bob012345 said:
Thanks. When I say something seems funny, I don't mean wrong or unphysical but rather surprising. For example, even though the highly relativistic rocket is almost 100% efficient converting most of the beam energy into rocket kinetic energy, the actual numbers were shocking. Adding a gigajoule has almost no effect at beta=0.99 but has a huge effect at low speeds even when the conversion is very inefficient.
Regarding the beam having less energy, in the Earth frame, I accounted for the energy with the redshift. That energy to the ship doesn't just evaporate. If we stick in that frame, the difference must go to the ship. I can see the acceleration and power go down but energy must be conserved.
This brings up a related question. I tried applying the work energy theorem in the relativistic regime. I have no problems with the relativistic kinetic energy difference but the integration force over distance got unwieldy. Then I realized than no books I have seen have relativistic kinematics covered. I don't mean Lorentz transformations, I mean in one frame where the acceleration changes for a fixed force because the mass increases. I couldn't match the integrated work with the change in relativistic energy.
A minor but important for communication nit:
wiki said:
Kinematics is the branch of
classical mechanics which describes the
motion of points (alternatively "particles"), bodies (objects), and systems of bodies without consideration of the masses of those objects nor the forces that may have caused the motion.
So I suspect you're bemoaning the lack of a good introductory textbook treatment of relativistic dynamics, something that treats forces & masses.
Most textbook treatments of relativistic forces that I've seen are fairly advanced, and use 4-vectors. You should be able to find a treatment of relativistic momentum and energy, though.
While it does not include a derivation of the results or explain the dyanamics, there's a good FAQ article with some equations for the relativistic rocket,
http://math.ucr.edu/home/baez/physics/Relativity/SR/Rocket/rocket.html, that might be of interest.
An approach I find useful for gaining insight is to take a detour into rapidity. See for instance the wiki article
https://en.wikipedia.org/wiki/Rapidity. I'm not sure if there's a good textbook treatment, I seem to recall that Rindler's textbook discussed it some (and it's cited in the wiki article). I think Rindler also treats the accelerated rocket, too, but I can't be certain, I don't have it handy to check. If you can track it down (interlibrary loan, perhaps) it's probably worth looking at, though I can't guarantee it'll answer your question. It's also not necessarily the most modern treatment.
One easy approach is to find the acceleration of the rocket in it's own frame. This is called the proper acceleration. This takes care of all the dynamics issues, once you know the acceleration of the rocket/mirror in its own frame, you can use the principles of kinematics to describe the motion of the rocket in the lab frame (though it may take a bit of work).
Because the rocket isn't moving in its own frame, one can use one's knowledge of Newtonian physics to work out the proper acceleration of the rocket. Once this is known, one can figure out the velocity using the idea of rapidity.
Rapidity, w, is defined as (see the wiki for instance, and I think Rindler's textbook?):
$$w = arctanh \, \beta = arctanh \, v/c$$
where w is the rapidity, v is the velocity, c is the speed of light, and ##\beta = v/c## is convenient (but not necessary), the ratio of v/c.
Because rapidites add, one can write:
$$w = a \tau$$
when the proper acceleration is constant, and when the proper accelration varies with (proper) time, one writes:
$$w(\tau) = \int a(\tau) d\tau$$
One still to find the proper acceleration a. If one consider a pulse of light with some momentum p, and it reflects off a mirror, one knows that the mirror gets a change in momentum of 2p. And it's important to realize that the invariant mass of the mirror (or solar sail + rocket) isn't changed by this process. One does need to know the energy and momentum of the light pulse in the rocket frame, though. So one needs to understand how the doppler shift changes the energy and momentum. One approach to this is to realize that energy and momentum transform via the Lorentz transform, i.e. as a 4-vector. One can possibly work around the need for doing this by figuring out how the frequency ##\nu## transforms and using ##E = h \nu##. One also needs to figure out their arrival rate of the pulses at the rocket/mirror (this is done with the relativistic doppler shift formula). Additionally, one needs to know that for light, E = pc.