Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores

Przemyslaw Dera, Barbara Lavina, Lauren A. Borkowski, Vitali B. Prakapenka, Stephen R. Sutton, Mark L. Rivers, Robert T Downs, Nabil Z. Boctor, Charles T. Prewitt

Research output: Contribution to journalArticle

13 Citations (Scopus)

Abstract

High-pressure and high-temperature behavior of synthetic Ni2P has been studied in a laser-heated diamond anvil cell up to 50 GPa and 2200 K. Incongruent melting associated with formation of pyrite-type NiP2 and amorphous Ni-P alloy was found at an intermediate pressure range, between 6.5 and 40 GPa. Above 40 GPa, Ni2P melts congruently. At room conditions, Ni2P has hexagonal C22-type structure, and without heating it remains in this structure to at least 50 GPa. With a bulk modulus .K0 = 201(8) GPa and K' = 4.2(6 Ni2P is noticeably less compressible than hep Fe, as well as all previously described iron phosphides, and its presence in the Earth core would favorably lower the core density. In contrast to Fe2P, the c/a ratio in Ni2P decreases on compression because of the lack of ferromagnetic interaction along the c direction. Lack of the C22→C23 transition in Ni2P rules out a stabilizing effect of Ni on the orthorhombic phase of natural (Fe1-xNix)P allabogdanite.

Original languageEnglish (US)
Article numberB03201
JournalJournal of Geophysical Research: Space Physics
Volume114
Issue number3
StatePublished - Mar 4 2009

Fingerprint

planetary cores
core (planetary)
Earth core
diamond anvil cell
phosphides
bulk modulus
pyrites
anvils
rooms
pyrite
melting
laser
Earth (planet)
diamonds
compression
melt
heating
iron
Diamond
cells

ASJC Scopus subject areas

  • Geochemistry and Petrology
  • Geophysics
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Dera, P., Lavina, B., Borkowski, L. A., Prakapenka, V. B., Sutton, S. R., Rivers, M. L., ... Prewitt, C. T. (2009). Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores. Journal of Geophysical Research: Space Physics, 114(3), [B03201].

Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores. / Dera, Przemyslaw; Lavina, Barbara; Borkowski, Lauren A.; Prakapenka, Vitali B.; Sutton, Stephen R.; Rivers, Mark L.; Downs, Robert T; Boctor, Nabil Z.; Prewitt, Charles T.

In: Journal of Geophysical Research: Space Physics, Vol. 114, No. 3, B03201, 04.03.2009.

Research output: Contribution to journalArticle

Dera, Przemyslaw ; Lavina, Barbara ; Borkowski, Lauren A. ; Prakapenka, Vitali B. ; Sutton, Stephen R. ; Rivers, Mark L. ; Downs, Robert T ; Boctor, Nabil Z. ; Prewitt, Charles T. / Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores. In: Journal of Geophysical Research: Space Physics. 2009 ; Vol. 114, No. 3.
@article{ef03cc4bdf6649869555c20c122e107e,
title = "Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores",
abstract = "High-pressure and high-temperature behavior of synthetic Ni2P has been studied in a laser-heated diamond anvil cell up to 50 GPa and 2200 K. Incongruent melting associated with formation of pyrite-type NiP2 and amorphous Ni-P alloy was found at an intermediate pressure range, between 6.5 and 40 GPa. Above 40 GPa, Ni2P melts congruently. At room conditions, Ni2P has hexagonal C22-type structure, and without heating it remains in this structure to at least 50 GPa. With a bulk modulus .K0 = 201(8) GPa and K' = 4.2(6 Ni2P is noticeably less compressible than hep Fe, as well as all previously described iron phosphides, and its presence in the Earth core would favorably lower the core density. In contrast to Fe2P, the c/a ratio in Ni2P decreases on compression because of the lack of ferromagnetic interaction along the c direction. Lack of the C22→C23 transition in Ni2P rules out a stabilizing effect of Ni on the orthorhombic phase of natural (Fe1-xNix)P allabogdanite.",
author = "Przemyslaw Dera and Barbara Lavina and Borkowski, {Lauren A.} and Prakapenka, {Vitali B.} and Sutton, {Stephen R.} and Rivers, {Mark L.} and Downs, {Robert T} and Boctor, {Nabil Z.} and Prewitt, {Charles T.}",
year = "2009",
month = "3",
day = "4",
language = "English (US)",
volume = "114",
journal = "Journal of Geophysical Research: Space Physics",
issn = "2169-9380",
publisher = "Wiley-Blackwell",
number = "3",

}

TY - JOUR

T1 - Structure and behavior of the barringerite Ni end-member, Ni2P, at deep Earth conditions and implications for natural Fe-Ni phosphides in planetary cores

AU - Dera, Przemyslaw

AU - Lavina, Barbara

AU - Borkowski, Lauren A.

AU - Prakapenka, Vitali B.

AU - Sutton, Stephen R.

AU - Rivers, Mark L.

AU - Downs, Robert T

AU - Boctor, Nabil Z.

AU - Prewitt, Charles T.

PY - 2009/3/4

Y1 - 2009/3/4

N2 - High-pressure and high-temperature behavior of synthetic Ni2P has been studied in a laser-heated diamond anvil cell up to 50 GPa and 2200 K. Incongruent melting associated with formation of pyrite-type NiP2 and amorphous Ni-P alloy was found at an intermediate pressure range, between 6.5 and 40 GPa. Above 40 GPa, Ni2P melts congruently. At room conditions, Ni2P has hexagonal C22-type structure, and without heating it remains in this structure to at least 50 GPa. With a bulk modulus .K0 = 201(8) GPa and K' = 4.2(6 Ni2P is noticeably less compressible than hep Fe, as well as all previously described iron phosphides, and its presence in the Earth core would favorably lower the core density. In contrast to Fe2P, the c/a ratio in Ni2P decreases on compression because of the lack of ferromagnetic interaction along the c direction. Lack of the C22→C23 transition in Ni2P rules out a stabilizing effect of Ni on the orthorhombic phase of natural (Fe1-xNix)P allabogdanite.

AB - High-pressure and high-temperature behavior of synthetic Ni2P has been studied in a laser-heated diamond anvil cell up to 50 GPa and 2200 K. Incongruent melting associated with formation of pyrite-type NiP2 and amorphous Ni-P alloy was found at an intermediate pressure range, between 6.5 and 40 GPa. Above 40 GPa, Ni2P melts congruently. At room conditions, Ni2P has hexagonal C22-type structure, and without heating it remains in this structure to at least 50 GPa. With a bulk modulus .K0 = 201(8) GPa and K' = 4.2(6 Ni2P is noticeably less compressible than hep Fe, as well as all previously described iron phosphides, and its presence in the Earth core would favorably lower the core density. In contrast to Fe2P, the c/a ratio in Ni2P decreases on compression because of the lack of ferromagnetic interaction along the c direction. Lack of the C22→C23 transition in Ni2P rules out a stabilizing effect of Ni on the orthorhombic phase of natural (Fe1-xNix)P allabogdanite.

UR - http://www.scopus.com/inward/record.url?scp=67649861656&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=67649861656&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:67649861656

VL - 114

JO - Journal of Geophysical Research: Space Physics

JF - Journal of Geophysical Research: Space Physics

SN - 2169-9380

IS - 3

M1 - B03201

ER -