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Phys. Rev. B 76, 104403 (2007) [7 pages]

Electronic structures and low-dimensional magnetic properties of the ordered rocksalt oxides Na3Cu2SbO6 and Na2Cu2TeO6

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Shahab Derakhshan1,2,*, Heather L. Cuthbert1,2, and John E. Greedan1,2
1Chemistry Department, McMaster University, 1280 Main Street West, Hamilton, Ontario, Canada L8S 4M1
2Brockhouse Institute for Materials Research at McMaster University, 1280 Main Street West, Hamilton, Ontario, Canada L8S 4M1

Badiur Rahaman3 and Tanusri Saha-Dasgupta3
3S.N. Bose National Centre for Basic Sciences, JD Block, Sector III, Salt Lake City, Kolkata 700098, India

Received 8 March 2007; published 5 September 2007

The ordered rocksalt-type oxide Na3Cu2SbO6 was synthesized and its magnetic properties were investigated. The broad peak in the temperature-dependent magnetic susceptibility data near 92 K is indicative of the dominant low-dimensional short-range antiferromagnetic (AF) behavior. The data are very well fitted with the AF-AF alternating linear chain model with J1k=−79 K and J2J1=0.39. The high-temperature data (T>300 K) exhibit Curie-Weiss behavior with a Weiss temperature of −55(2) K. These results are very similar to those reported for the isostructural oxide Na2Cu2TeO6 [ J. Xu et al. Inorg. Chem. 44 5042 (2005)]. Recently, it was shown [ Y. Miura et al. J. Phys. Soc. Jpn. 75 847071 (2006)] that an AF-ferromagnetic (F) linear chain model gives an equally good fit to the low-temperature data for both compounds and that further analysis of magnetic heat capacity data supports the AF-F model. We reinvestigate this proposal by computing the intersite hopping integrals using both the tight-binding spin dimer analysis and the Nth-order muffin-tin-orbital downfolding procedure for both compounds. The calculations support the AF-AF model for the antimonide. Further, the Weiss temperatures derived from the high-temperature experimental data, T>300 K, are also consistent with the J values derived from the AF-AF model but not with those obtained from the AF-F alternative.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.76.104403
DOI:
10.1103/PhysRevB.76.104403
PACS:
75.40.−s

*Author to whom correspondence should be addressed. derakh@mcmaster.ca