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        <parTitl xml:lang="en">CHASAM 2026: Datasets for Chalmers School on Atomic Modeling</parTitl>
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    <citation>
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        <titl xml:lang="sv"></titl>
        <parTitl xml:lang="en">CHASAM 2026: Datasets for Chalmers School on Atomic Modeling</parTitl>
        <IDNo agency="SND">doi-10-5281-zenodo-22252488-0</IDNo>
        <IDNo agency="DOI">https://doi.org/10.5281/zenodo.22252488</IDNo>
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        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Fransson, Erik</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Berger, Esmée</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Lindgren, Eric</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Uddén, Felix</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Svensson, Lucas</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Hainer, Tobias</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Berger, Ethan</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Ngoipala, Apinya</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Wiktor, Julia</AuthEnty>
        <AuthEnty xml:lang="en" affiliation="Department of Physics and Astronomy, Chalmers University of Technology">Erhart, Paul</AuthEnty>
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    <stdyInfo>
      <subject />
      <abstract xml:lang="en" contentType="abstract">MD trajectories used in the hands-on notebooks of the CHASAM 2026 school, https://chasam.materialsmodeling.org/. All runs were done with GPUMD using a NEP potential. Each archive unpacks into a directory of the same name, holding the input structure (model.xyz), the NEP model (nep.txt), the GPUMD input (run.in) and the trajectory (dump.xyz).

Files

Archive
System
Ensemble
Temperature
Supercell
Frames

CsPbI3_NPT_T650to1_size12_nframes2000.tar.gz
CsPbI3
NPT
650 K to 1 K
12x12x12, 8640 atoms
2000

CsPbI3_NVE_T600_size4_nframes100000.tar.gz
CsPbI3
NVE
600 K
4x4x4, 320 atoms
100000

CsPbI3_NVT_T650_size18_nframes500.tar.gz
CsPbI3
NVT
650 K
18x18x18, 29160 atoms
500

FAPI_md-run-active-learning.tar.gz
FAPbI3
NPT
1 K to 600 K
2x2x2, 96 atoms
2000</abstract>
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        <restrctn xml:lang="en">Access to data through an external actor. Data are freely accessible.</restrctn>
        <restrctn xml:lang="sv">Åtkomst till data via extern aktör. Data är fritt tillgängliga.</restrctn>
        <conditions elementVersion="info:eu-repo-Access-Terms vocabulary">openAccess</conditions>
      </useStmt>
    </dataAccs>
    <othrStdyMat />
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