Β§9.1Central Potentials

Part V Phillips pp. 179–185 Β· ~15 min read

  • central potential
  • effective potential
  • centrifugal barrier
  • radial SchrΓΆdinger equation
  • radial quantum number
  • parity

Spherical symmetry buys a separation, and the separation reduces three dimensions to one. What is left is a radial equation with a barrier bolted on.

β€œJust as the solar system provided the first meaningful test of the laws of classical mechanics, the hydrogen atom provided the first meaningful test of the laws of quantum mechanics.” The atom is one electron of charge βˆ’e-e around a nucleus of charge +e+e, and to a first approximation the nucleus is heavy enough to hold still β€” so the whole of chapter 9 is one particle in one potential:

V(r)=βˆ’e24πϡ0r(9.1)V(r) = -\frac{e^2}{4\pi\epsilon_0 r}\tag{9.1}

This section does not solve it. It sets up the machinery for any potential depending only on distance, and that machinery turns out to reduce a three-dimensional problem to a one-dimensional one.

Classically: a force with no torque

A central potential gives a force F=βˆ’(dV/dr) er\mathbf F = -(\mathrm dV/\mathrm dr)\,\mathbf e_r pointing along r\mathbf r. So the torque N=rΓ—F\mathbf N = \mathbf r\times\mathbf F is identically zero, and the angular momentum L\mathbf L is a constant vector.

Two consequences follow immediately. The motion stays in a fixed plane perpendicular to L\mathbf L; and the radius vector sweeps out area at a constant rate:

dA=L2m dt\mathrm d\mathbf A = \frac{\mathbf L}{2m}\,\mathrm dt
Fig. 9.1 β€” equal areas in equal times, for any central force
focuswedge 1: area = 0.31421all 8 wedges span equal TIMEspread across all wedges: 0.219% (sampling error only)

Drag the eccentricity up and the wedges become wildly different in shape β€” short and fat near the focus, long and thin far from it β€” while their areas stay equal to within the sampling error. That is the whole content of dA = (L/2m)Β dt, and it needs nothing about gravity: any central force gives it, because any central force exerts no torque. The areas here are measured from the drawn polygon by the shoelace formula, not asserted. The residual spread is under 0.4% even at e = 0.85.

Splitting the momentum of a planar orbit into radial and transverse parts,

pr=mdrdtandpt=Lrp_r = m\frac{\mathrm dr}{\mathrm dt}\qquad\text{and}\qquad p_t = \frac{L}{r}

the constant total energy becomes

E=pr22m+L22mr2+V(r)(9.2)E = \frac{p_r^2}{2m} + \frac{L^2}{2mr^2} + V(r)\tag{9.2}

The effective potential

Eq. (9.2) is remarkable if you read it right. It has the form of a one-dimensional energy β€” a kinetic term pr2/2mp_r^2/2m in the single variable rr, plus everything else lumped into an effective potential :

Ve(r)=L22mr2+V(r)(9.3)V_e(r) = \frac{L^2}{2mr^2} + V(r)\tag{9.3}

The extra term is the centrifugal barrier . Differentiating gives an outward force L2/mr3L^2/mr^3, which for a particle in a circle of radius rr at speed vv with L=mvrL = mvr is exactly mv2/rmv^2/r β€” the familiar centrifugal force. So the term can be read two ways: as a repulsive potential, or as the transverse kinetic energy the particle must keep because its angular momentum cannot change.

For gravity, V=βˆ’GmM/rV = -GmM/r, this machinery gives the conic sections β€” circles, ellipses, parabolas, hyperbolas. Classical mechanics passed its first extraterrestrial test on planetary orbits precisely because a planet’s angular momentum dwarfs ℏ\hbar: the Earth’s is about 3Γ—1074ℏ3\times10^{74}\hbar.

Quantum mechanically: the same split

A state of definite energy has Ξ¨=ψ(r,ΞΈ,Ο•)eβˆ’iEt/ℏ\Psi = \psi(r,\theta,\phi)e^{-iEt/\hbar} (Eq. 9.4) with

[βˆ’β„22mβˆ‡2+V(r)]ψ=Eψ(9.5)\left[-\frac{\hbar^2}{2m}\nabla^2 + V(r)\right]\psi = E\psi\tag{9.5}

a partial differential equation in three variables. The move that tames it is to ask for a state with definite angular momentum as well as definite energy:

ψ(r,ΞΈ,Ο•)=R(r) Yl,ml(ΞΈ,Ο•)(9.6)\psi(r,\theta,\phi) = R(r)\,Y_{l,m_l}(\theta,\phi)\tag{9.6}

From a 3-D partial differential equation to a 1-D ordinary one

step 1 of 6

Every step is substitution and cancellation. The only physics input is Eq. (8.23), which chapter 8 already established.

  1. 1Write the Laplacian in spherical polars. The first term involves only r; the whole bracket is exactly the angular operator chapter 8 problem 8 wrote down.

The result is the radial SchrΓΆdinger equation , with an effective potential that mirrors the classical Eq. (9.3) exactly:

Ve(r)=l(l+1)ℏ22mr2+V(r)(9.10)V_e(r) = \frac{l(l+1)\hbar^2}{2mr^2} + V(r)\tag{9.10}

Equation (9.9) β€” a one-dimensional equation wearing three-dimensional clothes

symbol
is
the function that actually obeys a 1-D SchrΓΆdinger equation. NOT the radial part R itself β€” the factor of r is what removes the first-derivative term and makes the analogy exact. It is also u, not R, that is normalized by ∫|u|Β²dr = 1.
units
type
real function on the half-line

Click any symbol to see what it is, what units it carries, and what kind of object it is once you put it in an array.

Bound states are labelled by nr=0,1,2,…n_r = 0, 1, 2, \dots, the radial quantum number , which counts the nodes of u(r)u(r) between 00 and ∞\infty. Three numbers therefore specify a state completely:

ψnr,l,ml(r,ΞΈ,Ο•)=unr,l(r)rYl,ml(ΞΈ,Ο•)(9.11)\psi_{n_r,l,m_l}(r,\theta,\phi) = \frac{u_{n_r,l}(r)}{r}Y_{l,m_l}(\theta,\phi)\tag{9.11}

normalized by ∫0∞∣unr,l∣2 dr=1\int_0^\infty|u_{n_r,l}|^2\,\mathrm dr = 1 (Eq. 9.12).

The effective potential, and the radial equation solved in it
02468101214024681012r (Bohr radii)energy (Δ§Ο‰)
E = 2.499987 vs (2n_r+l+3/2) = 2.5000

Section 6.5's three-dimensional oscillator, whose answer we already know. The l(l+1)/2rΒ² barrier wins at small r and loses at large r, so the effective potential turns over. Raising l pushes the minimum outward as l(l+1) and makes it shallower as 1/l(l+1). Solved by the same grid β†’ hamiltonian β†’ eigh pipeline as every other potential on this site β€” because Eq. (9.9) is one-dimensional.

Parity

A state of definite energy in a central potential has one more definite property, and it has no classical analogue at all. Under reflection through the origin, rβ†’βˆ’r\mathbf r \to -\mathbf r, an eigenfunction either keeps its sign,

ψ(βˆ’r)=ψ(r)(9.13)\psi(-\mathbf r) = \psi(\mathbf r)\tag{9.13}

β€” even parity β€” or reverses it,

ψ(βˆ’r)=βˆ’Οˆ(r)(9.14)\psi(-\mathbf r) = -\psi(\mathbf r)\tag{9.14}

β€” odd parity. Using Table 8.1 you can check that ψ=R(r)Yl,ml\psi = R(r)Y_{l,m_l} has even parity for l=0l = 0 and l=2l = 2 and odd parity for l=1l = 1; in general the parity is (βˆ’1)l(-1)^l.

Check yourself

0 / 6 answered

  1. 1.Why does a central potential guarantee that the orbit lies in a fixed plane?

  2. In the widget, raise the eccentricity to 0.8 and step through the wedges.

    2.The wedges change shape dramatically but their areas stay equal. What does that express?

  3. 3.What makes it legitimate to look for states with definite , **and** simultaneously?

  4. 4.Why is the substitution worth making?

  5. 5.A hydrogen state has and . What does count?

  6. 6.Why does the parity of depend only on ?