diff --git a/Docs/source/refs.bib b/Docs/source/refs.bib index 65545dfca87..8d001cf971e 100644 --- a/Docs/source/refs.bib +++ b/Docs/source/refs.bib @@ -60,20 +60,22 @@ @article{Turner2013 year = {2013} } -@article{winske2022hybrid, -archivePrefix = {arXiv}, -author = {D. Winske and Homa Karimabadi and Ari Le and N. Omidi and Vadim Roytershteyn and Adam Stanier}, -eprint = {2204.01676}, -journal = {arXiv}, -primaryClass = {physics.plasm-ph}, -title = {{Hybrid codes (massless electron fluid)}}, -year = {2022} +@Inbook{WinskeInBook2023, +author = {Winske, Dan and Karimabadi, Homa and Le, Ari Yitzchak and Omidi, Nojan Nick and Roytershteyn, Vadim and Stanier, Adam John}, +bookTitle = {Space and Astrophysical Plasma Simulation: Methods, Algorithms, and Applications}, +doi = {10.1007/978-3-031-11870-8_3}, +editor = {B{\"u}chner, J{\"o}rg}, +isbn = {978-3-031-11870-8}, +pages = {63--91}, +publisher = {Springer International Publishing}, +title = {{Hybrid-Kinetic Approach: Massless Electrons}}, +year = {2023} } -@incollection{NIELSON1976, +@incollection{Nielson1976, author = {Clair W. Nielson and H. Ralph Lewis}, booktitle = {Controlled Fusion}, -doi = {https://doi.org/10.1016/B978-0-12-460816-0.50015-4}, +doi = {10.1016/B978-0-12-460816-0.50015-4}, editor = {John Killeen}, issn = {0076-6860}, pages = {367--388}, diff --git a/Docs/source/theory/kinetic_fluid_hybrid_model.rst b/Docs/source/theory/kinetic_fluid_hybrid_model.rst index 69797352bee..55bce704fbb 100644 --- a/Docs/source/theory/kinetic_fluid_hybrid_model.rst +++ b/Docs/source/theory/kinetic_fluid_hybrid_model.rst @@ -19,7 +19,7 @@ of light. Many authors have described variations of the kinetic ion & fluid electron model, generally referred to as particle-fluid hybrid or just hybrid-PIC models. The implementation -in WarpX follows the outline from :cite:t:`c-winske2022hybrid`. +in WarpX follows the outline from :cite:t:`kfhm-WinskeInBook2023`. This description follows mostly from that reference. Model @@ -29,7 +29,7 @@ The basic justification for the hybrid model is that the system to which it is applied is dominated by ion kinetics, with ions moving much slower than electrons and photons. In this scenario two critical approximations can be made, namely, neutrality (:math:`n_e=n_i`) and the Maxwell-Ampere equation can be simplified by -neglecting the displacement current term :cite:p:`c-NIELSON1976`, giving, +neglecting the displacement current term :cite:p:`kfhm-Nielson1976`, giving, .. math:: @@ -168,4 +168,4 @@ The isothermal limit is given by :math:`\gamma = 1` while :math:`\gamma = 5/3` (default) produces the adiabatic limit. .. bibliography:: - :keyprefix: c- + :keyprefix: kfhm-