Difference between revisions of "Fieldscan enlev.m"
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{{DISPLAYTITLE:fieldscan_enlev.m}} | {{DISPLAYTITLE:fieldscan_enlev.m}} | ||
| − | + | Plots a user-specified number of the lowest energy levels of the system as a function of the applied magnetic field. The energies are obtained using the Arnoldi method. | |
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==Syntax== | ==Syntax== | ||
fieldscan_enlev(spin_system,parameters) | fieldscan_enlev(spin_system,parameters) | ||
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==Arguments== | ==Arguments== | ||
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| − | ''Version 2. | + | ''Version 2.2, authors: [[Ilya Kuprov]], [[Elizaveta Suturina]]'' |
Revision as of 14:19, 22 August 2018
Plots a user-specified number of the lowest energy levels of the system as a function of the applied magnetic field. The energies are obtained using the Arnoldi method.
Contents
Syntax
fieldscan_enlev(spin_system,parameters)
Arguments
parameters.fields - two-element vector in Tesla,
ordered as [from to]
parameters.npoints - number of points in the scan
parameters.orientation - system orientation, three-
element vector containing
Euler angles in radians,
ordered as [alp bet gam]
parameters.nstates - number of lowest energy states
to solve for
Outputs
This function plots a graph.
Examples
See quartet_levels.m, triple_dy_levels.m, and dy_lft_single_2.m files in examples/giant_spin directory.
Notes
The function runs in parallel over the values of the applied magnetic field. The sys.magnet parameter is used for internal normalisation and must be set to exactly 1 Tesla.
See also
eqmag.m, stevens.m, stev2sph.m, fieldscan_magn.m, fieldsweep.m
Version 2.2, authors: Ilya Kuprov, Elizaveta Suturina
