CFDFEAGURU said:
Hello all,
Thanks for the advice and definitions above. Here is the problem given in Hartle's book. This is problem 5 in chapter 3.
Consider the functional
S[x(t)] = \int[(dx(t)/dt)^2+x^2(t)]dt
The integral is from zero to T. (Can someone show me how to create an integral with the limits of integration in LaTex?)
Find the curve x(t) satisfying the conditions x(0)=0, x(T)=1. which makes S[x(t)] an extremum. What is the extremum value of S[x(t)]? Is it a maximum or a minimum?
Note: This is not a homework problem. I am teaching myself GR and I just need some help here.
Any help on this would be greatly appreciated.
Thanks
Matt
Quick hair splitting note: With regard to earlier discussion on definitions the notation used:
S[x(t)]
is really bad (but common) since a.) it implies S is a function (via composition) of t which relates to b.) t is a variable of integration and shouldn't appear anywhere outside the integral in which it is defined. It should rather read
S[x]
Focusing on this distinction may help better understand the process about which you asked.
With regard to latexing integral limits, when you want to put limits on latex integral simply use the sub-script, super-script ops.
\int_a^b f(x)dx
parses to:
\int_a^b f(x)dx
similarly with \sum in Sigma summation notation.
Now with regard to finding the extremum of the action, this is the classic variation problem in the derivation of the Euler-Lagrange equations. See http://en.wikipedia.org/wiki/Euler%E2%80%93Lagrange_equation"
For a given Action Lagrangian:
S[x] = \int_{0}^{T}L(x(t),\dot{x}(t)) dt
the classic solution to the extremum problem \delta S = 0[/tex] <br />
is that x must satisfy the E-L equations:<br />
\frac{d}{dt} \left( \frac{\partial L}{\partial \dot{x}} \right) = \frac{\partial L}{\partial x}<br />
Note that if x is a vector this form still holds for each component. Simply view it as having a suppressed index<br />
x\ \to x_\mu,\quad \dot{x}\to \dot{x}_\mu.<br />
<br />
The term in parenthesis of the RHS of the E-L equation:<br />
P=\frac{\partial L}{\partial \dot{x}}<br />
is called the <i>canonical momentum</i> and the right hand side of the equation is called the <i>canonical force</i> so that the E-L equation takes the classic form:<br />
\dot{P} = F<br />
and you'll note for Lagrangians of the form:<br />
L(\dot{x},x) = \frac{1}{2}\dot{x}^2 - V(x)<br />
you get the usual:<br />
P = m\dot{x}, \quad F = - \frac{\partial V}{\partial x}<br />
However you can apply to more exotic systems where you have say an x dependend "mass" or linear terms with respect to the velocity.<br />
<br />
Finally in GR and other field theories you will in the canonical treatment of the fields you will have a lagrangian density where now not just t but (t,x,y,z) are the independent variables of integration. The form of the Euler-Lagrange equations is still the same form if you look at it right.<br />
<br />
[EDIT] Oops! Forgot to mention that your boundary conditions simply become boundary conditions on the E-L equations. Since the E-L equations are second order differential equations you will have two free variables of integration for which you can solve to satisy the BC.