PlanetPhysics/Total Energy of a System of Particles

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Let us multiply the equation of [[../CosmologicalConstant/|motion]] of the k th [[../Particle/|particle]] scalarly with d𝐫dt, and sum over all the particles. Then

kmkd2𝐫kdt2d𝐫kdt=ddt12kmk(d𝐫kdt)2=k𝐅kd𝐫kdt+kjϵjk𝐅jkd𝐫kdt

Integrating between the times t0 and t:

12kmk(d𝐫kdt)t212kmk(d𝐫kdt)t02=rk(t0)rk(t)k𝐅kd𝐫k+rk(t0)rk(t)kj𝐅jkd𝐫k

The left member represents the total change in [[../KineticEnergy/|kinetic energy]] of the [[../SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence/|system]], the right member gives the [[../Work/|work]] done by the internal and external [[../Thrust/|forces]]. But it is by no means the case that the work done by the internal forces cancels out in calculating the [[../CosmologicalConstant/|energy]], as one might expect it to do. The kinetic energy may be divided into two parts, each of which has a physical meaning. If we introduce a second coordinate system, whose origin O is at the [[../CenterOfGravity/|center of gravity]] of the system, and if we denote all [[../PositionVector/|radius vectors]] referred to this system by primes, we have

𝐫k=𝐫¯+𝐫k

Then, identically,

k12mk(d𝐫kdt)2=12(d𝐫¯dt)2kmk+d𝐫¯dtkmkdr𝐀dt+12kmk(dr𝐀dt)2

The second sum on the right vanishes, however, since mk𝐫k/M is, by equation (3), the radius vector of the center of gravity, and this, by hypothesis, is zero in the primed coordinates. The first term on the right represents the kinetic energy of the system, considering the entire [[../Mass/|mass]] to be concentrated at the center of gravity. The last term gives the kinetic energy of motion of the system referred to the center of gravity, when considered at rest. Thus, we may say:

The total kinetic energy is equal to the \htmladdnormallink{translational kinetic energy {http://planetphysics.us/encyclopedia/KineticEnergy.html} of the entire mass, considered concentrated at the center of gravity, plus the energy of motion of the parts of the system relative to the center of gravity}.

We further assume that the internal forces are such that they are derivable from a potential. The potential of the force operating between the points j and k is a [[../Bijective/|function]] of the distance between the two points, and therefore of their coordinates:

Ujk=Ujk(𝐫jk)=Ujk((xjxk)2+(yjyk)2+(zjzk)2)

The force acting on k is obtained by taking j to be fixed, and considering k to move in the potential [[../CosmologicalConstant2/|field]] given by the point function Ujk; i.e. we consider the coordinates of j to be fixed, those of k to be variable. Then

𝐅jk=i^Ujkxkj^Ujkykk^Ujkzk=kUjk

in like manner,

𝐅kj=i^Ujkxjj^Ujkyjk^Ujkzj=jUjk=𝐅jk

The work done in causing small displacements of j and k is

𝐅jkd𝐫k+𝐅kjd𝐫j=(Ujkxkdxk+Ujkykdyk+Ujkzkdzk+Ujkxjdxj+Ujkyjdyj+Ujkzjdzj)=dUjk

The negative of the sum of 𝐅jkd𝐫k and 𝐅kjd𝐫j is therefore obtained by forming the total differential of Ujk, defined as a funtion of the six coordinates of the two points, in (11). If, then, we wish to introduce the internal potential into the right member of equation (9), we must write

kjϵjk𝐅jkd𝐫k=12ϵjkkjdUjk

It is readily seen that the factor 1/2 enters: If we start with point 1, and calculate the mutual energy Ujk between this and all the other points, k runs from 2 to N; but when we take point 2, we must start counting with 3, since the mutual effect of points 1 and 2 was already taken into account in dealing with point 1, and so on. Thus, in extending the summation over all combinations j and k, we must divide by two.

If the external forces have also a potential, the energy equation (9) becomes

T+kUk+12kjϵjkUjk=T(0)+kUk(0)+12kjϵjkUjk(0)=const.

where T denotes the kinetic energy. The sum of the kinetic energy and of the external and internal potential energy of a system is constant, if the external as well as the internal forces are conservative .

References

[1] Joos, Georg. "[[../PhysicalMathematics2/|Theoretical physics]]" 3rd Edition, Hafner Publishing Company; New York, 1954.

This entry is a derivative of the Public [[../Bijective/|domain]] work [1].

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