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The Principle of Mass Conservation in Classical Physics

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Exploring the principle of mass conservation in classical physics, this concept asserts that the mass of an isolated system remains constant over time, barring external forces. It underpins fluid dynamics and solid mechanics, and is crucial in chemistry for stoichiometry. Historical figures like Lomonosov and Lavoisier contributed to its development, while Einstein's relativity introduced mass-energy equivalence, expanding the principle to include energy conservation.

The Principle of Mass Conservation in Classical Physics

The principle of mass conservation is a cornerstone of classical physics, stating that the mass of an isolated system is constant over time if it is not influenced by external forces. This principle holds true when the energies involved are much less than the energy equivalent of the system's mass (given by E=mc^2, where c is the speed of light). In classical physics, mass is a conserved property, meaning it cannot be created or destroyed within an isolated system. This principle is essential for understanding the dynamics of physical systems and forms the basis for disciplines such as fluid dynamics and solid mechanics.
Classic brass scientific scale with two symmetrical plates and a large sphere on the right balanced by multiple small spheres on the left on a gray gradient background.

Continuity Equation and Mass Conservation

The mathematical expression of mass conservation in fluid dynamics and continuum mechanics is the continuity equation. In differential form, the equation is ∂ρ/∂t + ∇⋅(ρv) = 0, where ρ is the density, t is time, ∇⋅ is the divergence operator, and v is the velocity vector field of the fluid. The continuity equation states that the rate of change of mass within a volume is equal to the net flow of mass into or out of the volume. For a closed system, the total mass M remains constant over time, which can be expressed as dM/dt = 0, where M is the integral of density over the volume of the system.

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Mass conservation in isolated systems

In an isolated system, mass remains constant over time, unaffected by external forces.

01

Mass-energy equivalence formula

E=mc^2, where E is energy, m is mass, and c is the speed of light.

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Role of mass conservation in physics

Fundamental for understanding dynamics in fluid dynamics and solid mechanics.

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