Abstract
It is arguable that the most important scientific discovery of the 20th century is that one can discuss the whole universe in a rational way. After all, what could be more important than understanding everything that there is? The key technical tool which permits such a rational discussion is Einstein’s general theory of relativity. For the first time this theory provides us with the means to represent the layout of the universe in space and time in a manner which is also dynamically self consistent. Newtonian theory, with its emphasis on the fundamental role of world-wide inertial frames of reference, cannot do this. It is true that in the 1930’s so-called Newtonian models were constructed, bearing a close similarity to the relativistic models, but this was only possible if it was permitted for inertial frames centred on different points to be accelerating relative to one another. This is not strictly part of the Newtonian concept. Moreover, it was not possible to give a satisfactory discussion of the propagation of light in these Newtonian models, and since light (and radio waves) is the main tool of the astronomer in exploring the universe, this defect is catastrophic.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
A. Einstein, „Kosmologische Betrachtungen zur allgemeinen Relativitatstheorie“, Preuss. Akad. Wiss. Berlin, Sitzungsber. p. 142, 1917.
A. Einstein, as quoted by G. Gamow “My World Line”, p. 44 (Vilzing Press, New York) 1970.
A. Friedmann, „Uber die Kriimmung des Raumes“, Z. Phys. 10, p. 377, (1922).
E.P. Hubble, “NGC 6822 a remote stellar system”, Astrophys. J. 62, p. 409, (1925).
E.P. Hubble, “A relation between distance and radial velocity among extragalactic nebulae”, Proc. Nat. Acad. Sci. U.S. 15, p. 169, (1929).
E. P. Hubble, “The Realm of the Nebulae”, New Haven, Yale Univ. Press, 1936.
H.P. Robertson, “Kinematics and world structure”, Astrophys. J. 82, p. 248, (1935).
A. G. Walker, “On Riemannian spaces with spherical symmetry about a line and isotropy in general relativity”, J. Math. Oxford Ser. 6, 81 (1935).
A. Einstein, W. de Sitter, “On the relation between the expansion of the universe”, Proc. Nat. Acad. Sci. 18, 213 (1932).
H. Bondi und T. Gold, “The steady-state theory of the expanding universe”, Mon. Not. R. Astron. Soc. 108, p. 252 (1948).
F. Hoyle, “A new model for the expanding universe”, Mon. Not. R. Astron. Soc. 108, p. 372, (1948).
A. A. Penzias und R. W. Wilson, “A measurement of excess antenna temperature at 4080 Mc/s”, Astrophys. J. 142, p. 419 (1965).
R.H. Dicke, P.J. Peebles, P. G. Roll und D. T. Wilkinson, “Cosmic-black-body radiation”, Astrophys. J. 142, p. 414 (1965).
G. Gamow, “The evolution of the universe”, Nature 162, p. 680, (1948).
R.A. Alpher und R. C. Herman, “Evolution of the universe”, Nature 162, p. 774 (1948).
G.M. Smoot, M. V. Gorenstein und R. A. Midler, “Detection of anisotropy in the cosmic blackbody radiation”, Phys. Rev. Lett. 39, 14, p. 898 (1977).
S.W. Hawking und R. Penrose, “The singularity of gravitational collapse and cosmology”, Proc. R. Soc. London A 314, p. 529 (1969).
Editor information
Rights and permissions
Copyright information
© 1979 Friedr. Vieweg & Sohn Verlagsgesellschaft mbH, Braunschweig
About this chapter
Cite this chapter
Sciama, D.W. (1979). Cosmology. In: Aichelburg, P.C., Sexl, R.U. (eds) Albert Einstein. Vieweg+Teubner Verlag. https://doi.org/10.1007/978-3-322-91080-6_2
Download citation
DOI: https://doi.org/10.1007/978-3-322-91080-6_2
Publisher Name: Vieweg+Teubner Verlag
Print ISBN: 978-3-528-08425-7
Online ISBN: 978-3-322-91080-6
eBook Packages: Springer Book Archive