Undergrad A good reference sheet/manual about Einstein index notation?

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The discussion centers on the challenges of understanding Einstein index notation, particularly in complex examples involving derivatives. The user seeks a comprehensive reference sheet or manual that covers advanced topics like derivation rules and integration, as existing resources only address basic principles. They express confusion over specific notations, such as the interpretation of ##\partial^2##, and the implications of derivatives on indexed quantities. The user hopes for a cheatsheet that clarifies legitimate substitutions and prefactors, as well as exercises with solutions to build confidence. Overall, the need for more detailed resources on Einstein notation and its applications in theoretical physics is emphasized.
Gan_HOPE326
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I'm not used to Einstein notation and I'm struggling a bit with the more complex examples of it. I got the general gist of it and can follow the basic cases but get sometimes a bit lost when there are a lot of indexes and calculus is involved. All primers I've found online for now only give the basic rules - sum over repeated indices, Kronecker delta, Levi-Civita symbol, and that's it. Is there some good 'reference sheet' I could use to look up more sophisticated cases like those involving derivation rules? I realize they can easily be derived from considering the represented sum, and in some cases I manage to do that, but the convenience of the notation should be to avoid having to write sums explicitly all the time, and knowing the rule beforehand I could at least work out why and how it applies and then trust it going forward. Thanks!
 
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Can you give an example of the type of relation that you would like to have a reference for?
 
Orodruin said:
Can you give an example of the type of relation that you would like to have a reference for?

Mostly derivatives. I struggled quite a bit some days ago with understanding how you got from the relativistic EM Lagrangian

$$\mathcal{L} = -\frac{1}{4}F_{\mu\nu}F^{\mu\nu}$$

to the kernel of the action integral used in QFT

$$\frac{1}{2}A_\mu(\partial^2g^{\mu\nu}-\partial^\mu\partial^\nu)A_\nu$$

Part of this was because of not realising an integration by parts was happening in the process (I actually made a previous thread about it) but part of it was confusion about the meaning for example of ##\partial^2##, whether it was meant to represent ##\partial_\mu\partial_\mu## or ##\partial_\mu\partial^\mu##. Similarly today I ran into a case in which a derivative of a product of indexed quantities gives an additional factor of 2 - which is pretty obvious when carrying out the sum, but I would have probably missed if I didn't expand, and for more complex expressions that might become annoying (luckily for me, this one was simply a toy model of GR in 1+1 spacetime, so not many indices).

I guess what I'd hope for is some cheatsheet especially for derivation and integration. Which substitutions are legitimate to carry out, which prefactors appear and such. I imagine most people get this kind of knowledge through doing exercises in their relativity course, but unfortunately since I'm working on this on my own I don't get that luxury, and theory books I put my hands on tend to skim over all this. In alternative, a good reference for exercises with solutions I can carry out to learn more the basics and feel more confident with it would do the trick as well I guess.
 
Gan_HOPE326 said:
whether it was meant to represent ##\partial_\mu\partial_\mu## or ##\partial_\mu\partial^\mu##.
Well, ##\partial_\mu\partial_\mu## doesn't make sense because you're not allowed to repeat an index unless one is "downstairs" and the other is "upstairs".
 
DrGreg said:
Well, ##\partial_\mu\partial_\mu## doesn't make sense because you're not allowed to repeat an index unless one is "downstairs" and the other is "upstairs".

Fair enough, yeah.
 
MOVING CLOCKS In this section, we show that clocks moving at high speeds run slowly. We construct a clock, called a light clock, using a stick of proper lenght ##L_0##, and two mirrors. The two mirrors face each other, and a pulse of light bounces back and forth betweem them. Each time the light pulse strikes one of the mirrors, say the lower mirror, the clock is said to tick. Between successive ticks the light pulse travels a distance ##2L_0## in the proper reference of frame of the clock...

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