Equations of Motion with Covariant Derivatives and Momentum Density

In summary, the geodesic equation of motion can be written compactly as:-The "Covariant derivative" can be used to generalize the Newton equation of motion without forces or potentials.
  • #1
lokofer
106
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If for the "geodesic" equation of motion we have the compact form:

[tex] \nabla _ u u =0 [/tex] usign the "Covariant derivative"... as a generalization of Newton equation with F=0 (no force or potential) [tex] \frac{du}{ds}=0 [/tex] where "u" is the 4-dimensional momentum...

My question is if we can put the Equation of motion [tex] \R _\mu \nu =0 [/tex] as the "LIe derivative" or " Covariant derivative" or another Tensor, vector or similar involving the "momentum density" [tex] \pi _a b [/tex] and the metric elements [tex] g_ ab [/tex]
 
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  • #2
If the mass (invariant mass) is a constant, just multiply thorugh by m, and you have the covariant derivative of the energy-momentum 4 vector being 0.

I.e
[tex]\nabla_u u = 0 \Rightarrow \nabla_u (m u) = 0 \Rightarrow \nabla_u P = 0[/tex]

In component notation
[tex]
\nabla_u P^i = u^j \nabla_j P^i = 0
[/tex]

which makes it clear this gives 4 equations, one for each component of the energy-momentum 4-vector.

The notation for the covariant derivative [itex]\nabla_a[/itex] seems funny at first, but it's extremely useful. Let's say we have a scalar quantity x, and we want to find how fast it changes with time. With an ordinary derivative operator, we write dx/dt. With the covariant derivative operator, one writes [itex]\nabla_t x = t^a \nabla_a x[/itex], where t is a unit vector in the time direction. The covariant derivative operator actually generates a vector from the scalar. One must take the dot product of this vector with the direction one desires the derivative in order to get a scalar quantity. The reason for not doing a contraction automatically is that it can be ambiguous. Sometimes one sees the contracted covariant derivative written with a capital D to make the notation more simlar, but the math is the same.
 
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  • #3
-Thank you..by the way if we have the Lagrangian [tex] L= \sqrt (-g) R [/tex]

can you split the Lagrangian into a "Kinetic" and a "potential" part?..

- And What would be the "Euler-Lagrange" equation for Einstein Lagrangian?..i think you have:

[tex] \sum_{i=1,2,3,0} \partial _ {x_i }( \frac{ \partial L}{ \partial g_ab} - \frac{ \partial L}{ \partial g_ab} [/tex] or something similar.
 
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FAQ: Equations of Motion with Covariant Derivatives and Momentum Density

What is the significance of covariant derivatives in equations of motion?

Covariant derivatives are important in equations of motion because they allow us to take into account the effects of curved space-time. In other words, they take into account the fact that space and time are not flat and that the laws of physics may vary from one point to another. This is especially important in general relativity, where the curvature of space-time is a fundamental aspect of the theory.

How do covariant derivatives differ from ordinary derivatives?

Covariant derivatives are specifically designed to account for the curvature of space-time, while ordinary derivatives are used in flat, Euclidean space. Covariant derivatives also take into account the frame of reference in which the equations of motion are being described, while ordinary derivatives do not.

What is momentum density and why is it important in equations of motion?

Momentum density is a mathematical quantity that represents the momentum per unit volume of a system. It is important in equations of motion because it allows us to track how the momentum of a system changes over time. In theories such as general relativity, momentum density is a key component in understanding the dynamics of particles and fields in curved space-time.

Can equations of motion with covariant derivatives be used in all situations?

No, equations of motion with covariant derivatives are specifically designed for use in theories that involve curved space-time, such as general relativity. In situations where space-time is flat and the laws of physics are constant, ordinary derivatives are sufficient for describing the motion of particles.

What are some practical applications of equations of motion with covariant derivatives?

Equations of motion with covariant derivatives have a wide range of applications in physics, particularly in the fields of general relativity and particle physics. They are used to describe the motion of particles and fields in curved space-time, as well as in the study of cosmology, black holes, and other astrophysical phenomena. They are also essential in the development of quantum field theories that take into account the effects of curved space-time.

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