Efficient High-order Mass-conserving and Energy-balancing Schemes for Schrödinger-Poisson Equations

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Main Authors: Rajvanshi, Manvendra Pratap, Ketcheson, David I.
Format: Preprint
Published: 2026
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author Rajvanshi, Manvendra Pratap
Ketcheson, David I.
author_facet Rajvanshi, Manvendra Pratap
Ketcheson, David I.
contents We study relaxation-based approaches for conserving mass and energy in the numerical solution of Schrödinger-Poisson (SP) type systems. Relaxation-based methods offer a general approach that can be applied as post-time step processing to achieve conservation with any time-stepping scheme. Here we study two types of relaxation techniques applied to implicit-explicit Runge-Kutta schemes, with Fourier collocation in space. We also study SP equations with time-varying coefficients (which appear naturally in cosmology) where energy is not conserved but satisfies a balance equation. We show that the fully-discrete system conserves both mass and energy (or satisfies the balance equation in case of time-varying coefficients), up to rounding errors. The effectiveness of these methods is demonstrated via numerical examples, including a three-dimensional cosmological simulation.
format Preprint
id arxiv_https___arxiv_org_abs_2604_05940
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Efficient High-order Mass-conserving and Energy-balancing Schemes for Schrödinger-Poisson Equations
Rajvanshi, Manvendra Pratap
Ketcheson, David I.
Computational Physics
Numerical Analysis
We study relaxation-based approaches for conserving mass and energy in the numerical solution of Schrödinger-Poisson (SP) type systems. Relaxation-based methods offer a general approach that can be applied as post-time step processing to achieve conservation with any time-stepping scheme. Here we study two types of relaxation techniques applied to implicit-explicit Runge-Kutta schemes, with Fourier collocation in space. We also study SP equations with time-varying coefficients (which appear naturally in cosmology) where energy is not conserved but satisfies a balance equation. We show that the fully-discrete system conserves both mass and energy (or satisfies the balance equation in case of time-varying coefficients), up to rounding errors. The effectiveness of these methods is demonstrated via numerical examples, including a three-dimensional cosmological simulation.
title Efficient High-order Mass-conserving and Energy-balancing Schemes for Schrödinger-Poisson Equations
topic Computational Physics
Numerical Analysis
url https://arxiv.org/abs/2604.05940