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Conservation laws in elasticity. II. Linear homogeneous isotropic elastostatics
 Arch. Rational Mech. Anal
, 1984
"... In 1956 ESHELBY, [5], introduced his celebrated energymomentum tensor in his study of lattice defects. This tensor had the useful property of providing nontrivial pathindependent integrals for the equations of finite elasticity, or, in other words, providing densities of nontrivial conservation la ..."
Abstract

Cited by 22 (8 self)
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In 1956 ESHELBY, [5], introduced his celebrated energymomentum tensor in his study of lattice defects. This tensor had the useful property of providing nontrivial pathindependent integrals for the equations of finite elasticity, or, in other words, providing densities of nontrivial conservation
Note on the energymomentum tensor
, 2008
"... This note provides an explicit proof of the equivalence of the Belinfante’s energymomentum tensor and the metric energymomentum tensor for general mixed tensorspinor fields. 1 ..."
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This note provides an explicit proof of the equivalence of the Belinfante’s energymomentum tensor and the metric energymomentum tensor for general mixed tensorspinor fields. 1
EnergyMomentum Tensor on Foliations
, 2007
"... In this paper, we give a new lower bound for the eigenvalues of the Dirac operator on a compact spin manifold. This estimate is motivated by the fact that in its limiting case a skewsymmetric tensor (see Equation (1.6)) appears that can be identified geometrically with the O’Neill tensor of a Riema ..."
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Cited by 6 (2 self)
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In this paper, we give a new lower bound for the eigenvalues of the Dirac operator on a compact spin manifold. This estimate is motivated by the fact that in its limiting case a skewsymmetric tensor (see Equation (1.6)) appears that can be identified geometrically with the O’Neill tensor of a
energymomentum tensor
, 2004
"... In recent papers [13], we have discussed matter symmetries of nonstatic spherically symmetric spacetimes, static plane symmetric spacetimes and cylindrically symmetric static spacetimes. These have been classified for both cases when the energymomentum tensor is nondegenerate and also when it is ..."
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In recent papers [13], we have discussed matter symmetries of nonstatic spherically symmetric spacetimes, static plane symmetric spacetimes and cylindrically symmetric static spacetimes. These have been classified for both cases when the energymomentum tensor is nondegenerate and also when
as the energymomentum tensor
, 1997
"... A forgotten argument by Gordon uniquely selects Abraham’s tensor ..."
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