Probability amplitude in Heisenberg e Schrodinger pictures

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Discussion Overview

The discussion revolves around the relationship between the Schrödinger and Heisenberg pictures in quantum mechanics, specifically focusing on how to express the probability amplitude for a system transitioning between states in both frameworks. Participants explore the mathematical formulations and implications of these two representations.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant states that the probability for a system to be in a state | φ⟩ at time t'' is given by the norm of ⟨φ|ψ(t'')⟩ in the Schrödinger picture.
  • Another participant emphasizes that the probability is the squared modulus of the expression and suggests that understanding the connection between the two pictures is essential for deriving results.
  • A participant explains the time evolution of state kets in the Schrödinger picture and notes that observables are time-independent, leading to a specific formulation for the probability of measuring an eigenvalue.
  • In the Heisenberg picture, it is noted that states remain constant while operators evolve with time, with a detailed derivation provided for the probability expression that aligns with the Schrödinger picture result.
  • One participant interprets the overlap ⟨ψ(t)|φ⟩ as the desired quantity, discussing the role of projection operators in both pictures and how time evolution is represented differently.
  • Another participant mentions that to make the probability measurable, one of the vectors must be an eigenvector of a dynamical quantity, highlighting the relationship between state vectors and eigenvectors over time.

Areas of Agreement / Disagreement

Participants generally agree on the mathematical equivalence of the probability expressions in both pictures, but there are nuances in how they interpret the role of time evolution and the nature of the projection operators. Some aspects remain contested, particularly regarding the implications of these formulations.

Contextual Notes

There are assumptions regarding the Hamiltonian's time independence and the nature of the states and observables that are not fully explored. The discussion also does not resolve how these concepts apply in scenarios with explicitly time-dependent Hamiltonians.

AdeBlackRune
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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 Schrödinger picture. But how i can write the same thing in the Heisenberg picture?
 
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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.
 

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