diff --git a/docs/_includes/head.html b/docs/_includes/head.html new file mode 100644 index 000000000..f8c9eddbc --- /dev/null +++ b/docs/_includes/head.html @@ -0,0 +1,3 @@ + + {% include mathjax.html %} + \ No newline at end of file diff --git a/docs/_includes/mathjax.html b/docs/_includes/mathjax.html new file mode 100644 index 000000000..3623af010 --- /dev/null +++ b/docs/_includes/mathjax.html @@ -0,0 +1,15 @@ + + \ No newline at end of file diff --git a/docs/_posts/2024-09-20-tensile-instability-p2.md b/docs/_posts/2024-09-20-tensile-instability-p2.md index 02ce7ec6f..100588d3b 100644 --- a/docs/_posts/2024-09-20-tensile-instability-p2.md +++ b/docs/_posts/2024-09-20-tensile-instability-p2.md @@ -17,7 +17,7 @@ If only the hourglass modes have contribution, one may require that all the numerical simulations which are identified as tensile instability become numerically stable if only the method preventing hourglass is applied. -

Zigzag +

Zigzag

Fig. 2. Illustration of zero energy modes by considering a simple case. The particles are uniformly distributed along the x-axis, and change from time step n to time step n + 1