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PRLTAO 0031-9007 10.1103/PhysRevLett.82.1012
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J. S. Gardner, S. R. Dunsiger, B. D. Gaulin, M. J. P. Gingras, J. E. Greedan, R. F. Kiefl, M. D. Lumsden, W. A. MacFarlane, N. P. Raju, J. E. Sonier, I. Swainson, and Z. Tun, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett. 82.1012 82, 1012 (1999).
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0345802558
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PRBMDO 0163-1829 10.1103/PhysRevB.68.180401
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J. S. Gardner, A. Keren, G. Ehlers, C. Stock, E. Segal, J. M. Roper, B. Fak, M. B. Stone, P. R. Hammar, D. H. Reich, and B. D. Gaulin, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.68.180401 68, 180401 (R) (2003).
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Reich, D.H.10
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3
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84988755547
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PRBMDO 0163-1829 10.1103/PhysRevB.64.224416
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J. S. Gardner, B. D. Gaulin, A. J. Berlinsky, P. Waldron, S. R. Dunsiger, N. P. Raju, and J. E. Greedan, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.64.224416 64, 224416 (2001).
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4
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34347353184
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PRBMDO 0163-1829 10.1103/PhysRevB.75.212404
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S. H. Curnoe, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.75.212404 75, 212404 (2007)
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Y. Yamashita and K. Ueda, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.85.4960 85, 4960 (2000)
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PRLTAO 0031-9007 10.1103/PhysRevLett.99.237202
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J. P. C. Ruff, B. D. Gaulin, J. P. Castellan, K. C. Rule, J. P. Clancy, J. Rodriguez, and H. A. Dabkowska, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.99.237202 99, 237202 (2007).
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11
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4243800935
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Similar models were discussed in PRLTAO 0031-9007 10.1103/PhysRevLett.81. 2356
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Similar models were discussed in F. Mila, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.81.2356 81, 2356 (1998)
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PRBMDO 0163-1829 10.1103/PhysRevB.65.024415
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H. Tsunetsugu, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.65.024415 65, 024415 (2001).
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K. C. Rule, J. P. C. Ruff, B. D. Gaulin, S. R. Dunsiger, J. S. Gardner, J. P. Clancy, M. J. Lewis, H. A. Dabkowska, I. Mirebeau, P. Manuel, Y. Qiu, and J. R. D. Copley, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.96.177201 96, 177201 (2006).
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JUPSAU 0031-9015 10.1143/JPSJ.71.599
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17
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52949118395
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The (2, 0, 0) peak is likely present for several other rare-earth titinates, including the spin ice Ho2 Ti2 O7, which implies that it is not due to coupling with the spin.
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The (2, 0, 0) peak is likely present for several other rare-earth titinates, including the spin ice Ho2 Ti2 O7, which implies that it is not due to coupling with the spin. B. Gaulin (private communication).
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Gaulin, B.1
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18
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0005984228
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0038-5646
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I. V. Aleksandrov, B. V. Lidskiǐ, L. G. Mamsurova, M. G. Neǐgauz, K. S. Pigal'skiǐ, K. K. Pukhov, N. G. Trusevich, and L. G. Shcherbakova, Sov. Phys. JETP 62, 1287 (1985). 0038-5646
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19
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0034261175
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PRBMDO 0163-1829 10.1103/PhysRevB.62.6496
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M. J. P. Gingras, B. C. den Hertog, M. Faucher, J. S. Gardner, S. R. Dunsiger, L. J. Chang, B. D. Gaulin, N. P. Raju, and J. E. Greedan, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.62.6496 62, 6496 (2000).
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Greedan, J.E.9
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20
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52949127878
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The singlet state | A1 〉 is also a ground state of JX when j=0, but has a higher energy when j=0.
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The singlet state | A1 〉 is also a ground state of JX when j=0, but has a higher energy when j=0.
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-
-
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21
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52949087088
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Including the singlet state (see Ref.).
-
Including the singlet state (see Ref.).
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23
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46149085876
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PRBMDO 0163-1829 10.1103/PhysRevB.77.214310
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T. T. A. Lummen, I. P. Handayani, M. C. Donker, D. Fausti, G. Dhalenne, P. Berthet, A. Revcolevschi, and P. H. M. van Loosdrecht, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.77.214310 77, 214310 (2008).
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Revcolevschi, A.7
Van Loosdrecht, P.H.M.8
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