2007
DOI: 10.1063/1.2719144
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Absolute time derivatives

Abstract: A four dimensional treatment of nonrelativistic space-time gives a natural frame to deal with objective time derivatives. In this framework some well known objective time derivatives of continuum mechanics appear as Lie-derivatives. Their coordinatized forms depends on the tensorial properties of the relevant physical quantities. We calculate the particular forms of objective time derivatives for scalars, vectors, covectors and different second order tensors from the point of view of a rotating observer. The r… Show more

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Cited by 12 publications
(12 citation statements)
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References 39 publications
(60 reference statements)
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“…These requirements make (1) a diffeomorphism, i.e., a time-dependent flow of curvilinear coordinates 25,29,39,40,48 whose motion in space resembles in toto a physical fluid flow of classical mechanics. Einstein called these coordinate systems "reference-mollusks" 11 .…”
Section: The Conjugate Flowmentioning
confidence: 99%
“…These requirements make (1) a diffeomorphism, i.e., a time-dependent flow of curvilinear coordinates 25,29,39,40,48 whose motion in space resembles in toto a physical fluid flow of classical mechanics. Einstein called these coordinate systems "reference-mollusks" 11 .…”
Section: The Conjugate Flowmentioning
confidence: 99%
“…If the tensor z bc is split to components according to (7), then -y is the intensive quantity related to the mass density, -yb is the intensive quantity belonging to the momentum density pb, -ybc is the intensive quantity related to the energy density tensor ebc . One can pull closer the treatment to the usual approach assuming…”
Section: Thermostatics Of Motion or Thermostatodynamicsmentioning
confidence: 99%
“…However, the space is relative also in this case, it is different for different observers: the so-called non-relativistic space-time is Galilean relativistic. With the help of the notions of special relativistic space-time, the heuristic concepts of our everyday experience can be clarified and an exact mathematical model of Galilean relativistic space-time can be formulated [1,2,3,4,5,6,7].…”
Section: Introductionmentioning
confidence: 99%
“…• The weakly nonlocal extension of the constitutive state space is a safe procedure, because the gradient is a covector, that does not depend on the motion, e.g., does not transform by a Galilean transformation [63,64].…”
Section: The Entropy Principle In Classical Irreversible Thermodynamicsmentioning
confidence: 99%