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{{Other uses|Rotation operator (disambiguation)}} | |||
{{Quantum mechanics}} | |||
This article concerns the '''[[rotation]] [[Operator (physics)|operator]]''', as it appears in [[quantum mechanics]]. | |||
==Quantum mechanical rotations== | |||
With every physical rotation R, we postulate a quantum mechanical rotation operator D(R) which rotates quantum mechanical states. | |||
:<math>| \alpha \rangle_R = D(R) |\alpha \rangle</math> | |||
In terms of the generators of rotation, | |||
:<math>D (\mathbf{\hat n},\phi) = \exp \left( -i \phi \frac{\mathbf{\hat n} \cdot \mathbf J }{ \hbar} \right)</math> | |||
Please see [http://students.washington.edu/tkarin/rotations.pdf "rotations in quantum mechanics"] for details. | |||
==The translation operator== | |||
The [[rotation]] [[Operator (physics)|operator]] <math>\,\mbox{R}(z, \theta)</math>, with the first argument <math>\,z</math> indicating the rotation [[Cartesian coordinate system|axis]] and the second <math>\,\theta</math> the rotation angle, can operate through the [[Displacement operator|translation operator]] <math>\,\mbox{T}(a)</math> for infinitesimal rotations as explained below. This is why, it is first shown how the translation operator is acting on a particle at position x (the particle is then in the [[quantum state|state]] <math>|x\rangle</math> according to [[Quantum Mechanics]]). | |||
Translation of the particle at position x to position x+a: <math>\mbox{T}(a)|x\rangle = |x + a\rangle</math> | |||
Because a translation of 0 does not change the position of the particle, we have (with 1 meaning the [[identity function|identity operator]], which does nothing): | |||
:<math>\,\mbox{T}(0) = 1</math> | |||
:<math>\,\mbox{T}(a) \mbox{T}(da)|x\rangle = \mbox{T}(a)|x + da\rangle = |x + a + da\rangle = \mbox{T}(a + da)|x\rangle \Rightarrow</math> | |||
:<math>\,\mbox{T}(a) \mbox{T}(da) = \mbox{T}(a + da)</math> | |||
[[Taylor series|Taylor]] development gives: | |||
:<math>\,\mbox{T}(da) = \mbox{T}(0) + \frac{d\mbox{T}(0)}{da} da + ... = 1 - \frac{i}{h}\ p_x\ da</math> | |||
with | |||
:<math>\,p_x = i h \frac{d\mbox{T}(0)}{da}</math> | |||
From that follows: | |||
:<math>\,\mbox{T}(a + da) = \mbox{T}(a) \mbox{T}(da) = \mbox{T}(a)\left(1 - \frac{i}{h} p_x da\right) \Rightarrow</math> | |||
:<math>\,[\mbox{T}(a + da) - \mbox{T}(a)]/da = \frac{d\mbox{T}}{da} = - \frac{i}{h} p_x \mbox{T}(a)</math> | |||
This is a [[differential equation]] with the solution <math>\,\mbox{T}(a) = \mbox{exp}\left(- \frac{i}{h} p_x a\right)</math>. | |||
Additionally, suppose a [[Hamilton's equations|Hamiltonian]] <math>\,H</math> is independent of the <math>\,x</math> position. Because the translation operator can be written in terms of <math>\,p_x</math>, and <math>\,[p_x,H]=0</math>, we know that <math>\,[H,\mbox{T}(a)]=0</math>. This result means that linear [[momentum]] for the system is conserved. | |||
==In relation to the orbital angular momentum== | |||
Classically we have for the [[angular momentum]] <math>\,l = r \times p</math>. This is the same in [[quantum mechanics]] considering <math>\,r</math> and <math>\,p</math> as operators. Classically, an infinitesimal rotation <math>\,dt</math> of the vector r=(x,y,z) about the z-axis to r'=(x',y',z) leaving z unchanged can be expressed by the following infinitesimal translations (using [[Taylor series|Taylor approximation]]): | |||
:<math>\,x' = r \cos(t + dt) = x - y dt + ...</math> | |||
:<math>\,y' = r \sin(t + dt) = y + x dt + ...</math> | |||
From that follows for states: | |||
:<math>\,\mbox{R}(z, dt)|r\rangle</math><math>= \mbox{R}(z, dt)|x, y, z\rangle</math><math>= |x - y dt, y + x dt, z\rangle</math><math>= \mbox{T}_x(-y dt) \mbox{T}_y(x dt)|x, y, z\rangle</math><math>= \mbox{T}_x(-y dt) \mbox{T}_y(x dt)|r\rangle</math> | |||
And consequently: | |||
:<math>\,\mbox{R}(z, dt) = \mbox{T}_x (-y dt) \mbox{T}_y(x dt)</math> | |||
Using <math>\,T_k(a) = \exp\left(- \frac{i}{h}\ p_k\ a\right)</math> from above with <math>\,k = x,y</math> and Taylor development we get: | |||
:<math>\,\mbox{R}(z, dt) = \exp\left[- \frac{i}{h}\ (x p_y - y p_x) dt\right]</math><math>= \exp\left(- \frac{i}{h}\ l_z dt\right) = 1 - \frac{i}{h} l_z dt + ...</math> | |||
with l<sub>z</sub> = x p<sub>y</sub> - y p<sub>x</sub> the z-component of the angular momentum according to the classical [[cross product]]. | |||
To get a rotation for the angle <math>\,t</math>, we construct the following differential equation using the condition <math>\mbox{R}(z, 0) = 1</math>: | |||
:<math>\,\mbox{R}(z, t + dt) = \mbox{R}(z, t) \mbox{R}(z, dt) \Rightarrow</math> | |||
:<math>\,[\mbox{R}(z, t + dt) - \mbox{R}(z, t)]/dt = d\mbox{R}/dt</math><math>\,= \mbox{R}(z, t) [\mbox{R}(z, dt) - 1]/dt</math><math>\,= - \frac{i}{h} l_z \mbox{R}(z, t) \Rightarrow</math> | |||
:<math>\,\mbox{R}(z, t) = \exp\left(- \frac{i}{h}\ t\ l_z\right)</math> | |||
Similar to the translation operator, if we are given a Hamiltonian <math>\,H</math> which rotationally symmetric about the z axis, <math>\,[l_z,H]=0</math> implies <math>\,[\mbox{R}(z,t),H]=0</math>. This result means that angular momentum is conserved. | |||
For the spin angular momentum about the y-axis we just replace <math>\,l_z</math> with <math>\,S_y = \frac{h}{2} \sigma_y</math> and we get the [[spin (physics)|spin]] rotation operator <math>\,\mbox{D}(y, t) = \exp\left(- i \frac{t}{2} \sigma_y\right)</math>. | |||
==Effect on the spin operator and quantum states== | |||
{{Main|Spin (physics)#Spin and rotations}} | |||
Operators can be represented by [[Matrix (mathematics)|matrices]]. From [[linear algebra]] one knows that a certain matrix <math>\,A</math> can be represented in another [[basis (linear algebra)|basis]] through the transformation | |||
:<math>\,A' = P A P^{-1}</math> | |||
where <math>\,P</math> is the basis transformation matrix. If the vectors <math>\,b</math> respectively <math>\,c</math> are the z-axis in one basis respectively another, they are perpendicular to the y-axis with a certain angle <math>\,t</math> between them. The spin operator <math>\,S_b</math> in the first basis can then be transformed into the spin operator <math>\,S_c</math> of the other basis through the following transformation: | |||
:<math>\,S_c = \mbox{D}(y, t) S_b \mbox{D}^{-1}(y, t)</math> | |||
From standard quantum mechanics we have the known results <math>\,S_b |b+\rangle = \frac{\hbar}{2} |b+\rangle</math> and <math>\,S_c |c+\rangle = \frac{\hbar}{2} |c+\rangle</math> where <math>\,|b+\rangle</math> and <math>\,|c+\rangle</math> are the top spins in their corresponding bases. So we have: | |||
:<math>\,\frac{\hbar}{2} |c+\rangle = S_c |c+\rangle = \mbox{D}(y, t) S_b \mbox{D}^{-1}(y, t) |c+\rangle \Rightarrow</math> | |||
:<math>\,S_b \mbox{D}^{-1}(y, t) |c+\rangle = \frac{\hbar}{2} \mbox{D}^{-1}(y, t) |c+\rangle</math> | |||
Comparison with <math>\,S_b |b+\rangle = \frac{\hbar}{2} |b+\rangle</math> yields <math>\,|b+\rangle = D^{-1}(y, t) |c+\rangle</math>. | |||
This means that if the state <math>\,|c+\rangle</math> is rotated about the y-axis by an angle <math>\,t</math>, it becomes the state <math>\,|b+\rangle</math>, a result that can be generalized to arbitrary axes. It is important, for instance, in [[Sakurai's Bell inequality]]. | |||
==See also== | |||
*[[Symmetry in quantum mechanics]] | |||
*[[Spherical basis]] | |||
==References== | |||
*L.D. Landau and E.M. Lifshitz: ''Quantum Mechanics: Non-Relativistic Theory'', Pergamon Press, 1985 | |||
*P.A.M. Dirac: ''The Principles of Quantum Mechanics'', Oxford University Press, 1958 | |||
*R.P. Feynman, R.B. Leighton and M. Sands: ''The Feynman Lectures on Physics'', Addison-Wesley, 1965 | |||
*Karin, Todd. [http://students.washington.edu/tkarin/rotations.pdf ''Rotations in Quantum Mechanics.''] Unpublished Work. | |||
==See also== | |||
*[[Optical phase space]] | |||
{{Physics operator}} | |||
{{DEFAULTSORT:Rotation Operator (Quantum Mechanics)}} | |||
[[Category:Rotational symmetry]] | |||
[[Category:Quantum mechanics]] |
Revision as of 12:30, 15 January 2014
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This article concerns the rotation operator, as it appears in quantum mechanics.
Quantum mechanical rotations
With every physical rotation R, we postulate a quantum mechanical rotation operator D(R) which rotates quantum mechanical states.
In terms of the generators of rotation,
Please see "rotations in quantum mechanics" for details.
The translation operator
The rotation operator , with the first argument indicating the rotation axis and the second the rotation angle, can operate through the translation operator for infinitesimal rotations as explained below. This is why, it is first shown how the translation operator is acting on a particle at position x (the particle is then in the state according to Quantum Mechanics).
Translation of the particle at position x to position x+a:
Because a translation of 0 does not change the position of the particle, we have (with 1 meaning the identity operator, which does nothing):
Taylor development gives:
with
From that follows:
This is a differential equation with the solution .
Additionally, suppose a Hamiltonian is independent of the position. Because the translation operator can be written in terms of , and , we know that . This result means that linear momentum for the system is conserved.
In relation to the orbital angular momentum
Classically we have for the angular momentum . This is the same in quantum mechanics considering and as operators. Classically, an infinitesimal rotation of the vector r=(x,y,z) about the z-axis to r'=(x',y',z) leaving z unchanged can be expressed by the following infinitesimal translations (using Taylor approximation):
From that follows for states:
And consequently:
Using from above with and Taylor development we get:
with lz = x py - y px the z-component of the angular momentum according to the classical cross product.
To get a rotation for the angle , we construct the following differential equation using the condition :
Similar to the translation operator, if we are given a Hamiltonian which rotationally symmetric about the z axis, implies . This result means that angular momentum is conserved.
For the spin angular momentum about the y-axis we just replace with and we get the spin rotation operator .
Effect on the spin operator and quantum states
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Operators can be represented by matrices. From linear algebra one knows that a certain matrix can be represented in another basis through the transformation
where is the basis transformation matrix. If the vectors respectively are the z-axis in one basis respectively another, they are perpendicular to the y-axis with a certain angle between them. The spin operator in the first basis can then be transformed into the spin operator of the other basis through the following transformation:
From standard quantum mechanics we have the known results and where and are the top spins in their corresponding bases. So we have:
This means that if the state is rotated about the y-axis by an angle , it becomes the state , a result that can be generalized to arbitrary axes. It is important, for instance, in Sakurai's Bell inequality.
See also
References
- L.D. Landau and E.M. Lifshitz: Quantum Mechanics: Non-Relativistic Theory, Pergamon Press, 1985
- P.A.M. Dirac: The Principles of Quantum Mechanics, Oxford University Press, 1958
- R.P. Feynman, R.B. Leighton and M. Sands: The Feynman Lectures on Physics, Addison-Wesley, 1965
- Karin, Todd. Rotations in Quantum Mechanics. Unpublished Work.
See also
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