EOS interpolation
Shared infrastructure for PALEOS-format tables: file readers (load_paleos_table for the 2-phase format, load_paleos_unified_table for the single-file-per-material format), the log-uniform grid builder used by both, and the inner kernels _fast_bilinear (O(1) bilinear lookup) and _paleos_clamp_temperature (per-cell temperature clamp to the table's valid range). These kernels are called millions of times per Zalmoxis solve, so they avoid np.interp binary searches by exploiting the log-uniform grid. The cache populated by _ensure_unified_cache is reused across calls within the same process.
interpolation
Shared interpolation helpers for PALEOS EOS tables.
Provides table loading, bilinear interpolation, and per-cell temperature clamping used by all PALEOS-based EOS lookups.
load_paleos_table(eos_file)
Load a PALEOS MgSiO3 table and build RegularGridInterpolator objects.
The PALEOS tables have 10 columns (SI units): P, T, rho, u, s, cp, cv, alpha, nabla_ad, phase_id(string). The grid is log-uniform in both P and T with 150 points per decade. Some grid cells are missing (unconverged corners), filled with NaN. A P=0 row may exist and is excluded for log interpolation.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
eos_file
|
str
|
Path to the PALEOS table file. |
required |
Returns:
| Type | Description |
|---|---|
dict
|
Cache entry with keys:
- |
Source code in src/zalmoxis/eos/interpolation.py
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load_paleos_unified_table(eos_file)
Load a unified PALEOS table (single file per material) and build interpolators.
The unified tables use the same 10-column format as the 2-phase tables (P, T, rho, u, s, cp, cv, alpha, nabla_ad, phase_id) but contain all stable phases for a material in a single file. The thermodynamically stable phase at each (P, T) is encoded in the phase column.
In addition to density and nabla_ad interpolators, this function extracts the liquidus boundary from the phase column: for each pressure row, it finds the lowest temperature where the phase is 'liquid'.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
eos_file
|
str
|
Path to the unified PALEOS table file. |
required |
Returns:
| Type | Description |
|---|---|
dict
|
Cache entry with keys:
- |
Source code in src/zalmoxis/eos/interpolation.py
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_fast_bilinear(log_p, log_t, grid, cached)
O(1) bilinear interpolation on a log-uniform grid (scalar).
Optimized for the hot path: called ~2M times per structure solve. Uses direct floor indexing (no rounding, no max/min builtins).
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
log_p
|
float
|
log10 of pressure, already clamped to grid bounds. |
required |
log_t
|
float
|
log10 of temperature, already clamped to valid range. |
required |
grid
|
ndarray
|
2D array of values, shape (n_p, n_t). |
required |
cached
|
dict
|
Cache entry with grid metadata. |
required |
Returns:
| Type | Description |
|---|---|
float
|
Interpolated value. NaN if any corner is NaN. |
Source code in src/zalmoxis/eos/interpolation.py
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fast_bilinear_batch(log_p_arr, log_t_arr, grid, cached)
Vectorized O(1) bilinear interpolation on a log-uniform grid.
Batch version of _fast_bilinear for arrays of query points.
Uses numpy vectorized operations instead of Python loops, giving
5-10x speedup over calling _fast_bilinear in a loop or using
scipy RegularGridInterpolator for small-to-medium batches.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
log_p_arr
|
ndarray
|
1D array of log10(pressure) values. |
required |
log_t_arr
|
ndarray
|
1D array of log10(temperature) values (same length as log_p_arr). |
required |
grid
|
ndarray
|
2D array of values, shape (n_p, n_t). |
required |
cached
|
dict
|
Cache entry with grid metadata. |
required |
Returns:
| Type | Description |
|---|---|
ndarray
|
Interpolated values. NaN where any corner is NaN. |
Source code in src/zalmoxis/eos/interpolation.py
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_paleos_clamp_temperature(log_p, log_t, cached)
Clamp log10(T) to the per-pressure valid range of a PALEOS table.
Uses O(1) index computation on the log-uniform pressure grid instead of np.interp (which does binary search on 1000+ elements). This is called millions of times in the scalar ODE path.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
log_p
|
float
|
log10 of pressure in Pa (already clamped to table bounds). |
required |
log_t
|
float
|
log10 of temperature in K. |
required |
cached
|
dict
|
PALEOS cache entry. |
required |
Returns:
| Type | Description |
|---|---|
float
|
Clamped log10(T). |
bool
|
True if clamping was applied. |
Source code in src/zalmoxis/eos/interpolation.py
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_ensure_unified_cache(eos_file, interpolation_functions)
Ensure a unified PALEOS table is loaded into the interpolation cache.
Tries loading from a binary pickle cache first (fast), then falls back to the text table (slow). Saves a pickle cache after the first text load.
Parameters:
| Name | Type | Description | Default |
|---|---|---|---|
eos_file
|
str
|
Path to the unified PALEOS table file. |
required |
interpolation_functions
|
dict
|
Shared interpolation cache. |
required |
Returns:
| Type | Description |
|---|---|
dict
|
The cache entry for this file. |
Source code in src/zalmoxis/eos/interpolation.py
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