Understanding Euler-Lagrange Equations: Lagrangian Density & Vector Field

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The discussion revolves around the application of Euler-Lagrange equations to a specific Lagrangian density for a neutral vector field, leading to the equations of motion. The user expresses confusion regarding the treatment of indices in the Lagrangian, particularly why derivatives yield different indices and the implications for differentiation. Clarification is sought on the notation, specifically the distinction between upper and lower indices when differentiating the scalar product of the vector field. Additionally, recommendations for introductory texts on tensor algebra tailored for physicists are requested, with one user suggesting Schaum's Tensor Calculus despite noting some typographical errors. Understanding the proper treatment of indices is emphasized as crucial for accurate calculations in this context.
Spinny
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Here's the problem. For a neutral vector field V_{\mu} we have the Lagrangian density

\mathcal{L} = -\frac{1}{2}(\partial_{\mu}V_{\nu})(\partial^{\mu}V^{\nu})+\frac{1}{2}(\partial_{\mu}V^{\mu})(\partial_{\nu}V^{\nu})+\frac{1}{2}m^2V_{\mu}V^{\mu}

We are then going to use the Euler-Lagrange equations to show that (for m\neq 0)

\partial_{\mu}\partial^{\mu}V^{\nu}+m^2V^{\nu} = 0 \quad;\quad \partial^{\mu}V_{\mu} = 0

Now, the Euler-Lagrange equation (as I found in the textbook) is

\frac{\partial \mathcal{L}}{\partial \varphi}-\partial_{\mu}\frac{\partial \mathcal{L}}{\partial(\partial_{\mu}\varphi)} = 0

My problem here, with what at first glance would appear to be a rather simple problem, is that I'm confused by all the indices! I haven't a lot of experience working like this, in fact this is all new to me, so I don't quite know how or where to start.

I can, however, give a specific example of what I don't understand, just to get things started.

The first part seemed at first easy enough, as the Lagrangian only contains one part with V_{\mu} which is

\frac{1}{2}m^2V_{\mu}V^{\mu}

and from what I've understood V_{mu}V^{\mu} is just the square of each of the components of the vector, so that when you derivate it with respect to V_{\mu}, I thought you'd get something like

m^2V^{\mu}

but the text says m^2 V^{\nu} which brings up two question, first of all, why is it \nu and not \mu, and why is it an upper index, rather than a lower one?

Furthermore I was wondering if anyone could recommend a good book introductory book about tensor algebra and such, preferably one intended for physicists rather than mathematicians. (It doesn't have to be a book on just about tensors, as long as it contains a good introduction to tensors.)
 
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It matters whether you differentiate the scalar V_{\mu}V^{\mu} wrt the covector V_{\nu} or wrt the vector V^{\nu}. That's why the indices must be treated with great care.

Daniel.
 
Hi Spinny,

I worked my way through Schaum's Tensor Calculus which I found very good except for quite a few typos.

Regards


TerryW
 

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