Condition to minimum unceirtainty

Sections9
  1. Condition of coherent state
  2. Check
  3. Expectation value of amplitude
  4. Static noise
  5. Momentum variance
  6. Static noise for momentum
  7. Uncertainty product
  8. One more condition
  9. Non-coherent state

Condition of coherent state§

Coherent state have sinusoidal expectation value and static noise, which means

{⟨x⟩=X0cos⁡(ωt−ϕ)⟨p⟩=P0sin⁡(ωt−ϕ)∂tσx2=0∂tσp2=0\begin{cases} \braket{x}&=X_0\cos(\omega t - \phi)\\ \braket{p}&=P_0\sin(\omega t - \phi)\\ \partial_t\sigma^2_x &= 0\\ \partial_t\sigma^2_p &= 0\\ \end{cases}

let's check if this is the sufficient condition for minimum uncertainty

Check§

Unpack everything

Expectation value of amplitude§

Without conceptual connection to the coherent state, let's just call

⟨a⟩=αe−iϕ\braket{a}=\alpha e^{-i\phi}

Note, the derivation below show why should the magnitude be constant

The expectation value of the position,

⟨x⟩=ℏ2mω⟨ψ∣a^eiωt+a^†e−iωt∣ψ⟩=ℏ2mω(⟨a⟩eiωt+⟨a⟩∗e−iωt)=2ℏα2mωcos⁡(ωt−ϕ)\begin{align*} \braket{x}&=\sqrt{\frac{\hbar}{2m\omega}}\bra{\psi}\hat{a}e^{i\omega t}+\hat{a}^\dagger e^{-i\omega t}\ket{\psi}\\ &=\sqrt{\frac{\hbar}{2m\omega}}\left(\braket{a}e^{i\omega t}+\braket{a}^* e^{-i\omega t}\right)\\ &=\sqrt{\frac{2\hbar \alpha^2}{m\omega}}\cos(\omega t - \phi)\\ \end{align*}

If the magnitude of the expectation value is non constant, then this will not be sinusoidal. As the expectation value of the annihilation operator is sufficient to calculate the expectation value of momentum. Let's just have the result as

⟨p⟩=2ℏmωα2sin⁡(ωt−ϕ)\braket{p}=\sqrt{2\hbar m \omega\alpha^2}\sin(\omega t - \phi)

For future use, let's also calculate ⟨x2⟩\braket{x^2} And call

⟨a2⟩=A2e−2iγ\braket{a^2}=A^2e^{-2i\gamma} ⟨x2⟩=ℏ2mω⟨ψ∣a^2e2iωt+(a^†)2e−2iωt+{a^,a^†}∣ψ⟩=ℏ2mω(⟨a2⟩e2iωt+⟨a2⟩∗e−2iωt+2n+1)=ℏmω(A2cos⁡(2ωt−2γ)+n+12)\begin{align*} \braket{x^2}&=\frac{\hbar}{2m\omega}\bra{\psi}\hat{a}^2e^{2i\omega t}+\left(\hat{a}^\dagger\right)^2 e^{-2i\omega t}+\{\hat{a},\hat{a}^\dagger\}\ket{\psi}\\ &=\frac{\hbar}{2m\omega}\left(\braket{a^2}e^{2i\omega t}+\braket{a^2}^* e^{-2i\omega t}+2n+1\right)\\ &=\frac{\hbar}{m\omega}\left(A^2\cos(2\omega t - 2\gamma)+n+\frac{1}{2}\right)\\ \end{align*}

And

⟨x⟩2=ℏα2mω(1+cos⁡(2ωt−2ϕ))\braket{x}^2=\frac{\hbar \alpha^2}{m\omega}\left(1+\cos(2\omega t - 2\phi)\right)

Static noise§

∂tσx2=∂t⟨x2⟩−∂t⟨x⟩2\partial_t\sigma_x^2=\partial_t\braket{x^2}-\partial_t\braket{x}^2

Take the time derivative of each term

∂t⟨x2⟩=−2ℏA2msin⁡(2ωt−2γ)\partial_t \braket{x^2}=-\frac{2\hbar A^2}{m}\sin(2\omega t -2\gamma)

And

∂t⟨x⟩2=−2ℏα2msin⁡(2ωt−2ϕ)\partial_t \braket{x}^2=-\frac{2\hbar\alpha^2}{m}\sin(2\omega t - 2\phi)

Thus

∂tσx2=∂t⟨x2⟩−∂t⟨x⟩2=−2ℏA2msin⁡(2ωt−2γ)+2ℏα2msin⁡(2ωt−2ϕ)=2ℏm[α2sin⁡(2ωt−2ϕ)−A2sin⁡(2ωt−2γ)].\begin{align*} \partial_t \sigma_x^2 &= \partial_t \braket{x^2} - \partial_t \braket{x}^2 \\[4pt] &= -\frac{2\hbar A^2}{m}\sin(2\omega t - 2\gamma) + \frac{2\hbar\alpha^2}{m}\sin(2\omega t - 2\phi) \\[4pt] &= \frac{2\hbar}{m}\Bigl[ \alpha^2 \sin(2\omega t - 2\phi) - A^2 \sin(2\omega t - 2\gamma) \Bigr]. \end{align*}

Momentum variance§

⟨p2⟩=−ℏmω2[⟨a^2⟩e2iωt+⟨a^2⟩∗e−2iωt−(2n+1)]=−ℏmω2[2A2cos⁡(2ωt−2γ)−(2n+1)]=ℏmω(n+12−A2cos⁡(2ωt−2γ)).\begin{align*} \braket{p^2} &= -\frac{\hbar m \omega}{2} \Bigl[ \braket{\hat{a}^2} e^{2i\omega t} + \braket{\hat{a}^2}^* e^{-2i\omega t} - (2n+1) \Bigr] \\[4pt] &= -\frac{\hbar m \omega}{2} \Bigl[ 2A^2\cos(2\omega t - 2\gamma) - (2n+1) \Bigr] \\[4pt] &= \hbar m \omega \Bigl( n + \frac12 - A^2\cos(2\omega t - 2\gamma) \Bigr). \end{align*} ⟨p⟩2=2ℏmω α2sin⁡2(ωt−ϕ)=ℏmω α2[1−cos⁡(2ωt−2ϕ)].\begin{align*} \braket{p}^2 &= 2\hbar m \omega\,\alpha^2 \sin^2(\omega t - \phi) \\[4pt] &= \hbar m \omega\,\alpha^2 \bigl[1 - \cos(2\omega t - 2\phi)\bigr]. \end{align*}

Hence

σp2=⟨p2⟩−⟨p⟩2=ℏmω[n+12−α2+α2cos⁡(2ωt−2ϕ)−A2cos⁡(2ωt−2γ)].\sigma_p^2 = \braket{p^2} - \braket{p}^2 = \hbar m \omega\Bigl[ n + \tfrac12 - \alpha^2 + \alpha^2\cos(2\omega t - 2\phi) - A^2\cos(2\omega t - 2\gamma) \Bigr].

Static noise for momentum§

∂tσp2=2ℏmω2[A2sin⁡(2ωt−2γ)−α2sin⁡(2ωt−2ϕ)].\partial_t \sigma_p^2 = 2\hbar m \omega^2 \Bigl[ A^2 \sin(2\omega t - 2\gamma) - \alpha^2 \sin(2\omega t - 2\phi) \Bigr].

Imposing ∂tσp2=0\partial_t \sigma_p^2 = 0 and ∂tσx2=0\partial_t \sigma_x^2 = 0 gives, for all tt,

A2sin⁡(2ωt−2γ)=α2sin⁡(2ωt−2ϕ).A^2 \sin(2\omega t - 2\gamma) = \alpha^2 \sin(2\omega t - 2\phi).

Equality for all times forces

A2=α2andγ=ϕ(modπ).\boxed{A^2 = \alpha^2 \qquad\text{and}\qquad \gamma = \phi \pmod{\pi}}.

Uncertainty product§

Substituting A=αA = \alpha, γ=ϕ\gamma = \phi,

σx2=ℏmω(n+12−α2),σp2=ℏmω(n+12−α2),\sigma_x^2 = \frac{\hbar}{m\omega}\bigl(n + \tfrac12 - \alpha^2\bigr), \qquad \sigma_p^2 = \hbar m\omega \bigl(n + \tfrac12 - \alpha^2\bigr), σxσp=ℏ(n+12−α2).\sigma_x \sigma_p = \hbar\left(n + \frac12 - \alpha^2\right).

Since n=⟨a^†a^⟩≥∣⟨a^⟩∣2=α2n = \braket{\hat{a}^\dagger \hat{a}} \ge |\braket{\hat{a}}|^2 = \alpha^2,

σxσp≥ℏ2,\sigma_x \sigma_p \ge \frac{\hbar}{2},

Where we can see, n≥α2n \ge \alpha^2 with equality iff n=α2n = \alpha^2.

We already show that the ground state in this system ( note that ground state is not defined by n=0n=0 but rather the lowest energy state possible ) have been shifted. Or even better, all state is shifted uniformly

One more condition§

So, one additional condition needed:

n=α2⟨a^†a^⟩=⟨a^⟩⟨a^†⟩⟨(a^−⟨a^⟩)†(a^−⟨a^⟩)⟩=0.\begin{align*} n &= \alpha^2 \\ \braket{\hat{a}^\dagger \hat{a}} &= \braket{\hat{a}}\braket{\hat{a}^\dagger} \\ \braket{(\hat{a} - \braket{\hat{a}})^\dagger (\hat{a} - \braket{\hat{a}})} &= 0 . \end{align*}

For a pure state this means (a^−⟨a^⟩)∣ψ⟩=0(\hat{a} - \braket{\hat{a}}) |\psi\rangle = 0, i.e. ∣ψ⟩|\psi\rangle is an eigenstate of a^\hat{a}. Or so called, the coherent state.

Non-coherent state§

From this point of view, well maybe we can drop the condition that the noise must be stable, which since we know coherent state isn't that, n=α2n=\alpha^2 must also be droped. Thus, now

σx2=ℏmω(A2cos⁡(2ωt−2γ)+n+12−α2−α2cos⁡(2ωt−2ϕ))\sigma^2_x = \frac{\hbar}{m\omega}\left(A^2\cos(2\omega t - 2\gamma)+n+\frac{1}{2}-\alpha^2-\alpha^2\cos(2\omega t - 2\phi)\right) σp2=ℏmω(n+12−α2+α2cos⁡(2ωt−2ϕ)−A2cos⁡(2ωt−2γ))\sigma^2_p = \hbar m \omega\left( n + \frac{1}{2} - \alpha^2 + \alpha^2\cos(2\omega t - 2\phi) - A^2\cos(2\omega t - 2\gamma) \right)

This simplifies to

mωσx2=ℏ[sinh⁡2r+12+Rcos⁡(2ωt−δ)]m\omega\sigma_x^2 = \hbar\Bigl[ \sinh^2{r} + \tfrac12 + R \cos(2\omega t - \delta) \Bigr] 1mωσp2=ℏ[sinh⁡2r+12−Rcos⁡(2ωt−δ)]\frac{1}{m\omega}\sigma_p^2 = \hbar \Bigl[ \sinh^2{r} + \tfrac12 - R \cos(2\omega t - \delta)\Bigr]

where

R=A4+α4−2A2α2cos⁡(2γ−2ϕ),δ=arctan⁡2 ⁣(A2sin⁡2γ−α2sin⁡2ϕ,  A2cos⁡2γ−α2cos⁡2ϕ).R = \sqrt{ A^4 + \alpha^4 - 2A^2\alpha^2\cos(2\gamma - 2\phi) }, \qquad \delta = \arctan2\!\bigl( A^2\sin 2\gamma - \alpha^2\sin 2\phi,\; A^2\cos 2\gamma - \alpha^2\cos 2\phi \bigr).

And

n−α2=sinh⁡2rn-\alpha^2 = \sinh^2{r}

( Which indeed is quite arbitrary currently, we will derive this later )

This is the squeezed state under free harmonic oscillating force, where the uncertainty of xx and pp oscillate and squeezed into each others periodically.

This gives

σx2σp2=ℏ2[(sinh⁡2r+12)2−R2cos⁡2(2ωt−δ)]\sigma_x^2 \sigma_p^2 = \hbar^2 \Bigl[ \bigl( \sinh^2{r} + \tfrac12 \bigr)^2 - R^2 \cos^2(2\omega t - \delta) \Bigr]

Hence the uncertainty product is

σxσp=ℏ (sinh⁡2r+12)2−R2cos⁡2(2ωt−δ).\sigma_x \sigma_p = \hbar \, \sqrt{ \left( \sinh^2{r} + \frac{1}{2} \right)^2 - R^2 \cos^2(2\omega t - \delta) }.

Which is also oscillating. And periodically dipped to minimum uncertainty.

Discussion

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