Conservation of Energy of the Center of Mass

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SUMMARY

The discussion centers on the conservation of energy in the context of the center of mass for a system of particles, specifically two particles in an external field. The energy of the system is expressed as $$E=\frac{1}{2}m_1|\vec{v}_1|^2+\frac{1}{2}m_2|\vec{v}_2|^2+V(\vec{r}_1)+V(\vec{r}_2)+V'(|\vec{r}_2-\vec{r}_1|)$$, with the conclusion that both the total energy and the energy of the center of mass are conserved, represented by $$\frac{dE}{dt}=0$$ and $$\frac{dE'}{dt}=0$$ respectively. The discussion raises questions about the conditions under which this conservation holds, particularly in cases involving non-potential interactions like magnetic forces, and references Noether's Theorem as a potential framework for understanding these conservation laws.

PREREQUISITES
  • Understanding of classical mechanics principles, particularly energy conservation.
  • Familiarity with potential energy concepts in physics.
  • Knowledge of Noether's Theorem and its implications for conservation laws.
  • Basic mathematical skills to interpret equations involving vectors and derivatives.
NEXT STEPS
  • Research the implications of Noether's Theorem on conservation laws in physics.
  • Explore the role of magnetic forces in energy conservation and their mathematical representation.
  • Study the conditions under which energy conservation applies to systems with non-potential interactions.
  • Examine advanced topics in classical mechanics related to the center of mass and energy conservation.
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Students and professionals in physics, particularly those studying classical mechanics, energy conservation, and theoretical physics. This discussion is beneficial for anyone looking to deepen their understanding of conservation laws and their applications in various physical systems.

Luke Tan
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In classical mechanics, the energy of a system of particles (say with 2 particles) in an external field is given by
$$E=\frac{1}{2}m_1|\vec{v}_1|^2+\frac{1}{2}m_2|\vec{v}_2|^2+V(\vec{r}_1)+V(\vec{r}_2)+V'(|\vec{r}_2-\vec{r}_1|)$$
Where V is the potential energy of the external field, and V' is the energy of interaction between the two particles. It is well known that ##\frac{dE}{dt}=0##, or that energy is conserved.

However, the energy of the center of mass is surprisingly also conserved
$$E'=\frac{1}{2}(m_1+m_2)(\frac{m_1\vec{v}_1+m_2\vec{v}_2}{m_1+m_2})^2+V(\frac{m_1\vec{r}_1+m_2\vec{r}_2}{m_1+m_2})$$
$$\frac{dE'}{dt}=0$$

This makes sense as macroscopically, everything is just made out of tiny particles and if this identity doesn't hold there would be no concept of a macroscopic object being treated as a particle.

However, is there any proof that the energy of the center of mass is conserved, based directly on the fact that the energy of the system is conserved? What are the conditions? For example, if the interactions between the particles in the system could not be described by a potential ##V'(|\vec{r}_2-\vec{r}_1|)##, such as in the case of magnetic forces, would this still hold? Must ##V## be linear in the coordinates?

In addition, does this hold for other quantities? For example, if every particle ##i## had a quantity ##\Omega_i(\vec{r}_i,\vec{p}_i)## associated with it such that ##\frac{d}{dt}(\sum_i \Omega_i(\vec{r}_i,\vec{p}_i))=0##, would ##\frac{d}{dt}\Omega(\vec{r}_{cm},\vec{p}_{cm})=0##?

Thanks!
 
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anorlunda said:
There is a simpler approach. Are you familiar with Noether's Theorem?
Not really, I know that it states that for every symmetry there is an associated conservation law and I have used it before for simpler conservation laws such as the conservation of momentum and angular momentum, but I don't really see how I would apply it to this.
 

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