From Vlasov-Poisson to Schr\"odinger-Poisson: dark matter simulation with a quantum variational time evolution algorithm
Luca Cappelli, Francesco Tacchino, Giuseppe Murante, Stefano Borgani, and Ivano Tavernelli

TL;DR
This paper introduces a quantum algorithm using a variational real-time evolution approach to simulate the Schr"odinger-Poisson equations for dark matter, potentially improving the scalability of cosmological simulations compared to traditional methods.
Contribution
The authors develop a novel quantum circuit framework for solving the non-linear Schr"odinger-Poisson equations, connecting quantum solutions to classical Poisson problems and analyzing the impact of nonlinearity and resolution.
Findings
Discovered an empirical logarithmic relationship between qubits and spatial scale.
Designed quantum circuits linking Poisson and Schr"odinger solutions.
Analyzed how nonlinearity affects observable variance.
Abstract
Cosmological simulations describing the evolution of density perturbations of a self-gravitating collisionless Dark Matter (DM) fluid in an expanding background, provide a powerful tool to follow the formation of cosmic structures over wide dynamic ranges. The most widely adopted approach, based on the N-body discretization of the collisionless Vlasov-Poisson (VP) equations, is hampered by an unfavorable scaling when simulating the wide range of scales needed to cover at the same time the formation of single galaxies and of the largest cosmic structures. The dynamics described by the VP equations is limited by the rapid increase of the number of resolution elements which is required to simulate an ever growing range of scales. Recent studies showed an interesting mapping of the 6-dimensional+1 (6D+1) VP problem into a more amenable 3D+1 non-linear Schr\"odinger-Poisson (SP) problem for…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena
