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'''Amplitude amplification''' is a technique in [[quantum computing]] which generalizes the idea behind
the [[Grover's algorithm|Grover's search algorithm]], and gives rise to a family of
[[quantum algorithm]]s.
It was discovered by [[Gilles Brassard]] and
[[Peter Høyer]] in 1997,
<ref name="brassard1997">
{{cite journal
|author=Gilles Brassard, Peter Høyer
|date=June 1997
|title=An exact quantum polynomial-time algorithm for Simon's problem
|journal=Proceedings of Fifth Israeli Symposium on Theory of Computing and Systems
|pages=12–23
|publisher=IEEE Computer Society Press
|arxiv=quant-ph/9704027
|bibcode = 1997quant.ph..4027B }}
</ref>
and independently rediscovered by [[Lov K. Grover|Lov Grover]] in 1998.
<ref name="grover1998">
{{cite journal
|author=Grover, Lov K.
|date=May 1998
|title=Quantum Computers Can Search Rapidly by Using Almost Any Transformation
|journal=Phys. Rev. Lett.
|volume=80
|issue=19
|pages=4329–4332
|doi=10.1103/PhysRevLett.80.4329
|bibcode=1998PhRvL..80.4329G
|arxiv = quant-ph/9712011 }}
</ref>
 
In a quantum computer, amplitude amplification can be used to obtain a
quadratic speedup over several classical algorithms.
 
== Algorithm ==
 
The derivation presented here roughly follows the one given in
.<ref name="brassard2000">
{{cite arxiv
|author=Gilles Brassard, Peter Høyer, Michele Mosca, Alain Tapp
|date=2000-05-15
|title=Quantum Amplitude Amplification and Estimation
|class=quant-ph
|eprint=quant-ph/0005055
}}
</ref>
Assume we have an N-dimensional [[Hilbert space]] <math>\mathcal{H}</math>
representing the [[mathematical formulation of quantum mechanics|state space]] of our quantum system, spanned by the
orthonormal computational basis states <math>B := \{ |k\rangle \}_{k=0}^{N-1}</math>.
Furthermore assume we have a [[Hermitian]] [[projection operator]] <math>P: \mathcal{H} \to \mathcal{H}</math>.
Alternatively, <math>P</math> may be given in terms of a
Boolean [[Oracle_machine#Definitions|oracle]] function
<math>\chi:\mathbb{Z} \to \{0,1\}</math>
and an orthonormal operational basis
<math>B_{\text{op}} := \{|\omega_k\rangle \}_{k=0}^{N-1}</math>,
in which case
:<math>P := \sum_{\chi(k)=1} |\omega_k \rangle \langle \omega_k|</math>.
<math>P</math> can be used to partition
<math>\mathcal{H}</math> into a direct sum of two mutually orthogonal subspaces,
the ''good'' subspace <math>\mathcal{H}_1</math> and
the ''bad'' subspace <math>\mathcal{H}_0</math>:
:<math>
\begin{align}
\mathcal{H}_1 &:= \text{Image}\; P &= \operatorname{span}\{|\omega_k\rangle \in B_{\text{op}} \;|\; \chi(x) = 1\},\\
\mathcal{H}_0 &:= \text{Ker} \; P &= \operatorname{span}\{|\omega_k\rangle \in B_{\text{op}} \;|\; \chi(x) = 0\}.
\end{align}
</math>
 
Given a normalized state vector <math>|\psi\rangle \in \mathcal{H}</math> which has nonzero overlap with both subspaces, we can
uniquely decompose it as
:<math>|\psi\rangle = \sin(\theta) |\psi_1\rangle  +\cos(\theta) |\psi_0\rangle</math>,
where <math>\theta = \arcsin\left( \left| P |\psi\rangle \right| \right) \in [0, \pi/2]</math>,
and
<math>|\psi_1\rangle</math> and <math>|\psi_0\rangle</math> are the
normalized projections of  <math>|\psi\rangle</math> into the
subspaces <math>\mathcal{H}_1</math> and <math>\mathcal{H}_0</math>,
respectively.
This decomposition defines a two-dimensional subspace
<math>\mathcal{H}_\psi</math>, spanned by the vectors
<math>|\psi_0\rangle</math> and <math>|\psi_1\rangle</math>.
<!-- (The degenerate case, where<math>|\psi\rangle</math> lies entirely in one of the subspaces ...) -->
The probability of finding the system in a ''good'' state when measured
is <math>\sin^2(\theta)</math>.
 
Define a unitary operator
<math>Q(\psi, P) := -S_\psi S_P \,\!</math>,
where
:<math>
\begin{align}
S_\psi &= I -2|\psi\rangle \langle\psi|\quad \text{and}\\
S_P    &= I -2 P.
\end{align}
</math>
<math>S_P</math> flips the phase of the states in the ''good'' subspace, whereas
<math>S_\psi</math> flips the phase of the initial state <math>|\psi\rangle</math>.
 
The action of this operator on <math>\mathcal{H}_\psi</math> is given by
:<math>Q |\psi_0\rangle = -S_\psi |\psi_0\rangle = (2\cos^2(\theta)-1)|\psi_0\rangle +2 \sin(\theta) \cos(\theta) |\psi_1\rangle</math> and
:<math>Q |\psi_1\rangle =  S_\psi |\psi_1\rangle = -2 \sin(\theta) \cos(\theta) |\psi_0\rangle +(1-2\sin^2(\theta))|\psi_1\rangle</math>.
Thus in the <math>\mathcal{H}_\psi</math> subspace <math>Q</math>
corresponds to a rotation by the angle <math>2\theta\,\!</math>:
:<math>Q = \begin{pmatrix}
\cos(2\theta) & \sin(2\theta)\\
-\sin(2\theta) & \cos(2\theta)
\end{pmatrix}</math>.
 
<!-- Outside <math>\mathcal{H}_\psi</math> the operator <math>Q</math> acts simply as <math>-S_\chi</math>...-->
 
Applying <math>Q</math> <math>n</math> times on the state
<math>|\psi\rangle</math>
gives
:<math>Q^n |\psi\rangle = \cos((2n+1) \theta) |\psi_0\rangle +\sin((2n+1)\theta) |\psi_1\rangle</math>,
rotating the state between the ''good'' and ''bad'' subspaces.
After <math>n</math> iterations the probability of finding the
system in a ''good'' state is <math>\sin^2((2n+1)\theta)\,\!</math>.<br/>
The probability is maximized if we choose
:<math>n = \left\lfloor\frac{\pi}{4\theta}\right\rfloor</math>.
Up until this point each iteration increases the amplitude of the ''good'' states, hence
the name of the technique.
 
== Applications ==
 
Assume we have an unsorted database with N elements, and an oracle function
<math>\chi</math> which can recognize the ''good'' entries we are searching for, and <math>B_{\text{op}} = B</math> for simplicity.
 
If there are G such entries in the database in total, then we can find them by
initializing the quantum computer into a uniform superposition
:<math>|\psi\rangle = \frac{1}{\sqrt{N}} \sum_{k=0}^{N-1} |k\rangle</math>
of all the database elements,
and running the above algorithm. In this case the overlap of the initial state with the ''good'' subspace is equal to the
square root of the frequency of the ''good'' entries in the database, <math>\sin(\theta) = |P |\psi\rangle|= \sqrt{G/N}</math>.
If <math>\sin(\theta) \ll 1</math>, we can approximate the number of required iterations as
:<math>n = \left\lfloor\frac{\pi}{4\theta}\right\rfloor
\approx \left\lfloor\frac{\pi}{4 \sin(\theta)}\right\rfloor
= \left\lfloor\frac{\pi}{4} \sqrt{\frac{N}{G}}\right\rfloor = O(\sqrt{N}).
</math>
Measuring the state will now give one of the ''good'' entries with a high probability. Since each application of <math>S_P</math> requires a single oracle query (assuming that the oracle is implemented as a quantum gate),
we can find a ''good'' entry with just <math>O(\sqrt{N})</math> oracle queries, thus obtaining a quadratic speedup over the best possible classical algorithm.
 
If we set G to one, the above scenario essentially reduces to the original Grover search.
 
== References ==
{{reflist}}
 
{{Quantum computing}}
 
{{DEFAULTSORT:Amplitude Amplification}}
[[Category:Quantum algorithms]]
[[Category:Search algorithms]]

Revision as of 14:23, 18 June 2013

Amplitude amplification is a technique in quantum computing which generalizes the idea behind the Grover's search algorithm, and gives rise to a family of quantum algorithms. It was discovered by Gilles Brassard and Peter Høyer in 1997, [1] and independently rediscovered by Lov Grover in 1998. [2]

In a quantum computer, amplitude amplification can be used to obtain a quadratic speedup over several classical algorithms.

Algorithm

The derivation presented here roughly follows the one given in .[3] Assume we have an N-dimensional Hilbert space representing the state space of our quantum system, spanned by the orthonormal computational basis states B:={|k}k=0N1. Furthermore assume we have a Hermitian projection operator P:. Alternatively, P may be given in terms of a Boolean oracle function χ:{0,1} and an orthonormal operational basis Bop:={|ωk}k=0N1, in which case

P:=χ(k)=1|ωkωk|.

P can be used to partition into a direct sum of two mutually orthogonal subspaces, the good subspace 1 and the bad subspace 0:

1:=ImageP=span{|ωkBop|χ(x)=1},0:=KerP=span{|ωkBop|χ(x)=0}.

Given a normalized state vector |ψ which has nonzero overlap with both subspaces, we can uniquely decompose it as

|ψ=sin(θ)|ψ1+cos(θ)|ψ0,

where θ=arcsin(|P|ψ|)[0,π/2], and |ψ1 and |ψ0 are the normalized projections of |ψ into the subspaces 1 and 0, respectively. This decomposition defines a two-dimensional subspace ψ, spanned by the vectors |ψ0 and |ψ1. The probability of finding the system in a good state when measured is sin2(θ).

Define a unitary operator Q(ψ,P):=SψSP, where

Sψ=I2|ψψ|andSP=I2P.

SP flips the phase of the states in the good subspace, whereas Sψ flips the phase of the initial state |ψ.

The action of this operator on ψ is given by

Q|ψ0=Sψ|ψ0=(2cos2(θ)1)|ψ0+2sin(θ)cos(θ)|ψ1 and
Q|ψ1=Sψ|ψ1=2sin(θ)cos(θ)|ψ0+(12sin2(θ))|ψ1.

Thus in the ψ subspace Q corresponds to a rotation by the angle 2θ:

Q=(cos(2θ)sin(2θ)sin(2θ)cos(2θ)).


Applying Q n times on the state |ψ gives

Qn|ψ=cos((2n+1)θ)|ψ0+sin((2n+1)θ)|ψ1,

rotating the state between the good and bad subspaces. After n iterations the probability of finding the system in a good state is sin2((2n+1)θ).
The probability is maximized if we choose

n=π4θ.

Up until this point each iteration increases the amplitude of the good states, hence the name of the technique.

Applications

Assume we have an unsorted database with N elements, and an oracle function χ which can recognize the good entries we are searching for, and Bop=B for simplicity.

If there are G such entries in the database in total, then we can find them by initializing the quantum computer into a uniform superposition

|ψ=1Nk=0N1|k

of all the database elements, and running the above algorithm. In this case the overlap of the initial state with the good subspace is equal to the square root of the frequency of the good entries in the database, sin(θ)=|P|ψ|=G/N. If sin(θ)1, we can approximate the number of required iterations as

n=π4θπ4sin(θ)=π4NG=O(N).

Measuring the state will now give one of the good entries with a high probability. Since each application of SP requires a single oracle query (assuming that the oracle is implemented as a quantum gate), we can find a good entry with just O(N) oracle queries, thus obtaining a quadratic speedup over the best possible classical algorithm.

If we set G to one, the above scenario essentially reduces to the original Grover search.

References

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Template:Quantum computing

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