I Distance between two light pulses

member 743765
If a source emits a light pulse then waited one second and sent another pulse does the distance between the two pulses remain constant ? If yes is that mean their relative speed is zero? But why when we use lorentz transformation their relative speeds gives us zero over zero but if they travel in opposite directions their relative speed is c which agrees with special relativity?
 
Physics news on Phys.org
phyahmad said:
If a source emits a light pulse then waited one second and sent another pulse does the distance between the two pulses remain constant ?
Yes, assuming they're going in the same direction.
phyahmad said:
If yes is that mean their relative speed is zero?
No. It means that the difference in their coordinate velocities in your chosen frame is zero, which means that it will be zero in all frames. I usually call this quantity "closing rate" or "separation rate", although I don't think there's a universally accepted term.

The relative velocity of two objects is the velocity measured by one of the other in the rest frame of the first one. Light does not have a rest frame, so "velocity relative to light" isn't defined.

Note that relative velocity and separation rate are always equal in Newtonian physics, but not relativity.
phyahmad said:
But why when we use lorentz transformation their relative speeds gives us zero over zero but if they travel in opposite directions their relative speed is c which agrees with special relativity?
Lorentz transforms to a frame with speed ##v=\pm c## are not defined. Thus derived formulae such as the velocity transform (which is what I think you are using here) are not valid. That's why you get contradictory answers when you plug in ##+c## and ##-c##.
 
Last edited:
  • Like
Likes Dale and member 743765
phyahmad said:
But why when we use lorentz transformation their relative speeds gives us zero over zero but if they travel in opposite directions their relative speed is c which agrees with special relativity?
It should be undefined regardless of the direction. Light doesn’t have an inertial rest frame. You may want to check your math with the Lorentz transform for the opposite direction case
 
  • Like
Likes member 743765
Ibix said:
Yes, assuming they're going in the same direction.
And that we are in flat spacetime (i.e., no gravitating masses are present) and are using an inertial frame.
 
phyahmad said:
But why when we use lorentz transformation their relative speeds gives us zero over zero but if they travel in opposite directions their relative speed is c which agrees with special relativity?
To follow up on this. The Lorentz transform to an inertial frame moving at velocity ##v## with respect to the unprimed inertial frame is $$ct'=\frac{c t- v x/c}{\sqrt{1-v^2/c^2}}$$$$x'=\frac{x-vt}{\sqrt{1-v^2/c^2}}$$ For an object traveling at velocity ##u## in the unprimed frame we get ##x=ut## which gives $$ct'=\frac{c t- v u t/c}{\sqrt{1-v^2/c^2}}$$$$x'=\frac{u t-vt}{\sqrt{1-v^2/c^2}}$$

So, for the "perspective of light" we would have ##v=c## which gives $$ct'=\frac{c t- u t}{\sqrt{1-c^2/c^2}}=\frac{c t- u t}{0}=undefined$$$$x'=\frac{u t-ct}{\sqrt{1-c^2/c^2}}=\frac{u t-ct}{0}=undefined$$ Regardless of ##u##
 
  • Like
Likes PeroK and member 743765
I asked a question here, probably over 15 years ago on entanglement and I appreciated the thoughtful answers I received back then. The intervening years haven't made me any more knowledgeable in physics, so forgive my naïveté ! If a have a piece of paper in an area of high gravity, lets say near a black hole, and I draw a triangle on this paper and 'measure' the angles of the triangle, will they add to 180 degrees? How about if I'm looking at this paper outside of the (reasonable)...
From $$0 = \delta(g^{\alpha\mu}g_{\mu\nu}) = g^{\alpha\mu} \delta g_{\mu\nu} + g_{\mu\nu} \delta g^{\alpha\mu}$$ we have $$g^{\alpha\mu} \delta g_{\mu\nu} = -g_{\mu\nu} \delta g^{\alpha\mu} \,\, . $$ Multiply both sides by ##g_{\alpha\beta}## to get $$\delta g_{\beta\nu} = -g_{\alpha\beta} g_{\mu\nu} \delta g^{\alpha\mu} \qquad(*)$$ (This is Dirac's eq. (26.9) in "GTR".) On the other hand, the variation ##\delta g^{\alpha\mu} = \bar{g}^{\alpha\mu} - g^{\alpha\mu}## should be a tensor...
Back
Top