This lattice intro gives the matrix for a scalar field as $$\sum_{x,y} \varphi(x) (\delta_{x+a\hat{\mu},y} + \delta_{x-a\hat{\mu},y} - 2 \delta_{xy})\varphi(y)$$
But that would give $$\sum \varphi(x) \varphi(x+a\hat \mu) + \varphi(x) \varphi(x - a\hat\mu) - 2\varphi(x)^2$$
I don't think the lattice version cares at all about that. The measure is really just $\prod_x \mathrm{d}\phi_x$, there's no fancy Wiener measure or somesuch involved.
@ACuriousMind A bilinear form on any Lie algebra---in the case the algebra is simple it is non-degenerate and I think compactness guarantees it's negative semi-definite
Hopefully the method will just be the same as doing the path integral for a point particle from $x_1$ to $x_2$, except it will be from field configuration at x $\varphi_1$ to $\varphi_2$
@Slereah You integrate over a region in field space. Usually, the integral is over all of field space. What exactly do you mean by "integrating between two boundary conditions"?
Well...you'd need to know how to compute a path integral in the first place for that. Usually you just use its formal properties, you don't actually evaluate it
Also, I have a slight feeling that the space of fields obeying a certain boundary condition might be a zero measure set in the cases where the measure is actually well-defined.
I.e. you're not using a measure on the space of paths and restrict to certain subsets, you're defining a new measure for every integral with a different boundary condition
So one should expect the same for the path integral - you can't just say "I want to integrate over just these fields", you have to define your integral from scratch if you change the boundary conditions.
I mean, the Faddeev-Popov trick of just writing a $\delta$ function works for physicists, but the actual thing to do is to quotient out the gauge orbits out of the space of all fields and then integrate over that quotient.
@Danu I have a suspicion it has to do with physicists usually using a scaled version of the field, you get the usual physics action from $\frac{1}{g^2}\int F\wedge{\star} F$ by rescaling the field (or rather the Lie algebra generators) with $g$, which of course also rescales the Killing form.
There are tons of procedures in QFT that are done only in one formalism every time and it annoys me that it's so rare that people try to prove it for all of them
Einstein synchronisation (or Poincaré–Einstein synchronisation) is a convention for synchronising clocks at different places by means of signal exchanges. This synchronisation method was used already by telegraphers in the middle 19th century, but was popularized by Henri Poincaré and Albert Einstein who applied it to light signals and recognized its fundamental role in relativity theory. Its principal value is for clocks within a single inertial frame.
== Einstein ==
According to Albert Einstein's prescription from 1905, a light signal is sent at time from clock 1 to clock 2 and immediately back...
@JohnRennie OK. Points E and A are 8 ly apart. Ship S travels at 0.8 c past point A. S and E want to synchronize to t=0 the instant that happens. Possible?
@barrycarter In principle yes. S and A can synchonise because they are at the same point. A and E can synchronise (eventually) because they are in ther same inertial frame.
@JohnRennie OK. So S and A synch easily. For E, because it's 8 ly away, when they first see S pass A (at their time t=8), they declare the synch time to be t = what?
@barrycarter I feel you're probing for a signifance that isn't there. E knows how far they are from A and therefore how long a signal takes to get from A to E.
@barrycarter Well, he could say: I know A set their clock to zero when S passed, that happened 8 years ago, so if I set my clock to +8 years now I'm guaranteed to have my clock synchronised with A.
@barrycarter Because for space-like separated events, there's always a frame where they are simultaneous, and for time-like separated events, there's always a frame where they happen at the same point. You may not like it, but this is fact.
@barrycarter ?? Given two events the proper distance is just the (Minkowski) length of the four vector joining them. The proper time is this length divided by $c$.
Take the spacetiem points in the ship frame that mark the start and end of the journey and calculate $\tau$. Lorentz transform those points into the Earth frame and once again calculate $\tau$. The two values will match.
How can I be sure of this? Because the Lorentz transforms are derived from the invariance of $\tau$.
@barrycarter You're doing the wrong thing, you don't use the distance traveled or the time it took to compute the spacetime interval. You use the coordinates of the start point and the end point
Remember our discussion about the Lorentz contraction not matching what you found by Lorentz transforming the points? You're doing the same thing again, expecting the contraction to yield something it is not supposed to yield.
@barrycarter Okay, but I'm telling you we've essentially had the same discussion before - you're confusing time dilation and Lorentz contraction with the actual result of the Lorentz transformations
@JohnRennie Yeah, I know, it is an inevitable product of teaching relativity through thought experiments and paradoxes instead of axiomatically as we do with every other established theory-
We might be using two different definitions. The proper (non Minkowski) distance between two events is the distance between them to an observer who is stationary with respect to those two points. Yes?
If the two points are simulataneous in the rest frame of the observer then the proper length will simply be the distance between them because it reduces to $s^2 = 0 + \Delta x^2 + \Delta y^2 + \Delta z^2$
And if two events are simultaneous in one observer's rest frame, they can not be simultaneous in another observer's rest frame (different velocity), right?
Similarly, if two events occur at the same xyz coordinate for one observer, they won't for another (which is actually fairly obvious, even without relativity).
@JohnRennie Right, but since there is 0 distance (for him) between these two points, 4.8 years is in some sense the "proper time" (in heavy quotes) of the journey?
The proper time for an observer is exactly the elapsed time recorded by a clock carried by that observer. This is true in accelerated frames as well, and even in GR.
If two points have a time-like separation i.e. you can go from one to the other slower than light, then there is no frame in which the two points are simultaneous.
If $s^2 > 0$ there is a frame in which the two points have the same time coordinate. If $s^2 < 0$ there is a frame in which the two points have the same spatial coordinates.
I have studied some quantum field theory and gauge theory but I am definitely not an expert. I am aware that in quantizing electrodynamics one has to fix a gauge. I have read that for general gauge theory there are additional complications that arise and require things like Faddeev-Popov ansatz o...
@ACuriousMind My anecdotal experience is that users will come up with close reasons for those anyway. (I say this as I'm trudging through 50 close reviews...)
@Qmechanic Yes. The first question is a historical one, the second is trivially answered with "Yes.", and the third is a duplicate, as you point out; Neither of these three questions are related in a way that would require them to be asked jointly.