diff --git a/doc/RTD/source/HydroSchemes/index.rst b/doc/RTD/source/HydroSchemes/index.rst
index 3b511e03c0d0e92c6b663050d4c85df87860316f..d77649ee608bc17796339d2019e1b9e391f7eecf 100644
--- a/doc/RTD/source/HydroSchemes/index.rst
+++ b/doc/RTD/source/HydroSchemes/index.rst
@@ -2,7 +2,7 @@
    Josh Borrow 4th April 2018
 
 .. _hydro:
-   
+
 Hydrodynamics Schemes
 =====================
 
@@ -39,8 +39,8 @@ In case the case of a 2 loop scheme, SWIFT removes the gradient loop and the ext
    sphenix_sph
    gasoline_sph
    phantom_sph
+   remix_sph
    adaptive_softening
    gizmo
    shadowswift
    adding_your_own
-
diff --git a/doc/RTD/source/HydroSchemes/remix_sph.rst b/doc/RTD/source/HydroSchemes/remix_sph.rst
new file mode 100644
index 0000000000000000000000000000000000000000..e1a05fc8e21c98837d62690cbb42ebdf0880fcba
--- /dev/null
+++ b/doc/RTD/source/HydroSchemes/remix_sph.rst
@@ -0,0 +1,94 @@
+.. REMIX SPH
+    Thomas Sandnes, 13th May 2025
+
+.. _remix_sph:
+
+REMIX SPH
+==============================================
+
+.. toctree::
+   :maxdepth: 2
+   :hidden:
+   :caption: Contents:
+
+REMIX is an SPH scheme designed to alleviate effects that typically suppress
+mixing and instability growth at density discontinuities in SPH simulations
+(Sandnes et al. 2025). REMIX addresses this problem by directly targeting sources
+of kernel smoothing error and discretisation error, resulting in a generalised,
+material-independent formulation that improves the treatment both of
+discontinuities within a single material, for example in an ideal gas, and of
+interfaces between dissimilar materials. The scheme combines:
+
++ An evolved density estimate to avoid the kernel smoothing error in the
+  standard SPH integral density estimate;
++ Thermodynamically consistent, conservative equations of motion, with
+  free functions chosen to limit zeroth-order error;
++ Linear-order reproducing kernels with grad-h terms and a vacuum interface
+  treatment;
++ A "kernel normalising term" to avoid potential accumulation of error in
+  the evolved density estimate, such that densities would be no longer
+  representative of the distribution of particle masses in the simulation volume;
++ Advanced artificial viscosity and diffusion schemes with linear reconstruction
+  of quantities to particle midpoints, and a set of novel improvements to
+  effectively switch between treatments for shock-capturing under compression and
+  noise-smoothing in shearing regions.
+
+To configure with this scheme, use
+
+.. code-block:: bash
+
+  ./configure --with-hydro=remix --with-equation-of-state=planetary
+
+
+This scheme allows multiple materials,
+meaning that different SPH particles can be assigned different
+`equations of state <equations_of_state.html>`_ (EoS).
+Every SPH particle then requires and carries the additional ``MaterialID`` flag
+from the initial conditions file. This flag indicates the particle's material
+and which EoS it should use. Note that configuring with
+``--with-equation-of-state=planetary`` is required for this scheme, although
+for simulations that use a single, ideal gas EoS, setting all MaterialIDs to
+``0`` and including
+
+.. code-block:: yaml
+
+  EoS:
+      planetary_use_idg_def:    1
+
+in the parameter file are the only EoS-related additions needed compared with
+other non-Planetary hydro schemes. Note also that since densities are evolved in
+time, initial particle densities are required in initial conditions.
+
+We additionally recommend configuring with ``--with-kernel=wendland-C2`` and with
+
+.. code-block:: yaml
+
+  SPH:
+    resolution_eta:        1.487
+
+in the parameter file for improved hydrodynamic behaviour and since this is the
+configuration used for the validation simulations of Sandnes et al. (2025).
+
+
+The current implementation of the REMIX hydro scheme has been validated for
+planetary applications and in hydrodynamic test cases and does not include all
+necessary functionality for e.g. cosmological simulations.
+
+Default parameters used in the artificial viscosity and diffusion schemes and the
+normalising term are:
+
+.. code-block:: c
+
+  #define const_remix_visc_alpha 1.5f
+  #define const_remix_visc_beta 3.f
+  #define const_remix_visc_epsilon 0.1f
+  #define const_remix_visc_a 2.0f / 3.0f
+  #define const_remix_visc_b 1.0f / 3.0f
+  #define const_remix_difn_a_u 0.05f
+  #define const_remix_difn_b_u 0.95f
+  #define const_remix_difn_a_rho 0.05f
+  #define const_remix_difn_b_rho 0.95f
+  #define const_remix_norm_alpha 1.0f
+  #define const_remix_slope_limiter_exp_denom 0.04f
+
+These can be changed in ``src/hydro/REMIX/hydro_parameters.h``.
diff --git a/doc/RTD/source/Planetary/hydro_scheme.rst b/doc/RTD/source/Planetary/hydro_scheme.rst
index f0c787dce100142ecbe9b650fbee4d2110f34676..50d86e11944edbdb6828c64eb0a841b78b8c028b 100644
--- a/doc/RTD/source/Planetary/hydro_scheme.rst
+++ b/doc/RTD/source/Planetary/hydro_scheme.rst
@@ -16,5 +16,15 @@ and which EoS it should use.
 The Balsara viscosity switch is used by default, but can be disabled by
 compiling SWIFT with ``make CFLAGS=-DPLANETARY_SPH_NO_BALSARA``.
 
-Note: the boundary-improvement methods presented in Ruiz-Bonilla+2022 are
-in the process of being improved for release with better documentation etc soon.
+Note: the boundary-improvement method presented in Ruiz-Bonilla+2022 can be
+accessed on the ``planetary_imbalance_RB22`` git branch.
+
+.. _planetary_remix_hydro:
+
+REMIX SPH
+======================
+
+REMIX is an SPH scheme designed to alleviate effects that typically suppress
+mixing and instability growth at density discontinuities in SPH simulations
+(Sandnes et al. 2025). For more information on what is included in the REMIX
+scheme and how to configure SWIFT to use REMIX, see: :ref:`remix_sph`.
diff --git a/doc/RTD/source/Planetary/index.rst b/doc/RTD/source/Planetary/index.rst
index 15e2daedd9d53e22ac645b2e56b29f555b6af7cf..23997d67d67095837edaf2ac00311368316b8f15 100644
--- a/doc/RTD/source/Planetary/index.rst
+++ b/doc/RTD/source/Planetary/index.rst
@@ -22,11 +22,19 @@ and ``DemoImpact/``. Check out their `README.md` files for more info.
 The tabulated equation of state files can be downloaded there using
 ``EoSTables/get_eos_tables.sh``.
 
-To run planetary or similar simulations, SWIFT should be configured to use
-the planetary hydrodynamics scheme and equations of state:
-``--with-hydro=planetary`` and ``--with-equation-of-state=planetary``.
-These allow for multiple materials to be used,
-chosen from the several available equations of state.
+To run planetary or similar simulations with a traditional SPH formulation,
+SWIFT should be configured to use the planetary hydrodynamics scheme and
+equations of state: ``--with-hydro=planetary`` and
+``--with-equation-of-state=planetary``. These allow for multiple materials to be
+used, chosen from the several available equations of state. Planetary
+simulations can also be carried out using the more advanced :ref:`remix_sph` scheme,
+which improves the treatment of mixing and material interfaces
+(Sandnes et al. 2025). To configure within REMIX, use ``--with-hydro=remix`` and
+``--with-equation-of-state=planetary``. Note that REMIX simulations require
+initial particle densities in the initial conditions. We also recommend
+configuring with ``--with-kernel=wendland-C2`` and with ``resolution_eta: 1.487``
+in the parameter file for improved hydrodynamic behaviour and since this is the
+configuration used for the validation simulations of Sandnes et al. (2025).
 
 .. toctree::
    :maxdepth: 1