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Its Explanation and Proof |
Noether's Theorem states that if the Lagrangian function for a physical system is not affected by changes in the coordinate system used to describe them, then there will be a corresponding conservation law. For example, if the Lagrangian is independent of the location of the origin then the system will preserve (or conserve) linear momentum. If it is independent of the base time then energy is conserved. If it is independent of the angle of measurement then angular momentum is is conserved.
First the nature of the Langrangian for a physical system must be explained.
Let K be the kinetic energy of a system and V its potential energy. The Lagrangian L for the system is defined as the difference between the kinetic and the potenial energy of the system; i.e., L = K − V.
A condition of a physical system is described by n coordinates {q_{1}, q_{2}, …, q_{n}} and their time derivatives {v_{1}, v_{2}, …, v_{n}}, where v_{n}=dq_{n}/dt. For example, a body in a vertical, uniform gravitational field would be described by one dimension, its height z. Its kinetic energy would be T=½mv² where m is the body's mass. Its potential energy is V=mgz, where g is the acceleration due to gravity. Thus the Lagrangian function for the body is L(z,v)=½mv²−mgz.
A physical systems evolves over some period of time from 0 to T such that the integral of its Lagrangian
is a minimum.
The determination of the trajectory of the system, {q_{i}(t) for i=1,…,n} is a problem in the calculus of variations. The result from the calculus of variations is that for the Lagrangian integral to be an extreme, a maximum or a minimum, at each instant of time
This is known as the Euler-Lagrange equation.
For the example of a body in a uniform gravitational field L(z,v)=½mv²−mgz. Thus the Euler-Lagrange equation is that
Suppose there is no gravitational field; i.e., g=0. Then d(mv)/dt=0 and hence the momentum mv is constant. In other words, if the Lagrangian is independent of the height z, or more generally, location in a particular direction then momentum in that direction is conserved.
Consider next the more complex system of a particle of mass m at the end of a mass-less lever arm of length r which is free to rotate about an axis. Let θ be the angle of the lever arm with respect to the horizontal. The linear velocity is then v=r(dθ/dt)=rω. Thus the kinetic energy is K=½mr²ω². (The quantity mr² is called the moment of inertia and denoted I. Thus the kinetic energy could be expressed as K==½Iω². The potential energy is V=mgrsin(θ) where g is the acceleration due to gravity. Therefore the Lagrangian function is L(θ,ω)=½Iω²−mgrsin(θ). The Euler-Lagrange equation for this system is
To work toward a solution multiply each side of the above equation by the corresponding side of the equation ω=dθ/dt. The result is
The above equation can be solved for ω(t)=dθ/dt and the result, in principle, integrated to obtain θ(t).
For a third example, consider an object with a moment of inertia of I spinning about its own axis. Its kinetic energy is then ½Iω² where ω is its angular velocity. There is no potenial energy so the Lagrangian is independent of the angle of position θ. Thus the angular momentum (∂L/∂ω)=Iω is conserved.
In general, the momentum p_{i} associated with a coordinate q_{i} is defined as
With this defintion the Euler-Lagrange equation can be expressed as
Thus if the Lagrangian is independent of q_{i}; i.e., ∂L/∂q_{i}=0; then dp_{i}/dt=0; i.e., p_{i} is constant over time and is said to be conserved.
Noether's Theorem is a generalization of the above. Suppose the coordinates {q_{i}} are a function of a continuous parameter s. According to Noether's Theorem if the Lagrangian is independent of s then there is a quantity that is conserved.
Proof:
Consider a quantity (∂q_{i}/∂s) and its product with the corresponding momentum p_{i}. Call this product H_{i}; i.e.,
Now consider the time derivative of H_{i}:
The order of the differentiations (by t and by s) in the second term on the right may be interchanged to give
Since
the time derivative of H_{i} reduces to
But the right-hand-side of this equation is merely the rate of change of L having to do with the effect of a change in s. It is the change in L which occurs as a result of the effect of the change in s on q_{i} and v_{i}. A change in s may affect all of the coordinates and not just one. If everything is summed over the n coordinates the result is the total derivative of L with respect to s; i.e.,
The left-hand-side is just dH/dt where H=ΣH_{i}. Thus if L is independent of s; i.e., dL/ds=0; then dH/dt=0 and thus H is constant over time; i.e., H is conserved.
Reconsider the case of a body moving in a uniform gravitational field. In that case L(z,v)=½mv²−mgz. Then p=∂L/∂v=mv. Now let the parameter s be just time t. Thus (∂z/∂s)=dz/dt=v. Therefore H=(mv)v=mv²=2K. In this case there is no reason to expect dL/dt to be zero and therefore kinetic energy per se would not be conserved.
First note that the kinetic energy K depends only the v's and does not depend the q's. Furthermore the dependence of K upon the v's is quadratic and such that if all of the v's are multiplied by a factor λ the value of K is multiplied by λ². Thus the kinetic energy function K(v_{1},…,v_{n}) is homogeneous of degree 2.
The potential energy V usually depends only upon the q's.
Now consider the time derivative of the Lagrangian function; i.e.,
By the Euler-Lagrange equation
This means the previous equation can be expressed as
This means that the expression in the square brackets is constant over time; i.e., it is a conserved quantity. Let it be designated J.
If potential energy function V is independent of the v's and also independent of time t then
However K is a homogeneous function of degree 2 so by Euler's Theorem
Thus
So the conserved quantity J is total energy.
The Hamiltonian H for a system is defined in terms of the Lagrangian as
The equations for the dynamics of the system are then
where F_{qi} represents nonconservative external forces or dissipative forces such as frictions that are not represented in terms of the gradients of the potential energy function V. If the kinetic energy function depends only upon products of the v_{i} then H is just the total energy of the system. Then the dynamic equations reduce to
For such systems it immediately follows that if ∂L/∂q_{i}=0 and hence ∂H/∂q_{i}=0 that dp_{i}/dt=0 and therefore p_{i} is conserved. Also if ∂L/∂t=0 then total energy H is conserved.
More generally if
That is to say, momenta changes only due to nonconservative external and dissipative forces.
The Hamiltonian approach to dynamics was generalized by the great Russian mathematician Lev Pontryagin in terms of Optimal Control Theory and the Maximum Principle.
In the above the illustrations of Noether's Theorem involved taking a specific change and showing the conserved quantity. Noether's Theorem is more general. It says that if a transformation of the coordinate system satisfies certain condition, namely being continuous, then necessarily there exist a quantity that is conserved. The exact quantity may not be known but nevertheless it is known that it exists. There may be other transformations, such as the inversion between right and left-handed coordinate systems, which leave the Lagrangian function unchanged but for which there are not conserved quantities.
To go further it is convenient to express the spatial, velocity and momenta coordinates as the vectors Q, V and P, respectively. Then the Lagrangian function is L(Q,V) and the Hamiltonian function is H(Q,P). Now the effect of transformation T on the coordinates is expressed as Q'=T(Q) with a corresponding transformation of the velocities V'=T(V) and of the momenta P'=P(T).
The transformation T could be linear translations or rotations. It could also be a scalar dilation or inflation in Q'=λQ where λ is a scalar. This would be of interest because the universe appears to be undergoing such an inflation.
(To be continued.)
Noether's Theorem applies for continuous transformations of the coordinate system such as linear translations, rotations or time shifts. There are no explicit quantities conserved as a result of the independence of the system to coordinate transformations such as parity transformation (transformations between right-handed and left-handed coordinate systems).
(To be continued.)
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