Invariants of the stress energy tensor

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SUMMARY

The discussion focuses on the invariants of the stress-energy tensor, particularly in the context of ideal fluids characterized by their internal-energy density (##\epsilon##) and pressure (##P##). The energy-momentum tensor is expressed in a covariant form as ##T^{\mu \nu} = (\epsilon + P) u^{\mu} u^{\nu} - P \eta^{\mu \nu}##, with two key invariants identified: ##u_{\mu} u_{\nu} T^{\mu \nu} = \epsilon## and ##\eta_{\mu \nu} T^{\mu \nu} = \epsilon - 3P##. The discussion also touches on the local conservation of energy represented by ##\nabla_\mu T^{\mu\nu} = 0## and the implications of eigenvalues for (1,1) tensors, asserting that these properties hold true across all coordinate systems.

PREREQUISITES
  • Understanding of the stress-energy tensor in general relativity
  • Familiarity with covariant tensor notation and transformations
  • Knowledge of fluid dynamics, particularly ideal fluids
  • Basic concepts of eigenvalues and eigenvectors in linear algebra
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  • Research the properties of the energy-momentum tensor in general relativity
  • Study the implications of eigenvalues for different types of tensors
  • Explore the role of the trace of the stress-energy tensor in physical theories
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Physicists, particularly those specializing in general relativity, fluid dynamics, and theoretical physics, will benefit from this discussion on the invariants of the stress-energy tensor.

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Does anyone know of a set of invariants for the stress energy tensor? In particular, I would like to know if there is a small set of linearly independent invariants, each of which (or at least some of which) have a clear physical meaning.
 
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It depends on which situation you look at.

Take an ideal fluid. It's characterized by an equation of state and a fluid four-velocity field ##u^{\mu}##. The energy-momentum tensor is defined through 2 invariants (or rather scalar fields): the internal-energy density and pressure in the local rest frames of the fluid cells, ##\epsilon## and ##P##. At one space-time point in the restframe the components read
$$T^{* \mu \nu}=\mathrm{diag}(\epsilon,P,P,P).$$
Since ##u^{* \mu}=(1,0,0,0)## and ##\eta^{*\mu \nu}=(1,-1,-1,-1)## you can write this in manifestly covariant form as
$$T^{* \mu \nu}=(\epsilon+P) u^{*\mu} u^{* \nu}-P \eta^{* \mu \nu}.$$
Since ##u^{\mu}## are four-vector components, and ##\eta^{* \mu \nu}=\eta^{\mu \nu}## are invariant tensor components (under Lorentz boosts), the equation holds in any frame,
$$T^{\mu \nu} =(\epsilon+P) u^{\mu} u^{\nu} - P \eta^{\mu \nu}.$$
The invariants (scalar fields) in this case are
$$u_{\mu} u_{\nu} T^{\mu \nu}=\epsilon$$
and
$$\eta_{\mu \nu} T^{\mu \nu}=\epsilon-3P.$$
Of course the latter scalar ("the trace") is one you can define for any energy-momentum tensor. For a free electromagnetic field or a fluid of massless particles it vanishes (in the classical-field theory approximation) because of the scale invariance of free electromagnetic fields and massless particles making up an ideal fluid.
 
Do you know if there are other invariants for a more general stress energy tensor or only for a perfect fluid?
 
Like any (1,1) tensor, the invariants should just be the eigenvalues or combinations thereof? This is reflected in #2 where the assumption of an ideal fluid makes three of the eigenvalues equal so that you only have two independent ones.
 
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Does ##\nabla_\mu T^{\mu\nu}=0## count? It's the local conservation of energy, and is four invariants constructed from the stress-energy tensor.
 
Orodruin said:
Like any (1,1) tensor, the invariants should just be the eigenvalues or combinations thereof?
Is that true in all coordinate systems or just in locally inertial coordinates?
 
I rather thought the invariants would be ##T^u{}_u## and perhaps ##*T^u{}_u##, where ##*T^{cd} = \epsilon^{abcd}T_{ab}##. But that was mainly from a discussion of an anti-symmetric tensor, I'm not sure what difference symmetry might make.
 
pervect said:
I rather thought the invariants would be ##T^u{}_u## and perhaps ##*T^u{}_u##, where ##*T^{cd} = \epsilon^{abcd}T_{ab}##. But that was mainly from a discussion of an anti-symmetric tensor, I'm not sure what difference symmetry might make.
Well, to start ##T## is not a 2-form. Since it is symmetric, ##*T## would be zero trivially.

The trace of ##T## is indeed an invariant as it is the sum of eigenvalues.

Dale said:
Is that true in all coordinate systems or just in locally inertial coordinates?
Eigenvalues of a (1,1) tensor do not depend on the coordinates. The coordinate independent eigenvector equation is ##T(V)=\lambda V##.
 
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Orodruin said:
The coordinate independent eigenvector equation is ##T(V)=\lambda V##.
So in coordinate notation that is ##g_{\nu\xi}T^{\mu\nu}V^{\xi}=\lambda V^{\mu}##
 
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Dale said:
So in coordinate notation that is ##g_{\nu\xi}T^{\mu\nu}V^{\xi}=\lambda V^{\mu}##
Yes.
 
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