3 ms·
Neat, thank you for posting this. It is nicely organized, and while most HN readers would find §2 pretty steep, the content of §2.1.4 (Massless particles), §2.
by raattgift 5y ago
Neat, thank you for posting this.
It is nicely organized, and while most HN readers would find §2 pretty steep, the content of §2.1.4 (Massless particles), §2.3.2 (Geodesics and affine parameters) and §2.3.4 (Massless particles and the Speed of Light) are concise technical answers to a HN FAQ which is essentially "according to relativity, do photons experience no time?". Really frequently "asked". (tl;dr answer: yes, they certainly do, you just write their "time" down differently from that of massive particles. The difference in their time ("affine time") tells you observable things -- for instance the difference in quantum wavefunction phase, or the difference in redshift, just as does the difference in proper time for electron (anti)neutrinos when e.g. leaving the cores of stars or neutron stars, or traversing cosmological distances).
(The missing pieces here are defining a momentum p^\mu = \dot X^\mu where the \dot is the derivative with respect to the affine time, much as the author has actually done in §2.3.3 (Massive Particles), and one of the energy-momentum relations like de Broglie's E = hc / \lambda or \lambda = h / p).
§2.3.5 is another good trio of answers to the HN FAQ about the twin paradox, and I agree with the author that the geodesic analysis is more attractive, namely "both Alice and Bob's paths in spacetime begin and end at the same point, but Alice follows a timelike geodesic, while Bob follows a timelike path which is not a geodesic" (emphasis mine). "Since timelike geodesics are exactly the timelike paths which maximize proper time, the proper time experienced by Alice must be larger than the proper time experienced by Bob. Therefore, Alice must be the older twin." That's really all it takes to resolve the apparent paradox. (However, c.f. "Too Many Analyses" in the excellent <https://math.ucr.edu/home/baez/physics/Relativity/SR/TwinParadox/twin_vase.html https://math.ucr.edu/home/baez/physics/Relativity/SR/TwinPar...>).
I'm slightly surprised that in skimming the later sections (which I plan to peruse) I did not notice the author discussing the <https://en.wikipedia.org/wiki/Causality_conditions https://en.wikipedia.org/wiki/Causality_conditions> and the causal ladder discussed therein, and only engaged directly with with (in §3.1.3) global hyperbolicity, although some of the many references in §7 might. I suppose that at 60ish pages the author did not want to commit into turning an extensive set of lecture notes into a comprehensive textbook, which is fine.
Finally, it has been several years since Bob Geroch's "democracy of causal cones" Faster Than Light? paper <https://arxiv.org/abs/1005.1614 https://arxiv.org/abs/1005.1614>, and exposure to that likely would affect the end of this paper's §4.3 ("Tachyons and Time Travel") which deals specifically with faster-than-light.
P.S.: (2019)
- cygx 5y agoI'd also add Recami's Tachyon Kinematics and Causality: A Systematic Thorough Analysis of the Tachyon Causal Paradoxes to the reading list. However, as this is a paper from the 80s, it's probably only available behind a paywall...
- raattgift 5y agoThanks, added to the reading list. The 1980s typesetting is fun to see. Skimming quickly through, the Wheelerian text around eq (53) is fascinating, although I think I prefer an ADM-ish IV approach to thinking about the spacetime "suffering" from objects with these worldtubes, and thinking about the presence of a researcher reading a book by candlelight, all of which has worldlines similar to what is discussed in that part of Recami's paper. In that approach, a "Eulerian" snapshot observer notes two "copies" of the researcher on some slice, each with different candle-sizes and page numbers, while a more patient Eulerian observer may note one copy is reading backwards near a growing candle. However, Recami's consideration of a "Lagrangian" observer is certainly provocative if one starts to wonder what happens to his "traveller" across cosmological distances -- in that regime, one encounters arrow-of-time/statmech problems that sharpen in nonvacuum. (I will however need some time to absorb the points about apparent vacuum decay in Recami §7.7, among other goodies in the paper). Finally, yes, it was behind a paywall, but <https://sci-hub.se/https://link.springer.com/article/10.1007/BF00733092 https://sci-hub.se/https://link.springer.com/article/10.1007...> of course -- it's even easier to read that way, even if one has springerlink access. :-)