Simulating sparse Hamiltonians with star decompositions
Andrew M. Childs, Robin Kothari

TL;DR
This paper introduces an improved quantum algorithm for simulating sparse Hamiltonians by decomposing them into star-structured components, resulting in better query complexity than previous methods.
Contribution
It presents a novel decomposition technique into star graphs and an efficient simulation algorithm with reduced complexity for sparse Hamiltonians.
Findings
Achieves lower query complexity than previous algorithms.
Decomposes sparse Hamiltonians into star-structured components.
Provides an efficient simulation method for quantum systems.
Abstract
We present an efficient algorithm for simulating the time evolution due to a sparse Hamiltonian. In terms of the maximum degree d and dimension N of the space on which the Hamiltonian H acts for time t, this algorithm uses (d^2(d+log* N)||Ht||)^{1+o(1)} queries. This improves the complexity of the sparse Hamiltonian simulation algorithm of Berry, Ahokas, Cleve, and Sanders, which scales like (d^4(log* N)||Ht||)^{1+o(1)}. To achieve this, we decompose a general sparse Hamiltonian into a small sum of Hamiltonians whose graphs of non-zero entries have the property that every connected component is a star, and efficiently simulate each of these pieces.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
