Interaction Picture

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## Definition

### State vectors

### Operators

#### Hamiltonian operator

#### Density matrix

### Time-evolution

#### Time-evolution of states

#### Time-evolution of operators

#### Time-evolution of the density matrix

## Expectation values

## Use

## Summary comparison of evolution in all pictures

## References

## See also

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

Interaction Picture

In quantum mechanics, the **interaction picture** (also known as the **Dirac picture** after Paul Dirac) is an intermediate representation between the Schrödinger picture and the Heisenberg picture. Whereas in the other two pictures either the state vector or the operators carry time dependence, in the interaction picture both carry part of the time dependence of observables.^{[1]} The interaction picture is useful in dealing with changes to the wave functions and observables due to interactions. Most field-theoretical calculations^{[2]} use the interaction representation because they construct the solution to the many-body Schrödinger equation as the solution to the free-particle problem plus some unknown interaction parts.

Equations that include operators acting at different times, which hold in the interaction picture, don't necessarily hold in the Schrödinger or the Heisenberg picture. This is because time-dependent unitary transformations relate operators in one picture to the analogous operators in the others.

The interaction picture is a special case of unitary transformation applied to the Hamiltonian and state vectors.

Operators and state vectors in the interaction picture are related by a change of basis (unitary transformation) to those same operators and state vectors in the Schrödinger picture.

To switch into the interaction picture, we divide the Schrödinger picture Hamiltonian into two parts:

Any possible choice of parts will yield a valid interaction picture; but in order for the interaction picture to be useful in simplifying the analysis of a problem, the parts will typically be chosen so that *H*_{0,S} is well understood and exactly solvable, while *H*_{1,S} contains some harder-to-analyze perturbation to this system.

If the Hamiltonian has *explicit time-dependence* (for example, if the quantum system interacts with an applied external electric field that varies in time), it will usually be advantageous to include the explicitly time-dependent terms with *H*_{1,S}, leaving *H*_{0,S} time-independent. We proceed assuming that this is the case. If there *is* a context in which it makes sense to have *H*_{0,S} be time-dependent, then one can proceed by replacing by the corresponding time-evolution operator in the definitions below.

A state vector in the interaction picture is defined as^{[3]}

where |*?*_{S}(*t*)?is the state vector in the Schrödinger picture.

An operator in the interaction picture is defined as

Note that *A*_{S}(*t*) will typically not depend on t and can be rewritten as just *A*_{S}. It only depends on t if the operator has "explicit time dependence", for example, due to its dependence on an applied external time-varying electric field.

For the operator *H*_{0} itself, the interaction picture and Schrödinger picture coincide:

This is easily seen through the fact that operators commute with differentiable functions of themselves. This particular operator then can be called *H*_{0} without ambiguity.

For the perturbation Hamiltonian *H*_{1,I}, however,

where the interaction-picture perturbation Hamiltonian becomes a time-dependent Hamiltonian, unless [*H*_{1,S}, *H*_{0,S}] = 0.

It is possible to obtain the interaction picture for a time-dependent Hamiltonian *H*_{0,S}(*t*) as well, but the exponentials need to be replaced by the unitary propagator for the evolution generated by *H*_{0,S}(*t*), or more explicitly with a time-ordered exponential integral.

The density matrix can be shown to transform to the interaction picture in the same way as any other operator. In particular, let *?*_{I} and *?*_{S} be the density matrices in the interaction picture and the Schrödinger picture respectively. If there is probability *p _{n}* to be in the physical state |

Transforming the Schrödinger equation into the interaction picture gives

which states that in the interaction picture, a quantum state is evolved by the interaction part of the Hamiltonian as expressed in the interaction picture^{[4]}.

If the operator *A*_{S} is time-independent (i.e., does not have "explicit time dependence"; see above), then the corresponding time evolution for *A*_{I}(*t*) is given by

In the interaction picture the operators evolve in time like the operators in the Heisenberg picture with the Hamiltonian *H* = *H*_{0}.

The evolution of the density matrix in the interaction picture is

in consistency with the Schrödinger equation in the interaction picture.

For a general operator , the expectation value in the interaction picture is given by

Using the density-matrix expression for expectation value, we will get

The purpose of the interaction picture is to shunt all the time dependence due to *H*_{0} onto the operators, thus allowing them to evolve freely, and leaving only *H*_{1,I} to control the time-evolution of the state vectors.

The interaction picture is convenient when considering the effect of a small interaction term, *H*_{1,S}, being added to the Hamiltonian of a solved system, *H*_{0,S}. By utilizing the interaction picture, one can use time-dependent perturbation theory to find the effect of *H*_{1,I},^{[5]}^{:355ff} e.g., in the derivation of Fermi's golden rule,^{[5]}^{:359-363} or the Dyson series^{[5]}^{:355-357} in quantum field theory: in 1947, Shin'ichir? Tomonaga and Julian Schwinger appreciated that covariant perturbation theory could be formulated elegantly in the interaction picture, since field operators can evolve in time as free fields, even in the presence of interactions, now treated perturbatively in such a Dyson series.

For a time-independent Hamiltonian *H _{S}*, where H0,S is Free Hamiltonian,

Evolution | Picture
| ||

of: | Heisenberg | Interaction | Schrödinger |

Ket state | constant | ||

Observable | constant | ||

Density matrix | constant |

**^**Albert Messiah (1966).*Quantum Mechanics*, North Holland, John Wiley & Sons. ISBN 0486409244; J. J. Sakurai (1994).*Modern Quantum Mechanics*(Addison-Wesley) ISBN 9780201539295.**^**J. W. Negele, H. Orland (1988), Quantum Many-particle Systems, ISBN 0738200522.**^**The Interaction Picture, lecture notes from New York University.**^**Quantum Field Theory for the Gifted Amateur, Chapter 18 - for those who saw this being called the Schwinger-Tomonaga equation, this is not the Schwinger-Tomonaga equation. That is a generalization of the Schrödinger equation to arbitrary space-like foliations of spacetime.- ^
^{a}^{b}^{c}Sakurai, J. J.; Napolitano, Jim (2010),*Modern Quantum Mechanics*(2nd ed.), Addison-Wesley, ISBN 978-0805382914

- L.D. Landau; E.M. Lifshitz (1977).
*Quantum Mechanics: Non-Relativistic Theory*. Vol. 3 (3rd ed.). Pergamon Press. ISBN 978-0-08-020940-1.Online copy

- Townsend, John S. (2000).
*A Modern Approach to Quantum Mechanics, 2nd ed*. Sausalito, California: University Science Books. ISBN 1-891389-13-0.

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

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