Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-23T22:17:51.132Z Has data issue: false hasContentIssue false

SPACE–TIME STRUCTURE AND SPINOR GEOMETRY

Published online by Cambridge University Press:  01 October 2008

GEORGE SZEKERES
Affiliation:
School of Mathematics, University of New South Wales, Sydney 2052, Australia (deceased)
LINDSAY PETERS*
Affiliation:
Pacific Knowledge Systems, Australian Technology Park, Sydney 1430, Australia (email: [email protected])
*
For correspondence; e-mail: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The structure of space–time is examined by extending the standard Lorentz connection group to its complex covering group, operating on a 16-dimensional “spinor” frame. A Hamiltonian variation principle is used to derive the field equations for the spinor connection. The result is a complete set of field equations which allow the sources of the gravitational and electromagnetic fields, and the intrinsic spin of a particle, to appear as a manifestation of the space–time structure. A cosmological solution and a simple particle solution are examined. Further extensions to the connection group are proposed.

Type
Research Article
Copyright
Copyright © Australian Mathematical Society 2009

References

[1]Benn, I. M. and Tucker, R. W., An introduction to spinors and geometry with applications in physics (Adam Hilger, Bristol, 1987).Google Scholar
[2]Eddington, A. S., Relativity theory of protons and electrons (Cambridge University Press, Cambridge, 1935).Google Scholar
[3]Hehl, F. W., von der Heyde, P., Kerlick, G. D. and Nester, J. M., “General relativity with spin and torsion: foundation and prospects”, Rev. Modern Phys. 48 (1976) 393416.CrossRefGoogle Scholar
[4]Kibble, T. W. B., “Lorentz invariance and the gravitational field”, J. Math. Phys. 2 (1961) 212221.CrossRefGoogle Scholar
[5]Luehr, C. P., Rosenbaum, M., Ryan, M. P. Jr and Shepley, L. C., “Nonstandard vector connections given by nonstandard spinor connections”, J. Math. Phys. 18 (1976) 965970.CrossRefGoogle Scholar
[6]Lynch, J. T., “Stability of a Kahler-type neutrino-gravitational field”, Nuovo Cimento Soc. Ital. Fis. B 114 (1999) 11051120.Google Scholar
[7]Lynch, J. T., “General relativistic fields of an isolated spin-half charged particle near the spin axis with application to the rest-mass of the electron and positron”, Nuovo Cimento Soc. Ital. Fis. B 114 (1999) 11391156.Google Scholar
[8]Palatini, A., “Invariant deduction of the gravitational equations from the principle of Hamilton”, in Cosmology and gravitation (Bologna, 1979), Volume 58 of NATO Adv. Study Inst. Ser. B: Physics (Plenum, New York, London, 1980). (Translation from Italian by R. Hojman and C. Mukku of “Deduzione invariantiva delle equazioni gravitazionali dal principio di Hamilton”, Rend. Circ. Mat. Palermo. 43 (1919) 203.)Google Scholar
[9]Peters, L., “Solutions of field equations in general relativity with spinor connection”, Ph. D. Thesis, School of Mathematics, University of New South Wales, 1983.Google Scholar
[10]Schrödinger, E., Space-time structure (Cambridge University Press, Cambridge, 1950).Google Scholar
[11]Sciama, D. W., “The physical structure of general relativity”, Rev. Modern Phys. 36 (1964) 463469 1103 (erratum).CrossRefGoogle Scholar
[12]Szekeres, G., “Spinor geometry and general field theory”, J. Math. Mech. 6 (1957) 471517.Google Scholar
[13]Weyl, H., “Reine infinitesimalgeometrie”, Math. Z. 2 (1918) 384411.CrossRefGoogle Scholar