Data for Observation of a Dynamic Magneto-chiral Instability in Photoexcited Tellurium
A newer version of this dataset is available.
View the latest version.
Dataset Description |
*NOTE*: This dataset has been updated to V3 to include theoretical mode in addition to the experimental data and analysis. Please visit the V3 version: https://doi.org/10.13012/B2IDB-1409842_V3
Each folder contains the raw data (.mat), the oscillator parameters obtained through linear prediction algorithm (.mat), and the plot-generating code (.m). The code plots the raw data, the fit to the processed data, and the amplified modes.
|
Subject |
Physical Sciences |
Keywords |
magneto-chiral instability; THz emission; THz spectroscopy; nonequilibrium states; emergent phenomena; Weyl semiconductor; tellurium; ultrafast spectrscopy; photoexcitation |
License |
CC BY |
Funder |
U.S. Department of Energy (DOE)-Grant:Award No.DE-SC0021238 |
Corresponding Creator |
Yijing Huang |
Downloaded |
151 times |
| Version | DOI | Comment | Publication Date |
|---|---|---|---|
| 3 | 10.13012/B2IDB-1409842_V3 | Included theoretical mode in addition to the experimental data and analysis. Updated the "License". Added new files. Updated and renamed "publication_data.zip" (in V2) to "data_and_analysis.zip" | 2025-09-25 |
| 2 | 10.13012/B2IDB-1409842_V2 | Changed the figure legend, which was previously a typo in v1. | 2025-05-06 |
| 1 | 10.13012/B2IDB-1409842_V1 | 2025-02-03 |
Contact the Research Data Service for help interpreting this log.
| Dataset | update: {"all_globus"=>[nil, true]} | 2026-01-16T15:39:02Z |
| Dataset | update: {"all_medusa"=>[nil, true]} | 2026-01-16T15:36:54Z |
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| RelatedMaterial | update: {"link"=>["https://doi.org/10.13012/B2IDB-1409842_V2", "https://doi.org/10.13012/B2IDB-1409842_V3"], "citation"=>[" (2025): Data for Observation of a Dynamic Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign. https://doi.org/10.13012/B2IDB-1409842_V2", "Huang, Yijing; Abboud, Nick (2025): Data for Observation of a Dynamic Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign. https://doi.org/10.13012/B2IDB-1409842_V3"]} | 2026-01-15T06:13:13Z |
| Creator | update: {"family_name"=>["Mahmood", "Abboud"], "given_name"=>["Fahad", "Nick"], "email"=>["fahad@illinois.edu", "nka2@illinois.edu"]} | 2026-01-15T06:13:13Z |
| Dataset | update: {"description"=>["<b>*NOTE*: This dataset has been updated to V3 to include theoretical mode in addition to the experimental data and analysis. Please visit the V3 version: https://doi.org/10.13012/B2IDB-1409842_V3</b>\r\nThe data and code provided in this dataset can be used to generate plots that show the results of linear prediction algorithm and the amplified modes, supporting the key argument of the manuscript. \r\nIt is divided into five subfolders, each corresponding to one combination of external condition (magnetic field B, temperature), scan parameter (temperature, magnetic field B), pump laser polarization (linear s, linear p, and circular), and sample orientation ( B parallel to c axis, B perpendicular to c axis):\r\n1) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_parallel_c_linear_spump_sprobe_field).\r\n2) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_parallel_c_linear_spump_sprobe_temperature).\r\n3) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_perp_c_linear_spump_sprobe_field).\r\n4) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_perp_c_linear_spump_sprobe_temperature).\r\n5) B parallel to c axis, circular pump polarization (left circularly polarized LCP and right circularly polarized RCP), linear THz emission polarization in s, field dependence (B_parallel_c_LCPRCP_pump_sprobe_field).\r\n\r\nEach folder contains the raw data (.mat), the oscillator parameters obtained through linear prediction algorithm (.mat), and the plot-generating code (.m). The code plots the raw data, the fit to the processed data, and the amplified modes.\r\nCodes are written in MATLAB R2024a; the working directory of each code should be the corresponding subfolder that contains it. ", "<b>*NOTE*: This dataset has been updated to V3 to include theoretical mode in addition to the experimental data and analysis. Please visit the V3 version: <a href=\"https://doi.org/10.13012/B2IDB-1409842_V3\">https://doi.org/10.13012/B2IDB-1409842_V3</a></b>\r\nThe data and code provided in this dataset can be used to generate plots that show the results of linear prediction algorithm and the amplified modes, supporting the key argument of the manuscript. \r\nIt is divided into five subfolders, each corresponding to one combination of external condition (magnetic field B, temperature), scan parameter (temperature, magnetic field B), pump laser polarization (linear s, linear p, and circular), and sample orientation ( B parallel to c axis, B perpendicular to c axis):\r\n1) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_parallel_c_linear_spump_sprobe_field).\r\n2) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_parallel_c_linear_spump_sprobe_temperature).\r\n3) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_perp_c_linear_spump_sprobe_field).\r\n4) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_perp_c_linear_spump_sprobe_temperature).\r\n5) B parallel to c axis, circular pump polarization (left circularly polarized LCP and right circularly polarized RCP), linear THz emission polarization in s, field dependence (B_parallel_c_LCPRCP_pump_sprobe_field).\r\n\r\nEach folder contains the raw data (.mat), the oscillator parameters obtained through linear prediction algorithm (.mat), and the plot-generating code (.m). The code plots the raw data, the fit to the processed data, and the amplified modes.\r\nCodes are written in MATLAB R2024a; the working directory of each code should be the corresponding subfolder that contains it. "]} | 2026-01-14T17:26:03Z |
| RelatedMaterial | update: {"note"=>[nil, ""]} | 2026-01-14T17:25:04Z |
| Dataset | update: {"description"=>["The data and code provided in this dataset can be used to generate plots that show the results of linear prediction algorithm and the amplified modes, supporting the key argument of the manuscript. \r\nIt is divided into five subfolders, each corresponding to one combination of external condition (magnetic field B, temperature), scan parameter (temperature, magnetic field B), pump laser polarization (linear s, linear p, and circular), and sample orientation ( B parallel to c axis, B perpendicular to c axis):\r\n1) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_parallel_c_linear_spump_sprobe_field).\r\n2) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_parallel_c_linear_spump_sprobe_temperature).\r\n3) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_perp_c_linear_spump_sprobe_field).\r\n4) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_perp_c_linear_spump_sprobe_temperature).\r\n5) B parallel to c axis, circular pump polarization (left circularly polarized LCP and right circularly polarized RCP), linear THz emission polarization in s, field dependence (B_parallel_c_LCPRCP_pump_sprobe_field).\r\n\r\nEach folder contains the raw data (.mat), the oscillator parameters obtained through linear prediction algorithm (.mat), and the plot-generating code (.m). The code plots the raw data, the fit to the processed data, and the amplified modes.\r\nCodes are written in MATLAB R2024a; the working directory of each code should be the corresponding subfolder that contains it. ", "<b>*NOTE*: This dataset has been updated to V3 to include theoretical mode in addition to the experimental data and analysis. Please visit the V3 version: https://doi.org/10.13012/B2IDB-1409842_V3</b>\r\nThe data and code provided in this dataset can be used to generate plots that show the results of linear prediction algorithm and the amplified modes, supporting the key argument of the manuscript. \r\nIt is divided into five subfolders, each corresponding to one combination of external condition (magnetic field B, temperature), scan parameter (temperature, magnetic field B), pump laser polarization (linear s, linear p, and circular), and sample orientation ( B parallel to c axis, B perpendicular to c axis):\r\n1) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_parallel_c_linear_spump_sprobe_field).\r\n2) B parallel to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_parallel_c_linear_spump_sprobe_temperature).\r\n3) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, field dependence (B_perp_c_linear_spump_sprobe_field).\r\n4) B perpendicular to c axis, linear pump polarization in s, linear THz emission polarization in s, temperature dependence (B_perp_c_linear_spump_sprobe_temperature).\r\n5) B parallel to c axis, circular pump polarization (left circularly polarized LCP and right circularly polarized RCP), linear THz emission polarization in s, field dependence (B_parallel_c_LCPRCP_pump_sprobe_field).\r\n\r\nEach folder contains the raw data (.mat), the oscillator parameters obtained through linear prediction algorithm (.mat), and the plot-generating code (.m). The code plots the raw data, the fit to the processed data, and the amplified modes.\r\nCodes are written in MATLAB R2024a; the working directory of each code should be the corresponding subfolder that contains it. "], "external_files_link"=>[nil, ""], "external_files_note"=>[nil, ""]} | 2026-01-14T17:25:04Z |
| RelatedMaterial | create: {"material_type"=>"Dataset", "availability"=>nil, "link"=>"https://doi.org/10.13012/B2IDB-1409842_V2", "uri"=>"10.13012/B2IDB-1409842_V2", "uri_type"=>"DOI", "citation"=>" (2025): Data for Observation of a Dynamic Magneto-chiral Instability in Photoexcited Tellurium. University of Illinois Urbana-Champaign. https://doi.org/10.13012/B2IDB-1409842_V2", "dataset_id"=>2859, "selected_type"=>"Dataset", "datacite_list"=>"IsPreviousVersionOf", "note"=>nil, "feature"=>nil} | 2025-04-23T03:56:29Z |
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| Creator | update: {"family_name"=>["Fahad ", "Mahmood"], "given_name"=>["Mahmood", "Fahad"]} | 2025-02-13T05:02:37Z |
| Dataset | update: {"title"=>["Data for Observation of a Magneto-chiral Instability in Photoexcited Tellurium", "Data for Observation of a Dynamic Magneto-chiral Instability in Photoexcited Tellurium"]} | 2025-02-05T18:33:14Z |
| Dataset | update: {"publication_state"=>["file embargo", "released"]} | 2025-02-03T14:00:07Z |
| Dataset | update: {"publication_state"=>["released", "file embargo"]} | 2025-02-01T03:14:36Z |
| Dataset | update: {"publication_state"=>["file embargo", "released"]} | 2025-02-01T03:14:35Z |
| Funder | update: {"grant"=>["", "Award No.DE-SC0021238"]} | 2025-02-01T03:14:35Z |
| Dataset | update: {"publication_state"=>["released", "file embargo"]} | 2025-02-01T03:11:32Z |
| Dataset | update: {"publication_state"=>["file embargo", "released"]} | 2025-02-01T03:11:31Z |
| Funder | destroy: {"name"=>"U.S. Department of Energy (DOE)", "identifier"=>"", "identifier_scheme"=>"", "grant"=>"", "dataset_id"=>2859, "code"=>"DOE"} | 2025-02-01T03:11:31Z |
| Dataset | update: {"publication_state"=>["released", "file embargo"]} | 2025-01-31T16:48:26Z |
| Dataset | update: {"publication_state"=>["file embargo", "released"]} | 2025-01-31T16:48:26Z |
| Dataset | update: {"title"=>["Data for \"Observation of a Magneto-chiral Instability in Photoexcited Tellurium\"", "Data for Observation of a Magneto-chiral Instability in Photoexcited Tellurium"]} | 2025-01-31T16:48:25Z |