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https://github.com/triqs/dft_tools
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f7fad85fca
This is an iteration over the doc mainly thank to Priyanka. I fixed another couple of details on the way.
222 lines
7.4 KiB
ReStructuredText
222 lines
7.4 KiB
ReStructuredText
.. index::
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single: Green's functions; block Green's function
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module: gf_imfreq
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module: gf_refreq
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module: gf_imtime
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module: gf_retime
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module: gf_legendre
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.. _blockgreen:
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The blocks: matrix-valued Green's functions
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===============================================
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In this section, we present the matrix-valued Green's functions,
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i.e. the blocks of the full local Green's function.
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They are available in various flavours:
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.. toctree::
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:maxdepth: 1
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block/GfImTime
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block/GfImFreq
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block/GfReTime
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block/GfReFreq
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block/GfLegendre
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They have many common properties, which we now present.
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Operations
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--------------------------------------------
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Block Green's functions support various simple operations.
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.. note::
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All these operations compute the array of data, but also, if present in the object, the high frequency expansion tail automatically.
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* compound operators, `+=`, `-=`, `*=`, `\=`: the RHS can be a Green's function of the same type or an expression
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* arithmetic operations : `+`, `-`, `*`, `/`, e.g.::
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g = g1 + 2*g2
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* inversion, e.g.::
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inv = inverse(g)
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g2 = inverse(inverse(g) - sigma) # this is Dyson's equation
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Slicing
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--------
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Just like numpy arrays, the Green's function can be sliced, *when the indices are integers* (otherwise it is meaningless).
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The syntax is the regular python/numpy syntax, so a simple example will be enough here::
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>>> from pytriqs.gf.local import *
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>>> g = GfImFreq(indices = [1,2,3], beta = 50, n_points = 1000, name = "imp")
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>>> g[1:3:,1:3]
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GfImFreq imp : Beta = 50.000; IndicesL = [1, 2], IndicesR = [1, 2]
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>>> g[1,1]
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GfImFreq imp : Beta = 50.000; IndicesL = [1], IndicesR = [1]
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>>> g[2:3,2:3]
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GfImFreq imp : Beta = 50.000; IndicesL = [2], IndicesR = [2]
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Assignment: <<= or = operator
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--------------------------------------------
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Because python always uses references, one cannot simply use the = operator
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to assign some expression into a Green's function.
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Therefore, we introduced the <<= operator ::
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g <<= RHS
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This sets the data and tail of g with the RHS.
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* If RHS is Green's function, it must be of the same type and size must match
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* If RHS is a formal expression, it must be of the same size
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To simplify the notation, in the case where one accesses the Green's function with a [ ] operation,
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the = sign is possible and equivalent to the `<<=` operator.
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.. warning::
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Don't use the = operator without the brackets: it has its normal python meaning, i.e.
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reaffecting the reference.
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Let us illustrate this issue on a simple example::
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from pytriqs.gf.local import *
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# Create the Matsubara-frequency Green's function
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g = GfImFreq(indices = [1], beta = 50, n_points = 1000, name = "imp")
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g <<= inverse( Omega + 0.5 ) # correct
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g[1,1] = inverse( Omega + 0.5 ) # correct (it uses __setitem__).
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However, the following line is almost certainly NOT what you have in mind::
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g = inverse( Omega + 0.5 )
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* The reference g is reassigned to the object `inverse( Omega + 0.5 )`, which is not a block Green's function but a lazy expression.
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* The block created earlier is destroyed immediately.
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Lazy expressions
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----------------
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To initialize the Green's function, one can use lazy_expression, made of Green's functions, `descriptors`
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assembled with basic operations.
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:ref:`descriptors<descriptors>` are abstract objects that do not contain data, but describe a simple function and
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can be evaluated, can compute the high-frequency expansion, and so on. For example:
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* `Omega`: is the function :math:`f(\omega) = \omega`.
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* `SemiCircular(D)`: is a Green's function corresponding to free fermions with a semi circular density of states of half-bandwith `D`.
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* `Wilson`: is a Green's function corresponding to fermions with a flat density of states of half-bandwidth `D`.
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.. toctree::
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:maxdepth: 1
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descriptors
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shelve / pickle
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---------------
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Green's functions are `picklable`, i.e. they support the standard python serialization techniques.
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* It can be used with the `shelve <http://docs.python.org/library/shelve.html>`_ and `pickle <http://docs.python.org/library/pickle.html>`_ module::
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import shelve
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s = shelve.open('myfile','w')
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s['G'] = G # G is stored in the file.
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* It can be sent/broadcasted/reduced over mpi ::
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from pytriqs.utility import MPI
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mpi.send (G, destination)
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.. warning::
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Shelve is not a portable format, it may change from python version to another (and it actually does).
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For portability, we recommend using the HDF5 interface for storing data on disks.
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Plot options
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------------
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There is one important option that you will find very useful when plotting Green's functions, which we
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saw already in the previous section:
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* `RI` = 'R' or 'I' or 'S'
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It tells the plotter, what part of the Green's function you want to plot. 'R' for the real part, 'I'
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for the imaginary part, and 'S' for the spectral function, :math:`-1/\pi{\rm Im}G`. Of course,
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depending on the type of Green's function under consideration, one or more of these options do not make a lot of sense, e.g.
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calculating the spectral function of an imaginary-time Green's function is not useful.
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Direct access to data points and tails [not for the Legendre version]
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-----------------------------------------------------------------------------
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Data points can be accessed via the properties ``data`` and ``tail`` respectively.
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``data`` returns an array object and so does ``tail[i]``::
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g.data
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.. warning::
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Be careful when manipulating data directly to keep consistency between
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the function and the tail.
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Basic operations do this automatically, so use them as much as possible.
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.. _greentails:
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Direct access to the tails
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--------------------------
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All block Green's function come together with a **Tail** object that describes its
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large-frequency behavior. In other words, for large :math:`|z|`, the Green's function
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behaves like
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.. math::
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g(z) \sim ... + M_{-1} z + M_0 + \frac{M_1}{z} + \frac{M_2}{z^2} + ...
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where :math:`M_i` are matrices with the same dimensions as :math:`g`.
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* Tails can be accessed with the ``tail`` property. Moreover, in order
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to have access to :math:`M_i`, one uses the bracket. For example::
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>>> g = GfImFreq(indices = ['eg1','eg2'], beta = 50, n_points = 1000, name = "egBlock")
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>>> g <<= 2.0
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>>> print g.tail[0]
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TO BE UPDATED
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Here ``g.tail[0]`` is a diagonal matrix with 2 on the diagonal, corresponding to :math:`M_0`.
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* Some operations (sum over frequencies, Fourier) uses these tails to regulate the sum,
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so it is necessary to always keep the consistency between the array of data and the tail expansion.
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* Fortunately, in all basic operations on the blocks, these tails are computed automatically.
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For example, when adding two Green functions, the tails are added, and so on.
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* However, if you modify the ``data`` or the ``tail`` manually, you lose this guarantee.
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So you have to set the tail properly yourself (or be sure that you will not need it later).
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For example::
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g = GfImFreq(indices = ['eg1','eg2'], beta = 50, n_points = 1000, name = "egBlock")
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g <<= Function(lambda x: 3/x)
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g.tail.zero()
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g.tail[1] = numpy.array( [[3.0,0.0], [0.0,3.0]] )
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The third line sets all the :math:`M_i` to zero, while the second puts :math:`M_1 = diag(3)`. With
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the tail set correctly, this Green's function can be used safely.
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.. warning::
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The library will not be able detect tails that are incorrectly set.
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Calculations *may* be wrong in this case.
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