Skip to content

Conversation

@Guo-astro
Copy link
Contributor

@Guo-astro Guo-astro commented Jan 8, 2026

Summary

Adds the complete Newtonian physics mode for GSPH.

Headers

  • NewtonianConfig: solver configuration for Newtonian hydro
  • NewtonianEOS: ideal gas equation of state interface
  • NewtonianFieldNames: field naming constants
  • NewtonianForceKernel: force computation interface
  • NewtonianMode: PhysicsMode implementation
  • NewtonianTimestepper: CFL-based timestepping
  • forces.hpp: force math functions
  • ReconstructConfig: interface reconstruction settings
  • RiemannConfig: Riemann solver configuration

Riemann Solvers

  • RiemannBase: abstract Riemann solver interface
  • HLL: Harten-Lax-van Leer approximate Riemann solver
  • Iterative: exact iterative Riemann solver

Sources

Complete implementations for all Newtonian components.

Dependencies

Depends on #1523 (core infrastructure)

@github-actions
Copy link

github-actions bot commented Jan 8, 2026

Thanks @Guo-astro for opening this PR!

You can do multiple things directly here:
1 - Comment pre-commit.ci run to run pre-commit checks.
2 - Comment pre-commit.ci autofix to apply fixes.
3 - Add label autofix.ci to fix authorship & pre-commit for every commit made.
4 - Add label light-ci to only trigger a reduced & faster version of the CI (need the full one before merge).
5 - Add label trigger-ci to create an empty commit to trigger the CI.

Once the workflow completes a message will appear displaying informations related to the run.

Also the PR gets automatically reviewed by gemini, you can:
1 - Comment /gemini review to trigger a review
2 - Comment /gemini summary for a summary
3 - Tag it using @gemini-code-assist either in the PR or in review comments on files

@gemini-code-assist
Copy link

Summary of Changes

Hello @Guo-astro, I'm Gemini Code Assist1! I'm currently reviewing this pull request and will post my feedback shortly. In the meantime, here's a summary to help you and other reviewers quickly get up to speed!

This pull request introduces a comprehensive Newtonian physics mode for the GSPH (Godunov Smoothed Particle Hydrodynamics) simulation framework. It establishes a robust foundation for simulating non-relativistic hydrodynamics, featuring a modular design that allows for configurable equations of state, advanced Riemann solvers for inter-particle force calculations, and flexible spatial reconstruction techniques. The new mode integrates a kick-drift-kick (KDK) leapfrog timestepping scheme, ensuring accurate and stable evolution of particle states.

Highlights

  • Core Newtonian Physics Mode: Introduction of NewtonianMode to implement standard GSPH with leapfrog time integration, handling the full timestep sequence.
  • Configurable Physics Components: New configuration structures for Newtonian hydro (NewtonianConfig), equation of state (NewtonianEOS), and field naming (NewtonianFieldNames).
  • Advanced Riemann Solvers: Integration of multiple Riemann solvers, including an exact iterative solver (van Leer 1997) and an approximate HLL solver, with configurable settings (RiemannConfig).
  • Spatial Reconstruction Options: Support for different spatial reconstruction methods, such as PiecewiseConstant and MUSCL with various slope limiters (ReconstructConfig).
  • Modular Force and Timestepping: Dedicated modules for force computation (NewtonianForceKernel, forces.hpp) and CFL-based leapfrog time integration (NewtonianTimestepper).
Using Gemini Code Assist

The full guide for Gemini Code Assist can be found on our documentation page, here are some quick tips.

Invoking Gemini

You can request assistance from Gemini at any point by creating a comment using either /gemini <command> or @gemini-code-assist <command>. Below is a summary of the supported commands on the current page.

Feature Command Description
Code Review /gemini review Performs a code review for the current pull request in its current state.
Pull Request Summary /gemini summary Provides a summary of the current pull request in its current state.
Comment @gemini-code-assist Responds in comments when explicitly tagged, both in pull request comments and review comments.
Help /gemini help Displays a list of available commands.

Customization

To customize Gemini Code Assist for GitHub experience, repository maintainers can create a configuration file and/or provide a custom code review style guide (such as PEP-8 for Python) by creating and adding files to a .gemini/ folder in the base of the repository. Detailed instructions can be found here.

Limitations & Feedback

Gemini Code Assist may make mistakes. Please leave feedback on any instances where its feedback is incorrect or counter productive. You can react with 👍 and 👎 on @gemini-code-assist comments. If you're interested in giving your feedback about your experience with Gemini Code Assist for Github and other Google products, sign up here.

You can also get AI-powered code generation, chat, as well as code reviews directly in the IDE at no cost with the Gemini Code Assist IDE Extension.

Footnotes

  1. Review the Privacy Notices, Generative AI Prohibited Use Policy, Terms of Service, and learn how to configure Gemini Code Assist in GitHub here. Gemini can make mistakes, so double check it and use code with caution.

Copy link

@gemini-code-assist gemini-code-assist bot left a comment

Choose a reason for hiding this comment

The reason will be displayed to describe this comment to others. Learn more.

Code Review

This pull request introduces the complete Newtonian physics mode for GSPH, including configurations for the solver, equation of state, field names, force kernels, and timesteppers. It also adds support for different Riemann solvers and reconstruction methods. The changes are extensive and well-structured, providing a solid foundation for Newtonian hydrodynamics within the SHAMROCK framework. All provided comments offer valid and useful feedback, addressing areas where consistency, maintainability, and completeness could be improved, particularly regarding the dynamic selection of Riemann solvers and the use of named constants for field identifiers.

@Guo-astro Guo-astro changed the title [GSPH] Add complete Newtonian physics mode [GSPH 2/7] Newtonian physics mode Jan 8, 2026
@Guo-astro
Copy link
Contributor Author

/gemini review

Copy link

@gemini-code-assist gemini-code-assist bot left a comment

Choose a reason for hiding this comment

The reason will be displayed to describe this comment to others. Learn more.

Code Review

This pull request introduces a comprehensive Newtonian physics mode for GSPH, including configurations, timestepping, EOS, and force computations with various Riemann solvers. The overall structure is well-designed, using modern C++ features like std::variant for flexible configuration. However, there are several areas for improvement. The implementation currently hardcodes the choice of Riemann solver and reconstruction method, bypassing the flexible configuration system that was also introduced. There's also significant code duplication in the force kernels and a minor inconsistency in the EOS implementation. Additionally, a performance improvement opportunity exists in the force calculation loop. Addressing these points will make the new module more robust, maintainable, and aligned with the configurable design.

@Guo-astro Guo-astro force-pushed the pr/gsph-newtonian-physics branch from 45e892a to e51d1f4 Compare January 9, 2026 07:06
Core Infrastructure:
- PhysicsMode base class for strategy pattern implementation
- ForceKernelBase for common force computation interface
- PhysicsModeFactory for creating physics mode instances
- FieldNames.hpp as SSOT for field naming

Modular Components:
- BoundaryHandler: boundary condition processing
- BuildTrees: tree construction
- ComputeCFL: CFL timestep calculation
- ComputeGradients: gradient computation
- ComputeOmega: omega factor computation
- GhostCommunicator: MPI ghost communication
- IterateSmoothingLengthVolume: h-iteration
- NeighbourCache: caching neighbor interactions
- FunctorNode: generic functor nodes

Refactors the monolithic GSPH Solver into modular components,
preparing for physics mode decoupling (Newtonian vs SR).
The ForceKernelBase template class was designed as a Template Method pattern
base but was never used - NewtonianForceKernel and SRForceKernel are standalone
implementations with their own buffer management appropriate for their physics.

The hardcoded CommonBuffers design (buf_density, buf_pressure, etc.) does not
accommodate SR physics which requires distinct lab-frame vs rest-frame field
naming (N_LABFRAME, LORENTZ_FACTOR, ENTHALPY, etc.).
These fields have physics-specific meanings:
- Newtonian: single frame quantities
- SR: lab-frame vs rest-frame distinction

Each physics mode now defines its own field constants with
appropriate semantic names in their respective FieldNames headers.
Headers:
- NewtonianConfig: solver configuration for Newtonian hydro
- NewtonianEOS: ideal gas equation of state interface
- NewtonianFieldNames: field naming constants
- NewtonianForceKernel: force computation interface
- NewtonianMode: PhysicsMode implementation for Newtonian hydro
- NewtonianTimestepper: CFL-based timestepping
- forces.hpp: force math functions
- ReconstructConfig: interface reconstruction settings
- RiemannConfig: Riemann solver configuration

Riemann Solvers:
- RiemannBase: abstract Riemann solver interface
- HLL: Harten-Lax-van Leer approximate Riemann solver
- Iterative: exact iterative Riemann solver

Sources:
- Complete implementations for all Newtonian components

This implements the Newtonian physics mode for GSPH using
the strategy pattern for physics decoupling.
Energy fields have physics-specific meanings and are now defined
directly in NewtonianFieldNames.hpp rather than imported from
the common FieldNames.hpp.
Headers:
- SRConfig: solver configuration for SR hydro
- SREOS: relativistic equation of state interface
- SRFieldNames: field naming constants for SR fields
- SRForceKernel: force computation interface for SR
- SRMode: PhysicsMode implementation for SR hydro
- SRPrimitiveRecovery: conservative to primitive variable recovery
- SRTimestepper: relativistic CFL-based timestepping
- forces.hpp: SR force math functions

Sources:
- SREOS.cpp: relativistic EOS implementation
- SRForceKernel.cpp: SR force kernel implementation
- SRPrimitiveRecovery.cpp: Newton-Raphson primitive recovery
- SRTimestepper.cpp: SR timestep computation

This implements the core SR physics components for GSPH.
SR physics defines its own XYZ, VXYZ, AXYZ, UINT, DUINT constants
directly rather than importing from the common FieldNames.hpp.
This clarifies the physical meaning (lab-frame quantities for SR).
Recovery Methods:
- RecoveryBase: abstract interface for primitive recovery
- NewtonRaphson: Newton-Raphson iterative recovery algorithm

Riemann Solvers:
- RiemannBase: abstract SR Riemann solver interface
- Exact: exact relativistic Riemann solver (Pons 2000)

Mode Implementation:
- SRMode.cpp: complete SR physics mode orchestration
  - Ghost field setup for SR variables
  - Primitive recovery from conserved variables
  - Force computation with relativistic corrections
  - Integration of SR equations

This completes the Special Relativistic GSPH implementation
following Kitajima 2024 formulation.
Solver Changes:
- Solver.hpp/cpp: Refactored to use PhysicsMode strategy pattern
- SolverConfig.hpp/cpp: Updated config for physics mode selection
- Model.hpp/cpp: Updated model registration

Storage & IO:
- SolverStorage.hpp: Updated field storage for physics modes
- VTKDump.hpp/cpp: Physics-aware VTK output

Python Bindings:
- pyGSPHModel.cpp: Extended bindings for SR configuration
  - physics_mode selection (newtonian/sr)
  - SR-specific parameters (gamma, initial conditions)

Build System:
- CMakeLists.txt: Updated for new physics module structure

This integrates the modular physics modes into the GSPH solver,
enabling runtime selection between Newtonian and SR physics.
Newtonian Tests:
- sod_tube_gsph.py: Sod shock tube validation
- blast_wave_gsph.py: Extreme blast wave test

SR Tests (Kitajima 2024 benchmark suite):
- problem1_sod.py: Relativistic Sod shock tube
- problem2_blast.py: Relativistic blast wave
- problem3_strong_blast.py: Strong relativistic blast
- problem4_ultra_relativistic.py: Ultra-relativistic regime
- problem5_tangent_velocity.py: Tangential velocity test
- problem6_2d_sod.py: 2D relativistic Sod tube
- problem7_kh_instability.py: Kelvin-Helmholtz instability

Common:
- sr/__init__.py: SR test utilities
- kitajima_plotting.py: Plotting helpers for Kitajima benchmarks

All tests use:
- ctx.collect_data() for direct memory access (no pyvista)
- Strict tolerances (~1e-8) for regression testing
- Analytic solutions for validation
Unit Tests:
- GSPHForceTests.cpp: Update for new physics structure
- GSPHRiemannTests.cpp: Update Riemann solver tests

SPH Module Fixes:
- IterateSmoothingLengthDensity: Improve h-iteration logging
- BasicSPHGhosts.cpp: Fix ghost handling

Math:
- sphkernels.hpp: Minor kernel fixes

MHD Placeholder:
- MHDConfig.hpp: Placeholder for future MHD physics mode
- NewtonianMode: add compute_omega_newtonian() using standard SPH (no c_smooth)
- SRMode: use SRIterateSmoothingLength with Kitajima volume-based approach
- Remove shared ComputeOmega module (each mode now owns this)
- Remove legacy UpdateDerivs (replaced by NewtonianForceKernel)
- Move IterateSmoothingLengthVolume to physics/sr/SRIterateSmoothingLength
- Update CMakeLists.txt sources

This fixes the density/pressure error regression caused by c_smooth=1.2
being incorrectly applied to Newtonian mode.
…ult (1.0)

SR's volume-based h-iteration (Kitajima Eq. 232-233) requires c_smooth > 1
to smooth h variation across discontinuities. The SR-specific value was
defined in SRConfig but not transferred to the shared config.
The Riemann solver and force computation code has been moved to
the physics/newtonian/ and physics/sr/ directories. The math/ folder
contained duplicate/orphaned code that is no longer used.
Remove deprecated include of math/riemann/iterative.hpp (now deleted)
and update hllc_solver call to use solve_hll from the new location
in physics/newtonian/riemann/HLL.hpp.
@Guo-astro Guo-astro force-pushed the pr/gsph-newtonian-physics branch from c95ae36 to 26ad744 Compare January 9, 2026 07:48
Guo-astro and others added 2 commits January 9, 2026 19:56
Run buildbot/update_authors.py to add --no git blame-- annotations
to author headers as required by CI checks.
Remove SolverCallbacks struct and have PhysicsMode evaluate nodes
directly via storage.solver_graph. This aligns with solvergraph design:
- Branching happens at init time (node registration)
- Flow is visible as graph structure
- No runtime callback creation

Changes:
- Register Solver method nodes in init_solver_graph()
- Delete SolverCallbacks struct from PhysicsMode.hpp
- Update evolve_timestep() signature (remove callbacks param)
- NewtonianMode/SRMode evaluate nodes directly via storage.solver_graph

Co-Authored-By: Claude Opus 4.5 <noreply@anthropic.com>
@Guo-astro Guo-astro closed this Jan 9, 2026
Sign up for free to join this conversation on GitHub. Already have an account? Sign in to comment

Projects

None yet

Development

Successfully merging this pull request may close these issues.

2 participants