of fractional integration and dieren tiation (i.e., integration and dieren tiation of an arbitrary real
Irving Ezra Segal (1918-1998) has proposed some axioms for mathematical cosmology. These are here re-examined and Segal's redshift formula and energy conservation in the Einstein universe are

## References

SHOWING 1-10 OF 14 REFERENCES

• Physics
• 1973
The theory of the causal structure of a general space-time is developed, and is used to study black holes and to prove a number of theorems establishing the inevitability of singualarities under certain conditions.
• Physics
• 1997
We test and reject the claim of Segal and coworkers that the correlation of redshifts and flux densities in a complete sample of IRAS galaxies favors a quadratic redshift-distance relation over the
• I. Segal
• Physics
Proceedings of the National Academy of Sciences of the United States of America
• 1976
The derivation of the redshift (z)-distance (r) relation in the chronometric theory of the Cosmos is amplified and this deviation and the (quantum) dispersion in redshift are shown to be unobservably small.
• Physics
• 1992
This paper presents an easily applied permutation test for H0, closely related to Lyden-Bell's (1971) estimate of the marginal distribution of truncated data. The test is applied to two
All tensors of contravariant valency two, which are divergence free on one index and which are concomitants of the metric tensor, together with its first two derivatives, are constructed in the
Es ist wohlbekannt, das die Poissonsche Differentialgleichung $$\Delta \phi = 4\pi K\varrho$$ (1) in Verbindung mit der Bewegungsgleichung des materiellen Punktes die Newtonsche
• Physics
• 1993
The local redshift-distance (z-r) power laws, z∞r p , of exponents p=1, 2, which are predicted respectively by generic big bang cosmology and chronometric cosmology, are tested on flux- and