Understand
We begin with the time-dependent electric and magnetic dipole solution of Maxwell's equations in Minkowski space.
- This Maxwell field is then used to determine the behavior of the gravitational field (the Weyl tensor) as a second-order perturbation off of the Minkowski background.
- From the Weyl tensor we go on and find the spin-coefficients and the full metric in this approximation.
- The physical meaning of many of the relations is discussed.
Built on
Newman, E., Penrose, R., Journal of Mathematical Physics, 3
1962
Earlier work this paper cites.
Bondi, H., van de Burg, M.G.J., Metzner, A.W.K. Proc. Roy. Soc., London Ser
1962
Earlier work this paper cites.
Landau, L. and Lifschitz, E. M., Classical Theory of Fields,
1962
Earlier work this paper cites.
Newman, E.T., Tod, K.P. , in General Relativity and Gravitation, Vol. 2
1980
Earlier work this paper cites.
Similar
Newman, E.T., Classical and Quantum Gravity, 21
2004
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Bramson, B., Proceedings of the Royal Society,
2006
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Kozameh, C., Newman, E.T., Silva-Ortigoza, G., Classical and Quantum Gravity, 23
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Then
Newman, E.T. ,Silva-Ortigoza, G., Classical and Quantum Grav
2006
Later among the works it cites.
Kozameh, C., Newman, E.T., Silva-Ortigoza, G., Classical and Quantum Gravity, 24
2007
Later among the works it cites.
Kozameh, C., Newman, E.T., Silva-Ortigoza, G., Classical and Quantum Gravity,
2008
Closest in time.
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