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Groups > sci.physics.relativity > #359554 > unrolled thread
| Started by | RichD <r_delaney2001@yahoo.com> |
|---|---|
| First post | 2015-08-03 13:10 -0700 |
| Last post | 2015-08-04 15:50 +0000 |
| Articles | 5 — 4 participants |
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EM in warped space RichD <r_delaney2001@yahoo.com> - 2015-08-03 13:10 -0700
Re: EM in warped space John Heath <heathjohn2@gmail.com> - 2015-08-03 15:25 -0700
Re: EM in warped space John Heath <heathjohn2@gmail.com> - 2015-08-03 15:36 -0700
Re: EM in warped space Tom Roberts <tjroberts137@sbcglobal.net> - 2015-08-03 20:18 -0500
Re: EM in warped space Bohuš Matuška <bohu@paranetnet.net> - 2015-08-04 15:50 +0000
| From | RichD <r_delaney2001@yahoo.com> |
|---|---|
| Date | 2015-08-03 13:10 -0700 |
| Subject | EM in warped space |
| Message-ID | <ac9aedec-9881-4adf-b1be-adf754cbf1a6@googlegroups.com> |
I wonder, what happens to the Maxwell eqs., and the solutions, in a high gravity gradient, in GR? A diagram would be better, but anyway... postulate a G field which intensifies linearly in the x-direction; constant in y and z directions. Place a linear antenna, with circular symmetry in its gain, in this space. The antenna might be oriented along the x axis, or alternatively, along the y axis. What does the radiated wave look like? It's basically a schoolboy problem. Can somebody run out and find me a schoolboy? -- Rich
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| From | John Heath <heathjohn2@gmail.com> |
|---|---|
| Date | 2015-08-03 15:25 -0700 |
| Message-ID | <d1a6a305-e7f1-4b52-8515-7e248fdc16c1@googlegroups.com> |
| In reply to | #359554 |
Hi Richard Good question. I see this as similar to the position offset of stars close to the sun in the famous Einstein experiment. In this case the photons were falling into the sun's gravity offsetting their perceived position. As this test was successful it can be assumed the same would happen in your experiment. As the g field intensifies linearly in the x-direction a round EM field should be egg shaped with the pointed end in the direction of the increasing gravitational field when viewed at right angles from the X or y direction.The buzz word for an intensifying gravitational field is gravity gradient. This is similar to another question you had regarding time dilation from the center of the earth to outer space. I have a nifty graph that plots this out in detail and including both SR and GR time dilation from the center of earth to well out into space. Will have to find the link in another post so it will come later. On Monday, August 3, 2015 at 4:10:59 PM UTC-4, RichD wrote: > I wonder, what happens to the Maxwell eqs., and > the solutions, in a high gravity gradient, in GR? > > A diagram would be better, but anyway... postulate > a G field which intensifies linearly in the x-direction; > constant in y and z directions. > > Place a linear antenna, with circular symmetry in > its gain, in this space. The antenna might be > oriented along the x axis, or alternatively, along > the y axis. What does the radiated wave look like? > > It's basically a schoolboy problem. > Can somebody run out and find me a schoolboy? > > > -- > Rich
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| From | John Heath <heathjohn2@gmail.com> |
|---|---|
| Date | 2015-08-03 15:36 -0700 |
| Message-ID | <6ae03e2f-f789-4394-adb4-abba81060db3@googlegroups.com> |
| In reply to | #359572 |
There ya go http://tinyurl.com/pzvvf42 On Monday, August 3, 2015 at 6:25:08 PM UTC-4, John Heath wrote: > Hi Richard > > Good question. I see this as similar to the position offset of stars close to the sun in the famous Einstein experiment. In this case the photons were falling into the sun's gravity offsetting their perceived position. As this test was successful it can be assumed the same would happen in your experiment. As the g field intensifies linearly in the x-direction a round EM field should be egg shaped with the pointed end in the direction of the increasing gravitational field when viewed at right angles from the X or y direction.The buzz word for an intensifying gravitational field is gravity gradient. This is similar to another question you had regarding time dilation from the center of the earth to outer space. I have a nifty graph that plots this out in detail and including both SR and GR time dilation from the center of earth to well out into space. Will have to find the link in another post so it will come later. > > On Monday, August 3, 2015 at 4:10:59 PM UTC-4, RichD wrote: > > I wonder, what happens to the Maxwell eqs., and > > the solutions, in a high gravity gradient, in GR? > > > > A diagram would be better, but anyway... postulate > > a G field which intensifies linearly in the x-direction; > > constant in y and z directions. > > > > Place a linear antenna, with circular symmetry in > > its gain, in this space. The antenna might be > > oriented along the x axis, or alternatively, along > > the y axis. What does the radiated wave look like? > > > > It's basically a schoolboy problem. > > Can somebody run out and find me a schoolboy? > > > > > > -- > > Rich
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| From | Tom Roberts <tjroberts137@sbcglobal.net> |
|---|---|
| Date | 2015-08-03 20:18 -0500 |
| Message-ID | <9oudnfdXI7hjj13InZ2dnUU7_82dnZ2d@giganews.com> |
| In reply to | #359554 |
On 8/3/15 8/3/15 3:10 PM, RichD wrote: > I wonder, what happens to the Maxwell eqs., and > the solutions, in a high gravity gradient, in GR? Here are Maxwell's equations in flat spacetime, written in the language of differential forms: dF = 0 *d*F = J Here d is the exterior derivative, * is the Hodge dual operator, F is the Maxwell 2-form, and J is the current 1-form. In terms of the electromagnetic potential 1-form A: F = dA Here are the corresponding Einstein-Maxwell equations in curved spacetime such that the energy density of the EM fields is negligible (compared to other mass/energy that determines the geometry): dF = 0 *d*F = J Yes, they are the same, including the meanings of all the symbols. This shows the advantages of using advanced mathematics: the usual 4 Maxwell's equations become two equations, the two equations relating E and B to A and \phi become a single equation, and the equations are valid in curved manifolds. > A diagram would be better, but anyway... postulate > a G field which intensifies linearly in the x-direction; > constant in y and z directions. > > Place a linear antenna, with circular symmetry in > its gain, in this space. The antenna might be > oriented along the x axis, or alternatively, along > the y axis. What does the radiated wave look like? Assuming that the energy density of the EM source and field is negligible compared to the mass/energy that determines the geometry of the manifold, and assuming weak gravitation (e.g. as in the solar system), the EM wave will be Doppler shifted in frequency and wavelength, in the usual way. As the EM field is continuous, this Doppler shift in the wavelength implies a corresponding "bending" of the direction of propagation in suitable circumstances. Tom Roberts
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| From | Bohuš Matuška <bohu@paranetnet.net> |
|---|---|
| Date | 2015-08-04 15:50 +0000 |
| Message-ID | <mpqn07$8vs$1@speranza.aioe.org> |
| In reply to | #359582 |
Tom Roberts wrote: > On 8/3/15 8/3/15 3:10 PM, RichD wrote: >> I wonder, what happens to the Maxwell eqs., and the solutions, in a >> high gravity gradient, in GR? > > Here are Maxwell's equations in flat spacetime, written in the language > of differential forms: > dF = 0 *d*F = J > Here d is the exterior derivative, * is the Hodge dual operator, F is > the Maxwell 2-form, and J is the current 1-form. In terms of the > electromagnetic potential 1-form A: > F = dA > > > Here are the corresponding Einstein-Maxwell equations in curved > spacetime such that the energy density of the EM fields is negligible > (compared to other mass/energy that determines the geometry): > dF = 0 *d*F = J > Yes, they are the same, including the meanings of all the symbols. No, they are not the same. The former was Maxwell, the later Einstein is added to it: Einstein-Maxwell.
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