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Braket notation 7/8 https://en.wikipedia.org/wiki/Braket_notation reference science, encyclopedia 2026-05-05T14:40:03.882193+00:00 kb-cron
      |
    
    ψ
    ⟩
    
      |
    
    ϕ
    ⟩
    
    ,
    
    
      |
    
    ψ
    ⟩
    ⊗
    
      |
    
    ϕ
    ⟩
    
    ,
    
    
      |
    
    ψ
    ϕ
    ⟩
    
    ,
    
    
      |
    
    ψ
    ,
    ϕ
    ⟩
    
    .
  

{\displaystyle |\psi \rangle |\phi \rangle \,,\quad |\psi \rangle \otimes |\phi \rangle \,,\quad |\psi \phi \rangle \,,\quad |\psi ,\phi \rangle \,.}

See quantum entanglement and the EPR paradox for applications of this product.

== The unit operator == Consider a complete orthonormal system (basis),

    {
    
      e
      
        i
      
    
     
    
      |
    
     
    i
    ∈
    
      N
    
    }
    
    ,
  

{\displaystyle \{e_{i}\ |\ i\in \mathbb {N} \}\,,}

for a Hilbert space H, with respect to the norm from an inner product ⟨·,·⟩. From basic functional analysis, it is known that any ket

      |
    
    ψ
    ⟩
  

{\displaystyle |\psi \rangle }

can also be written as

      |
    
    ψ
    ⟩
    =
    
      ∑
      
        i
        ∈
        
          N
        
      
    
    ⟨
    
      e
      
        i
      
    
    
      |
    
    ψ
    ⟩
    
      |
    
    
      e
      
        i
      
    
    ⟩
    ,
  

{\displaystyle |\psi \rangle =\sum _{i\in \mathbb {N} }\langle e_{i}|\psi \rangle |e_{i}\rangle ,}

with ⟨·|·⟩ the inner product on the Hilbert space. From the commutativity of kets with (complex) scalars, it follows that

      ∑
      
        i
        ∈
        
          N
        
      
    
    
      |
    
    
      e
      
        i
      
    
    ⟩
    ⟨
    
      e
      
        i
      
    
    
      |
    
    =
    
      I
    
  

{\displaystyle \sum _{i\in \mathbb {N} }|e_{i}\rangle \langle e_{i}|=\mathbb {I} }

must be the identity operator, which sends each vector to itself. This, then, can be inserted in any expression without affecting its value; for example

            ⟨
            v
            
              |
            
            w
            ⟩
          
          
            
            =
            ⟨
            v
            
              |
            
            
              (
              
                
                  ∑
                  
                    i
                    ∈
                    
                      N
                    
                  
                
                
                  |
                
                
                  e
                  
                    i
                  
                
                ⟩
                ⟨
                
                  e
                  
                    i
                  
                
                
                  |
                
              
              )
            
            
              |
            
            w
            ⟩
          
        
        
          
          
            
            =
            ⟨
            v
            
              |
            
            
              (
              
                
                  ∑
                  
                    i
                    ∈
                    
                      N
                    
                  
                
                
                  |
                
                
                  e
                  
                    i
                  
                
                ⟩
                ⟨
                
                  e
                  
                    i
                  
                
                
                  |
                
              
              )
            
            
              (
              
                
                  ∑
                  
                    j
                    ∈
                    
                      N
                    
                  
                
                
                  |
                
                
                  e
                  
                    j
                  
                
                ⟩
                ⟨
                
                  e
                  
                    j
                  
                
                
                  |
                
              
              )
            
            
              |
            
            w
            ⟩
          
        
        
          
          
            
            =
            ⟨
            v
            
              |
            
            
              e
              
                i
              
            
            ⟩
            ⟨
            
              e
              
                i
              
            
            
              |
            
            
              e
              
                j
              
            
            ⟩
            ⟨
            
              e
              
                j
              
            
            
              |
            
            w
            ⟩
            
            ,
          
        
      
    
  

{\displaystyle {\begin{aligned}\langle v|w\rangle &=\langle v|\left(\sum _{i\in \mathbb {N} }|e_{i}\rangle \langle e_{i}|\right)|w\rangle \\&=\langle v|\left(\sum _{i\in \mathbb {N} }|e_{i}\rangle \langle e_{i}|\right)\left(\sum _{j\in \mathbb {N} }|e_{j}\rangle \langle e_{j}|\right)|w\rangle \\&=\langle v|e_{i}\rangle \langle e_{i}|e_{j}\rangle \langle e_{j}|w\rangle \,,\end{aligned}}}

where, in the last line, the Einstein summation convention has been used to avoid clutter. In quantum mechanics, it often occurs that little or no information about the inner product ⟨ψ|φ⟩ of two arbitrary (state) kets is present, while it is still possible to say something about the expansion coefficients ⟨ψ|ei⟩ = ⟨ei|ψ⟩* and ⟨ei|φ⟩ of those vectors with respect to a specific (orthonormalized) basis. In this case, it is particularly useful to insert the unit operator into the bracket one time or more. For more information, see Resolution of the identity,

        I
      
    
    =
    ∫
    
    d
    x
     
    
      |
    
    x
    ⟩
    ⟨
    x
    
      |
    
    =
    ∫
    
    d
    p
     
    
      |
    
    p
    ⟩
    ⟨
    p
    
      |
    
    ,
  

{\displaystyle {\mathbb {I} }=\int \!dx~|x\rangle \langle x|=\int \!dp~|p\rangle \langle p|,}

where

      |
    
    p
    ⟩
    =
    ∫
    d
    x
    
      
        
          
            e
            
              i
              x
              p
              
                /
              
              ℏ
            
          
          
            |
          
          x
          ⟩
        
        
          2
          π
          ℏ
        
      
    
    .
  

{\displaystyle |p\rangle =\int dx{\frac {e^{ixp/\hbar }|x\rangle }{\sqrt {2\pi \hbar }}}.}

Since ⟨x|x⟩ = δ(x x), plane waves follow,

    ⟨
    x
    
      |
    
    p
    ⟩
    =
    
      
        
          e
          
            i
            x
            p
            
              /
            
            ℏ
          
        
        
          2
          π
          ℏ
        
      
    
    .
  

{\displaystyle \langle x|p\rangle ={\frac {e^{ixp/\hbar }}{\sqrt {2\pi \hbar }}}.}

In his book (1958), Ch. III.20, Dirac defines the standard ket which, up to a normalization, is the translationally invariant momentum eigenstate

      |
    
    ϖ
    ⟩
    =
    
      lim
      
        p
        →
        0
      
    
    
      |
    
    p
    ⟩
  

{\textstyle |\varpi \rangle =\lim _{p\to 0}|p\rangle }

in the momentum representation, i.e.,

          p
          ^
        
      
    
    
      |
    
    ϖ
    ⟩
    =
    0
  

{\displaystyle {\hat {p}}|\varpi \rangle =0}

. Consequently, the corresponding wavefunction is a constant,

    ⟨
    x
    
      |
    
    ϖ
    ⟩
    
      
        2
        π
        ℏ
      
    
    =
    1
  

{\displaystyle \langle x|\varpi \rangle {\sqrt {2\pi \hbar }}=1}

, and

      |
    
    x
    ⟩
    =
    δ
    (
    
      
        
          x
          ^
        
      
    
    
    x
    )
    
      |
    
    ϖ
    ⟩
    
      
        2
        π
        ℏ
      
    
    ,
  

{\displaystyle |x\rangle =\delta ({\hat {x}}-x)|\varpi \rangle {\sqrt {2\pi \hbar }},}

as well as

      |
    
    p
    ⟩
    =
    exp
    
    (
    i
    p
    
      
        
          x
          ^
        
      
    
    
      /
    
    ℏ
    )
    
      |
    
    ϖ
    ⟩
    .
  

{\displaystyle |p\rangle =\exp(ip{\hat {x}}/\hbar )|\varpi \rangle .}

Typically, when all matrix elements of an operator such as

    ⟨
    x
    
      |
    
    A
    
      |
    
    y
    ⟩
  

{\displaystyle \langle x|A|y\rangle }

are available, this resolution serves to reconstitute the full operator,

    ∫
    d
    x
    
    d
    y
    
    
      |
    
    x
    ⟩
    ⟨
    x
    
      |
    
    A
    
      |
    
    y
    ⟩
    ⟨
    y
    
      |
    
    =
    A
    
    .
  

{\displaystyle \int dx\,dy\,|x\rangle \langle x|A|y\rangle \langle y|=A\,.}

== Notation used by mathematicians == The object physicists are considering when using braket notation is a Hilbert space (a complete inner product space). Let

    (
    
      
        H
      
    
    ,
    ⟨
    ⋅
    ,
    ⋅
    ⟩
    )
  

{\displaystyle ({\mathcal {H}},\langle \cdot ,\cdot \rangle )}

be a Hilbert space and h ∈ H a vector in H. What physicists would denote by |h⟩ is the vector itself. That is,

      |
    
    h
    ⟩
    ∈
    
      
        H
      
    
    .
  

{\displaystyle |h\rangle \in {\mathcal {H}}.}

Let H* be the dual space of H. This is the space of linear functionals on H. The embedding

    Φ
    :
    
      
        H
      
    
    ↪
    
      
        
          H
        
      
      
        
      
    
  

{\displaystyle \Phi :{\mathcal {H}}\hookrightarrow {\mathcal {H}}^{*}}

is defined by

    Φ
    (
    h
    )
    =
    
      φ
      
        h
      
    
  

{\displaystyle \Phi (h)=\varphi _{h}}

, where for every h ∈ H the linear functional

      φ
      
        h
      
    
    :
    
      
        H
      
    
    →
    
      C
    
  

{\displaystyle \varphi _{h}:{\mathcal {H}}\to \mathbb {C} }

satisfies for every g ∈ H the functional equation

      φ
      
        h
      
    
    (
    g
    )
    =
    ⟨
    h
    ,
    g
    ⟩
    =
    ⟨
    h
    
    g
    ⟩
  

{\displaystyle \varphi _{h}(g)=\langle h,g\rangle =\langle h\mid g\rangle }

. Notational confusion arises when identifying φh and g with ⟨h| and |g⟩ respectively. This is because of literal symbolic substitutions. Let

      φ
      
        h
      
    
    =
    H
    =
    ⟨
    h
    
  

{\displaystyle \varphi _{h}=H=\langle h\mid }

and let g = G = |g⟩. This gives

      φ
      
        h
      
    
    (
    g
    )
    =
    H
    (
    g
    )
    =
    H
    (
    G
    )
    =
    ⟨
    h
    
      |
    
    (
    G
    )
    =
    ⟨
    h
    
      |
    
    
      
        (
      
    
    
      |
    
    g
    ⟩
    
      
        )
      
    
    
    .
  

{\displaystyle \varphi _{h}(g)=H(g)=H(G)=\langle h|(G)=\langle h|{\bigl (}|g\rangle {\bigr )}\,.}