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This material derives the quantization scheme that exists for particles in a central force field when the orbital angular momentum is quantized. Relativistic conditions are assumed.
Consider a single particle of mass m traveling in a circular orbit of radius r. Let the central force be given by the formula
This is still a completely general case although it is presumed that the force is carried by particles, such as photons or pi mesons, and hence there is a 1/r² dependence. K stands for the force constant and f(r) is a dimensionless quantity. For forces carried by a particle that does not decay such a the electrostatic force or gravity the quantity f(r)=1. For a force carried by a decaying particle such as a meson the quantity f(r) is of the form e^{λr}. The force may be a combination of nuclear force, electrostatic force and gravity. The force may be an attraction or a repulsion, depending upon the sign of K.
For a circular orbit the attractive force must balance the centrifugal force; i.e.,
where c is the speed of light.
Angular momentum is equal to mvr so its quantization is
where n is an integer and h is Planck's constant divided by 2π.
Expressing v as βc this quantization condition along with the condition for a circular orbit are:
The division of the first equation by the second results in
so that if the quantization of r is determined then the quantization of velocity is given by
the above expression. The quantity (K/(hc)) is a dimensionless constant that may be
denoted as γ, a characteristic of the force field. Thus the general relationship, which applies
in both the relativistic and nonrelativistic case, is
For the electrostatic force γ is the fine structure constant 1/137.036. An estimate of γ for the nuclear force is 1.5217246. For more on this quantity γ see Force Constants.
Under relativistic conditions the mass of the particle is given by
The angular momentum condition then takes the form
For convenience let nh/(m_{0}cr) be denoted as D.
The previous equation may be solved for β² as
On the other hand from the general expression previously found for β
Equating the two expressions for β² gives
Replacing D by its defition and carrying out some simple algebraic manipulation gives
The quantity hc/(m_{0}c²) has special significance but it has the
dimensions of length. Let r_{0} be some significant unit of length. The variable r then can
be expressed as r=zr_{0}.
The quantization condition then takes the form
Now let (hc/(r_{0}m_{0}c²)=μ.
The quantization condition then takes the form
The function f(r) could be a constant or it could be e^{−λr}, in which case r_{0}=1/λ. In that case f(zr_{0})=e^{−z}. Let f(zr_{0}) be denoted as φ(z). Then the quantization condition takes the form
This is the condition sought for the quantization of z and r.
The constant hc is equal 3.1616×10^{26} kg m³/s².
For a proton m_{0}c² = 1.503353×10^{10} kg m²/s² (joules).
Then for r_{0}=(0.5)1.522×10^{15} m, the nondimensional constant μ = 27.635116 and μ² = 763.7.
As stated previously an estimate of γ for the nuclear force is 1.5217246 and hence γ²=2.31564583.
For a given value of n the quantization condition may have one solution, no solution or more than one solution.
Let N be the set of values of n for which the quantization condition has solutions and R the set
{r_{n}, n∈N}. Then the set of allowable β's B={β_{n}, n∈N} is given
by β_{n}=f(r_{n})/(nhc).
The kinetic energies κ_{n} are given by
The potential energies are given by
The change in potential energy from n to n1 can be approximated by the trapezoidal rule; i.e., ΔV is approximately equal to ½K[f(r_{n1})/r_{n1}² + f(r_{n})/r_{n}²]Δr.
When a transition in n results in a lower potential energy some of that energy loss goes into an increase in kinetic energy but some of it goes into the energy of an emitted photon. The energy of the emitted photon is then −ΔV  ΔKE and its frequency ν is then given by
The spectrum of the system is the set of ν's for transitions from n_{1} to n_{2} for n_{1} and n_{2} belonging to N.
Some insights into the relationships the spectrum to changes in the angular momentum can be obtained by looking at the partial derivatives of the quantities with respect to n and using the approximation Δy=(∂y/∂n)Δn for Δn=±1.
What is known concerning the potential energy V is that
Likewise it is known that
From the equation β=γf(r)/n it follows that
All that remains is to evaluate (∂r/∂n). For this exercise it is convenient to put the quantization equation γ²φ²(z)[z² + n²μ²] = n^{4}μ² into a simpler form by dividing through by n²μ² and defining (z/(nμ)) as ζ. This results in
Taking the derivative of this equation with respect to n gives
A factor of 2 can be cancelled.
(To be continued.)
For the case in which m=m_{0}, the circular orbit condition gives
When this value of v is substituted into the angular momentum quantization conditon the result is
Division of both sides by hc gives
This is the quantization conditon for the nonrelativistic case.
Thus, if φ(z)=1 then
Then the potential energy is proportional to 1/n² and likewise the kinetic energy. So higher levels of the angular momentum quantum number correspond to greater orbit radii.
For the relativistic case the quantization conditions with φ(z)=1 reduces to
A quantization scheme for particles in a central force field has been established based upon the quantization of angular momentum. This scheme applies for any formula for the central force. The quantization of angular momentum establishes quantization for potential and kinetic energy such that a change in state results in incompatible changes in potential and kinetic energy and the difference must be reconciled by the emission or absorption of a photon.
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