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Interferometers...: Testing Relativistic Gravity in Space - download pdf or read online

By David P. Landau, Kurt Binder

ISBN-10: 0521842387

ISBN-13: 9780521842389

Lawsuits of a gathering on Gyros, Clocks, Interferometers...: checking out basic Relativity in area, held in undesirable Honnef from August 21-27, 1999. subject matters coated contain the Lense-Thirring impression, the detection of gravitational waves, trying out the equivalence precept, electromagnetic box and gravity, and clocks and rods in gravitational fields.

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Since S a is an axial vector and, according to (48) a rest–frame quantity, it is identified with the spin of the Dirac particle. 40 C. L¨ ammerzahl and G. Neugebauer Therefore, the only independent normalized quantities are the normalized current ˆj µ = ¯bγ µ b = v µ and the normalized spin–vector S µ = ¯bγ5 γ µ b. The propagation equations (46) for b and ¯b then give propagation equations for j µ and S µ : Dv v = 0 , Dv S = 0 . (52) (53) Therefore the direction of the spin is parallely propagated along the path of the Dirac particle.

30] resonator Wuppertal (microwaves) A. De Marchi [17] dynamic et al. free pendulum Torino Wei-Tou Ni Fabry–P´erot et al. [33] resonator Taiwan (optical) F. Nolting beam balance et al. [26] Z¨ urich H. Parks Fabry–P´erot et al. resonator Colorado (optical) J. P. Schwarz free fall et al. 6735 rel. 6873 1400 first results under construction working on improvements under construction published results The second technique is called force compensation method. A electromagnetic force is applied to the torsion pendulum in order to prevent the torsion fiber from twisting.

L¨ ammerzahl and G. Neugebauer Since M µν is symmetric, we must have P µ = mv µ with m := P 0 /v 0 . Therefore M µν = m v µ v ν , and, consequently, we get from (15) Dv (mv) = 0. From this and the fact that v is a normalized 4–velocity, g(v, v) = −1, we get Dv m = 0 which means that m is the mass of the particle which is constant. Then we also have the geodesic equation for the center–of–mass trajectory: Dv v = 0 . (20) The spinning particle. This kind of particle is defined by Tµρ d3 x = 0 and δxµ Tνρ d3 x = 0; all other moments vanish.

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Interferometers...: Testing Relativistic Gravity in Space by David P. Landau, Kurt Binder


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