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Spin-two massless-particle radiation as a gravitational effect

โœ Scribed by R.H Good Jr.


Publisher
Elsevier Science
Year
1971
Tongue
English
Weight
506 KB
Volume
62
Category
Article
ISSN
0003-4916

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โœฆ Synopsis


The theory for a spin-two massless-particle field interacting with sources is developed, in parallel with Maxwell's theory for photons interacting with charges. In the spin-two case there are two fields Eij and &, which are symmetric traceless tensors of opposite parity. Whereas a Maxwell source must be a conserved current, the spin-two source is built up in a certain way from a conserved stress-energy-momentum tensor. Polarization effects of the radiation are much the same as for electromagnetic fields; there are plane polarized, circularly polarized, and intermediate cases possible. It is suggested that a nonrelativistic test object detects the radiation through the effect of the Eij field on the object's quadrupole and octupole moments.


๐Ÿ“œ SIMILAR VOLUMES


Massless spinning test particles in a gr
โœ Bahram Mashhoon ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 250 KB

The classical equations of motion of a massless spinning test particle are derived as a limiting case of Mathisson-Papapetrou equations. It is shown that when a particular supplementary condition is assumed the particle follows a null geodesic and the spin is either parallel or antiparallel to the d