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| author | Claudius "keldu" Holeksa <mail@keldu.de> | 2025-11-12 16:29:47 +0100 |
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| committer | Claudius "keldu" Holeksa <mail@keldu.de> | 2025-11-12 16:29:47 +0100 |
| commit | ce35f47f1407590c55551f792c05620c454870c3 (patch) | |
| tree | 4f26d01eb556c8646c602d9491972284ab3b1ff2 /typst | |
| parent | 7b17a9eeac41d6be4840efc964e5d0d2e749cf58 (diff) | |
| download | phd-fluid_mechanics_report-ce35f47f1407590c55551f792c05620c454870c3.tar.gz | |
progress
Diffstat (limited to 'typst')
| -rw-r--r-- | typst/main.typ | 4 |
1 files changed, 2 insertions, 2 deletions
diff --git a/typst/main.typ b/typst/main.typ index 3e5c415..50f2dca 100644 --- a/typst/main.typ +++ b/typst/main.typ @@ -244,11 +244,11 @@ Van-Der-Waal forces and electromagnetic repulsion where the final particle-parti #math.equation( block:true, $ F_"ij"^"DLVO"_"pp" = ( - A_"iLj" r_"ij" / (6h^2_"ij") + 64 pi epsilon_0 epsilon_r r_"ij" kappa (k_B T / (Z e)) ^2\ -tanh ( Z e psi / (4k_B T) ) ^2 +tanh ( Z e psi / (4k_B T) ) ^2 $ ) -== Discusion +== Discussion The particles forming arches are often inherently unstable. Slight fluctuations in flow rate, local velocity gradients or the particle shape can impact the particle arch formation and restore partial flow. |