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A relativistic electromagnetism example
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This video shows an example of a particle moving in a uniform electric field.
1. First we use the classical law of motion: F=ma. According to this law uniform force means uniform acceleration, and the particle can reach the speed of light, and continue to accelerate. According to relativity, this can't be true.
2. The classical law can also be formulated: F=d/dt mv. Meaning: the change of momentum is proportional to the force. This works also in relativity, only this time the mass m is changing. It grows as the velocity grows. This makes it harder for it to increase its velocity further. This prevents it from ever reaching the speed of light.
3. Now we switch to a different point of view: an observer moving at 60% the speed of light to the left. This observer views the same scene, but from this point of view the particle and the hoop have an initial velocity of 60% the speed of light to the right. If we used the F=ma law, then the particle would have accelerated downwards, while v_x would remain at a steady 0.6. But with the relativistic law something different happens: the x momentum, m v_x, remains constant, because there's no force along the x direction. But m grows, so it means v_x diminishes. The hoop however floats steadily at 0.6, so the particle falls short. This can't be true of course, the second observer is watching the same scene: the particle should pass through the hoop.
4. The 4th scene fixes that. According to relativity, when we switch between points of view we should transform the electromagnetic field. In our example, this means the electric field grows by 25%, and a magnetic field shows up. The 'x' marks shown in the video are a common convention for a vector field pointing into the screen, along a Z axis that is not shown. The magnetic force is perpendicular to the magnetic field and to the particle's velocity. It provides just the right amount of pull along the x-axis to keep v_x steady.
5. The 5th scene is a sneak peek into visualization of tensors part 2, due in August.
1. First we use the classical law of motion: F=ma. According to this law uniform force means uniform acceleration, and the particle can reach the speed of light, and continue to accelerate. According to relativity, this can't be true.
2. The classical law can also be formulated: F=d/dt mv. Meaning: the change of momentum is proportional to the force. This works also in relativity, only this time the mass m is changing. It grows as the velocity grows. This makes it harder for it to increase its velocity further. This prevents it from ever reaching the speed of light.
3. Now we switch to a different point of view: an observer moving at 60% the speed of light to the left. This observer views the same scene, but from this point of view the particle and the hoop have an initial velocity of 60% the speed of light to the right. If we used the F=ma law, then the particle would have accelerated downwards, while v_x would remain at a steady 0.6. But with the relativistic law something different happens: the x momentum, m v_x, remains constant, because there's no force along the x direction. But m grows, so it means v_x diminishes. The hoop however floats steadily at 0.6, so the particle falls short. This can't be true of course, the second observer is watching the same scene: the particle should pass through the hoop.
4. The 4th scene fixes that. According to relativity, when we switch between points of view we should transform the electromagnetic field. In our example, this means the electric field grows by 25%, and a magnetic field shows up. The 'x' marks shown in the video are a common convention for a vector field pointing into the screen, along a Z axis that is not shown. The magnetic force is perpendicular to the magnetic field and to the particle's velocity. It provides just the right amount of pull along the x-axis to keep v_x steady.
5. The 5th scene is a sneak peek into visualization of tensors part 2, due in August.
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