198 lines
7.1 KiB
ReStructuredText
198 lines
7.1 KiB
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Photo-Electron Diffraction (PED)
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Introduction
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============
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In PhotoElectron Diffraction, an incoming photon, with an energy in the X-ray range is absorbed by
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an atom of the sample. A core electron of the absorbing atom is emitted and will eventually escape
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from the sample after many scattering events toward a detector. This photo-electron is detected at
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a given kinetic energy and for a given position (polar angle and azimutal angle) of the detector with
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respect to the sample (see figure below). The distribution of electrons as a function of the sample
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polar or azimutal angles contains chemically resolved informations about the crystallography in the
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immediate proximity of the surface sample. This spectroscopy can also be done on Auger electrons. In
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this case, the technique is named Auger Electron Diffraction.
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.. _ped_full_picture:
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.. figure:: ../../full_picture.png
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:align: center
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:width: 80%
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The Full picture of a photoelectron diffraction process. a) The geometry of
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the experiment. b) A view of the multiple scattering process and c) Atomic
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energy level sketch of the normal and Auger photoemission process.
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Quick reference
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===============
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To quickly start with MsSpec and Python, the easiest way is to read the :ref:`tutorials` section.
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Here we summurize all the steps to perform a PED simulation:
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1. :ref:`Build your cluster <step1>` (thanks to the ASE python package)
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2. :ref:`Create a calculator <step2>` with :py:func:`MSSPEC`
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3. :ref:`Set the parameters <step3>` of your calculation.
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4. :ref:`Attach <step4>` your cluster to the calculator
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5. :ref:`Choose the absorber <step5>`
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6. :ref:`Compute <step6>` a scan
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7. :ref:`Plot <step7>` the results
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.. _step1:
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Build your cluster
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------------------
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Building a cluster means creating a list of atoms with their given positions in x, y, z coordinates.
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It is easily done thanks to the `ase Python package <https://wiki.fysik.dtu.dk/ase/index.html>`_.
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Because most of spectroscopies have a source and a detector in the same hemispherical space, a cluster
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is often shaped as an half sphere. To create such atomic arrangements, special helper functions are provided
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in the :py:mod:`utils` module.
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For example to create an MgO cluster:
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.. literalinclude:: MgO.py
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:linenos:
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:lines: 1-15
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.. only:: html
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will produce a cluster of 519 atoms like this:
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.. figure:: MgO.gif
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:align: center
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:width: 60%
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The shape of a typical (yet quite large) cluster used for a calculation (519 atoms of MgO).
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.. only:: latex
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will produce a cluster of 519 atoms like this:
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.. figure:: MgO.png
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:align: center
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:width: 60%
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The shape of a typical (yet quite large) cluster used for a calculation (519 atoms of MgO).
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.. _step2:
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Create a calculator
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-------------------
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To create a claculator, you will use the :py:func:`calculator.MSSPEC` function. This function takes 4
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keyword arguments:
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- **spectroscopy**, to specify the kind of spectroscopy. This is a string and
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can be one of 'PED' for PhotoElectron Diffraction, 'AED' for Auger Electron
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Diffraction, 'APECS' for Auger PhotoElectron Coincidence Spectroscopy or
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'EXAFS' for Extended X-Ray Absorption Fine Structure.
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- **algorithm**, to choose between the matrix inversion method with the string
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'inversion' (best suited for lower kinetic energies < 100 eV), or the series
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expansion technique with 'expansion' or the correlation-expansion with
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'correlation'.
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- **polarization** to specify the light polarization. 'linear_qOz' or 'linear_xOy'
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for a linearly polarized light with the polarization vector in the :math:`(\vec{q}Oz)`
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or in the :math:`(xOy)` plane respectively. Finally choose 'circular' for circularly
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polarized light.
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- **folder**. Enter here the name of the folder used for temporary files.
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The function returns a calculator object, so for example. To create a calculator for PhotoElectron
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Diffraction with the matrix inversion method:
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.. code-block:: python
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calc = MSSPEC(spectroscopy = 'PED', algorithm = 'inversion')
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.. _step3:
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Set the parameters
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------------------
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A calculator has many parameters. They fall into 4 categories:
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* Muffin-tin parameters, to tweak the potential used for the phase shifts calculation
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* T-Matrix parameters, to control the T-matrix calculation
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* Calculation parameters, to tune the multiple scattering calculation: add atomic vibrations,
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add some filters to speed up the process, control the parameters of the series expansion method...
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* Spectroscopy dependent parameters. These parameters control -- for example -- the light source,
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the detector...
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Each set of parameters is accessible through properties of the calculator object. For example, to tweak
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the interstitial value of the Muffin Tin potential, use:
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>>> calc.muffintin_parameters.interstitial_potential = 12.1
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To change the source energy, use:
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>>> calc.source_parameters.energy = 1253.0
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All options are detailed in :ref:`this section <allparameters>`
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.. _step4:
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Attach your cluster
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-------------------
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Very easy! Juste use the :py:func:`set_atoms` function like this:
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.. code-block:: python
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calc.set_atoms(cluster)
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.. _step5:
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Choose the absorber
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-------------------
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Set the absorber attribute of your cluster to the index of the atom you want it to be the absorber.
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For example if the first atom of your cluster is the absorber
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.. code-block:: python
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cluster.absorber = 0
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The best way is to use a function to find the index based on the xyz coordinates of the atom. For
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example to choose the closest atom of the origin:
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.. code-block:: python
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cluster.absorber = get_atom_index(cluster, 0, 0, 0)
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:py:func:`get_atom_index` is in the :py:mod:`utils` package so do not forget to import it. The
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first argument is the cluster you will look for and the 3 next parameters are the x, y and z
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coordinates.
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.. _step6:
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Compute
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-------
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You can compute 5 kinds of scans in PED spectroscopy:
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* A polar scan, with the :py:func:`get_theta_scan` method of the calculator object
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* An azimutal scan, with the :py:func:`MSSPEC.get_phi_scan` method
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* A stereographic scan, with the :py:func:`MSSPEC.get_theta_phi_scan` method
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* An energy scan, with the :py:func:`MSSPEC.get_energy_scan` method
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* The scattering factor, with the :py:func:`MSSPEC.get_scattering_factors` method
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All these functions are used and detailed in the :ref:`tutorials <tutorials>`.
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.. _step7:
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Plot the results
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----------------
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Normally, the output of the previous functions is a :py:class:`iodata.Data` object. You can see
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the results by typing:
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>>> data = calc.get_theta_scan(...) # a polar scan for example
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>>> data.view() # will popup a graphical window
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