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[doc] Remove todos in doc

This commit is contained in:
Manuel 2018-12-04 09:36:52 -05:00
parent b14e802859
commit d8488efd98
7 changed files with 4 additions and 86 deletions
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2
doc/conf.py.in
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@ -19,7 +19,7 @@ extensions = ['sphinx.ext.autodoc',
source_suffix = '.rst'
project = u'TRIQS DFTTools'
copyright = u'2011-2013, M. Aichhorn, L. Pourovskii, V. Vildosola, C. Martins'
copyright = u'2011-2019'
version = '@DFT_TOOLS_VERSION@'
mathjax_path = "@TRIQS_MATHJAX_PATH@/MathJax.js?config=default"

36
doc/tutorials.rst
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@ -14,42 +14,6 @@ A simple example: SrVO3
tutorials/srvo3
FeSe
----
.. toctree::
:maxdepth: 2
tutorials/fese
Magnetism: SrMnO3
-----------------
.. toctree::
:maxdepth: 2
tutorials/srmno3
Offdiagonals: LaTiO3
--------------------
.. toctree::
:maxdepth: 2
tutorials/latio3
Spin-orbit coupling: Sr2RuO4
----------------------------
.. toctree::
:maxdepth: 2
tutorials/sr2ruo4_soc
Full charge self consistency with Wien2k: :math:`\gamma`-Ce
-----------------------------------------------------------

8
doc/tutorials/fese.rst
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@ -1,8 +0,0 @@
.. _FeSe:
FeSe
====
Discuss 5-orbital setup.

7
doc/tutorials/latio3.rst
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@ -1,7 +0,0 @@
.. _LaTiO3:
LaTiO3
======
Discuss Off-diagonals, rotation of basis.

7
doc/tutorials/sr2ruo4_soc.rst
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@ -1,7 +0,0 @@
.. _Sr2RuO4:
Sr2RuO4
=======
Discuss addign SOC by hand to t2gs.

7
doc/tutorials/srmno3.rst
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@ -1,7 +0,0 @@
.. _SrMnO3:
SrMnO3
======
Discuss Magnetism, setup with flipping spins and so on.

23
doc/tutorials/srvo3.rst
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@ -1,6 +1,6 @@
.. _SrVO3:
We will discuss now how to set up a full working calculation,
On the example of SrVO3 we will discuss now how to set up a full working calculation,
including the initialization of the :ref:`CTHYB solver <triqscthyb:welcome>`.
Some additional parameter are introduced to make the calculation
more efficient. This is a more advanced example, which is
@ -14,9 +14,8 @@ rotational-invariant Slater interaction Hamiltonian (:download:`dft_dmft_cthyb_s
<images_scripts/dft_dmft_cthyb_slater.py>`). The user has to adapt these
scripts to his own needs. How to execute your script is described :ref:`here<runpy>`.
TODO: At the end of this section we also provide hdf5 archives for this example, including data as function of DMFT iterations.
The conversion will now be discussed in detail for the Wien2k and VASP packages. For more details we refer to the :ref:`documentation <conversion>`.
The conversion will now be discussed in detail for the Wien2k and VASP packages.
For more details we refer to the :ref:`documentation <conversion>`.
Wien2k
@ -66,16 +65,6 @@ text files to the hdf5 archive by::
This reads all the data, and stores everything that is necessary for the DMFT calculation in the file :file:`SrVO3.h5`.
VASP
====
DFT setup
---------
Wannier orbitals
----------------
The DMFT calculation
====================
@ -286,9 +275,3 @@ of the self energy and to stop (:emphasis:`fit_max_n`) before the noise fully ta
If it is difficult to find a reasonable fit in this region you should increase
your statistics (number of measurements). Keep in mind that :emphasis:`fit_min_n`
and :emphasis:`fit_max_n` also depend on :math:`\beta`.
Data for benchmark / comparison
-------------------------------
TODO: We should provide two h5 files, one fore Wien2k and one for VASP, with selfs for, say, 15 DMFT iterations. Then people can check what they are doing.