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
:
where is time-independent and is the possibly time-dependent interacting part of the Schrödinger picture.
To avoid subscripts, stands for in what follows.
In the interaction picture, the evolution operator {{mvar| U}} is defined by the equation:
:
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: Sakurai, Modern Quantum mechanics, 2.1.10
- Composition: Sakurai, Modern Quantum mechanics, 2.1.12
- Time Reversal: {{Clarify|reason=Not sure if this hypothesis is needed, why this is not in Sakurai ?|date=August 2023}}
- Unitarity: 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
:
In the interaction picture, the Hamiltonian is the same as the interaction potential and thus the equation can also be written in the interaction picture as
:
Caution: this time evolution equation is not to be confused with the Tomonaga–Schwinger equation.
The formal solution is
:
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, , and so the fields are time-ordered. It is useful to introduce an operator , called the time-ordering operator, and to define
:
The limits of the integration can be simplified. In general, given some symmetric function one may define the integrals
:
and
:
The region of integration of the second integral can be broken in sub-regions, defined by . Due to the symmetry of , the integral in each of these sub-regions is the same and equal to by definition. It follows that
:
Applied to the previous identity, this gives
:
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
:
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 can be expressed in terms of the state vector at time , for as
:
The inner product of an initial state at with a final state at in the Schrödinger picture, for is:
:
\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}}
:
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)