5c370c0b2a
GitOrigin-RevId: 33d1e753c82ffc557b4a585c77de43d4c922ebb5
85 lines
2.2 KiB
Nix
85 lines
2.2 KiB
Nix
{ lib
|
|
, stdenv
|
|
, fetchurl
|
|
, boost
|
|
, gfortran
|
|
, lhapdf
|
|
, ncurses
|
|
, perl
|
|
, python ? null
|
|
, swig
|
|
, yoda
|
|
, zlib
|
|
, withPython ? false
|
|
}:
|
|
|
|
stdenv.mkDerivation rec {
|
|
pname = "fastnlo-toolkit";
|
|
version = "2.5.0-2826";
|
|
|
|
src = fetchurl {
|
|
url = "https://fastnlo.hepforge.org/code/v25/fastnlo_toolkit-${version}.tar.gz";
|
|
sha256 = "sha256-7aIMYCOkHC/17CHYiEfrxvtSJxTDivrS7BQ32cGiEy0=";
|
|
};
|
|
|
|
buildInputs = [
|
|
boost
|
|
gfortran
|
|
gfortran.cc.lib
|
|
lhapdf
|
|
yoda
|
|
] ++ lib.optional withPython python
|
|
++ lib.optional (withPython && python.isPy3k) ncurses;
|
|
|
|
propagatedBuildInputs = [
|
|
zlib
|
|
] ++ lib.optional withPython swig;
|
|
|
|
preConfigure = ''
|
|
substituteInPlace ./fastnlotoolkit/Makefile.in \
|
|
--replace "-fext-numeric-literals" ""
|
|
|
|
# disable test that fails due to strict floating-point number comparison
|
|
echo "#!/usr/bin/env perl" > check/fnlo-tk-stattest.pl.in
|
|
chmod +x check/fnlo-tk-stattest.pl.in
|
|
'';
|
|
|
|
configureFlags = [
|
|
"--with-yoda=${yoda}"
|
|
] ++ lib.optional withPython "--enable-pyext";
|
|
|
|
enableParallelBuilding = true;
|
|
|
|
doCheck = true;
|
|
nativeCheckInputs = [
|
|
perl
|
|
lhapdf.pdf_sets.CT10nlo
|
|
];
|
|
preCheck = ''
|
|
patchShebangs --build check
|
|
'';
|
|
enableParallelChecking = false;
|
|
|
|
# None of our currently packaged versions of swig are C++17-friendly
|
|
# Use a workaround from https://github.com/swig/swig/issues/1538
|
|
env.CXXFLAGS="-D_LIBCPP_ENABLE_CXX17_REMOVED_FEATURES";
|
|
|
|
meta = with lib; {
|
|
homepage = "http://fastnlo.hepforge.org";
|
|
description = "Fast pQCD calculations for hadron-induced processes";
|
|
longDescription = ''
|
|
The fastNLO project provides computer code to create and evaluate fast
|
|
interpolation tables of pre-computed coefficients in perturbation theory
|
|
for observables in hadron-induced processes.
|
|
|
|
This allows fast theory predictions of these observables for arbitrary
|
|
parton distribution functions (of regular shape), renormalization or
|
|
factorization scale choices, and/or values of alpha_s(Mz) as e.g. needed
|
|
in PDF fits or in systematic studies. Very time consuming complete
|
|
recalculations are thus avoided.
|
|
'';
|
|
license = licenses.gpl3Plus;
|
|
maintainers = with maintainers; [ veprbl ];
|
|
platforms = platforms.unix;
|
|
};
|
|
}
|