arXiv (All)
open access
Three-body corrections to Brownian hard-sphere viscosity
For Brownian hard spheres without hydrodynamic interactions, we obtain a conditional enclosure between 1.8266948 and 1.8267157 for the third-order zero-shear Brownian viscosity coefficient. It applies when the physical three-body correction coincides with the finite-energy weak solution and the remo
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Black hole correspondences of quasi-topological gravity : Shadows, quasinormal modes, graybody factors#799392
- Black hole correspondences of quasi-topological gravity : Shadows, quasinormal modes, graybody factors#797969
- Machine Learning Unveils Finite-volume Energy Shifts in Three-body System#792948
- Machine Learning Unveils Finite-volume Energy Shifts in Three-body System#788944
- Strong constraints on the gravitational law from $Gaia$ DR3 wide binaries#1128487
Record · ID 1389894
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive