Difference between revisions of "Tutorial-v.1.0.0"
| Line 161: | Line 161: | ||
* You may download the above files (zipped file) from: | * You may download the above files (zipped file) from: | ||
| − | [[media: | + | [[media:C2H2_rt_response_output_v1_0_0.zip|Download zipped output files]] |
*Explanations of the output files, ''C2H2-RT.data'' and ''C2H2-ALP.data'', are given in: | *Explanations of the output files, ''C2H2-RT.data'' and ''C2H2-ALP.data'', are given in: | ||
Revision as of 08:50, 12 November 2017
Contents
- 1 Getting started
- 2 C2H2 (isolated molecules)
- 3 Crystalline silicon (periodic solids)
- 4 Light propagation in bulk silicon (Maxwell + TDDFT)
Getting started
Welcome to SALMON Tutorial!
In this tutorial, we explain the use of SALMON from the very beginning, taking a few samples that cover applications of SALMON in several directions. We assume that you are in the computational environment of UNIX/Linux OS. First you need to download and install SALMON in your computational environment. If you have not yet done it, do it following the instruction, download-v.1.0.0 and install and Run-v.1.0.0.
As described in Install and Run-v.1.0.0, you are required to prepare at least an input file and pseudopotential files to run SALMON. In the following, we present input files for several sample calculations and provide a brief explanation of the namelist variables that appear in the input files. You may modify the input files to execute for your own calculations. Pseudopotential files of elements that appear in the samples are also attached. We also present explanations of main output files.
We present 6 tutorials.
First 3 tutorials (Tutorial-1 ~ 3) are for an isolated molecule, acetylene C2H2. If you are interested in learning electron dynamics calculations in isolated systems, please look into these tutorials. In SALMON, we usually calculate the ground state solution first. This is illustrated in Tutorial-1. After finishing the ground state calculation, two tutorials of electron dynamics calculations are prepared. Tutorial-2 illustrates the calculation of linear optical responses in real time, obtaining polarizability and photoabsorption of the molecule. Tutorial-3 illustrates the calculation of electron dynamics in the molecule under a pulsed electric field.
Next 2 tutorials (Tutorial-4 ~ 5) are for a crystalline solid, silicon. If you are interested in learning electron dynamics calculations in extended periodic systems, please look into these tutorials. Since ground state calculations of small unit-cell systems are not computationally expensive and a time evolution calculation is usually much more time-consuming than the ground state calculation, we recommend to run the ground and the time evolution calculations as a single job. The following two tutorials are organized in that way. Tutorial-4 illustrates the calculation of linear response properties of crystalline silicon to obtain the dielectric function. Tutorial-5 illustrates the calculation of electron dynamics in the crystalline silicon induced by a pulsed electric field.
The final tutorial (Tutorial-6) is for an irradiation and a propagation of a pulsed light in a bulk silicon, coupling Maxwell equations for the electromagnetic fields of the pulsed light and the electron dynamics in the unit cells. This calculation is quite time-consuming and is recommended to execute using massively parallel supercomputers. Tutorial-6 illustrates the calculation of a pulsed, linearly polarized light irradiating normally on a surface of a bulk silicon.
C2H2 (isolated molecules)
Tutorial-1: Ground state of C2H2 molecule
In this tutorial, we learn the calculation of the ground state solution of acetylene (C2H2) molecule, solving the static Kohn-Sham equation. This tutorial will be useful to learn how to set up calculations in SALMON for any isolated systems such as molecules and nanoparticles. It should be noted that at present it is not possible to carry out the geometry optimization in SALMON. Therefore, atomic positions of the molecule are specified in the input file and are fixed during the calculations.
Input files
- To run the code, following files are used:
| file name | description |
| C2H2_gs.inp | input file that contain namelist variables and their values. |
| C_rps.dat | pseodupotential file for carbon atom |
| H_rps.dat | pseudopotential file for hydrogen atom |
- You may download the above 3 files (zipped file) from:
Download zipped input and pseudopotential files
- In the input file C2H2_gs.inp, namelists variables are specified. Most of them are mandatory to execute the ground state calculation. We present explanations of the namelist variables that appear in the input file in:
Explanation of C2H2_gs.inp file
- This will help you to prepare an input file for other systems that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| C2H2-info.data | information on ground state solution |
| dns.cube | a cube file for electron density |
| elf.cube | electron localization function (ELF) |
| psi1.cube, psi2.cube, ... | electron orbitals |
| dos.data | density of states |
| pdos1.data, pdos2.data, ... | projected density of states |
- You may download the above files (zipped file) from:
Download zipped output files
- Main results of the calculation such as orbital energies are included in C2H2.info. Explanations of the C2H2.info and other output files are described in:
Explanation of C2H2-info.data and other output files
Images
- We show several image that are created from the output files.
| image | files used to create the image |
| highest occupied molecular orbital (HOMO) | psi1.cube, psi2.cube, ... |
| electron density | dns.cube |
| electron localization function | elf.cube |
Tutorial-2: Polarizability and photoabsorption of C2H2 molecule
In this tutorial, we learn the linear response calculation in the acetylene (C2H2) molecule, solving the time-dependent Kohn-Sham equation. The linear response calculation provides the polarizability and the oscillator strength distribution of the molecule. This tutorial should be carried out after finishing the ground state calculation that was explained in Tutorial-1. In the calculation, an impulsive perturbation is applied to all electrons in the C2H2 molecule along the molecular axis which we take z axis. Then a time evolution calculation is carried out without any external fields. During the calculation, the electric dipole moment is monitored. After the time evolution calculation, a time-frequency Fourier transformation is carried out for the electric dipole moment to obtain the frequency-dependent polarizability. The imaginary part of the frequency-dependent polarizability is proportional to the oscillator strength distribution and the photoabsorption cross section.
Input files
- To run the code, following files are used. The ??? file is created in the ground state calculation. Pseudopotential files are already used in the ground state calculation. Therefore, C2H2_rt_response.inp that specifies namelist variables and their values for the linear response calculation is the only file that the users need to prepare.
| file name | description |
| C2H2_rt_response.inp | input file that contain namelist variables and their values. |
| C_rps.dat | pseodupotential file for Carbon |
| H_rps.dat | pseudopotential file for Hydrogen |
| ??? | binary file created in the ground state calculation |
- You may download the C2H2_rt_response.inp file (zipped file) from:
Download zipped input file
- In the input file C2H2_rt_response.inp, namelists variables are specified. Most of them are mandatory to execute the linear response calculation. We present explanations of the namelist variables that appear in the input file in:
Explanation of C2H2_rt_response.inp file
- This will help you to prepare the input file for other systems that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| C2H2-RT.data | components of the electric dipole moment as functions of time |
| C2H2-ALP.data | polarizability and oscillator strength distribution as functions of energy |
- You may download the above files (zipped file) from:
Download zipped output files
- Explanations of the output files, C2H2-RT.data and C2H2-ALP.data, are given in:
Explanation of C2H2-RT.data and C2H2-ALP.data
Tutorial-3: Electron dynamics in C2H2 molecule under a pulsed electric field
In this tutorial, we learn the calculation of the electron dynamics in the acetylene (C2H2) molecule under a pulsed electric field, solving the time-dependent Kohn-Sham equation. As outputs of the calculation, such quantities as the total energy and the electric dipole moment of the system as functions of time are calculated. This tutorial should be carried out after finishing the ground state calculation that was explained in Tutorial-1. In the calculation, a pulsed electric field that has cos^2 envelope shape is applied. The parameters that characterize the pulsed field such as magnitude, frequency, polarization direction, and carrier envelope phase are specified in the input file.
Input files
- To run the code, following files are used. The ??? file is created in the ground state calculation. Pseudopotential files are already used in the ground state calculation. Therefore, C2H2_rt_pulse.inp that specifies namelist variables and their values for the pulsed electric field calculation is the only file that the users need to prepare.
| file name | description |
| C2H2_rt_pulse.inp | input file that contain namelist variables and their values. |
| C_rps.dat | pseodupotential file for Carbon |
| H_rps.dat | pseudopotential file for Hydrogen |
| ??? | binary file created in the ground state calculation |
- You may download the C2H2_rt_pulse.inp file (zipped file) from:
Download zipped input file
- In the input file C2H2_rt_pulse.inp, namelists variables are specified. Most of them are mandatory to execute the calculation of electron dynamics induced by a pulsed electric field. We present explanations of the namelist variables that appear in the input file in:
Explanation of C2H2_rt_pulse.inp file
- This will help you to prepare the input file for other systems and other pulsed electric fields that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| C2H2-RT.data | components of the electric dipole moment as functions of time |
| C2H2-ALP.data | power spectrum that is obtained by a time-frequency Fourier transformation of the electric dipole moment |
- You may download the above files (zipped file) from:
Download zipped output files
- Explanations of the files are described in:
Explanation of C2H2-RT.data and C2H2-ALP.data
Crystalline silicon (periodic solids)
Tutorial-4: Dielectric function of crystalline silicon
In this tutorial, we learn the linear response calculation of the crystalline silicon of a diamond structure. Calculation is done in a cubic unit cell that contains eight silicon atoms. Since the ground state calculation costs much less computational time than the time evolution calculation, both calculations are successively executed. After finishing the ground state calculation, an impulsive perturbation is applied to all electrons in the unit cell along z direction. Since the dielectric function is isotropic in the diamond structure, calculated dielectric function should not depend on the direction of the perturbation. During the time evolution, electric current averaged over the unit cell volume is calculated. A time-frequency Fourier transformation of the electric current gives us a frequency-dependent conductivity. The dielectric function may be obtained from the conductivity using a standard relation.
Input files
- To run the code, following files are used:
| file name | description |
| input_lr_Si.inp | input file that contain namelist variables and their values. |
| Si_rps.dat | pseodupotential file for silicon |
- You may download the above 2 files (zipped file) from:
Download zipped input and pseudopotential files
- In the input file input_lr_Si.inp, namelists variables are specified. Most of them are mandatory to execute the calculation. We present explanations of the namelist variables that appear in the input file in:
Explanation of input_lr_Si.inp file
- This will help you to prepare the input file for other systems that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| Si_eigen.data | energy eigenvalues of orbitals |
| Si_k.data | information on k-points |
| Si_rt.data | electric field, vector potential, and current as functions of time |
| Si_e.out | ??? |
| Si_t.out | ??? |
| Si_lr.data | ??? |
- You may download the above files (zipped file) from:
Download zipped output files
- Explanations of the output files are described in:
Explanation of Si_eigen.data and Si_k.data Explanation of Si_rt.data, Si_e.out, and Si_t.out Explanation of Si_lr.data'
Tutorial-5: Electron dynamics in crystalline silicon under a pulsed electric field
In this tutorial, we learn the calculation of electron dynamics in a unit cell of crystalline silicon of a diamond structure. Calculation is done in a cubic unit cell that contains eight silicon atoms. Since the ground state calculation costs much less computational time than the time evolution calculation, both calculations are successively executed. After finishing the ground state calculation, a pulsed electric field that has cos^2 envelope shape is applied. The parameters that characterize the pulsed field such as magnitude, frequency, polarization, and carrier envelope phase are specified in the input file.
Input files
- To run the code, following files are used:
| file name | description |
| input_sc_Si.inp | input file that contain namelist variables and their values. |
| Si_rps.dat | pseodupotential file for Carbon |
- You may download the above 2 files (zipped file) from:
Download zipped input and pseudopotential files
- In the input file input_sc_Si.inp, namelists variables are specified. Most of them are mandatory to execute the calculation. We present explanations of the namelist variables that appear in the input file in:
Explanations for Si response input files
- This will help you to prepare the input file for other systems that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| Si_eigen.data | energy eigenvalues of orbitals |
| Si_k.data | information on k-points |
| Si_GS.out | information on the ground state |
| Si_rt.data | electric field, vector potential, and current as functions of time |
| Si_t.out | ??? |
| Si_j_ac.out | current, applied vector potential, and total vector potential |
- You may download the above files (zipped file) from:
Download zipped output files
- Explanations of the output files are described in:
Explanation of Si_eigen.data, Si_k.data, and Si_GS.out Explanation of Si_rt.data, Si_t.out, and Si_j_ac.out
Light propagation in bulk silicon (Maxwell + TDDFT)
Tutorial-6: Pulsed-light propagation through silicon thin film
In this tutorial, we learn the calculation of the propagation of a pulsed light through a thin film of crystalline silicon. We consider a silicon thin film of ?? nm thickness, and an irradiation of a few-cycle, linearly polarized pulsed light normally on the thin film. First, to set up initial orbitals, the ground state calculation is carried out. The pulsed light locates in the vacuum region in front of the thin film. The parameters that characterize the pulsed light such as magnitude and frequency are specified in the input file. The calculation ends when the reflected and transmitted pulses reach the vacuum region.
Input files
- To run the code, following files are used:
| file name | description |
| input_ms_Si.inp | input file that contain namelist variables and their values. |
| Si_rps.dat | pseodupotential file for silicon |
- You may download the above two files (zipped file) from:
Download zipped input and pseudopotential files
- In the input file input_ms_Si.inp, namelists variables are specified. Most of them are mandatory to execute the calculation. We present explanations of the namelist variables that appear in the input file in:
Explanations for Si response input files
- This will help you to prepare the input file for other systems that you want to calculate. A complete list of the namelist variables that can be used in input files can be found at ???.
Output files
- After the calculation, following output files are created in the directory that you run the code,
| file name | description |
| Si_Ac_??????.out | EM field and electron energy distribution at the macroscpic grid |
| Si_Ac_M_??????.out | Vector potential field and current density at individual macropoints |
- You may download the above files (zipped file) from:
Download zipped output files
