l^2 and lz share eigenfunctions, termed Y{lm} functions.
These functions are located on a provided sheet; Y_{lm} functions are on the right-hand side.
When l = 0, the only allowed value for m is 0.
If l = 1, there exist three m values: -1, 0, and +1.
If l = 2, five m values exist: -2, -1, 0, +1, +2.
If l = 3, seven m values exist, ranging from -3 to +3.
The number of m states is defined by 2l + 1. For instance, if l = 2, then 2(2) + 1 = 5, showing five states.
m cannot exceed l because the vector component cannot exceed the vector's magnitude. |m| \leq l
Eigenfunctions of lx and ly exist.
They manifest as linear combinations from the shared eigenfunctions of l^2 and lz, which are the Y{lm} functions.
Y{xlm} eigenfunction is the linear combination of the Y{zl} eigenfunctions.
Example: Y{x1-1} = d1 Y{z1-1} + d2 Y{z10} + d3 Y{z11}. This equation illustrates that \Delta lx \times \Delta l_y > 0.
Measurements:
Measuring the magnitude of l collapses part of the wave function by fixing the quantum number l.
Measuring one component of l further collapses the wave function.
One measurement collapses the wave function to a linear combination.
A subsequent measurement locks it into a specific state.
Once locked into a state with definite l and one component of l, measuring another component yields a distribution.
The Y{xlmx} functions are a linear combination of the Y{z} functions, represented as: Y{xlmx} = e1 Y{zl-1} + e2 Y{zl0} + e3 Y_{zl+1}
The value of m can be subscripted (e.g., mz, mx) to denote a measurement of a particular component of l.
For instance:
Y{z10} = e1 Y{x1-1} + e2 Y{x10} + e3 Y_{x11}
You cannot specify two components of angular momentum at the same time.
Measuring one component leads to a distribution if another component is then measured.
The variable y labels the function in terms of \theta and \phi.
Y_{lm} = \Theta(\theta) \Phi(\phi). It is a product of functions of \theta and \phi.
The term Y{lm} is a label or code for this function, and it's often written without parentheses: Y{lm}.
The sheet contains functions put on the board, it includes both \theta and \phi functions, making it abstract.
Example: For l = 0 and m_z = 0, the state is a constant, indicating spherical symmetry.
Since it is not a function of \theta or \phi, the probability distribution is spherically symmetric.
The solution is constant and \propto \frac{1}{\sqrt{4\pi}}. This constant normalizes the integral over all space:
\int |\Psi|^2 dV = \int |\Psi|^2 r^2 \sin(\theta) d\theta d\phi dr = 1
Constants ensure that integration yields a probability of 1.
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The Y{lm} functions are the shared eigenfunctions of l^2 and lz.
Each Y_{lm} is a product of a function of \theta and a function of \phi.
Even without a \phi dependence, the function can still be an eigenstate of the l_z operator.
The l_z operator only affects the \phi variable.
Every function on the chart is an eigenfunction of l^2.
The provided l^2 operator allows direct verification.
Each eigenfunction satisfies the eigenvalue problem for both the l^2 and l_z operators.
Shared eigenfunctions exist because the two operators commute.
For l = 1, there are three eigenfunctions.
The bottom number indicates the l quantum number, while the top number shows the ml or mz quantum number.
For l = 2, there are five eigenfunctions.
The bottom quantum number is l, determining the magnitude of the angular momentum vector.
The top quantum number represents the z-component.
Again, each function is a product of a function of \theta and a function of \phi.
The fact that components don't commute gives rise to equations of this form.
The component of angular momentum for y_{x1-1} is -1.
Reference is made to a diagram showing the rotation of angular momentum.
The representation of l_z = +1 aligns with the z-direction in the diagram.
Cones in the diagram represent different l_z states.
The states of l = 1 and m_z = +1 indicate the positive z-component.
If an angular momentum vector is in the -1 state, measuring the x-component results in a distribution.
There is no special distinction between the x and z.
The same argument applies to x axis relative to z.
y_{x1-1}: the length is 1.
mx = +1, mx = -1, and m_x = 0.
The inquiry was whether certain combinations could be ruled out; the answer is that the d values aren't always zero.
Symmetry dictates the z-component must be the same as state zero.
There should not be a higher probability of measuring momentum with the rightward component versus the leftward component.
These states do not inherently eliminate specific values.
The same principles apply to x, z, and y directions.
The non-commutation of components leads to relationships such as \Delta lx \Delta ly \propto l_z.
The x and y directions relate to the z direction.
\Delta lx = \Delta ly.
The relationship: \Delta lx^2 = \Delta ly^2 = \frac{1}{2} \langle l_z \rangle
Once a particle is fixed into an lz state, uncertainties in lx and l_y can be calculated.
The equation changes based on lz because when l is larger, the lz components increase, expanding the cone diagram.
The equation for the free particle problem:
-\frac{\hbar^2}{2m} \frac{1}{r} \frac{d}{dr} \left(r \frac{d}{dr} f(r) \right) + \frac{l^2}{2mr^2} + V(r, \theta, \phi) = E f(r)
Each operator acts on a function.
The Hamiltonian in spherical coordinates can be expressed this way.
The full l^2 operator is skipped because it's extensive.
The potential must be substituted and the differential equation solved.
Examples of potentials:
Free particle: V = 0
Coulomb potential: V = -k \frac{Qq}{r}
Particle in a spherical box:
V = 0 for r < R
V = \infty for r > R
Single step potential:V = 0 for r < R
jump to V = V_0 for r > R
Spherical harmonic oscillator: V = \frac{1}{2} k r^2
Each potential leads to different problems.
Eigenfunctions for the free particle are already known.
In Cartesian coordinates, the general solution is:
\Psi(x, y, z) = c1 e^{ikx x} e^{iky y} e^{ikz z}
Substituting x = r \sin(\theta) \cos(\phi), y = r \sin(\theta) \sin(\phi), and z = r \cos(\theta) would also represent an eigenfunction.
This method isn't helpful for understanding our theta and phi.
Choosing specific kx, ky, and k_z values breaks the symmetry of the problem.
We solve the differential equation in spherical coordinates.
f = R(r) Y_{lm}(\theta, \phi)
Substituting this solution into the original equation leads to several terms.
The potential term vanishes in the free particle case.
l^2 operator acting on its eigenfunction yields a constant times the eigenfunction.
The original equation simplifies to:
-\frac{\hbar^2}{2m} \frac{1}{r} \frac{d}{dr} \left(r \frac{d}{dr} R(r) Y{lm}(\theta, \phi) \right) + \frac{l^2}{2mr^2} R(r) Y{lm}(\theta, \phi) = E R(r) Y_{lm}(\theta, \phi)
Dividing each term by R(r) Y_{lm}(\theta, \phi) simplifies the equation.
The resulting differential equation depends on the value of l.
For l = 0, the equation simplifies significantly, where u(r)=rR(r).
The equation is:
-\frac{\hbar^2}{2m} \frac{d^2 u(r)}{dr^2} = E u(r)
Rearranging gives:
\frac{d^2 u(r)}{dr^2} = -\frac{2mE}{\hbar^2} u(r)
The constant is expected to be negative.
Trial solution: u(r) = C \cos(\alpha r)
Taking derivatives: \frac{d^2}{dr^2} C \cos(\alpha r) = -\alpha^2 C \cos(\alpha r)
Equating coefficients: \alpha^2 C \cos(\alpha r) = \frac{2mE}{\hbar^2} C \cos(\alpha r)
Therefore, R(r) = \frac{u(r)}{r} = \frac{C_1}{r} \cos(\alpha r) (for l=0).
One solution is proportional to \frac{\cos(\alpha r)}{r}.
R(r) = \frac{C_1}{r} \cos(\alpha r) \frac{1}{\sqrt{4\pi}}.
The graph of the radial function resembles a decreasing cosine wave.
Another solution is obtained using sine: R(r) = \frac{C_2}{r} \sin(\alpha r).
\lim_{x \to 0} \frac{\sin(x)}{x} = 1
Though \frac{\sin(x)}{x} goes to 1, the radial solution R(r) the function goes to positive infinity.
The probability of finding a particle is calculated by integrating the wave function squared.
When using r, theta, and phi, the volume element is dV = r^2 \sin(\theta) dr d\theta d\phi.
The Jacobian ensures the volume element is correctly accounted for.
The expression is:
P(r \text{ to } r + dr) = |\Psi|^2 r^2 \sin(\theta) dr d\theta d\phi
The radial component of a 3D probability density has units of (length)^{-3/2}.
* The wave function squared is a 3D probability density.
After plotting an equation squared, the function increases with the square of the radius. Right.
Therefore, the probability function will not blow up to infinity.
The momentum of the particle isn't specified.
For the 3D problem with x, y, and z, the energy eigenfunction also determines the momentum direction.
The original solution \Psi(x, y, z) = c1 e^{ikx x} e^{iky y} e^{ikz z} gave both energy and momentum components.
There are two factors here, magnitude and direction of energy, and also each component of momentum.
The Hamiltonian commutes with the px, py, and pz operators because they were shared eigenfunctions.
Not for one particular value of solutions that are complicated when it comes to measuring momentum.
The question is: if the momentum is measured, will a single vector be obtained, or will a distribution be observed?
The function is perfectly symmetric
The measurement of momentum would yield many values.
This function isn't an eigenfunction of the px operator.
All possible solutions could have momentum in any direction.