Dyson series#The Dyson operator

{{Short description|Expansion of the time evolution operator}}

In scattering theory, a part of mathematical physics, the Dyson series, formulated by Freeman Dyson, is a perturbative expansion of the time evolution operator in the interaction picture. Each term can be represented by a sum of Feynman diagrams.

This series diverges asymptotically, but in quantum electrodynamics (QED) at the second order the difference from experimental data is in the order of 10−10. This close agreement holds because the coupling constant (also known as the fine-structure constant) of QED is much less than 1.{{huh|date=December 2019|reason=This statement seems to imply that the series would converge, but we just said that it diverges. Provide a secondary reference discussing this with some context. Also, the fine structure constant is larger than 10^-3, and alpha^2 > 10^-5, so how does it follow that second order approximation in alpha is good to 10^-10?}}

Dyson operator

In the interaction picture, a Hamiltonian {{mvar|H}}, can be split into a free part {{math|H0}} and an interacting part {{math|VS(t)}} as {{math|H {{=}} H0 + VS(t)}}.

The potential in the interacting picture is

:V_{\mathrm I}(t) = \mathrm{e}^{\mathrm{i} H_{0}(t - t_{0})/\hbar} V_{\mathrm S}(t) \mathrm{e}^{-\mathrm{i} H_{0} (t - t_{0})/\hbar},

where H_0 is time-independent and V_{\mathrm S}(t) is the possibly time-dependent interacting part of the Schrödinger picture.

To avoid subscripts, V(t) stands for V_\mathrm{I}(t) in what follows.

In the interaction picture, the evolution operator {{mvar| U}} is defined by the equation:

:\Psi(t) = U(t,t_0) \Psi(t_0)

This is sometimes called the Dyson operator.

The evolution operator forms a unitary group with respect to the time parameter. It has the group properties:

  • Identity and normalization: U(t,t) = 1,Sakurai, Modern Quantum mechanics, 2.1.10
  • Composition: U(t,t_0) = U(t,t_1) U(t_1,t_0),Sakurai, Modern Quantum mechanics, 2.1.12
  • Time Reversal: U^{-1}(t,t_0) = U(t_0,t),{{Clarify|reason=Not sure if this hypothesis is needed, why this is not in Sakurai ?|date=August 2023}}
  • Unitarity: U^{\dagger}(t,t_0) U(t,t_0)=\mathbb{1}Sakurai, Modern Quantum mechanics, 2.1.11

and from these is possible to derive the time evolution equation of the propagator:Sakurai, Modern Quantum mechanics, 2.1 pp. 69-71

:i\hbar\frac d{dt} U(t,t_0)\Psi(t_0) = V(t) U(t,t_0)\Psi(t_0).

In the interaction picture, the Hamiltonian is the same as the interaction potential H_{\rm int}=V(t) and thus the equation can also be written in the interaction picture as

:i\hbar \frac d{dt} \Psi(t) = H_{\rm int}\Psi(t)

Caution: this time evolution equation is not to be confused with the Tomonaga–Schwinger equation.

The formal solution is

:U(t,t_0)=1 - i\hbar^{-1} \int_{t_0}^t{dt_1\ V(t_1)U(t_1,t_0)},

which is ultimately a type of Volterra integral.

Derivation of the Dyson series

An iterative solution of the Volterra equation above leads to the following Neumann series:

:

\begin{align}

U(t,t_0) = {} & 1 - i\hbar^{-1} \int_{t_0}^t dt_1V(t_1) + (-i\hbar^{-1})^2\int_{t_0}^t dt_1 \int_{t_0}^{t_1} \, dt_2 V(t_1)V(t_2)+\cdots \\

& {} + (-i\hbar^{-1})^n\int_{t_0}^t dt_1\int_{t_0}^{t_1} dt_2 \cdots \int_{t_0}^{t_{n-1}} dt_nV(t_1)V(t_2) \cdots V(t_n) +\cdots.

\end{align}

Here, t_1 > t_2 > \cdots > t_n, and so the fields are time-ordered. It is useful to introduce an operator \mathcal T, called the time-ordering operator, and to define

:U_n(t,t_0)=(-i\hbar^{-1} )^n \int_{t_0}^t dt_1 \int_{t_0}^{t_1} dt_2 \cdots \int_{t_0}^{t_{n-1}} dt_n\,\mathcal TV(t_1) V(t_2)\cdots V(t_n).

The limits of the integration can be simplified. In general, given some symmetric function K(t_1, t_2,\dots,t_n), one may define the integrals

:S_n=\int_{t_0}^t dt_1\int_{t_0}^{t_1} dt_2\cdots \int_{t_0}^{t_{n-1}} dt_n \, K(t_1, t_2,\dots,t_n).

and

:I_n=\int_{t_0}^t dt_1\int_{t_0}^t dt_2\cdots\int_{t_0}^t dt_nK(t_1, t_2,\dots,t_n).

The region of integration of the second integral can be broken in n! sub-regions, defined by t_1 > t_2 > \cdots > t_n. Due to the symmetry of K, the integral in each of these sub-regions is the same and equal to S_n by definition. It follows that

:S_n = \frac{1}{n!}I_n.

Applied to the previous identity, this gives

:U_n=\frac{(-i \hbar^{-1})^n}{n!}\int_{t_0}^t dt_1\int_{t_0}^t dt_2\cdots\int_{t_0}^t dt_n \, \mathcal TV(t_1)V(t_2)\cdots V(t_n).

Summing up all the terms, the Dyson series is obtained. It is a simplified version of the Neumann series above and which includes the time ordered products; it is the path-ordered exponential:Sakurai, Modern Quantum Mechanics, 2.1.33, pp. 72

:\begin{align}

U(t,t_0)&=\sum_{n=0}^\infty U_n(t,t_0)\\

&=\sum_{n=0}^\infty \frac{(-i\hbar^{-1})^n}{n!}\int_{t_0}^t dt_1\int_{t_0}^t dt_2\cdots\int_{t_0}^t dt_n \, \mathcal TV(t_1)V(t_2)\cdots V(t_n) \\

&=\mathcal T\exp{-i\hbar^{-1}\int_{t_0}^t{d\tau V(\tau)}}

\end{align}

This result is also called Dyson's formula. Tong 3.20, http://www.damtp.cam.ac.uk/user/tong/qft/qft.pdf The group laws can be derived from this formula.

Application on state vectors

The state vector at time t can be expressed in terms of the state vector at time t_0, for t>t_0, as

:|\Psi(t)\rangle=\sum_{n=0}^\infty {(-i\hbar^{-1})^n\over n!}\underbrace{\int dt_1 \cdots dt_n}_{t_{\rm f}\,\ge\, t_1\,\ge\, \cdots\, \ge\, t_n\,\ge\, t_{\rm i}}\, \mathcal{T}\left\{\prod_{k=1}^n e^{iH_0 t_k/\hbar}V(t_{k})e^{-iH_0 t_k/\hbar}\right \}|\Psi(t_0)\rangle.

The inner product of an initial state at t_i=t_0 with a final state at t_f=t in the Schrödinger picture, for t_f>t_i is:

:\begin{align}

\langle\Psi(t_{\rm i}) & \mid\Psi(t_{\rm f})\rangle=\sum_{n=0}^\infty {(-i\hbar^{-1})^n\over n!} \times \\

&\underbrace{\int dt_1 \cdots dt_n}_{t_{\rm f}\,\ge\, t_1\,\ge\, \cdots\, \ge\, t_n\,\ge\, t_{\rm i}}\, \langle\Psi(t_i)\mid e^{-iH_0(t_{\rm f}-t_1)/\hbar}V_{\rm S}(t_1)e^{-iH_0(t_1-t_2)/\hbar}\cdots V_{\rm S}(t_n) e^{-iH_0(t_n-t_{\rm i})/\hbar}\mid\Psi(t_i)\rangle

\end{align}

The S-matrix may be obtained by writing this in the Heisenberg picture, taking the in and out states to be at infinity:{{citation|title=The S-matrix in quantum electrodynamics|journal=Physical Review|year=1949|author=Dyson|volume=75 |issue=11 |pages=1736–1755 |doi=10.1103/PhysRev.75.1736 |bibcode=1949PhRv...75.1736D |url=https://journals.aps.org/pr/abstract/10.1103/PhysRev.75.1736|url-access=subscription}}

:\langle\Psi_{\rm out} \mid S\mid\Psi_{\rm in}\rangle= \langle\Psi_{\rm out}\mid\sum_{n=0}^\infty {(-i\hbar^{-1})^n\over n!} \underbrace{\int d^4x_1 \cdots d^4x_n}_{t_{\rm out}\,\ge\, t_n\,\ge\, \cdots\, \ge\, t_1\,\ge\, t_{\rm in}}\, \mathcal{T}\left\{ H_{\rm int}(x_1)H_{\rm int}(x_2)\cdots H_{\rm int}(x_n) \right\}\mid\Psi_{\rm in}\rangle.

Note that the time ordering was reversed in the scalar product.

See also

References

{{reflist}}

  • Charles J. Joachain, Quantum collision theory, North-Holland Publishing, 1975, {{ISBN|0-444-86773-2}} (Elsevier)

Category:Scattering theory

Category:Quantum field theory

Category:Freeman Dyson