# A quantum linear system algorithm for dense matrices

**Authors:** Leonard Wossnig, Zhikuan Zhao, Anupam Prakash

arXiv: 1704.06174 · 2018-02-07

## TL;DR

This paper introduces a quantum algorithm for solving dense linear systems with a runtime that improves quadratically over previous quantum methods, especially for matrices with bounded spectral norm, leveraging singular value estimation and efficient state preparation.

## Contribution

The paper presents a novel quantum linear system algorithm with sparsity-independent runtime scaling for dense matrices, improving efficiency over existing quantum algorithms.

## Key findings

- Achieves $	ilde{O}(	au 	ext{polylog}(n)/	extepsilon)$ runtime for dense matrices.
- Provides a quadratic speedup over previous quantum algorithms for dense matrices.
- Utilizes a memory architecture for efficient quantum state preparation.

## Abstract

Solving linear systems of equations is a frequently encountered problem in machine learning and optimisation. Given a matrix $A$ and a vector $\mathbf b$ the task is to find the vector $\mathbf x$ such that $A \mathbf x = \mathbf b$. We describe a quantum algorithm that achieves a sparsity-independent runtime scaling of $\mathcal{O}(\kappa^2 \|A\|_F \text{polylog}(n)/\epsilon)$, where $n\times n$ is the dimensionality of $A$ with Frobenius norm $\|A\|_F$, $\kappa$ denotes the condition number of $A$, and $\epsilon$ is the desired precision parameter. When applied to a dense matrix with spectral norm bounded by a constant, the runtime of the proposed algorithm is bounded by $\mathcal{O}(\kappa^2\sqrt{n} \text{polylog}(n)/\epsilon)$, which is a quadratic improvement over known quantum linear system algorithms. Our algorithm is built upon a singular value estimation subroutine, which makes use of a memory architecture that allows for efficient preparation of quantum states that correspond to the rows and row Frobenius norms of $A$.

## Full text

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## References

31 references — full list in the complete paper: https://tomesphere.com/paper/1704.06174/full.md

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Source: https://tomesphere.com/paper/1704.06174