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 Incoming links: Transmission probability

Put

k = \frac{2 m E}{ℏ}, K = \frac{2 m ( E + V _{0} )}{ℏ} .

ψ (x) = ⎩ ⎨ ⎧ A e^{ik x} + B e^{- ik x}, C e^{i K x} + D e^{- i K x}, F e^{ik x}, x < 0, 0 \leq x \leq a, x > a .

The first region contains the incident and reflected waves, while the final region contains only the transmitted wave.

Continuity of

ψ

and

ψ^{'}

T = \frac{∣ F ∣ ^{2}}{∣ A ∣ ^{2}} = [1 + \frac{( K ^{2} - k ^{2} ) ^{2}}{4 k ^{2} K ^{2}} sin^{2} (K a)]^{- 1} .

When

V_{0} = 3 E

, one has

K = 2 k

, and therefore

\frac{( K ^{2} - k ^{2} ) ^{2}}{4 k ^{2} K ^{2}} = \frac{9}{16}, K a = \frac{a 8 m E}{ℏ} .

T = \frac{16}{16 + 9 sin ^{2} ( a 8 m E /ℏ )} .

For one-dimensional quantum scattering,

t

is the complex amplitude of the outgoing transmitted wave relative to the incoming wave. The transmission probability is

∣ t ∣^{2}

times the ratio of transmitted and incident flux velocities; with equal asymptotic dispersion it is

∣ t ∣^{2}

r = 0

and a unit-modulus transmission amplitude whose phase shifts continuum quantization. The supersymmetric factorization of the one-soliton potential gives

t (k) = (k + im) / (k - im)

for its single-bound-state potential.