Integration in Sean Carroll's parallel propagator derivation

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SUMMARY

The discussion focuses on the integration process in Sean Carroll's derivation of the parallel propagator as outlined in Chapter 3 of his General Relativity Lecture Notes. The equation of interest is the differential equation for the parallel propagator, given by \(\frac{d}{d\lambda} P^\mu_{\;\;\; \rho}(\lambda,\lambda_0) = A^\mu_{\;\;\; \sigma} P^\sigma_{\;\;\; \rho}(\lambda,\lambda_0)\). The integration of both sides leads to the expression \(P^\mu_{\;\;\; \rho}(\lambda,\lambda_0) = \delta^\mu_\rho + \int_{\lambda_0}^\lambda A^\mu_{\;\;\; \sigma} (\eta) P^\sigma_{\;\;\; \rho}(\eta,\lambda_0) \; d \eta\), where the Kronecker delta ensures proper normalization. The discussion also addresses the iteration procedure and the component-wise nature of the integration and differentiation involved.

PREREQUISITES
  • Understanding of differential equations, specifically matrix differential equations.
  • Familiarity with the Kronecker delta and its role in linear algebra.
  • Knowledge of integration techniques in the context of vector-valued functions.
  • Basic concepts of general relativity and parallel transport.
NEXT STEPS
  • Study the derivation of the parallel propagator in Sean Carroll's General Relativity Lecture Notes, focusing on Chapter 3.
  • Learn about matrix differential equations and their solutions, particularly in the context of physics.
  • Explore the concept of vector-valued functions and their derivatives and integrals.
  • Investigate related mathematical frameworks, such as those discussed by Bachman regarding cells and chains.
USEFUL FOR

This discussion is beneficial for graduate students in physics, mathematicians working with differential equations, and researchers interested in the mathematical foundations of general relativity and parallel transport. It provides insights into the integration techniques used in theoretical physics.

Rasalhague
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Integration in Sean Carroll's "parallel propagator" derivation

Reading Chapter 3 of Sean Carroll's General Relativity Lecture Notes, I've followed it up to and including eq. 3.38.

\frac{d}{d\lambda} P^\mu_{\;\;\; \rho}(\lambda,\lambda_0) = A^\mu_{\;\;\; \sigma} P^\sigma_{\;\;\; \rho}(\lambda,\lambda_0).

Here, Carroll writes, "To solve this equation, first integrate both sides:

P^\mu_{\;\;\; \rho}(\lambda,\lambda_0) = \delta^\mu_\rho + \int_{\lambda_0}^\lambda A^\mu_{\;\;\; \sigma} (\eta) \; P^\sigma_{\;\;\; \rho}(\eta,\lambda_0) \; d \eta.

"The Kronecker delta, it is easy to see, provides the correct normalization for \lambda = \lambda_0."

I can see that this makes P the identity matrix in that case, but by what algebraic rule is it inserted. This is a definite integral, so shouldn't any constant of integration be canceled out?

Also, I don't understand the iteration procedure that follows. Doesn't the concept of integration already encode such a procedure, taken to a limit? Should I read this as (coordinate-dependent?, coordinate independent?) abstract index notation for a matrix equation inside the integral sign, or is each component function integrated separately? Is there a name for this procedure or the subject area that includes it? Can anyone recommend a book or website that explains the mathematical background. Sorry these questions are a bit vague. I'm not really sure what to ask.

I wonder if it's related to what Bachman calls cells and chains. Maybe I should read the rest of that chapter first.
 
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Write it as

\frac{dP(\lambda)}{d\lambda}=A(\lambda)P(\lambda)

The solution of this differential equation with the initial data P(\lambda_0)=I is

P(\lambda)=I+\int_{\lambda_0}^\lambda A(\lambda)P(\lambda)

First, check that indeed the initial value data are satisfied and then that the differential equation is also satisfied.

Now, add the indices remembering that

\left(\frac{dP(\lambda)}{d\lambda}\right)^\mu_\rho is the same as
\frac{dP^\mu_\rho(\lambda)}{d\lambda} and similarly on the RHS - matrix entries of the integral are integrals of matrix entries owing to the linearity of the integral. That is how we define derivatives and integrals of vector-valued functions.
 


Thanks again, arkajad! I get it now. Holding lambda_zero constant,

P(\lambda) - P(\lambda_0) = \int_{\lambda_0}^{\lambda} A(\eta) P(\eta) \; \mathrm{d}\eta

and

P(\lambda_0) = I[/itex]<br /> <br /> given what the parallel propagator has be defined to do, so<br /> <br /> P(\lambda) = I + \int_{\lambda_0}^{\lambda} A(\eta) P(\eta) \; \mathrm{d}\eta.<br /> <br /> Sean Carroll&#039;s eq. (3.39) is just this expressed with indices. And there&#039;s no ambiguity over the order of operations, because the derivatives and integrals are defined componentwise.
 

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