Electron spin resonance in S= 1 2 antiferromagnets at high temperature

Physical Review B - Condensed Matter and Materials Physics

Volumn 81, Issue 22, 2010, Pages

  El Shawish, S ^a   Cepas O ^b   Miyashita, S ^c  

^a JO EF STEFAN INSTITUTE   (Slovenia)

^b CNRS   (France)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 77956310122     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.81.224421     Document Type: Article

References (37)

1. P. W. Anderson and P. R. Weiss, Rev. Mod. Phys. 25, 269 (1953). 10.1103/RevModPhys.25.269
2. R. Kubo and K. Tomita, J. Phys. Soc. Jpn. 9, 888 (1954). 10.1143/JPSJ.9.888
3. H. Mori, Prog. Theor. Phys. 33, 423 (1965). 10.1143/PTP.33.423
4. R. Zwanzig, Phys. Rev. 124, 983 (1961). 10.1103/PhysRev.124.983
5. R. E. Dietz, F. R. Merritt, R. Dingle, Daniel Hone, B. G. Silbernagel, and Peter M. Richards, Phys. Rev. Lett. 26, 1186 (1971). 10.1103/PhysRevLett.26. 1186
6. H. Benner and J.-P. Boucher, in Magnetic Properties of Layered Transition Metal Compounds, edited by, L. J. de Jongh, (Kluwer, Dordrecht, 1990), p. 323.
7. M. Oshikawa and I. Affleck, Phys. Rev. Lett. 82, 5136 (1999). 10.1103/PhysRevLett.82.5136
8. J. Choukroun, J.-L. Richard, and A. Stepanov, Phys. Rev. Lett. 87, 127207 (2001). 10.1103/PhysRevLett.87.127207
9. M. Oshikawa and I. Affleck, Phys. Rev. B 65, 134410 (2002). 10.1103/PhysRevB.65.134410
10. I. Yamada, M. Nishi, and J. Akimitsu, J. Phys.: Condens. Matter 8, 2625 (1996). 10.1088/0953-8984/8/15/012
11. R. M. Eremina, M. V. Eremin, V. N. Glazkov, H.-A. Krug von Nidda, and A. Loidl, Phys. Rev. B 68, 014417 (2003). 10.1103/PhysRevB.68.014417
12. T. Kaplan, Z. Phys. B: Condens. Matter 49, 313 (1983) 10.1007/BF01301591
13. L. Shekhtman, O. Entin-Wohlman, and A. Aharony, Phys. Rev. Lett. 69, 836 (1992). 10.1103/PhysRevLett.69.836
14. M. V. Eremin, D. V. Zakharov, R. M. Eremina, J. Deisenhofer, H.-A. Krug von Nidda, G. Obermeier, S. Horn, and A. Loidl, Phys. Rev. Lett. 96, 027209 (2006). 10.1103/PhysRevLett.96.027209
15. M. V. Eremin, D. V. Zakharov, H.-A. Krug von Nidda, R. M. Eremina, A. Shuvaev, A. Pimenov, P. Ghigna, J. Deisenhofer, and A. Loidl, Phys. Rev. Lett. 101, 147601 (2008). 10.1103/PhysRevLett.101.147601
16. J. E. Gulley, Daniel Hone, D. J. Scalapino, and B. G. Silbernagel, Phys. Rev. B 1, 1020 (1970). 10.1103/PhysRevB.1.1020
17. G. F. Reiter and J.-P. Boucher, Phys. Rev. B 11, 1823 (1975). 10.1103/PhysRevB.11.1823
18. A. Zorko, D. Arčon, H. van Tol, L. C. Brunel, and H. Kageyama, Phys. Rev. B 69, 174420 (2004). 10.1103/PhysRevB.69.174420
19. O. Cépas, K. Kakurai, L. P. Regnault, T. Ziman, J. P. Boucher, N. Aso, M. Nishi, H. Kageyama, and Y. Ueda, Phys. Rev. Lett. 87, 167205 (2001). 10.1103/PhysRevLett.87.167205
20. Y. F. Cheng, O. Cépas, P. W. Leung, and T. Ziman, Phys. Rev. B 75, 144422 (2007). 10.1103/PhysRevB.75.144422
21. S. Miyashita, T. Yoshino, and A. Ogasahara, J. Phys. Soc. Jpn. 68, 655 (1999) 10.1143/JPSJ.68.655
22. A. Ogasahara and S. Miyashita, J. Phys. Soc. Jpn. 72, 44 (2003).
23. For a finite-size system, one could argue that there is no need for broadening as it is the exact result once the Hamiltonian is given. In fact there are many additional sources of natural broadening. Even if these were absent, experimentalists usually modulates the external field by a (very) small-frequency component, thus artificially broadening each peak.
24. T. Sakai, O. Cépas, and T. Ziman, J. Phys. Soc. Jpn. 69, 3521 (2000). 10.1143/JPSJ.69.3521
25. U. Brandt and K. Jacoby, Z. Phys. B 25, 181 (1976). 10.1007/BF01320179
26. J. H. H. Perk and H. W. Capel, Physica A 100, 1 (1980) 10.1016/0378-4371(80)90147-8
27. J. H. H. Perk and H. W. Capel, Physica A 92, 163 (1978). 10.1016/0378-4371(78)90026-2
28. A. Abragam and M. Goldmann, Nuclear Magnetism: Order and Disorder (Clarendon Press, Oxford, 1982), p. 30.
29. K. Fabricius and B. M. McCoy, Phys. Rev. B 57, 8340 (1998). 10.1103/PhysRevB.57.8340
30. At lower temperatures, this is not excluded though. Indeed it is possible that if a spin-nematic state develops at some critical temperature, the four-spin correlation function does slow down, whereas the spin-spin correlation function does not. If this is so, we would predict a strong change in the resonance line shape.
31. M. J. Hennessy, C. D. McElwee, and P. M. Richards, Phys. Rev. B 7, 930 (1973). 10.1103/PhysRevB.7.930
32. J.-P. Boucher, M. Ahmed Bakheit, M. Nechtschein, M. Villa, G. Bonera, and F. Borsa, Phys. Rev. B 13, 4098 (1976). 10.1103/PhysRevB.13.4098
33. T. T. P. Cheung and Z. G. Soos, J. Chem. Phys. 69, 3845 (1978). 10.1063/1.437050
34. O. Cépas, C. M. Fong, P. W. Leung, and C. Lhuillier, Phys. Rev. B 78, 140405 (R) (2008). 10.1103/PhysRevB.78.140405
35. A. Zorko, S. Nellutla, J. van Tol, L. C. Brunel, F. Bert, F. Duc, J. C. Trombe, M. A. de Vries, A. Harrison, and P. Mendels, Phys. Rev. Lett. 101, 026405 (2008). 10.1103/PhysRevLett.101.026405
36. For a review, see P. Mendels and F. Bert, J. Phys. Soc. Jpn. 79, 011001 (2010). 10.1143/JPSJ.79.011001
37. I. Rousochatzakis, S. R. Manmana, A. M. Läuchli, B. Normand, and F. Mila, Phys. Rev. B 79, 214415 (2009). 10.1103/PhysRevB.79.214415