Probability amplitude in Heisenberg e Schrodinger pictures

AdeBlackRune
Messages
9
Reaction score
0
Hi, this is my question:

suppose that at time t' our system is in the state | \psi(t')\rangle
The probability for the system to be in the state | \phi\rangle at the time t'' is the norm of
\langle \phi| \psi(t'')\rangle
This in the Schrodinger picture. But how i can write the same thing in the Heisenberg picture?
 
Physics news on Phys.org
The probability is actually the squared modulus of the expression you wrote. It's supposed to be a number independent of description/picture. You need to know how to connect the 2 pictures and then it's easy to get the result.
 
In the Schrödinger picture, the state ket evolves in time via

|\psi,t \rangle_S=\exp(-\mathrm{i} \hat{H} t) |\psi,0\rangle .

Here, I assume that the Hamiltonian of the system is not explicitly time dependent.

The observables like position, momentum, etc. are time-independent by definition. Thus, for any observable operator we have

\hat{O}_S(t)=\hat{O}(0).

Thus, also the eigenvectors are time-independent

|o,t \rangle_S=|o,0 \rangle.

The probability to measure the eigenvalue o is then given by

P(t,o)=|_S\langle o,t|\psi,t\rangle_S|^2=\langle o,0|\exp(-\mathrm{i} \hat{H} t) |\psi,0 \rangle..

In the Heisenberg picture, the states are constant in time:

|\psi,t \rangle_H=|\psi,0 \rangle.

The operators representing observables move with the full Hamiltonian,

\frac{d}{d t} \hat{O}_H(t)=\frac{1}{\mathrm{i}} [\hat{O}_H(t),\hat{H}].

The solution is

\hat{O}_H(t)=\exp(\mathrm{i} \hat{H} t) \hat{O}(0) \exp(-\mathrm{i} \hat{H} t),

and thus for the eigenvectors we have

|o,t \rangle_H=\exp( \mathrm{i} \hat{H} t) |o,0\rangle.

Thus again, we have

P(o,t)=|_H\langle o,t|\psi,t \rangle_H|^2=|\langle \exp( \mathrm{i} \hat{H} t) o,0|\psi,0 \rangle|^2 = |\langle o,0|\exp(- \mathrm{i} \hat{H} t)|\psi,0 \rangle|^2,

which is the same result as in the Schrödinger picture. The observable quantities do not depend on the picture of time evolution used, as it must be.
 
vanhees pretty much explained it.

You can also interpret it as follows:

The overlap

<br /> \langle \psi(t)| \phi\rangle \langle \phi| \psi(t)\rangle<br />

is basically what you want, modulus squared. Then

\hat{A}_S = | \phi\rangle \langle \phi|

is a projection operator onto the state | \phi\rangle [/tex] in the Schroedinger picture. So switching to the Heisenberg picture gives<br /> <br /> \hat{A}_H(t) = e^{iHt} \hat{A}_S e^{-iHt} = e^{iHt} | \phi\rangle \langle \phi|e^{-iHt}<br /> <br /> But e^{iHt} | \phi\rangle = |\phi(t)\rangle is just the time-evolved version of the state you are projecting on:<br /> <br /> \hat{A}_H(t) = | \phi(t)\rangle \langle \phi(t)|<br /> <br /> In effect, the time evolution switched from the state to the (projection) operator. The time dependence of the projection operator is hidden in the time-evolution of the state you are projecting on.
 
To make the probability measurable, one of the two vectors must be some dynamical quantity's eigenvector. As eigenvectors change with time in an opposite way to state vector, the product is identical in both picture.
 
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. Towards the end of the first lecture for the Qiskit Global Summer School 2025, Foundations of Quantum Mechanics, Olivia Lanes (Global Lead, Content and Education IBM) stated... Source: https://www.physicsforums.com/insights/quantum-entanglement-is-a-kinematic-fact-not-a-dynamical-effect/ by @RUTA
I am reading WHAT IS A QUANTUM FIELD THEORY?" A First Introduction for Mathematicians. The author states (2.4 Finite versus Continuous Models) that the use of continuity causes the infinities in QFT: 'Mathematicians are trained to think of physical space as R3. But our continuous model of physical space as R3 is of course an idealization, both at the scale of the very large and at the scale of the very small. This idealization has proved to be very powerful, but in the case of Quantum...
Thread 'Lesser Green's function'
The lesser Green's function is defined as: $$G^{<}(t,t')=i\langle C_{\nu}^{\dagger}(t')C_{\nu}(t)\rangle=i\bra{n}C_{\nu}^{\dagger}(t')C_{\nu}(t)\ket{n}$$ where ##\ket{n}## is the many particle ground state. $$G^{<}(t,t')=i\bra{n}e^{iHt'}C_{\nu}^{\dagger}(0)e^{-iHt'}e^{iHt}C_{\nu}(0)e^{-iHt}\ket{n}$$ First consider the case t <t' Define, $$\ket{\alpha}=e^{-iH(t'-t)}C_{\nu}(0)e^{-iHt}\ket{n}$$ $$\ket{\beta}=C_{\nu}(0)e^{-iHt'}\ket{n}$$ $$G^{<}(t,t')=i\bra{\beta}\ket{\alpha}$$ ##\ket{\alpha}##...
Back
Top