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The Fock space is an construction used in quantum mechanics to construct the space of a variable or unknown number of identical particles from a single particle . It is named after who first introduced it in his 1932 paper "Konfigurationsraum und zweite Quantelung" ("Configuration space and second quantization").M.C. Reed, , "Methods of Modern Mathematical Physics, Volume II", Academic Press 1975. Page 328.

Informally, a Fock space is the sum of a set of Hilbert spaces representing zero particle states, one particle states, two particle states, and so on. If the identical particles are , the -particle states are vectors in a of single-particle Hilbert spaces . If the identical particles are , the -particle states are vectors in an antisymmetrized tensor product of single-particle Hilbert spaces (see symmetric algebra and respectively). A general state in Fock space is a linear combination of -particle states, one for each .

Technically, the Fock space is (the completion of) the direct sum of the symmetric or antisymmetric tensors in the tensor powers of a single-particle Hilbert space , F_\nu(H)=\overline{\bigoplus_{n=0}^{\infty}S_\nu H^{\otimes n}} ~.

Here S_\nu is the operator that symmetrizes or antisymmetrizes a tensor, depending on whether the Hilbert space describes particles obeying bosonic (\nu = +) or fermionic (\nu = -) statistics, and the overline represents the completion of the space. The bosonic (or fermionic) Fock space can alternatively be constructed as (the Hilbert space completion of) the F_+(H) = \overline{S^*H} (or alternating tensors F_-(H) = \overline{ {\bigwedge}^* H}). For every basis of , there is a natural basis of the Fock space, the .


Definition
The Fock space is the (Hilbert) direct sum of of copies of a single-particle Hilbert space H

F_\nu(H)=\bigoplus_{n=0}^{\infty}S_\nu H^{\otimes n} = \Complex \oplus H \oplus \left(S_\nu \left(H \otimes H\right)\right) \oplus \left(S_\nu \left( H \otimes H \otimes H\right)\right) \oplus \cdots

Here \Complex, the , consists of the states corresponding to no particles, H the states of one particle, S_\nu (H\otimes H) the states of two identical particles etc.

A general state in F_\nu(H) is given by

|\Psi\rangle_\nu= |\Psi_0\rangle_\nu \oplus |\Psi_1\rangle_\nu \oplus |\Psi_2\rangle_\nu \oplus \cdots = a |0\rangle \oplus \sum_i a_i|\psi_i\rangle \oplus \sum_{ij} a_{ij}|\psi_i, \psi_j \rangle_\nu \oplus \cdots where

  • |0\rangle is a vector of length 1 called the vacuum state and a \in \Complex is a complex coefficient,
  • |\psi_i\rangle \in H is a state in the single particle Hilbert space and a_i \in \Complex is a complex coefficient,
  • |\psi_i , \psi_j \rangle_\nu = a_{ij} |\psi_i\rangle \otimes|\psi_j\rangle + a_{ji} |\psi_j\rangle\otimes|\psi_i\rangle \in S_\nu(H \otimes H), and a_{ij} = \nu a_{ji} \in \Complex is a complex coefficient, etc.

The convergence of this infinite sum is important if F_\nu(H) is to be a Hilbert space. Technically we require F_\nu(H) to be the Hilbert space completion of the algebraic direct sum. It consists of all infinite |\Psi\rangle_\nu = (|\Psi_0\rangle_\nu , |\Psi_1\rangle_\nu , |\Psi_2\rangle_\nu, \ldots) such that the norm, defined by the inner product is finite \| |\Psi\rangle_\nu \|_\nu^2 = \sum_{n=0}^\infty \langle \Psi_n |\Psi_n \rangle_\nu < \infty where the n particle norm is defined by \langle \Psi_n | \Psi_n \rangle_\nu = \sum_{i_1,\ldots i_n} \sum_{j_1, \ldots j_n} a_{i_1,\ldots, i_n}^* a_{j_1, \ldots, j_n} \langle \psi_{i_1}| \psi_{j_1} \rangle\cdots \langle \psi_{i_n}| \psi_{j_n} \rangle i.e., the restriction of the norm on the tensor product H^{\otimes n}

For two general states |\Psi\rangle_\nu= |\Psi_0\rangle_\nu \oplus |\Psi_1\rangle_\nu \oplus |\Psi_2\rangle_\nu \oplus \cdots = a |0\rangle \oplus \sum_i a_i|\psi_i\rangle \oplus \sum_{ij} a_{ij}|\psi_i, \psi_j \rangle_\nu \oplus \cdots, and |\Phi\rangle_\nu=|\Phi_0\rangle_\nu \oplus |\Phi_1\rangle_\nu \oplus |\Phi_2\rangle_\nu \oplus \cdots = b |0\rangle \oplus \sum_i b_i |\phi_i\rangle \oplus \sum_{ij} b_{ij}|\phi_i, \phi_j \rangle_\nu \oplus \cdots the on F_\nu(H) is then defined as \langle \Psi |\Phi\rangle_\nu := \sum_n \langle \Psi_n| \Phi_n \rangle_\nu = a^* b + \sum_{ij} a_i^* b_j\langle\psi_i | \phi_j \rangle +\sum_{ijkl}a_{ij}^*b_{kl}\langle \psi_i|\phi_k\rangle\langle\psi_j| \phi_l \rangle_\nu + \cdots where we use the inner products on each of the n-particle Hilbert spaces. Note that, in particular the n particle subspaces are orthogonal for different n.


Product states, indistinguishable particles, and a useful basis for Fock space
A of the Fock space is a state of the form

|\Psi\rangle_\nu=|\phi_1,\phi_2,\cdots,\phi_n\rangle_\nu = |\phi_1\rangle \otimes |\phi_2\rangle \otimes \cdots \otimes |\phi_n\rangle

which describes a collection of n particles, one of which has quantum state \phi_1, another \phi_2 and so on up to the nth particle, where each \phi_i is any state from the single particle Hilbert space H. Here juxtaposition (writing the single particle kets side by side, without the \otimes) is symmetric (resp. antisymmetric) multiplication in the symmetric (antisymmetric) . The general state in a Fock space is a linear combination of product states. A state that cannot be written as a convex sum of product states is called an .

When we speak of one particle in state \phi_i, we must bear in mind that in quantum mechanics identical particles are indistinguishable. In the same Fock space, all particles are identical. (To describe many species of particles, we take the tensor product of as many different Fock spaces as there are species of particles under consideration). It is one of the most powerful features of this formalism that states are implicitly properly symmetrized. For instance, if the above state |\Psi\rangle_- is fermionic, it will be 0 if two (or more) of the \phi_i are equal because the antisymmetric product |\phi_i \rangle |\phi_i \rangle = 0 . This is a mathematical formulation of the Pauli exclusion principle that no two (or more) fermions can be in the same quantum state. In fact, whenever the terms in a formal product are linearly dependent; the product will be zero for antisymmetric tensors. Also, the product of orthonormal states is properly orthonormal by construction (although possibly 0 in the Fermi case when two states are equal).

A useful and convenient basis for a Fock space is the occupancy number basis. Given a basis \{|\psi_i\rangle\}_{i = 0,1,2, \dots} of H, we can denote the state with n_0 particles in state |\psi_0\rangle, n_1 particles in state |\psi_1\rangle, ..., n_k particles in state |\psi_k\rangle, and no particles in the remaining states, by defining

|n_0,n_1,\ldots,n_k\rangle_\nu = |\psi_0\rangle^{n_0}|\psi_1\rangle^{n_1} \cdots |\psi_k\rangle^{n_k},

where each n_i takes the value 0 or 1 for fermionic particles and 0, 1, 2, ... for bosonic particles. Note that trailing zeroes may be dropped without changing the state. Such a state is called a . When the |\psi_i\rangle are understood as the steady states of a free field, the Fock states describe an assembly of non-interacting particles in definite numbers. The most general Fock state is a linear superposition of pure states.

Two operators of great importance are the creation and annihilation operators, which upon acting on a Fock state add or respectively remove a particle in the ascribed quantum state. They are denoted a^{\dagger}(\phi)\, for creation and a(\phi)for annihilation respectively. To create ("add") a particle, the quantum state |\phi\rangle is symmetric or exterior- multiplied with |\phi\rangle; and respectively to annihilate ("remove") a particle, an (even or odd) is taken with \langle\phi|, which is the adjoint of a^\dagger(\phi). It is often convenient to work with states of the basis of H so that these operators remove and add exactly one particle in the given basis state. These operators also serve as generators for more general operators acting on the Fock space, for instance the giving the number of particles in a specific state |\phi_i\rangle is a^{\dagger}(\phi_i)a(\phi_i).


Wave function interpretation
Often the one particle space H is given as L_2(X, \mu), the space of square-integrable functions on a space X with measure \mu (strictly speaking, the equivalence classes of square integrable functions where functions are equivalent if they differ on a ). The typical example is the with H = L_2(\R^3, d^3x) the space of square integrable functions on three-dimensional space. The Fock spaces then have a natural interpretation as symmetric or anti-symmetric square integrable functions as follows.

Let X^0 = \{*\} and X^1 = X, X^2 = X\times X , X^3 = X \times X \times X, etc. Consider the space of tuples of points which is the

X^* = X^0 \amalg X^1 \amalg X^2 \amalg X^3 \amalg \cdots .

It has a natural measure \mu^* such that \mu^*(X^0) = 1 and the restriction of \mu^* to X^n is \mu^n. The even Fock space F_+(L_2(X,\mu)) can then be identified with the space of symmetric functions in L_2(X^*, \mu^*) whereas the odd Fock space F_-(L_2(X,\mu)) can be identified with the space of anti-symmetric functions. The identification follows directly from the mapping L_2(X, \mu)^{\otimes n} \to L_2(X^n, \mu^n) \psi_1(x)\otimes\cdots\otimes\psi_n(x) \mapsto \psi_1(x_1)\cdots \psi_n(x_n).

Given wave functions \psi_1 = \psi_1(x), \ldots , \psi_n = \psi_n(x) , the Slater determinant

\Psi(x_1, \ldots x_n) = \frac{1}{\sqrt{n!}} \begin{vmatrix} \psi_1(x_1) & \cdots & \psi_n(x_1) \\ \vdots & \ddots & \vdots \\ \psi_1(x_n) & \cdots & \psi_n(x_n) \\ \end{vmatrix} is an antisymmetric function on X^n. It can thus be naturally interpreted as an element of the n-particle sector of the odd Fock space. The normalization is chosen such that \|\Psi\| = 1 if the functions \psi_1, \ldots, \psi_n are orthonormal. There is a similar "Slater permanent" with the determinant replaced with the permanent which gives elements of n-sector of the even Fock space.


Relation to the Segal–Bargmann space
Define the Segal–Bargmann space B_N of complex holomorphic functions square-integrable with respect to a :

\mathcal{F}^2\left(\Complex^N\right) = \left\{ f\colon\Complex^N\to\Complex \mid \Vert f\Vert_{\mathcal{F}^2(\Complex^N)} < \infty\right\}, where \Vert f\Vert_{\mathcal{F}^2(\Complex^N)} := \int_{\Complex^N}\vert f(\mathbf{z})\vert^2 e^{-\pi\vert \mathbf{z}\vert^2}\,d\mathbf{z}. Then defining a space B_\infty as the nested union of the spaces B_N over the integers N \ge 0 , Segal and Bargmann showed that B_\infty is isomorphic to a bosonic Fock space. The monomial x_1^{n_1}...x_k^{n_k} corresponds to the Fock state |n_0,n_1,\ldots,n_k\rangle_\nu = |\psi_0\rangle^{n_0}|\psi_1\rangle^{n_1} \cdots |\psi_k\rangle^{n_k}.


See also
  • Holomorphic Fock space
  • Creation and annihilation operators
  • Slater determinant
  • Wick's theorem
  • Noncommutative geometry
  • Grand canonical ensemble, thermal distribution over Fock space
  • Schrödinger functional


External links

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