% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@ARTICLE{JundullahHanafi:619990,
      author       = {Jundullah Hanafi, Muchammad Izzuddin and Bastonero, Lorenzo
                      and Murshed, Mohammad Mangir and Robben, Lars and Dononelli,
                      Wilke and Kirsch, Andrea and Marzari, Nicola and Gesing,
                      Thorsten M.},
      title        = {{S}ynthesis, structural and spectroscopic characterization
                      of defect-rich forsterite as a representative phase of
                      {M}artian regolith},
      journal      = {IUCrJ},
      volume       = {11},
      number       = {6},
      issn         = {2052-2525},
      address      = {Chester},
      publisher    = {[Verlag nicht ermittelbar]},
      reportid     = {PUBDB-2024-08073},
      pages        = {977-990},
      year         = {2024},
      abstract     = {Regolith draws intensive research attention because of its
                      importance as the basis for fabricating materials for future
                      human space exploration. Martian regolith is predicted to
                      consist of defect-rich crystal structures due to long-term
                      space weathering. The present report focuses on the
                      structural differences between defect-rich and defect-poor
                      forsterite (Mg2SiO4) – one of the major phases in Martian
                      regolith. In this work, forsterites were synthesized using
                      reverse strike co-precipitation and high-energy ball milling
                      (BM). Subsequent post-processing was also carried out using
                      BM to enhance the defects. The crystal structures of the
                      samples were characterized by X-ray powder diffraction and
                      total scattering using Cu and synchrotron radiation followed
                      by Rietveld refinement and pair distribution function (PDF)
                      analysis, respectively. The structural models were deduced
                      by density functional theory assisted PDF refinements,
                      describing both long-range and short-range order caused by
                      defects. The Raman spectral features of the synthetic
                      forsterites complement the ab initio simulation for an
                      in-depth understanding of the associated structural
                      defects.Keywords: Martian forsterite; crystal structures;
                      defects; DFT–PDF; Raman spectroscopy; X-ray powder
                      diffraction; ball milling.},
      cin          = {DOOR ; HAS-User},
      ddc          = {530},
      cid          = {I:(DE-H253)HAS-User-20120731},
      pnm          = {6G3 - PETRA III (DESY) (POF4-6G3) / DFG project
                      G:(GEPRIS)429360100 - Studien an in-situ Daten der totalen
                      Streufunktion: Bildungsmechanismen von ternären
                      multiferroischen Bismutferraten (429360100) / DFG project
                      G:(GEPRIS)390741603 - EXC 2077: Der Ozeanboden –
                      unerforschte Schnittstelle der Erde (390741603)},
      pid          = {G:(DE-HGF)POF4-6G3 / G:(GEPRIS)429360100 /
                      G:(GEPRIS)390741603},
      experiment   = {EXP:(DE-H253)P-P02.1-20150101},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {pmid:39465970},
      UT           = {WOS:001362462200008},
      doi          = {10.1107/S2052252524009722},
      url          = {https://bib-pubdb1.desy.de/record/619990},
}