From ac9389f5cbdaa2d0e16bb805c432498fb391fcf7 Mon Sep 17 00:00:00 2001 From: jtclemm Date: Mon, 20 Mar 2023 14:24:21 -0600 Subject: [PATCH] Slight rewrite --- doc/src/neighbor.rst | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/doc/src/neighbor.rst b/doc/src/neighbor.rst index bf9a13923c..b5ca4d15a8 100644 --- a/doc/src/neighbor.rst +++ b/doc/src/neighbor.rst @@ -66,7 +66,7 @@ instance in a dense binary system with a ratio of the size of the largest to smallest collection bin :math:`\lamda`, the computational costs of building a default neighbor list grows as :math:`\lamda^6` while the costs for *multi* grows as :math:`\lamda^3`, equivalent to the cost of force -evaluations, as identified in Monti et al. :ref:`(Monti) `. +evaluations, as argued in Monti et al. :ref:`(Monti) `. By default in *multi*, each atom type defines a separate collection of particles. For systems where two or more atom types have the same