<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>A reduced speed-of-light formulation of the magnetohydrodynamic-particle-in-cell method</dc:title><dc:creator>Ji, Suoqing; Hopkins, Philip F</dc:creator><dc:corporate_author/><dc:editor/><dc:description>ABSTRACT            A reduced speed-of-light (RSOL) approximation is a useful technique for magnetohydrodynamic (MHD)-particle-in-cell (PIC) simulations. With an RSOL, some ‘in-code’ speed-of-light $\tilde{c}$ is set to much lower values than the true c, allowing simulations to take larger time-steps (which are restricted by the Courant condition given the large CR speeds). However, due to the absence of a well-formulated RSOL implementation from the literature, with naive substitution of the true c with a RSOL, the CR properties in MHD-PIC simulations (e.g. CR energy or momentum density, gyro radius) vary artificially with respect to each other and with respect to the converged ($\tilde{c} \rightarrow c$) solutions, with different choices of a RSOL. Here, we derive a new formulation of the MHD-PIC equations with an RSOL and show that (1) it guarantees all steady-state properties of the CR distribution function, and background plasma/MHD quantities are independent of the RSOL $\tilde{c}$ even for $\tilde{c} \ll c$; (2) it ensures that the simulation can simultaneously represent the real physical values of CR number, mass, momentum, and energy density; (3) it retains the correct physical meaning of various terms like the electric field; and (4) it ensures the numerical time-step for CRs can always be safely increased by a factor $\sim c/\tilde{c}$. This new RSOL formulation should enable greater self-consistency and reduced CPU cost in simulations of CR–MHD interactions.</dc:description><dc:publisher/><dc:date>2022-09-27</dc:date><dc:nsf_par_id>10443253</dc:nsf_par_id><dc:journal_name>Monthly Notices of the Royal Astronomical Society</dc:journal_name><dc:journal_volume>516</dc:journal_volume><dc:journal_issue>4</dc:journal_issue><dc:page_range_or_elocation>5143 to 5147</dc:page_range_or_elocation><dc:issn>0035-8711</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1093/mnras/stac2523</dc:doi><dcq:identifierAwardId>2108318; 1713353</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>