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Template lambda for scalar calls #363

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c84f686
template ideal gas on eos lambda
jonahm-LANL Apr 17, 2024
3946c9b
Change LambdaIndexer to Indexer_t in eos_ideal
jonahm-LANL Apr 17, 2024
30534d7
davis use indexer_t
jonahm-LANL Apr 17, 2024
3aaa2cd
template gruneisen and eospac
jonahm-LANL Apr 17, 2024
9159b45
template-ify helm and jwl
jonahm-LANL Apr 17, 2024
8a7fe02
templateify eos_mgusup
jonahm-LANL Apr 17, 2024
92eb4dd
CC
jonahm-LANL Apr 17, 2024
96d98ae
templateify noble_abel
jonahm-LANL Apr 17, 2024
d36e7b4
templateify eos_powermg
jonahm-LANL Apr 17, 2024
35fc794
templateify sap polynomial
jonahm-LANL Apr 17, 2024
14fec2a
tempalteify eos_spiner
jonahm-LANL Apr 17, 2024
e4e39e6
templateify stellar collapse
jonahm-LANL Apr 17, 2024
286fefe
templateify stiff gas
jonahm-LANL Apr 17, 2024
f71358d
templateify vinet
jonahm-LANL Apr 17, 2024
c47bc56
templateify unitsystem
jonahm-LANL Apr 17, 2024
8bf8deb
templateify ramp
jonahm-LANL Apr 17, 2024
5103921
templateify relativistic eos
jonahm-LANL Apr 17, 2024
a69ab02
templateify shift and scale
jonahm-LANL Apr 18, 2024
cf4adca
make lambda an indexer
jonahm-LANL Apr 18, 2024
941da07
sfinae check for nullptr
jonahm-LANL Apr 18, 2024
49e38ef
apply sfinae check for null pointer
jonahm-LANL Apr 18, 2024
c840b90
add a check that indexers work
jonahm-LANL Apr 18, 2024
d04298f
formatting
jonahm-LANL Apr 18, 2024
d6fd188
CC
jonahm-LANL Apr 18, 2024
d272d7c
update docs and use more robust sfinae
jonahm-LANL Apr 18, 2024
5ea1111
constexpr and include utility
jonahm-LANL Apr 18, 2024
1254adf
CHANGELOG
jonahm-LANL Apr 18, 2024
df11689
python: update method signature
rbberger Apr 19, 2024
dc5f614
Merge branch 'main' into jmm/template-lambda
Yurlungur Apr 19, 2024
4ea36aa
no dereferencing indexers. they're not pointers necessarily.
jonahm-LANL Apr 19, 2024
b2ae8aa
potentially real dumb fix
jonahm-LANL Apr 19, 2024
35535a3
static casts. Static casts for everybody.
jonahm-LANL Apr 19, 2024
f519eb0
be REALLY explicit about wanting (Real*)(NULL)
jonahm-LANL Apr 19, 2024
d7f913e
add remove_cvref
jonahm-LANL Apr 22, 2024
e533122
Merge branch 'main' into jmm/template-lambda
Yurlungur Apr 22, 2024
1336455
Merge branch 'main' into jmm/template-lambda
Yurlungur Apr 23, 2024
e822af2
typo in commented out code
jonahm-LANL Apr 23, 2024
88f616b
static casts for everybody
jonahm-LANL Apr 23, 2024
3efad79
Merge branch 'main' into jmm/template-lambda
Yurlungur Apr 23, 2024
921d1c0
one more static cast for those at home
jonahm-LANL Apr 23, 2024
1eeed8a
add constexpr
jonahm-LANL Apr 24, 2024
019c5e4
Merge branch 'main' into jmm/template-lambda
Yurlungur Apr 25, 2024
32bcf9c
use array for host test of lambda, just to make the compiler stop com…
jonahm-LANL Apr 25, 2024
f594ee1
add constexpr function for generating nullptr of specific pointer type
jonahm-LANL Apr 25, 2024
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1 change: 1 addition & 0 deletions CHANGELOG.md
Original file line number Diff line number Diff line change
Expand Up @@ -21,6 +21,7 @@
- [[PR356]](https://github.com/lanl/singularity-eos/pull/356) Update CMake for proper Kokkos linking in Fortran interface

### Changed (changing behavior/API/variables/...)
- [[PR363]](https://github.com/lanl/singularity-eos/pull/363) Template lambda values for scalar calls

### Infrastructure (changes irrelevant to downstream codes)
- [[PR329]](https://github.com/lanl/singularity-eos/pull/329) Move vinet tests into analytic test suite
Expand Down
10 changes: 5 additions & 5 deletions doc/sphinx/src/using-closures.rst
Original file line number Diff line number Diff line change
Expand Up @@ -460,11 +460,11 @@ total specific internal energy in the problem, ``rho`` is an indexer
over densities, one per material. ``vfract`` is an indexer over volume
fractions, one per material. ``sie`` is an indexer over temperatures,
one per material. ``press`` is an indexer over pressures, one per
material. ``lambda`` is an indexer over lambda arrays, one ``Real *``
object per material. ``scratch`` is a pointer to pre-allocated scratch
memory, as described above. It is assumed enough scratch has been
allocated. Finally, the optional argument ``Tguess`` allows for host
codes to pass in an initial temperature guess for the solver. For more
material. ``lambda`` is an indexer over lambda arrays, one per
material. ``scratch`` is a pointer to pre-allocated scratch memory, as
described above. It is assumed enough scratch has been allocated.
Finally, the optional argument ``Tguess`` allows for host codes to
pass in an initial temperature guess for the solver. For more
information on initial guesses, see the section below.

The constructor for the ``PTESolverRhoU`` has the same structure:
Expand Down
141 changes: 102 additions & 39 deletions doc/sphinx/src/using-eos.rst
Original file line number Diff line number Diff line change
Expand Up @@ -77,7 +77,7 @@ method. ``get`` is templated and type deduction is not possible. You
must specify the type of the class you're pulling out of the
variant. For example:

.. code-block::
.. code-block:: cpp

auto my_ideal_gas = my_eos.get<singularity::IdealGas>();

Expand All @@ -91,7 +91,7 @@ The EOS model also allows some host-side introspection. The method
returns a string representing the equation of state an ``EOS`` object
currently is. For example:

.. code-block::
.. code-block:: cpp

auto tpe_str = my_ideal_gas.EosType();
// prints "IdealGas"
Expand Down Expand Up @@ -158,20 +158,16 @@ method, which can be called as, e.g.,

eos.Finalize();

Vector and Scalar API, Accessors
---------------------------------
Accessors and Indexers
-----------------------

Most ``EOS`` methods have both scalar and vector overloads, where the
scalar version returns a value, and the vector version modifies an
array. By default the vector version is called from host on device (if
``singularity-eos`` was compiled for device).

The vector API is templated to accept *accessors*. An accessor is any
object with a square bracket operator. One-dimensional arrays,
pointers, and ``std::vector<double>`` are all examples of what we call
an accessor. However, the value of an accessor is it doesn't have to
be an array. You can create an accessor class that wraps your
preferred memory layout, and ``singularity-eos`` will handle it
Many functions in ``singularity-eos`` accept **accessors**, also
called **indexers**. An accessor is any object with a square bracket
operator. One-dimensional arrays, pointers, and
``std::vector<double>`` are all examples of what we call an
accessor. However, the value of an accessor is it doesn't have to be
an array. You can create an accessor class that wraps your preferred
memory layout, and ``singularity-eos`` will handle it
appropriately. An accessor that indexes into an array with some stride
might look like this:

Expand All @@ -186,8 +182,20 @@ might look like this:
int stride_;
};

We do note, however, that vectorization may suffer if your underlying
data structure is not contiguous in memory.
The Vector API and the ``lambda`` optional arguments all use
accessors, as discussed below.

Vector and Scalar API
----------------------

Most ``EOS`` methods have both scalar and vector overloads, where the
scalar version returns a value, and the vector version modifies an
array. By default the vector version is called from host on device (if
``singularity-eos`` was compiled for device).

The vector API is templated to accept accessors. We do note, however,
that vectorization may suffer if your underlying data structure is not
contiguous in memory.

.. _eospac_vector:

Expand Down Expand Up @@ -246,7 +254,7 @@ decorated so that it may be evaluated on either host or device,
depending on desired use-case. Alternatively, you may use an anonymous
function with an `auto` argument as the input, e.g.,

.. code-block::
.. code-block:: cpp

// equivalent to [=], but with device markings
eos.Evaluate(PORTABLE_LAMBDA(auto eos) { /* my code snippet */ });
Expand Down Expand Up @@ -339,21 +347,25 @@ Lambdas and Optional Parameters
--------------------------------

Most methods for ``EOS`` objects accept an optional ``lambda``
parameter, which is a ``Real *``. Unless specified in :ref:`the
models section <models>`, this parameter does nothing. However, some
models require or benefit from additional information. For example
models with internal root finds can leverage initial guesses and
models with composition mixing parameters may need additional input to
return a meaningful state.
parameter, which is an accessor as discussed above. ``lambda[i]``
should return a real number unless ``lambda==nullptr``. Unless
specified in :ref:`the models section <models>`, this parameter does
nothing, and the default type is ``Real*`` with a default value of
``nullptr``

However, some models require or benefit from additional
information. For example models with internal root finds can leverage
initial guesses and models with composition mixing parameters may need
additional input to return a meaningful state.

``EOS`` models are introspective and can provide the desired/required
size of the lambda array with:

.. cpp:function:: int EOS::nlambda()

which is the desired size of the ``lambda`` array per scalar call. For
vector calls, there should be one such array per grid point. An
accessor for ``lambda`` should return a ``Real *`` pointer at each
vector calls, there should be one such accessor per grid point. A
vector accessor for ``lambda`` should return an accessor at each
index. A trivial example of such an indexer for ``lambda`` might be
the null indexer:

Expand Down Expand Up @@ -551,13 +563,17 @@ cgs. Unless specified, all functions work on device, if the code is
compiled appropriately. The exceptions are constructors,
``GetOnDevice``, and ``Finalize``, all of which are host-only.

.. cpp:function:: Real TemperatureFromDensityInternalEnergy(const Real rho, const Real sie, Rela &lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real TemperatureFromDensityInternalEnergy(const Real rho, const Real sie,
Indexer_t &&lambda = nullptr) const;

Returns temperature in Kelvin. Inputs are density in :math:`g/cm^3`
and specific internal energy in :math:`erg/g`. The vector equivalent
of this function is

.. code-block::
.. code-block:: cpp

template <typename RealIndexer, typename ConstRealIndexer, typename LambdaIndexer>
inline void
Expand All @@ -574,33 +590,57 @@ parameter is always last in the function signature. As they are all
almost exactly analogous to their scalar counterparts, we will mostly
not list the vector functions here.

.. cpp:function:: Real InternalEnergyFromDensityTemperature(const Real rho, const Real temperature, Real *lambda=nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real InternalEnergyFromDensityTemperature(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns specific internal energy in :math:`erg/g` given a density in
:math:`g/cm^3` and a temperature in Kelvin.

.. cpp:function:: Real PressureFromDensityTemperature(const Real rho, const Real temperature, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real PressureFromDensityTemperature(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns pressure in Barye given density in :math:`g/cm^3` and temperature in Kelvin.

.. cpp:function:: Real PressureFromDensityInternalEnergy(const Real rho, const Real temperature, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real PressureFromDensityInternalEnergy(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns pressure in Barye given density in :math:`g/cm^3` and specific
internal energy in :math:`erg/g`.

.. cpp:function:: Real SpecificHeatFromDensityTemperature(const Real rho, const Real temperature, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real SpecificHeatFromDensityTemperature(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns specific heat capacity at constant volume, in units of
:math:`erg/(g K)` in terms of density in :math:`g/cm^3` and
temperature in Kelvin.

.. cpp:function:: Real SpecificHeatFromDensityInternalEnergy(const Real rho, const Real sie, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real SpecificHeatFromDensityInternalEnergy(const Real rho, const Real sie,
Indexer_t &&lambda = nullptr) const;

returns specific heat capacity at constant volume, in units of
:math:`erg/(g K)` in terms of density in :math:`g/cm^3` and specific
internal energy in :math:`erg/g`.

.. cpp:function:: Real BulkModulusFromDensityTemperature(const Real rho, const Real temperature, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real BulkModulusFromDensityTemperature(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns the the bulk modulus

Expand All @@ -627,12 +667,20 @@ enthalpy by volume. The sound speed may also differ for, e.g., porous
models, where the pressure is less directly correlated with the
density.

.. cpp:function:: Real BulkModulusFromDensityInternalEnergy(const Real rho, const Real sie, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real BulkModulusFromDensityInternalEnergy(const Real rho, const Real sie,
Indexer_t &&lambda = nullptr) const;

returns the bulk modulus in units of :math:`g cm^2/s^2` given density
in :math:`g/cm^3` and specific internal energy in :math:`erg/g`.

.. cpp:function:: Real GruneisenParamFromDensityTemperature(const Real rho, const Real temperature, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real GruneisenParamFromDensityTemperature(const Real rho, const Real temperature,
Indexer_t &&lambda = nullptr) const;

returns the unitless Gruneisen parameter

Expand All @@ -642,14 +690,23 @@ returns the unitless Gruneisen parameter

given density in :math:`g/cm^3` and temperature in Kelvin.

.. cpp:function:: Real GruneisenParamFromDensityInternalEnergy(const Real rho, const Real sie, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
Real GruneisenParamFromDensityInternalEnergy(const Real rho, const Real sie,
Indexer_t &&lambda = nullptr) const;

returns the unitless Gruneisen parameter given density in
:math:`g/cm^3` and specific internal energy in :math:`erg/g`.

The function

.. cpp:function:: void ValuesAtReferenceState(Real &rho, Real &temp, Real &sie, Real &press, Real &cv, Real &bmod, Real &dpde, Real &dvdt, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
void ValuesAtReferenceState(Real &rho, Real &temp, Real &sie, Real &press,
Real &cv, Real &bmod, Real &dpde, Real &dvdt,
Indexer_t &&lambda = nullptr) const;

fills the density, temperature, specific internal energy, pressure,
and thermodynamic derivatives a specifically chosen characteristic
Expand All @@ -660,7 +717,13 @@ representative energy and density scale.

The function

.. cpp:function:: void FillEos(Real &rho, Real &temp, Real &energy, Real &press, Real &cv, Real &bmod, const unsigned long output, Real *lambda = nullptr) const;
.. code-block:: cpp

template <typename Indexer_t = Real*>
void FillEos(Real &rho, Real &temp, Real &energy,
Real &press, Real &cv, Real &bmod,
const unsigned long output,
Indexer_t &&lambda = nullptr) const;

is a a bit of a special case. ``output`` is a bitfield represented as
an unsigned 64 bit number. Quantities such ``pressure`` and
Expand Down
14 changes: 8 additions & 6 deletions python/module.hpp
Original file line number Diff line number Diff line change
Expand Up @@ -14,6 +14,7 @@
// clang-format off
#include <pybind11/pybind11.h>
#include <pybind11/numpy.h>
#include <singularity-eos/base/variadic_utils.hpp>
#include <singularity-eos/eos/eos.hpp>
#include <map>
#include <string>
Expand All @@ -24,17 +25,18 @@

namespace py = pybind11;
using namespace singularity;
using singularity::variadic_utils::np;

// Helper function to convert lambda numpy array to double* buffer
// With std::optional we would add support for a default value of lambda=None
template<typename T, PORTABLE_FUNCTION Real(T::*Func)(const Real, const Real, Real*) const>
template<typename T, PORTABLE_FUNCTION Real(T::*Func)(const Real, const Real, Real*&&) const>
Real two_params(const T& self, const Real a, const Real b, py::array_t<Real> lambda) {
return (self.*Func)(a, b, lambda.mutable_data());
}

template<typename T, PORTABLE_FUNCTION Real(T::*Func)(const Real, const Real, Real*) const>
template<typename T, PORTABLE_FUNCTION Real(T::*Func)(const Real, const Real, Real*&&) const>
Real two_params_no_lambda(const T& self, const Real a, const Real b) {
return (self.*Func)(a, b, nullptr);
return (self.*Func)(a, b, np<Real>());
}

class LambdaHelper {
Expand Down Expand Up @@ -326,7 +328,7 @@ py::class_<T> eos_class(py::module_ & m, std::string name) {
auto lambda = kwargs["lmbda"].cast<py::array_t<Real>>();
self.FillEos(s.density, s.temperature, s.specific_internal_energy, s.pressure, s.specific_heat, s.bulk_modulus, output, lambda.mutable_data());
} else {
self.FillEos(s.density, s.temperature, s.specific_internal_energy, s.pressure, s.specific_heat, s.bulk_modulus, output, nullptr);
self.FillEos(s.density, s.temperature, s.specific_internal_energy, s.pressure, s.specific_heat, s.bulk_modulus, output, np<Real>());
}
return s;
})
Expand All @@ -337,7 +339,7 @@ py::class_<T> eos_class(py::module_ & m, std::string name) {
})
.def("ValuesAtReferenceState", [](const T & self){
EOSState s;
self.ValuesAtReferenceState(s.density, s.temperature, s.specific_internal_energy, s.pressure, s.specific_heat, s.bulk_modulus, s.dpde, s.dvdt, nullptr);
self.ValuesAtReferenceState(s.density, s.temperature, s.specific_internal_energy, s.pressure, s.specific_heat, s.bulk_modulus, s.dpde, s.dvdt, np<Real>());
return s;
})

Expand All @@ -354,7 +356,7 @@ py::class_<T> eos_class(py::module_ & m, std::string name) {
}, py::arg("press"), py::arg("temp"), py::arg("lmbda"))
.def("DensityEnergyFromPressureTemperature", [](const T & self, const Real press, const Real temp) {
Real rho, sie;
self.DensityEnergyFromPressureTemperature(press, temp, nullptr, rho, sie);
self.DensityEnergyFromPressureTemperature(press, temp, np<Real>(), rho, sie);
return std::pair<Real, Real>(rho, sie);
}, py::arg("press"), py::arg("temp"))
.def("Finalize", &T::Finalize)
Expand Down
32 changes: 31 additions & 1 deletion singularity-eos/base/variadic_utils.hpp
Original file line number Diff line number Diff line change
@@ -1,5 +1,5 @@
//------------------------------------------------------------------------------
// © 2021-2023. Triad National Security, LLC. All rights reserved. This
// © 2021-2024. Triad National Security, LLC. All rights reserved. This
// program was produced under U.S. Government contract 89233218CNA000001
// for Los Alamos National Laboratory (LANL), which is operated by Triad
// National Security, LLC for the U.S. Department of Energy/National
Expand All @@ -16,13 +16,43 @@
#define SINGULARITY_EOS_BASE_VARIADIC_UTILS_HPP_

#include <type_traits>
#include <utility>

namespace singularity {
namespace variadic_utils {

// Some generic variatic utilities
// ======================================================================

// Useful for generating nullptr of a specific pointer type
template <typename T>
inline constexpr T *np() {
return nullptr;
}

// C++14 implementation of std::remove_cvref (available since C++20)
// credit to CJ + Diego
template <typename T>
struct remove_cvref {
typedef std::remove_cv_t<std::remove_reference_t<T>> type;
};

// Helper types
template <typename T>
using remove_cvref_t = typename remove_cvref<T>::type;

// SFINAE to check if a value is a null ptr
template <typename T, typename = typename std::enable_if<
std::is_pointer<remove_cvref_t<T>>::value>::type>
constexpr inline bool is_nullptr(T &&t) {
return std::forward<T>(t) == nullptr;
}
template <typename T, typename std::enable_if<
!std::is_pointer<remove_cvref_t<T>>::value>::type * = nullptr>
constexpr inline bool is_nullptr(T &&) {
return false;
}

// Backport of C++17 bool_constant.
// With C++17, can be replaced with
// using std::bool_constant
Expand Down
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