This library provides routines for constructing and working with the intermediate representation of correlation functions. It provides:
- on-the-fly computation of basis functions for arbitrary cutoff Λ
- basis functions and singular values are accurate to full precision
- routines for sparse sampling
Install via pip:
pip install sparse-ir
Install via conda:
conda install -c spm-lab sparse-ir
sparse-ir requires numpy, scipy, and pylibsparseir (a thin Python wrapper for the libsparseir C API).
To manually install the current development version, you can use the following:
# Only recommended for developers - no automatic updates! git clone https://github.com/SpM-lab/sparse-ir cd sparse-ir uv sync
Note: uv is a fast Python package manager. If you don't have it installed,
you can install it with pip install uv
or use pip install -e .
instead.
To build the documentation locally, first install the development dependencies:
uv sync --group doc
Then build the documentation:
uv run sphinx-build -M html doc _build/html
The documentation will be available in _build/html/html/index.html
.
Check out our comprehensive tutorial, where we self-contained notebooks for several many-body methods - GF(2), GW, Eliashberg equations, Lichtenstein formula, FLEX, ... - are presented.
Refer to the API documentation for more details on how to work with the python library.
There is also a Julia library and (currently somewhat restricted) C library with Fortran bindings available for the IR basis and sparse sampling.
Here is a full second-order perturbation theory solver (GF(2)) in a few lines of Python code:
# Construct the IR basis and sparse sampling for fermionic propagators import sparse_ir, numpy as np basis = sparse_ir.FiniteTempBasis('F', beta=10, wmax=8, eps=1e-6) stau = sparse_ir.TauSampling(basis) siw = sparse_ir.MatsubaraSampling(basis, positive_only=True) # Solve the single impurity Anderson model coupled to a bath with a # semicircular states with unit half bandwidth. U = 1.2 def rho0w(w): return np.sqrt(1-w.clip(-1,1)**2) * 2/np.pi # Compute the IR basis coefficients for the non-interacting propagator rho0l = basis.v.overlap(rho0w) G0l = -basis.s * rho0l # Self-consistency loop: alternate between second-order expression for the # self-energy and the Dyson equation until convergence. Gl = G0l Gl_prev = 0 while np.linalg.norm(Gl - Gl_prev) > 1e-6: Gl_prev = Gl Gtau = stau.evaluate(Gl) Sigmatau = U**2 * Gtau**3 Sigmal = stau.fit(Sigmatau) Sigmaiw = siw.evaluate(Sigmal) G0iw = siw.evaluate(G0l) Giw = 1/(1/G0iw - Sigmaiw) Gl = siw.fit(Giw)
You may want to start with reading up on the intermediate representation.
It is tied to the analytic continuation of bosonic/fermionic spectral
functions from (real) frequencies to imaginary time, a transformation mediated
by a kernel K
. The kernel depends on a cutoff, which you should choose to
be lambda_ >= beta * W
, where beta
is the inverse temperature and W
is the bandwidth.
One can now perform a singular value expansion on this kernel, which
generates two sets of orthonormal basis functions, one set v[l](w)
for
real frequency side w
, and one set u[l](tau)
for the same obejct in
imaginary (Euclidean) time tau
, together with a "coupling" strength
s[l]
between the two sides.
By this construction, the imaginary time basis can be shown to be optimal in terms of compactness.
This software is released under the MIT License. See LICENSE.txt for details.
If you find the intermediate representation, sparse sampling, or this software useful in your research, please consider citing the following papers:
- Hiroshi Shinaoka et al., Phys. Rev. B 96, 035147 (2017)
- Jia Li et al., Phys. Rev. B 101, 035144 (2020)
- Markus Wallerberger et al., SoftwareX 21, 101266 (2023)
If you are discussing sparse sampling in your research specifically, please also consider citing an independently discovered, closely related approach, the MINIMAX isometry method (Merzuk Kaltak and Georg Kresse, Phys. Rev. B 101, 205145, 2020).