Mathematical form of Mass Conservation for continuum body:
Integral form | Differential form | ||||
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where
t | time | \rho(t, {\bf r}) | continuum body spatial density distribution |
{\bf r } | position vector | {\bf u}(t, {\bf r) | continuum body spatial velocity distribution |
\Omega | space volume (could be finite or infinite) | \displaystyle \frac{dm_\Omega}{dt} | mass generation rate with the space volume \Omega |
\nabla | gradient operator | \displaystyle \frac{d\rho(t, {\bf r})}{dt} | volume-specific mass generation rate at a given point in space {\bf r } |
For the specific case of stationary process when density is not explicitly dependent on time:
(3) | \frac{\partial \rho}{\partial t} = 0 \rightarrow \nabla (\rho \, {\bf u}) = 0 |
For the specific case of finite number of mass generation locations the differential equation (2) takes form:
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where
{\bf r }_k | position vector of the k-th source/sink |
\dot m_k(t) | mass generation rate at k-th source/sink: \displaystyle \dot m_k(t) = \frac{dm_k}{dt} |
\delta ( \bf r ) | Dirac delta function |
Alternatively it can be written as:
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wehre
q_k(t) | volumetric value of body mass generation rate at k-th source/sink: \displaystyle q_k(t) = \frac{dV_k}{dt} |
See also
Natural Science / Physics / Mechanics / Continuum mechanics