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criticisms of the einstein field equation - Alpha Institute for Advanced ...

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CHAPTER 2. A REVIEW OF EINSTEIN CARTAN EVANS (ECE) . . .<br />

2.13 Appendix 4: Standard Tensorial Formulation<br />

<strong>of</strong> <strong>the</strong> Homogeneous Maxwell Heaviside<br />

Field Equations<br />

The standard tensorial <strong>for</strong>mulation developed in this appendix is:<br />

∂µ F µν = ∂ µ Fµν = 0 (2.1)<br />

and is needed as a baseline <strong>for</strong> <strong>the</strong> development <strong>of</strong> ECE <strong>the</strong>ory. The <strong>field</strong> tensor<br />

is defined as:<br />

⎡<br />

⎤<br />

F µν =<br />

⎢<br />

⎣<br />

0 cB 1 cB 2 cB 3<br />

−cB 1 0 −E 3 E 2<br />

−cB 2 E 3 0 −E 1<br />

−cB 3 −E 2 E 1 0<br />

⎥<br />

⎦ . (2.2)<br />

where, in standard covariant - contravariant notation and in S.I. units:<br />

<br />

1 ∂ ∂ ∂ ∂<br />

∂µ = , , , ,<br />

c ∂t ∂X ∂Y ∂Z<br />

(2.3)<br />

∂ µ <br />

1 ∂ ∂ ∂ ∂<br />

= , − , − , − ,<br />

c ∂t ∂X ∂Y ∂Z<br />

(2.4)<br />

x µ = (ct, X, Y, Z), (2.5)<br />

xµ = (ct, −X, −Y, −Z). (2.6)<br />

The metric and inverse metric tensors in Minkowski space-time are equal, and<br />

are given by:<br />

gµν = g µν =<br />

⎡<br />

⎢<br />

⎣<br />

1 0 0 0<br />

0 −1 0 0<br />

0 0 −1 0<br />

0 0 0 −1<br />

⎤<br />

⎥<br />

⎦ . (2.7)<br />

Indices are raised and lowered with <strong>the</strong> metric, <strong>for</strong> example:<br />

where<br />

Fµν = gµρ gνσ F ρσ<br />

(2.8)<br />

g00 = 1, g11 = g22 = g33 = −1 (2.9)<br />

and so on. There<strong>for</strong>e:<br />

F01 = g00 g11F 01 = − F 01 , F02 = − F 02 , F03 = − F 03<br />

65<br />

(2.10)

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