|  Configuration-Space Based Representations in Quantum Theory | 
Schrödinger Picture / Representation
  > s.a. representations in quantum theory; quantum field theory.
  * Idea: The representation
    on L2(\(\cal C\), dμ), where
    \(\cal C\) is the configuration space, in which states are time-dependent,
    observables time-independent.
  * Use: It is not convenient
    for the relativistic theory, since it treats time differently from the space
    coordinates.
  @ References:
    Hiley & Dennis a1809 [Dirac-Bohm picture];
    Stoica a1906
      [multi-layered field representation in 3D space].
Heisenberg Picture / Representation > s.a. quantum field theory.
  * Idea: The representation on
    L2(\(\cal C\), dμ) in which
    states are time-independent, and observables time-dependent operators.
  * Relationships: Compared to
    the Schrödinger representation,
ψH = exp{iHt/\(\hbar\)} ψS(t), and AH(t) = exp{iHt/\(\hbar\)} AS exp{−iHt/\(\hbar\)};
    the time evolution of the operators is given by i\(\hbar\) ∂AH/∂t
    = [AH, H]; The Hamiltonian operator is the same.
  * Advantages: Constant phase
    shifts in the operators due, e.g., to a constant potential are cancelled;
    The equations of motion for the operators are formally identical to
    the classical ones; It is convenient for relativistic theory.
  * Disadvantages: It
    is difficult to solve practical problems with it.
  @ Compared to Schrödinger representation:
    Faria et al PLA(02);
    Nikolić PLA(04)qp/03;
    de la Madrid qp/05-conf [for unbounded operators, and rigged Hilbert space];
    Solomon a0706 [in quantum field theory];
    Aharonov a1303-fs [and non-local quantum phenomena];
    Partovi a1305
      [and Eulerian vs Lagrangian descriptions of fluid dynamics];
    de Gosson a1404 [inequivalence];
    Franson & Brewster a1811 [limitations].
Interaction Picture / Representation
  * Idea: Both states and
    operators are time-dependent, with evolutions governed by different parts
    of the Hamiltonian:
H'I(t) ψI(t) = i\(\hbar\) ∂ψI(t)/∂t , and i\(\hbar\) ∂AI(t)/∂t = [AI(t), H0] ,
where H = H0 + H', a free and an interaction part, and the relationship with Schrödinger representation quantities is
ψI(t) = exp{iH0t/\(\hbar\)} ψS(t) , and H'I(t) = exp{iH0t/\(\hbar\)} H'S exp{−iH0t/\(\hbar\)} .
  * Advantage: Takes into
    account only the non-trivial evolution of states; The free H
    evolves the operators.
  * Disadvantage: It does
    not exist in general for a relativistic theory.
  * Remark: This representation
    is often implicitly used in ordinary quantum mechanics, when ignoring
    "the rest of the world".
  @ In quantum field theory: Biswas a0807 [transformation to free fields not unitary].
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