Three dimensions:

Three-dimensional infinite square well:
E = Ex + Ey + Ez.    E = nx2π2ħ2/(2mLx2)  + ny2π2ħ2/(2mLy2) + nz2π2ħ2/(2mLz2).  

Orbital angular momentum:
In three dimensions, for  a potential energy function U(x,y,z) = U(r), the solutions of the time-independent Schroedinger equation are
ψnlm(r,θ,ϕ) = Rnl(r)Ylm(θ,ϕ).

The spherical harmonics Ylm(θ,ϕ) are eigenfunctions of the operator L2, which is the operator for the square of the magnitude of the orbital angular momentum.
L2Ylm(θ,ϕ) = l(l+1)ħ2Ylm(θ,ϕ),  l = 0, 1, 2, ... .
The magnitude of the angular momentum is quantized.  The only possible outcomes of a measurement are  (l(l + 1)ħ2.

The Ylm(θ,ϕ) are also eigenfunctions of the operator Lz, which is the operator for the z-component of the orbital angular momentum.
LzYlm(θ,ϕ) = Ylm(θ,ϕ),  m = 0, ±1, ±2, ... ±l. 
The  z-component  of the angular momentum is quantized.  The only possible outcomes of a measurement are .

Tunneling:
The transmittance T is the probability that a particle will tunnel through a barrier. 
T = exp(-2bL) with b = (2m(U0-E)/
ħ2)1/2
T decreases as the difference between the height of the barrier U0 and the particle energy increases, and it is smaller for a more massive particle and for a wider barrier.