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|    Message 15,791 of 17,520    |
|    Lawrence Crowell to stargene    |
|    Re: Gravitational lensing of gravitons b    |
|    21 Aug 17 23:44:31    |
      From: goldenfieldquaternions@gmail.com              On Saturday, August 19, 2017 at 1:56:15 AM UTC-5, stargene wrote:       > Does gravitational lensing affect gravitons coming from distant       > sources?       >       > To ease visualization, I assume a straight line between (1) Observer,       > (2) Massive lensing object (~SMBH or galaxy), (3) a Distant source       > (~SMBH or galaxy). For photons, ideally, the angle of deflection       > witnessed by the observer is theta = 4GM / rc^2 , where G is the       > Newtonian gravitational constant, M the lensing mass, r the so-       > called "impact parameter" and c the speed of light.       >       > Since gravitons (which are generally posited to mediate gravitational       > interaction between two masses) interact with the grav=E2=80=99l field it=       self,       > not to mention with themselves (unlike other boson quanta), would       > their theta relation be different? Ie: If we could =E2=80=9Csee=E2=80=9D=        gravity,       > would we see a gravitational =E2=80=98ring=E2=80=99 similar to the Einste=       in Ring, and       > would it have the same angular distribution?       >       > If any distribution exists for gravitons, where could I find a good       > reference, and would it distinguish between gravitons of different       > energies?              You can think of a graviton in the weak field limit, where gravitons       do not interact with each other, as similar to a pair of photons       in an entangled triplet state. Just as this is lensed by a static       gravitational force, so too would a gravitational wave.              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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