nonlinear time-domain simulation model Search Results


90
COMSOL Inc finite-difference-time-domain (fdtd) method
Finite Difference Time Domain (Fdtd) Method, supplied by COMSOL Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
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finite-difference-time-domain (fdtd) method - by Bioz Stars, 2026-09
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Rsoft Inc finite-difference time-domain (fdtd) simulations
Finite Difference Time Domain (Fdtd) Simulations, supplied by Rsoft Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/fdtd+fullwave/10__1021_slash_nl500149h-39-11-24
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finite-difference time-domain (fdtd) simulations - by Bioz Stars, 2026-09
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Rsoft Inc finite difference time domain fdtd simulations
Finite Difference Time Domain Fdtd Simulations, supplied by Rsoft Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/finite+difference+time+domain+method/10__1063_slash_1__3567944-33-63-69
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finite difference time domain fdtd simulations - by Bioz Stars, 2026-09
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Rsoft Inc three-dimensional finite difference time domain simulation fdtd rsoft 9.0 fullwave
Three Dimensional Finite Difference Time Domain Simulation Fdtd Rsoft 9.0 Fullwave, supplied by Rsoft Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
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three-dimensional finite difference time domain simulation fdtd rsoft 9.0 fullwave - by Bioz Stars, 2026-09
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90
ANSYS inc 3d fdtd method
3d Fdtd Method, supplied by ANSYS inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/3d+fdtd+simulations/pmc12073108-64-9-14
Average 90 stars, based on 1 article reviews
3d fdtd method - by Bioz Stars, 2026-09
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ANSYS inc finite-difference time-domain (fdtd) simulation software
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Finite Difference Time Domain (Fdtd) Simulation Software, supplied by ANSYS inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/finite+difference+time+domain++fdtd++simulations/pmc09663599-152-20-32
Average 90 stars, based on 1 article reviews
finite-difference time-domain (fdtd) simulation software - by Bioz Stars, 2026-09
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90
ANSYS inc finite-difference time-domain simulations
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Finite Difference Time Domain Simulations, supplied by ANSYS inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/finite+difference+time+domain+method/pmc11127965__41467_2024_48621_MOESM1_ESM-4-11-19
Average 90 stars, based on 1 article reviews
finite-difference time-domain simulations - by Bioz Stars, 2026-09
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90
Verlag GmbH difference time domain (fdtd) simulations
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Difference Time Domain (Fdtd) Simulations, supplied by Verlag GmbH, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/finite+difference+time+domain++fdtd++simulations/10__1002_slash_adom__202000786-85-8-3
Average 90 stars, based on 1 article reviews
difference time domain (fdtd) simulations - by Bioz Stars, 2026-09
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96
MathWorks Inc real time domain simulation
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Real Time Domain Simulation, supplied by MathWorks Inc, used in various techniques. Bioz Stars score: 96/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/Simulink+Real-Time/10__3390_slash_en11123475-436-5-9
Average 96 stars, based on 1 article reviews
real time domain simulation - by Bioz Stars, 2026-09
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90
COMSOL Inc time-domain fem simulations comsol multiphysics
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Time Domain Fem Simulations Comsol Multiphysics, supplied by COMSOL Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/simulation+program+comsol+multiphysics/pm28915056-55-19-22
Average 90 stars, based on 1 article reviews
time-domain fem simulations comsol multiphysics - by Bioz Stars, 2026-09
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Remcom Inc finite difference time domain method xfdtd 6.3
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Finite Difference Time Domain Method Xfdtd 6.3, supplied by Remcom Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/xfdtd+software/pmc03245373-39-14-20
Average 90 stars, based on 1 article reviews
finite difference time domain method xfdtd 6.3 - by Bioz Stars, 2026-09
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Weidlinger Associates Inc time-domain finite-element method (fem) package pzflex
a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and <t>FDTD</t> simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .
Time Domain Finite Element Method (Fem) Package Pzflex, supplied by Weidlinger Associates Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/nonlinear+time-domain+simulation+model/pzflex+software/pmc05027576-148-7-13
Average 90 stars, based on 1 article reviews
time-domain finite-element method (fem) package pzflex - by Bioz Stars, 2026-09
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Image Search Results


a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and FDTD simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .

Journal: Nature Communications

Article Title: Coherent momentum control of forbidden excitons

doi: 10.1038/s41467-022-34740-5

Figure Lengend Snippet: a PL emission momentum distribution mapping with \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y axis. Four shining emission spots, located at the Γ-X line and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{x}}}}}}}$$\end{document} k x or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}$$\end{document} k y = 0.74 with C 4 symmetry, are clearly visible. b Polarization analysis of the PL emission momentum distribution in a . The four shining emission spots show radial polarization indicating they are from dark excitons. c Angle-resolved PL emission spectra mapping extracted from y-polarized PL emission momentum distribution mapping in b . It is clear to see the dark exciton directional emissions have small divergence angles at wavelengths of around 772 nm and towards oblique emission angles of around 48°. d The measured (red solid line) and FDTD simulated (dark green dashed line) PL intensity as a function of the in-plane momentum ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{{{{\bf{k}}}}}}}_{{{{{{\bf{y}}}}}}}/{{{{{\bf{k}}}}}}$$\end{document} k y / k ) along the y-direction. The full-width-half-maximum (FWHM) of the measured X D emission lobes is 7° indicating the ultra-low divergence angle of the directional emission. e Spectra extracted from oblique angles of 48° and 23° for the dark exciton emission and the bright exciton emission, respectively. f The simulated PL emission momentum distribution by the Lumerical FDTD. Four shining emission spots show high correspondence to the measured PL emission pattern in a .

Article Snippet: To further understand the coupling mechanism between the out-of-plane dipole and the Friedrich-Wintgen BIC supported by the PhC slab, a Finite-difference time-domain (FDTD) simulation was performed using commercial software (Lumerical FDTD Solutions, ANSYS Inc.) to show how the PhC slab selectively couples with the out-of-plane dipole and enhances their emission.

Techniques: