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https://github.com/paboyle/Grid.git
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183 lines
8.4 KiB
C++
183 lines
8.4 KiB
C++
/*
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* Example_plaquette.cc
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*
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* D. Clarke
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*
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* Here I just want to create an incredibly simple main to get started with GRID and get used
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* to its syntax. If the reader is like me, they vaguely understand something about lattice coding,
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* they don't know a ton of C++, don't know much of the fine details, and certainly know nothing about GRID.
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*
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* Once you've made a new executable, like this one, you can bootstrap.sh again. At this point,
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* the code should be able to find your new executable. You can tell that bootstrap.sh worked by
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* having a look at Make.inc. You should see your executable inside there.
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*
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* Warning: This code illustrative only, not well tested, and not meant for production use. The best
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* way to read this code is to start at the main.
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*
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*/
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// All your mains should have this
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#include <Grid/Grid.h>
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using namespace Grid;
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// This copies what already exists in WilsonLoops.h. The point here is to be pedagogical and explain in
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// detail what everything does so we can see how GRID works.
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template <class Gimpl> class WLoops : public Gimpl {
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public:
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// Gimpl seems to be an arbitrary class. Within this class, it is expected that certain types are
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// already defined, things like Scalar and Field. This macro includes a bunch of #typedefs that
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// implement this equivalence at compile time.
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INHERIT_GIMPL_TYPES(Gimpl);
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// Some example Gimpls can be found in GaugeImplementations.h, at the bottom. These are in turn built
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// out of GaugeImplTypes, which can be found in GaugeImplTypes.h. The GaugeImplTypes contain the base
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// field/vector/link/whatever types. These inherit from iScalar, iVector, and iMatrix objects, which
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// are sort of the building blocks for gerenal math objects. The "i" at the beginning of these names
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// indicates that they should be for internal use only. It seems like these base types have the
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// acceleration, e.g. SIMD or GPU or what-have-you, abstracted away. How you accelerate these things
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// appears to be controlled through a template parameter called vtype.
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// The general math/physics objects, such as a color matrix, are built up by nesting these objects.
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// For instance a general color matrix has two color indices, so it's built up like
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// iScalar<iScalar<iMatrix<vtype ...
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// where the levels going from the inside out are color, spin, then Lorentz indices. Scalars have
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// no indices, so it's what we use when such an index isn't needed. Lattice objects are made by one
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// higher level of indexing using iVector.
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// These types will be used for U and U_mu objects, respectively.
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typedef typename Gimpl::GaugeLinkField GaugeMat;
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typedef typename Gimpl::GaugeField GaugeLorentz;
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// U_mu_nu(x)
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static void dirPlaquette(GaugeMat &plaq, const std::vector<GaugeMat> &U, const int mu, const int nu) {
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// Calls like CovShiftForward and CovShiftBackward have 3 arguments, and they multiply together
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// the first and last argument. (Second arg gives the shift direction.) The CovShiftIdentityBackward
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// has meanwhile only two arguments; it just returns the shifted (adjoint since backward) link.
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plaq = Gimpl::CovShiftForward(U[mu],mu,
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// Means Link*Cshift(field,mu,1), arguments are Link, mu, field in that order.
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Gimpl::CovShiftForward(U[nu],nu,
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Gimpl::CovShiftBackward(U[mu],mu,
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// This means Cshift(adj(Link), mu, -1)
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Gimpl::CovShiftIdentityBackward(U[nu], nu))));
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}
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// tr U_mu_nu(x)
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static void traceDirPlaquette(ComplexField &plaq, const std::vector<GaugeMat> &U, const int mu, const int nu) {
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// This .Grid() syntax seems to get the pointer to the GridBase. Apparently this is needed as argument
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// to instantiate a Lattice object.
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GaugeMat sp(U[0].Grid());
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dirPlaquette(sp, U, mu, nu);
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plaq = trace(sp);
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}
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// sum_mu_nu tr U_mu_nu(x)
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static void sitePlaquette(ComplexField &Plaq, const std::vector<GaugeMat> &U) {
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ComplexField sitePlaq(U[0].Grid());
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Plaq = Zero();
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// Nd=4 and Nc=3 are set as global constants in QCD.h
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for (int mu = 1; mu < Nd; mu++) {
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for (int nu = 0; nu < mu; nu++) {
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traceDirPlaquette(sitePlaq, U, mu, nu);
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Plaq = Plaq + sitePlaq;
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}
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}
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}
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// sum_mu_nu_x Re tr U_mu_nu(x)
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static RealD sumPlaquette(const GaugeLorentz &Umu) {
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std::vector<GaugeMat> U(Nd, Umu.Grid());
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for (int mu = 0; mu < Nd; mu++) {
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// Umu is a GaugeLorentz object, and as such has a non-trivial Lorentz index. We can
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// access the element in the mu Lorentz index with this PeekIndex syntax.
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U[mu] = PeekIndex<LorentzIndex>(Umu, mu);
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}
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ComplexField Plaq(Umu.Grid());
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sitePlaquette(Plaq, U);
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// I guess this should be the line that sums over all space-time sites.
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auto Tp = sum(Plaq);
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// Until now, we have been working with objects inside the tensor nest. This TensorRemove gets
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// rid of the tensor nest to return whatever is inside.
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auto p = TensorRemove(Tp);
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return p.real();
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}
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// < Re tr U_mu_nu(x) >
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static RealD avgPlaquette(const GaugeLorentz &Umu) {
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// Real double type
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RealD sumplaq = sumPlaquette(Umu);
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// gSites() is the number of global sites. there is also lSites() for local sites.
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double vol = Umu.Grid()->gSites();
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// The number of orientations. 4*3/2=6 for Nd=4, as known.
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double faces = (1.0 * Nd * (Nd - 1)) / 2.0;
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return sumplaq / vol / faces / Nc;
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}
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};
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// Next we show an example of how to construct an input parameter class. We first inherit
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// from Serializable. Then all class data members have to be defined using the
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// GRID_SERIALIZABLE_CLASS_MEMBERS macro. This variadic macro allows for arbitrarily many
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// class data members. In the below case, we make a parameter file holding the configuration
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// name. Here, it expects the name to be labeled with "conf_name" in the configuration file.
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struct ConfParameters: Serializable {
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GRID_SERIALIZABLE_CLASS_MEMBERS(
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ConfParameters,
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std::string, conf_name);
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template <class ReaderClass>
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ConfParameters(Reader<ReaderClass>& Reader){
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// If we are reading an XML file, it should be structured like:
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// <grid>
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// <parameters>
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// <conf_name>l20t20b06498a_nersc.302500</conf_name>
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// </parameters>
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// </grid>
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read(Reader, "parameters", *this);
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}
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};
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// This syntax lets you pass command line arguments to main. An asterisk means that what follows is
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// a pointer. Two asterisks means what follows is a pointer to an array.
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int main (int argc, char **argv)
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{
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// This initializes Grid. Some command line options include
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// --mpi n.n.n.n
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// --threads n
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// --grid n.n.n.n
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Grid_init(&argc, &argv);
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// This is where you would specify a custom lattice size, if not from the command line. Here
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// Nd is a global quantity that is currently set to 4.
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Coordinate simd_layout = GridDefaultSimd(Nd,vComplex::Nsimd());
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Coordinate mpi_layout = GridDefaultMpi();
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Coordinate latt_size = GridDefaultLatt();
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// Instantiate the spacetime Grid on which everything will be built.
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GridCartesian GRID(latt_size,simd_layout,mpi_layout);
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// The PeriodicGimplD type is what you want for gauge matrices. There is also a LatticeGaugeFieldD
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// type that you can use, which will work perfectly with what follows.
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PeriodicGimplD::Field U(&GRID);
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// Here we read in the parameter file params.json to get conf_name. The last argument is what the
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// top organizational level is called in the param file.
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XmlReader Reader("Example_plaquette.xml",false, "grid");
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ConfParameters param(Reader);
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// Load a lattice from SIMULATeQCD into U. SIMULATeQCD finds plaquette = 0.6381995717
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FieldMetaData header;
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NerscIO::readConfiguration(U, header, param.conf_name);
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// Let's see what we find.
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RealD plaq = WLoops<PeriodicGimplD>::avgPlaquette(U);
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// This is how you make log messages.
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std::cout << GridLogMessage << std::setprecision(std::numeric_limits<Real>::digits10 + 1) << "Plaquette = " << plaq << std::endl;
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// To wrap things up.
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Grid_finalize();
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} |