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Re: Comparison of Gravitational waves with EM waves |
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| Jan26-06, 06:28 PM | #1 |
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Re: Comparison of Gravitational waves with EM waves
On Mon, 12 Dec 2005 ianparker2@gmail.com wrote:
> Maxwells Equations (spin = 1) state that the electric field is at right > angles to the direction of motion. A gravitational field can be along > the direction of motion. Moreover the tensor equations are quadrupolar. > If they were dipolar (Maxwell) the Earth could only circle the Sun for > 100 Million years. (30km/s = c/10,000). > > One year's Nobel prize for Physics was one by measuring the slowdown in > pulsar transmissions. It fitted a quadupolar model to 10-15%. I think you meant to say something like this: Maxwell's theory of EM predicts the existence of electromagnetic radiation which propagates as transverse waves at the speed of light, with polarization properties loosely described as spin-1. The strongest type of EM radiation in this theory is dipole radiation. Gtr predicts the existence of gravitational radiation which propagates as transverse waves at the speed of light, with polarization properties loosely described as spin-2. The strongest type of radiation in this theory is quadrupole radiation. Russell Hulse and Joseph Taylor were awarded the 1993 Nobel Prize in Physics for their observations of the remarkable binary pulsar PSR B1913+16, which they discovered in 1974. Their observations are consistent with the gtr prediction that gravitational radiation should carry off energy at a certain rate from this system, leading to orbital decay at a certain rate. This consistitutes an indirect confirmation of the existence of gravitational radiation. Other theories also predict such radiation. However, the LIGO/VIRGO/GEO interferometric detectors are designed to directly verify the existence of gravitational radiation, and they, with LISA (a proposed spaceborne detector) should give much information about their properties. This might confirm other gtr predictions while ruling out some alternatives (which predict different properties for gravitational waves), but more important, it might eventually lead to a new field of gravitational wave astronomy which should neatly complement electromagnetic astronomy. Your comment "a gravitational field can be along the direction of motion" might be a garbled version of something D'Inverno mentions about Petrov III versus Petrov N vacuum gravitational fields, but one should probably focus first on the basics: the linearized gtr treatment of weak gravitational waves in Minkowski vacuum background. "T. Essel" |
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