Covariant Derivative: A^μₛᵦ Definition & Use

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SUMMARY

The covariant derivative is defined as A^\mu_{\sigma} = \frac{\partial A^\mu}{\partial x_{\sigma}} + \Gamma^\mu_{\sigma \alpha}A^\alpha, where \Gamma^\mu_{\sigma \alpha} serves to adjust the ordinary derivative to ensure it transforms correctly under coordinate changes. This definition is essential in differential geometry and general relativity, as it allows for the proper behavior of vector fields under transformations. The discussion emphasizes that the covariant derivative is not merely a mathematical construct but is motivated by the need for consistency in tensor analysis and parallel transport.

PREREQUISITES
  • Understanding of tensor analysis and transformations
  • Familiarity with differential geometry concepts
  • Knowledge of general relativity principles
  • Basic calculus, specifically limits and derivatives
NEXT STEPS
  • Study the concept of parallel transport in differential geometry
  • Learn about the role of Christoffel symbols in tensor calculus
  • Explore the implications of covariant derivatives in general relativity
  • Investigate alternative definitions of derivatives, such as the Schwarzian derivative
USEFUL FOR

Mathematicians, physicists, and students of theoretical physics who are engaged in advanced studies of differential geometry, general relativity, or tensor calculus will benefit from this discussion.

  • #31
And back again into the loop: what exactly is the definition of covariant derivative you're starting from then? Because the problem seems to be you can't translate from your definition to this one.
 
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  • #32
For the "pictoral" approach I mentioned in more detail, if you can get a hold of MTW's book "Gravitation", it's discussed around pg 244 in chapter 10.

As far as the detailed answer to your question

A general vector x can be represented as x^i e_i, where the e_i are the basis vectors.

Thus in a cartesian coordinate system we would have as basis vectors e_x, e_y, e_z, in a cylindrical coordinate system we would have e_r, e_theta, e_z, etc etc.

The definition of the Christoffel symbols

\Gamma^{\mu}{}_{\sigma \alpha}[/itex] is that they describe how the basis vectors transform in terms of the basis vectors.<br /> <br /> i.e we take<br /> <br /> \nabla_{\sigma} e_{\alpha} <br /> <br /> and express it in terms of the basis vectors as<br /> <br /> \nabla_{\sigma} e_{\alpha} = \Gamma^{\mu}{}_{\alpha \sigma} e_{\mu}<br /> <br /> The rest is the chain rule. \nabla_{\sigma} A^{\mu}e_{\mu} = (\nabla_{\sigma}A^{\mu}) e_{\mu} +(\nabla_{\sigma}e_{\mu})A^{\mu}<br /> <br /> The first term gives the partial derivative, the second term gives the Christoffel symbols.
 
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