Start writing about finite systems.
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Using QPMS library for simulating finite systems
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Using QPMS library for simulating finite systems
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================================================
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The main C API for finite systems is defined in [scatsystem.h][], and the
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most relevant parts are wrapped into python modules. The central data structure
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defining the system of scatterers is [qpms_scatsys_t][],
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which holds information about particle positions and their T-matrices
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(provided by user) and about the symmetries of the system. Specifically, it
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keeps track about the symmetry group and how the particles transform
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under the symmetry operations.
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```
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#!/usr/bin/env python
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from qpms import Particle, CTMatrix, BaseSpec, FinitePointGroup, ScatteringSystem, TMatrixInterpolator, eV, hbar, c
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from qpms.symmetries import point_group_info
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import numpy as np
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import os
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import sys
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nm = 1e-9
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sym = FinitePointGroup(point_group_info['D2h'])
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bspec = BaseSpec(lMax = 2)
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tmfile = '/m/phys/project/qd/Marek/tmatrix-experiments/Cylinder/AaroBEC/cylinder_50nm_lMax4_cleaned.TMatrix'
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#outputdatadir = '/home/necadam1/wrkdir/AaroBECfinite_new'
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outputdatadir = '/u/46/necadam1/unix/project/AaroBECfinite_new'
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os.makedirs(outputdatadir, exist_ok = True)
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interp = TMatrixInterpolator(tmfile, bspec, symmetrise = sym, atol = 1e-8)
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# There is only one t-matrix in the system for each frequency. We initialize the matrix with the lowest frequency data.
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# Later, we can replace it using the tmatrix[...] = interp(freq) and s.update_tmatrices NOT YET; TODO
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omega = float(sys.argv[3]) * eV/hbar
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sv_threshold = float(sys.argv[4])
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# Now place the particles and set background index.
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px = 571*nm; py = 621*nm
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n = 1.51
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Nx = int(sys.argv[1])
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Ny = int(sys.argv[2])
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orig_x = (np.arange(Nx/2) + (0 if (Nx % 2) else .5)) * px
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orig_y = (np.arange(Ny/2) + (0 if (Ny % 2) else .5)) * py
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orig_xy = np.stack(np.meshgrid(orig_x, orig_y), axis = -1)
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tmatrix = interp(omega)
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particles = [Particle(orig_xy[i], tmatrix) for i in np.ndindex(orig_xy.shape[:-1])]
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ss = ScatteringSystem(particles, sym)
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k = n * omega / c
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for iri in range(ss.nirreps):
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mm_iri = ss.modeproblem_matrix_packed(k, iri)
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U, S, Vh = np.linalg.svd(mm_iri)
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print(iri, ss.irrep_names[iri], S[-1])
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starti = max(0,len(S) - np.searchsorted(S[::-1], sv_threshold, side='left')-1)
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np.savez(os.path.join(outputdatadir, 'Nx%d_Ny%d_%geV_ir%d.npz'%(Nx, Ny, omega/eV*hbar, iri)),
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S=S[starti:], omega=omega, Vh = Vh[starti:], iri=iri, Nx = Nx, Ny= Ny )
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# Don't forget to conjugate Vh before transforming it to the full vector!
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```
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[scatsystem.h]: @ref scatsystem.h
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[qpms_scatsys_t]: @ref qpms_scatsys_t
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