Hostname: page-component-8448b6f56d-wq2xx Total loading time: 0 Render date: 2024-04-25T02:34:05.747Z Has data issue: false hasContentIssue false

IV.—On Properties of Null Geodesics, and their Application to the Theory of Radiation

Published online by Cambridge University Press:  15 September 2014

Get access

Extract

In a previous paper an expression was given by one of us for the Doppler effect in a de Sitter universe. In the present communication an attempt is made to obtain a more general expression for the Doppler effect, and for this purpose certain results have been derived relating to the properties of null geodesics in a general Riemannian space. In the paper referred to, the problem of defining spatial distance in general space was discussed and certain formulæ suggested which satisfy the essential conditions associated with the idea of spatial distance. This problem has now been approached from a different standpoint, and a new formula of more general form is now put forward. In the final section of the present paper a physical interpretation is given of the theorem relating to null geodesics which is proved in the first section. This involves a discussion of the concept of energy in general relativity, in order that a decision may be arrived at as to what law governs the transference of energy by radiation from one point to another. It appears that when the simplest and most natural assumptions are made for this purpose, then these are precisely the assumptions which are necessary to ensure the general consistency of relativity with the principles of quantum theory. This is illustrated by an application to a statical universe, and to the reddening of light in an expanding universe.

Type
Proceedings
Copyright
Copyright © Royal Society of Edinburgh 1934

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

page 31 note * Whittaker, E. T., Proc. Roy. Soc., A, vol. cxxxiii, 1931, pp. 93105.CrossRefGoogle Scholar

page 33 note * This theorem is a generalisation of a theorem proved by J. L. Synge and A. J. M'Connell, Phil. Mag., (7), vol. v, 1928, pp. 241–263. Their theorem (equation (5.5) of their paper) may be obtained as a particular case of the one given here by supposing that the points C, C′ are correlated to each other by the condition that a certain parameter is to have the same value at C′ as it has at C. Reference may also be made to a paper by C. Lanczos, Zs.f. Physik, vol. xvii, 1923, pp. 168–189.

page 35 note * Whittaker, E. T., Proc. Roy. Soc., A, vol. cxxxiii, 1931, pp. 93105.CrossRefGoogle Scholar

page 36 note * In a forthcoming paper it is proved by H. S. Ruse that this definition of spatial distance is precisely equivalent to that previously given by him, Proc. Roy. Soc. Edin., vol. lii, 1932, pp. 183–194.

page 38 note * H. S. Ruse, loc. cit., § 5.

page 42 note * Eddington, Mathematical Theory of Relativity, 1924 (2nd ed.), § 56.

page 46 note * O. Heckmann, Göttingen Nachr. (Math. Phys.), 1931, pp. 126–130.