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(not exact)]] In Physics , Light loses Energy when it moves away from a massive body such as a star or a black hole. This effect reveals itself as a Gravitation al Redshift in the frequency of the light, and is observable as a shift of spectral lines towards the red end of the spectrum. Light coming from a region of weaker gravity shows a gravitational Blueshift . DEFINITION Background knowledge the reader may need to learn: What is Wavelength ? What is Frequency ? What is the Electromagnetic Spectrum ? Gravitational redshift is often denoted as the variable ''z''. Where: is the wavelength of the photon as measured by a distant observer. is the wavelength of the photon when measured at the source of emission. Gravitational redshift, the displacement of light towards the red, can be predicted using the formula provided in the theory of General Relativity ''(Albert Einstein: Relativity - Appendix - Appendix III - The Experimental Confirmation of the General Theory of Relativity)'': Where: is the displacement of spectral lines due to gravity as viewed by a far away observer in free space. is Netwon's Gravitational Constant (the variable used by Einstein himself). is the mass of the body which the light is escaping. is the speed of light. is the radial distance from the center from which the light originates. HISTORY The gravitational weakening of light from high-gravity stars was predicted by ). The effect of gravity on light was then explored by Laplace and Johann Georg Von Soldner (1801) before Einstein rederived the idea from scratch in his 1911 paper on light and gravitation. Einstein was accused by Lenard of plagiarism for not citing Soldner's earlier work - however, given that the idea had fallen so far into obscurity before Einstein resurrected it, it is entirely possible that Einstein was unaware of all previous work on the subject. In any case, Einstein went further and pointed out that a key consequence of gravitational shifts was Gravitational Time Dilation . This was a genuinely new and revolutionary idea. IMPORTANT THINGS TO STRESS
INITIAL VERIFICATION The Pound-Rebka Experiment of 1969 demonstrated the existence of gravitational redshift in spectral lines. This was documented by scientists of the Lyman Laboratory of Physics at Harvard University. APPLICATION Gravitational redshift is studied in many areas of Astrophysical research. EXACT SOLUTIONS A table of exact solutions for gravitational redshift consists of the following: The more often used exact solution is for gravitational redshift of non-rotating, uncharged masses which are spherically symmetric. The equation for this is: , where
GRAVITATIONAL REDSHIFT VS. GRAVITATIONAL TIME DILATION When using '' Special Relativity 's Relativistic Doppler relationships'' to calculate the change in energy and frequency (assuming no complicating Route-dependent effects such as those caused by the Frame-dragging of Rotating Black Holes ), then the Gravitational redshift and Blueshift frequency ratios are the inverse of each other, suggesting that the "seen" frequency-change corresponds to the Actual Difference In Underlying Clockrate . Route-dependence due to Frame-dragging ''may'' come into play, which invalidates this method and makes establishing globally-agreed differences in ''underlying'' clockrate can be more ''difficult'' though not necessarily impossible. While gravitational redshift refers to what is seen, Gravitational Time Dilation refers to what is deduced to be "really" happening once observational effects are taken into account. GENERAL RELATIVITY FOR EXPERTS Readers who are experts or students of GR may be interested in the Null Geodesic article and an article about Exact Solutions In General Relativity . PRIMARY SOURCES Einstein, Albert. "Relativity : the Special and General Theory." Project Gutenberg. |
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