This page is a convention-fixed translation sheet for closed-system quantum pictures. The general derivation is given in Picture Transformations . The broader Translation Table of Formulations compares pictures, kernels, path integrals, and phase-space methods conceptually; this page focuses narrowly on exact state-operator conversions and the signs that most often cause errors.
Let R ( t ) R(t) R ( t ) be differentiable and unitary. The formulas hold directly for finite matrices; for unbounded observables require the transformed domains and derivatives to exist. Define picture P P P from the Schrödinger picture by
∣ ψ P ( t ) ⟩ = R † ( t ) ∣ ψ S ( t ) ⟩ . \lvert\psi_P(t)\rangle
=
R^\dagger(t)
\lvert\psi_S(t)\rangle. ∣ ψ P ( t )⟩ = R † ( t ) ∣ ψ S ( t )⟩ .
To preserve matrix elements, transform observables and density operators as
A P ( t ) = R † ( t ) A S ( t ) R ( t ) , A_P(t)
=
R^\dagger(t)A_S(t)R(t), A P ( t ) = R † ( t ) A S ( t ) R ( t ) ,
ρ P ( t ) = R † ( t ) ρ S ( t ) R ( t ) . \rho_P(t)
=
R^\dagger(t)\rho_S(t)R(t). ρ P ( t ) = R † ( t ) ρ S ( t ) R ( t ) .
The transformed state obeys a Schrödinger equation with
H P ( t ) = R † ( t ) H S ( t ) R ( t ) − i ℏ R † ( t ) R ˙ ( t ) . H_P(t)
=
R^\dagger(t)H_S(t)R(t)
-
i\hbar R^\dagger(t)\dot R(t). H P ( t ) = R † ( t ) H S ( t ) R ( t ) − i ℏ R † ( t ) R ˙ ( t ) .
Every table below uses this dagger convention. Some sources instead define ∣ ψ P ⟩ = R ∣ ψ S ⟩ \lvert\psi_P\rangle=R\lvert\psi_S\rangle ∣ ψ P ⟩ = R ∣ ψ S ⟩ ; their formulas are valid but have the daggers and connection-term sign reversed.
Object
Schrödinger to picture P P P
Picture P P P to Schrödinger
state vector
∣ ψ P ⟩ = R † ∣ ψ S ⟩ \lvert\psi_P\rangle=R^\dagger\lvert\psi_S\rangle ∣ ψ P ⟩ = R † ∣ ψ S ⟩
∣ ψ S ⟩ = R ∣ ψ P ⟩ \lvert\psi_S\rangle=R\lvert\psi_P\rangle ∣ ψ S ⟩ = R ∣ ψ P ⟩
bra
⟨ ψ P ∣ = ⟨ ψ S ∣ R \langle\psi_P\rvert=\langle\psi_S\rvert R ⟨ ψ P ∣ = ⟨ ψ S ∣ R
⟨ ψ S ∣ = ⟨ ψ P ∣ R † \langle\psi_S\rvert=\langle\psi_P\rvert R^\dagger ⟨ ψ S ∣ = ⟨ ψ P ∣ R †
observable
A P = R † A S R A_P=R^\dagger A_SR A P = R † A S R
A S = R A P R † A_S=RA_PR^\dagger A S = R A P R †
density operator
ρ P = R † ρ S R \rho_P=R^\dagger\rho_SR ρ P = R † ρ S R
ρ S = R ρ P R † \rho_S=R\rho_PR^\dagger ρ S = R ρ P R †
energy observable
E P = R † H S R E_P=R^\dagger H_SR E P = R † H S R
H S = R E P R † H_S=RE_PR^\dagger H S = R E P R †
state generator
H P = R † H S R − i ℏ R † R ˙ H_P=R^\dagger H_SR-i\hbar R^\dagger\dot R H P = R † H S R − i ℏ R † R ˙
H S = R H P R † + i ℏ R ˙ R † H_S=RH_PR^\dagger+i\hbar\dot R R^\dagger H S = R H P R † + i ℏ R ˙ R †
evolution operator
U P ( t , t 0 ) = R † ( t ) U S ( t , t 0 ) R ( t 0 ) U_P(t,t_0)=R^\dagger(t)U_S(t,t_0)R(t_0) U P ( t , t 0 ) = R † ( t ) U S ( t , t 0 ) R ( t 0 )
U S ( t , t 0 ) = R ( t ) U P ( t , t 0 ) R † ( t 0 ) U_S(t,t_0)=R(t)U_P(t,t_0)R^\dagger(t_0) U S ( t , t 0 ) = R ( t ) U P ( t , t 0 ) R † ( t 0 )
The two endpoint factors in the evolution-operator row are essential. Setting R ( t 0 ) = I R(t_0)=I R ( t 0 ) = I is convenient, but it is a convention rather than an identity that holds for every transformation.
For pure states,
⟨ A ⟩ t = ⟨ ψ S ( t ) ∣ A S ( t ) ∣ ψ S ( t ) ⟩ = ⟨ ψ P ( t ) ∣ A P ( t ) ∣ ψ P ( t ) ⟩ . \begin{aligned}
\langle A\rangle_t
&=
\langle\psi_S(t)\rvert
A_S(t)
\lvert\psi_S(t)\rangle
\\
&=
\langle\psi_P(t)\rvert
A_P(t)
\lvert\psi_P(t)\rangle.
\end{aligned} ⟨ A ⟩ t = ⟨ ψ S ( t )∣ A S ( t ) ∣ ψ S ( t )⟩ = ⟨ ψ P ( t )∣ A P ( t ) ∣ ψ P ( t )⟩ .
For mixed states,
⟨ A ⟩ t = Tr [ ρ S ( t ) A S ( t ) ] = Tr [ ρ P ( t ) A P ( t ) ] . \begin{aligned}
\langle A\rangle_t
&=
\operatorname{Tr}
\left[
\rho_S(t)A_S(t)
\right]
\\
&=
\operatorname{Tr}
\left[
\rho_P(t)A_P(t)
\right].
\end{aligned} ⟨ A ⟩ t = Tr [ ρ S ( t ) A S ( t ) ] = Tr [ ρ P ( t ) A P ( t ) ] .
The second equality uses unitarity and cyclicity of the trace. A picture is a change of mathematical representatives, not a change in the predicted probability distribution.
Transition amplitudes are likewise invariant when endpoint states and the evolution operator are translated consistently:
⟨ ϕ P ( t ) ∣ U P ( t , t 0 ) ∣ ψ P ( t 0 ) ⟩ = ⟨ ϕ S ( t ) ∣ U S ( t , t 0 ) ∣ ψ S ( t 0 ) ⟩ . \langle\phi_P(t)\rvert
U_P(t,t_0)
\lvert\psi_P(t_0)\rangle
=
\langle\phi_S(t)\rvert
U_S(t,t_0)
\lvert\psi_S(t_0)\rangle. ⟨ ϕ P ( t )∣ U P ( t , t 0 ) ∣ ψ P ( t 0 )⟩ = ⟨ ϕ S ( t )∣ U S ( t , t 0 ) ∣ ψ S ( t 0 )⟩ .
Let U ( t , t 0 ) U(t,t_0) U ( t , t 0 ) be the full Schrödinger-picture evolution operator and choose
R ( t ) = U ( t , t 0 ) , R ( t 0 ) = I . R(t)=U(t,t_0),
\qquad
R(t_0)=I. R ( t ) = U ( t , t 0 ) , R ( t 0 ) = I .
Then
Object
Schrödinger picture
Heisenberg picture
state
∣ ψ S ( t ) ⟩ = U ( t , t 0 ) ∣ ψ S ( t 0 ) ⟩ \lvert\psi_S(t)\rangle=U(t,t_0)\lvert\psi_S(t_0)\rangle ∣ ψ S ( t )⟩ = U ( t , t 0 ) ∣ ψ S ( t 0 )⟩
∣ ψ H ⟩ = ∣ ψ S ( t 0 ) ⟩ \lvert\psi_H\rangle=\lvert\psi_S(t_0)\rangle ∣ ψ H ⟩ = ∣ ψ S ( t 0 )⟩
observable
A S ( t ) A_S(t) A S ( t )
A H ( t ) = U † ( t , t 0 ) A S ( t ) U ( t , t 0 ) A_H(t)=U^\dagger(t,t_0)A_S(t)U(t,t_0) A H ( t ) = U † ( t , t 0 ) A S ( t ) U ( t , t 0 )
density operator
ρ S ( t ) = U ρ S ( t 0 ) U † \rho_S(t)=U\rho_S(t_0)U^\dagger ρ S ( t ) = U ρ S ( t 0 ) U †
ρ H = ρ S ( t 0 ) \rho_H=\rho_S(t_0) ρ H = ρ S ( t 0 )
state generator
H S ( t ) H_S(t) H S ( t )
H H s t a t e = 0 H_H^{\rm state}=0 H H state = 0
state propagator
U ( t , t 0 ) U(t,t_0) U ( t , t 0 )
U H ( t , t 0 ) = I U_H(t,t_0)=I U H ( t , t 0 ) = I
The notation H H s t a t e = 0 H_H^{\rm state}=0 H H state = 0 means that the transformed state equation has zero generator. The Hamiltonian can still be treated as an observable,
H H o b s ( t ) = U † ( t , t 0 ) H S ( t ) U ( t , t 0 ) , H_H^{\rm obs}(t)
=
U^\dagger(t,t_0)H_S(t)U(t,t_0), H H obs ( t ) = U † ( t , t 0 ) H S ( t ) U ( t , t 0 ) ,
and it need not vanish. Keeping these two roles distinct avoids the misleading statement that “the Hamiltonian is zero in the Heisenberg picture.”
The inverse observable translation is
A S ( t ) = U ( t , t 0 ) A H ( t ) U † ( t , t 0 ) . A_S(t)
=
U(t,t_0)A_H(t)U^\dagger(t,t_0). A S ( t ) = U ( t , t 0 ) A H ( t ) U † ( t , t 0 ) .
The Heisenberg operator equation is
d A H d t = i ℏ [ H H o b s ( t ) , A H ( t ) ] + U † ( t , t 0 ) ∂ A S ∂ t U ( t , t 0 ) . \frac{dA_H}{dt}
=
\frac{i}{\hbar}
[H_H^{\rm obs}(t),A_H(t)]
+
U^\dagger(t,t_0)
\frac{\partial A_S}{\partial t}
U(t,t_0). d t d A H = ℏ i [ H H obs ( t ) , A H ( t )] + U † ( t , t 0 ) ∂ t ∂ A S U ( t , t 0 ) .
The last term is present when the Schrödinger-picture observable has explicit time dependence.
Split the Hamiltonian as
H S ( t ) = H 0 ( t ) + V ( t ) . H_S(t)
=
H_0(t)+V(t). H S ( t ) = H 0 ( t ) + V ( t ) .
Let U 0 ( t , t 0 ) U_0(t,t_0) U 0 ( t , t 0 ) solve
i ℏ ∂ U 0 ∂ t = H 0 ( t ) U 0 ( t , t 0 ) , U 0 ( t 0 , t 0 ) = I . i\hbar\frac{\partial U_0}{\partial t}
=
H_0(t)U_0(t,t_0),
\qquad
U_0(t_0,t_0)=I. i ℏ ∂ t ∂ U 0 = H 0 ( t ) U 0 ( t , t 0 ) , U 0 ( t 0 , t 0 ) = I .
Choose R ( t ) = U 0 ( t , t 0 ) R(t)=U_0(t,t_0) R ( t ) = U 0 ( t , t 0 ) . Then
Object
Schrödinger picture
Interaction picture
state
∣ ψ S ( t ) ⟩ \lvert\psi_S(t)\rangle ∣ ψ S ( t )⟩
∣ ψ I ( t ) ⟩ = U 0 † ( t , t 0 ) ∣ ψ S ( t ) ⟩ \lvert\psi_I(t)\rangle=U_0^\dagger(t,t_0)\lvert\psi_S(t)\rangle ∣ ψ I ( t )⟩ = U 0 † ( t , t 0 ) ∣ ψ S ( t )⟩
observable
A S ( t ) A_S(t) A S ( t )
A I ( t ) = U 0 † ( t , t 0 ) A S ( t ) U 0 ( t , t 0 ) A_I(t)=U_0^\dagger(t,t_0)A_S(t)U_0(t,t_0) A I ( t ) = U 0 † ( t , t 0 ) A S ( t ) U 0 ( t , t 0 )
density operator
ρ S ( t ) \rho_S(t) ρ S ( t )
ρ I ( t ) = U 0 † ( t , t 0 ) ρ S ( t ) U 0 ( t , t 0 ) \rho_I(t)=U_0^\dagger(t,t_0)\rho_S(t)U_0(t,t_0) ρ I ( t ) = U 0 † ( t , t 0 ) ρ S ( t ) U 0 ( t , t 0 )
state generator
H 0 ( t ) + V ( t ) H_0(t)+V(t) H 0 ( t ) + V ( t )
V I ( t ) = U 0 † ( t , t 0 ) V ( t ) U 0 ( t , t 0 ) V_I(t)=U_0^\dagger(t,t_0)V(t)U_0(t,t_0) V I ( t ) = U 0 † ( t , t 0 ) V ( t ) U 0 ( t , t 0 )
evolution operator
U ( t , t 0 ) U(t,t_0) U ( t , t 0 )
U I ( t , t 0 ) = U 0 † ( t , t 0 ) U ( t , t 0 ) U_I(t,t_0)=U_0^\dagger(t,t_0)U(t,t_0) U I ( t , t 0 ) = U 0 † ( t , t 0 ) U ( t , t 0 )
The inverse translations are
∣ ψ S ( t ) ⟩ = U 0 ( t , t 0 ) ∣ ψ I ( t ) ⟩ , \lvert\psi_S(t)\rangle
=
U_0(t,t_0)
\lvert\psi_I(t)\rangle, ∣ ψ S ( t )⟩ = U 0 ( t , t 0 ) ∣ ψ I ( t )⟩ ,
A S ( t ) = U 0 ( t , t 0 ) A I ( t ) U 0 † ( t , t 0 ) , A_S(t)
=
U_0(t,t_0)
A_I(t)
U_0^\dagger(t,t_0), A S ( t ) = U 0 ( t , t 0 ) A I ( t ) U 0 † ( t , t 0 ) ,
and similarly for ρ S \rho_S ρ S . The interaction-picture evolution satisfies
i ℏ ∂ U I ∂ t = V I ( t ) U I ( t , t 0 ) . i\hbar
\frac{\partial U_I}{\partial t}
=
V_I(t)U_I(t,t_0). i ℏ ∂ t ∂ U I = V I ( t ) U I ( t , t 0 ) .
No approximation has been made. Approximation enters only when U I U_I U I , V I V_I V I , or the Dyson series is truncated or simplified.
At t 0 t_0 t 0 , choose all three pictures to coincide. Since
U ( t , t 0 ) = U 0 ( t , t 0 ) U I ( t , t 0 ) , U(t,t_0)
=
U_0(t,t_0)U_I(t,t_0), U ( t , t 0 ) = U 0 ( t , t 0 ) U I ( t , t 0 ) ,
the interaction and Heisenberg representatives are related by U I U_I U I :
Object
Interaction to Heisenberg
Heisenberg to interaction
state
∣ ψ H ⟩ = U I † ( t , t 0 ) ∣ ψ I ( t ) ⟩ \lvert\psi_H\rangle=U_I^\dagger(t,t_0)\lvert\psi_I(t)\rangle ∣ ψ H ⟩ = U I † ( t , t 0 ) ∣ ψ I ( t )⟩
∣ ψ I ( t ) ⟩ = U I ( t , t 0 ) ∣ ψ H ⟩ \lvert\psi_I(t)\rangle=U_I(t,t_0)\lvert\psi_H\rangle ∣ ψ I ( t )⟩ = U I ( t , t 0 ) ∣ ψ H ⟩
observable
A H ( t ) = U I † ( t , t 0 ) A I ( t ) U I ( t , t 0 ) A_H(t)=U_I^\dagger(t,t_0)A_I(t)U_I(t,t_0) A H ( t ) = U I † ( t , t 0 ) A I ( t ) U I ( t , t 0 )
A I ( t ) = U I ( t , t 0 ) A H ( t ) U I † ( t , t 0 ) A_I(t)=U_I(t,t_0)A_H(t)U_I^\dagger(t,t_0) A I ( t ) = U I ( t , t 0 ) A H ( t ) U I † ( t , t 0 )
density operator
ρ H = U I † ( t , t 0 ) ρ I ( t ) U I ( t , t 0 ) \rho_H=U_I^\dagger(t,t_0)\rho_I(t)U_I(t,t_0) ρ H = U I † ( t , t 0 ) ρ I ( t ) U I ( t , t 0 )
ρ I ( t ) = U I ( t , t 0 ) ρ H U I † ( t , t 0 ) \rho_I(t)=U_I(t,t_0)\rho_HU_I^\dagger(t,t_0) ρ I ( t ) = U I ( t , t 0 ) ρ H U I † ( t , t 0 )
This direct conversion is often cleaner than translating back through the Schrödinger picture, especially in perturbative calculations.
For closed Schrödinger-picture evolution,
i ℏ d ρ S d t = [ H S , ρ S ] . i\hbar\frac{d\rho_S}{dt}
=
[H_S,\rho_S]. i ℏ d t d ρ S = [ H S , ρ S ] .
Under the general picture transformation,
i ℏ d ρ P d t = [ H P , ρ P ] . i\hbar\frac{d\rho_P}{dt}
=
[H_P,\rho_P]. i ℏ d t d ρ P = [ H P , ρ P ] .
The special cases are
d ρ H d t = 0 \frac{d\rho_H}{dt}=0 d t d ρ H = 0
and
i ℏ d ρ I d t = [ V I ( t ) , ρ I ( t ) ] . i\hbar\frac{d\rho_I}{dt}
=
[V_I(t),\rho_I(t)]. i ℏ d t d ρ I = [ V I ( t ) , ρ I ( t )] .
These formulas apply to closed-system unitary evolution. A reduced open-system state generally has additional dissipative or memory terms; changing picture then requires transforming the full generator, not only its Hamiltonian part.
For
A P ( t ) = R † ( t ) A S ( t ) R ( t ) , A_P(t)
=
R^\dagger(t)A_S(t)R(t), A P ( t ) = R † ( t ) A S ( t ) R ( t ) ,
the full derivative is
d A P d t = R † ∂ A S ∂ t R + R ˙ † A S R + R † A S R ˙ . \frac{dA_P}{dt}
=
R^\dagger
\frac{\partial A_S}{\partial t}
R
+
\dot R^\dagger A_SR
+
R^\dagger A_S\dot R. d t d A P = R † ∂ t ∂ A S R + R ˙ † A S R + R † A S R ˙ .
Define K P = i ℏ R † R ˙ K_P=i\hbar R^\dagger\dot R K P = i ℏ R † R ˙ . Then H P = E P − K P H_P=E_P-K_P H P = E P − K P , whereas
A ˙ P = i ℏ [ K P , A P ] + R † ( ∂ t A S ) R . \dot A_P=\frac{i}{\hbar}[K_P,A_P]+R^\dagger(\partial_t A_S)R. A ˙ P = ℏ i [ K P , A P ] + R † ( ∂ t A S ) R .
The operator’s picture motion is generated by K P K_P K P , not by the transformed state generator H P H_P H P . This distinction recovers fixed Schrödinger observables when R = I R=I R = I and moving Heisenberg observables when R = U R=U R = U .
If another source uses
∣ ψ ~ P ⟩ = R ∣ ψ S ⟩ , \lvert\widetilde\psi_P\rangle
=
R\lvert\psi_S\rangle, ∣ ψ P ⟩ = R ∣ ψ S ⟩ ,
then consistency requires
A ~ P = R A S R † , ρ ~ P = R ρ S R † , \widetilde A_P
=
RA_SR^\dagger,
\qquad
\widetilde\rho_P
=
R\rho_SR^\dagger, A P = R A S R † , ρ P = R ρ S R † ,
and
H ~ P = R H S R † + i ℏ R ˙ R † . \widetilde H_P
=
RH_SR^\dagger
+
i\hbar\dot R R^\dagger. H P = R H S R † + i ℏ R ˙ R † .
Do not borrow the state definition from one convention and the Hamiltonian formula from the other. A quick diagnostic is expectation-value invariance: inconsistent dagger placement fails immediately.
Transforming only the state. Observables or density operators must be translated consistently for predictions to agree.
Forgetting − i ℏ R † R ˙ -i\hbar R^\dagger\dot R − i ℏ R † R ˙ . A time-dependent frame has its own generator.
Using R ( t ) R(t) R ( t ) at both propagator endpoints. The correct factors are R † ( t ) R^\dagger(t) R † ( t ) and R ( t 0 ) R(t_0) R ( t 0 ) .
Assuming R ( t 0 ) = I R(t_0)=I R ( t 0 ) = I silently. Include the initial factor unless the convention is declared.
Saying the Heisenberg Hamiltonian is zero without qualification. The state generator vanishes; the Hamiltonian observable need not.
Dropping explicit operator time dependence. It survives as a separately transformed derivative term.
Treating H 0 H_0 H 0 as time independent by definition. A time-dependent solvable H 0 ( t ) H_0(t) H 0 ( t ) is allowed if its propagator U 0 U_0 U 0 is defined correctly.
Calling the interaction picture approximate. The picture is exact before any perturbative truncation.
Mixing the two common R R R conventions. This reverses daggers and the connection-term sign.
Applying closed-system density formulas to reduced open dynamics. Nonunitary terms must also be transformed.
L. E. Ballentine, Quantum Mechanics: A Modern Development , 2nd ed., World Scientific, 2014.
C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics , Wiley, 1977.
P. A. M. Dirac, The Principles of Quantum Mechanics , 4th ed., Oxford University Press, 1958.
J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics , 3rd ed., Cambridge University Press, 2020.
R. Shankar, Principles of Quantum Mechanics , 2nd ed., Springer, 1994.
Starting from ∣ ψ P ⟩ = R † ∣ ψ S ⟩ \lvert\psi_P\rangle=R^\dagger\lvert\psi_S\rangle ∣ ψ P ⟩ = R † ∣ ψ S ⟩ , derive H P H_P H P .
Solution
Differentiate the transformed state and use the Schrödinger equation:
i ℏ d d t ∣ ψ P ⟩ = i ℏ R ˙ † ∣ ψ S ⟩ + R † H S ∣ ψ S ⟩ = ( i ℏ R ˙ † R + R † H S R ) ∣ ψ P ⟩ . \begin{aligned}
i\hbar\frac{d}{dt}
\lvert\psi_P\rangle
&=
i\hbar\dot R^\dagger
\lvert\psi_S\rangle
+
R^\dagger H_S
\lvert\psi_S\rangle
\\
&=
\left(
i\hbar\dot R^\dagger R
+
R^\dagger H_SR
\right)
\lvert\psi_P\rangle.
\end{aligned} i ℏ d t d ∣ ψ P ⟩ = i ℏ R ˙ † ∣ ψ S ⟩ + R † H S ∣ ψ S ⟩ = ( i ℏ R ˙ † R + R † H S R ) ∣ ψ P ⟩ .
Differentiating R † R = I R^\dagger R=I R † R = I gives R ˙ † R = − R † R ˙ \dot R^\dagger R=-R^\dagger\dot R R ˙ † R = − R † R ˙ . Hence
H P = R † H S R − i ℏ R † R ˙ . H_P
=
R^\dagger H_SR
-
i\hbar R^\dagger\dot R. H P = R † H S R − i ℏ R † R ˙ .
Show that
U P ( t , t 0 ) = R † ( t ) U S ( t , t 0 ) R ( t 0 ) U_P(t,t_0)
=
R^\dagger(t)U_S(t,t_0)R(t_0) U P ( t , t 0 ) = R † ( t ) U S ( t , t 0 ) R ( t 0 )
maps the transformed initial state to the transformed final state.
Solution
The transformed initial state is
∣ ψ P ( t 0 ) ⟩ = R † ( t 0 ) ∣ ψ S ( t 0 ) ⟩ . \lvert\psi_P(t_0)\rangle
=
R^\dagger(t_0)
\lvert\psi_S(t_0)\rangle. ∣ ψ P ( t 0 )⟩ = R † ( t 0 ) ∣ ψ S ( t 0 )⟩ .
Then
U P ( t , t 0 ) ∣ ψ P ( t 0 ) ⟩ = R † ( t ) U S ( t , t 0 ) R ( t 0 ) R † ( t 0 ) ∣ ψ S ( t 0 ) ⟩ = R † ( t ) ∣ ψ S ( t ) ⟩ = ∣ ψ P ( t ) ⟩ . \begin{aligned}
U_P(t,t_0)
\lvert\psi_P(t_0)\rangle
&=
R^\dagger(t)U_S(t,t_0)
R(t_0)R^\dagger(t_0)
\lvert\psi_S(t_0)\rangle
\\
&=
R^\dagger(t)
\lvert\psi_S(t)\rangle
\\
&=
\lvert\psi_P(t)\rangle.
\end{aligned} U P ( t , t 0 ) ∣ ψ P ( t 0 )⟩ = R † ( t ) U S ( t , t 0 ) R ( t 0 ) R † ( t 0 ) ∣ ψ S ( t 0 )⟩ = R † ( t ) ∣ ψ S ( t )⟩ = ∣ ψ P ( t )⟩ .
Show that Tr ( ρ P A P ) = Tr ( ρ S A S ) \operatorname{Tr}(\rho_PA_P)=\operatorname{Tr}(\rho_SA_S) Tr ( ρ P A P ) = Tr ( ρ S A S ) .
Solution
Substitute the transformed operators:
Tr ( ρ P A P ) = Tr ( R † ρ S R R † A S R ) = Tr ( R † ρ S A S R ) = Tr ( ρ S A S R R † ) = Tr ( ρ S A S ) . \begin{aligned}
\operatorname{Tr}(\rho_PA_P)
&=
\operatorname{Tr}
\left(
R^\dagger\rho_SR
R^\dagger A_SR
\right)
\\
&=
\operatorname{Tr}
\left(
R^\dagger\rho_SA_SR
\right)
\\
&=
\operatorname{Tr}
\left(
\rho_SA_SRR^\dagger
\right)
\\
&=
\operatorname{Tr}(\rho_SA_S).
\end{aligned} Tr ( ρ P A P ) = Tr ( R † ρ S R R † A S R ) = Tr ( R † ρ S A S R ) = Tr ( ρ S A S R R † ) = Tr ( ρ S A S ) .
The third line uses cyclicity of the trace.
Derive A H = U I † A I U I A_H=U_I^\dagger A_IU_I A H = U I † A I U I from U = U 0 U I U=U_0U_I U = U 0 U I .
Solution
By definition,
A H = U † A S U A_H
=
U^\dagger A_SU A H = U † A S U
and
A I = U 0 † A S U 0 . A_I
=
U_0^\dagger A_SU_0. A I = U 0 † A S U 0 .
Using U = U 0 U I U=U_0U_I U = U 0 U I gives
A H = U I † U 0 † A S U 0 U I = U I † A I U I . \begin{aligned}
A_H
&=
U_I^\dagger U_0^\dagger
A_S
U_0U_I
\\
&=
U_I^\dagger A_IU_I.
\end{aligned} A H = U I † U 0 † A S U 0 U I = U I † A I U I .
A source defines ∣ ψ P ⟩ = R ∣ ψ S ⟩ \lvert\psi_P\rangle=R\lvert\psi_S\rangle ∣ ψ P ⟩ = R ∣ ψ S ⟩ but writes A P = R † A S R A_P=R^\dagger A_SR A P = R † A S R . Explain the failure.
Solution
With the stated state convention, the transformed bra is ⟨ ψ P ∣ = ⟨ ψ S ∣ R † \langle\psi_P\rvert=\langle\psi_S\rvert R^\dagger ⟨ ψ P ∣ = ⟨ ψ S ∣ R † . Expectation invariance requires
A P = R A S R † , A_P
=
RA_SR^\dagger, A P = R A S R † ,
because then
⟨ ψ P ∣ A P ∣ ψ P ⟩ = ⟨ ψ S ∣ A S ∣ ψ S ⟩ . \langle\psi_P\rvert A_P\lvert\psi_P\rangle
=
\langle\psi_S\rvert A_S\lvert\psi_S\rangle. ⟨ ψ P ∣ A P ∣ ψ P ⟩ = ⟨ ψ S ∣ A S ∣ ψ S ⟩ .
Using R † A S R R^\dagger A_SR R † A S R with the same state definition generally inserts extra powers of R R R and fails this test.