diff --git a/doc/pages/galactic_cosmic_rays.rst b/doc/pages/galactic_cosmic_rays.rst
index 0b83464a9..89e632a1a 100644
--- a/doc/pages/galactic_cosmic_rays.rst
+++ b/doc/pages/galactic_cosmic_rays.rst
@@ -36,6 +36,17 @@ changes, which can be modeled following the next examples.
 .. toctree::
    example_notebooks/Diffusion/AdiabaticCooling.ipynb
 
+Diffusive Shock Acceleration
+^^^^^^^^^^^^^^^^^^
+
+Diffusive shock acceleration or first order Fermi acceleration can be modeled
+in the diffusive picture as an interplay between diffusion, advection and 
+adiabatic cooling. Simple shock configurations are shown in the following 
+example notebook.
+
+.. toctree::
+   example_notebooks/acceleration/diffusive_shock_acceleration.ipynb
+
 Momentum Diffusion 
 ^^^^^^^^^^^^^^^^^^