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Dynamic compression of Ce and Pr with millisecond time-resolved X-ray diffraction.

Earl F O'Bannon Iii1, Rachel J Husband2, Bruce J Baer3

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Summary

Cerium and praseodymium exhibit distinct volume collapse transitions under pressure due to their differing electronic structures. Dynamic compression reveals kinetic differences, with cerium

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Area of Science:

  • Materials Science
  • Condensed Matter Physics
  • Solid State Chemistry

Background:

  • Cerium (Ce) and praseodymium (Pr) are rare-earth elements exhibiting unique electronic properties under pressure.
  • Both elements undergo a volume collapse transition driven by similar electronic mechanisms involving 4f electrons.
  • Despite similar mechanisms, Ce retains its crystal symmetry while Pr transforms to a lower symmetry orthorhombic structure.

Purpose of the Study:

  • To investigate the influence of strain/compression rate on the volume collapse phase transitions in Ce and Pr.
  • To explore the kinetic differences between the phase transformations in Ce and Pr under dynamic compression.
  • To elucidate the role of electronic structure and crystal symmetry in these pressure-induced transitions.

Main Methods:

  • Dynamic compression experiments utilizing a diamond anvil cell.
  • Systematic variation of strain/compression rates across four orders of magnitude.
  • Analysis of volume collapse phase transitions and their kinetic behavior.

Main Results:

  • Cerium's volume collapse transition could not be overdriven in pressure, indicating a rapid kinetic process.
  • Fast compression rates in praseodymium shifted the phase boundary to higher pressures, suggesting slower kinetics.
  • The observed kinetic differences are linked to the distinct outcomes of the volume collapse in Ce and Pr, particularly the change in crystal symmetry for Pr.

Conclusions:

  • The study highlights significant kinetic disparities in the volume collapse phase transitions of cerium and praseodymium.
  • Dynamic compression experiments reveal that praseodymium's phase transformation kinetics are considerably slower than cerium's.
  • These findings underscore the interplay between electronic structure, crystal symmetry, and the kinetics of pressure-induced phase transitions in rare-earth elements.