X-ray imaging of dispersive charge modes in a doped Mott insulator near the antiferromagnet/superconductor transition

Physical Review B - Condensed Matter and Materials Physics

Volumn 78, Issue 7, 2008, Pages

  Li, Y W ^a   Qian, D ^a   Wray, L ^a   Hsieh, D ^a   Xia, Y ^a   Kaga, Y ^b   Sasagawa, T ^b   Takagi, H ^b   Markiewicz, R S ^c   Bansil, A ^c   Eisaki, H ^d   Uchida, S ^b   Hasan, M Z ^a  

^a PRINCETON UNIVERSITY   (United States)

^b UNIVERSITY OF TOKYO   (Japan)

^c NORTHEASTERN UNIVERSITY   (United States)

^d NATIONAL INSTITUTE OF ADVANCED INDUSTRIAL SCIENCE AND TECHNOLOGY AIST   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 50049087923     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.78.073104     Document Type: Article

References (31)

1. M. Imada, A. Fujimori, and Y. Tokura, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.70.1039 70, 1039 (1998).
2. M. A. Kastner, R. J. Birgeneau, G. Shirane, and Y. Endoh, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.70.897 70, 897 (1998).
3. G. Blumberg, M. Kang, M. V. Klein, K. Kadowaki, and C. Kendziora, Science SCIEAS 0036-8075 10.1126/science.278.5342.1427 278, 1427 (1997).
4. M. Z. Hasan, E. D. Isaacs, Z.-X. Shen, L. L. Miller, K. Tsutsui, T. Tohyama, and S. Maekawa, Science SCIEAS 0036-8075 10.1126/science.288.5472.1811 288, 1811 (2000)
5. Y. J. Kim, J. P. Hill, C. A. Burns, S. Wakimoto, R. J. Birgeneau, D. Casa, T. Gog, and C. T. Venkataraman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.89.177003 89, 177003 (2002).
6. J. P. Hill, C.-C. Kao, W. A. L. Caliebe, M. Matsubara, A. Kotani, J. L. Peng, and R. L. Greene, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett. 80.4967 80, 4967 (1998)
7. P. Abbamonte, C. A. Burns, E. D. Isaacs, P. M. Platzman, L. L. Miller, S. W. Cheong, and M. V. Klein, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83.860 83, 860 (1999).
8. K. Tsutsui, T. Tohyama, and S. Maekawa, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83.3705 83, 3705 (1999)
9. T. P. Devereaux, G. E. D. McCormack, and J. K. Freericks, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.90.067402 90, 067402 (2003)
10. T. Nomura and J.-i. Igarashi, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.71.035110 71, 035110 (2005)
11. J. V. D. Brink and M. V. Veenendaal, Europhys. Lett. EULEEJ 0295-5075 10.1209/epl/i2005-10366-9 73, 121 (2006).
12. R. S. Markiewicz and A. Bansil, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.96.107005 96, 107005 (2006).
13. M. Z. Hasan, P. A. Montano, E. D. Isaacs, Z.-X. Shen, H. Eisaki, S. K. Sinha, Z. Islam, N. Motoyama, and S. Uchida, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.88.177403 88, 177403 (2002).
14. Y.-J. Kim, J. P. Hill, S. Komiya, Y. Ando, D. Casa, T. Gog, and C. T. Venkataraman, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.70.094524 70, 094524 (2004)
15. K. Ishii, K. Tsutsui, Y. Endoh, T. Tohyama, K. Kuzushita, T. Inami, K. Ohwada, S. Maekawa, T. Masui, S. Tajima, Y. Murakami, and J. Mizuki, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94.187002 94, 187002 (2005).
16. C. Kusko, R. S. Markiewicz, M. Lindroos, and A. Bansil, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.66.140513 66, 140513 (R) (2002).
17. H. Kusunose and T. M. Rice, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.91.186407 91, 186407 (2003).
18. D. Sénéchal and A.-M. S. Tremblay, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92.126401 92, 126401 (2004).
19. B. Kyung, V. Hankevych, A.-M. Daré, and A.-M. S. Tremblay, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.93.147004 93, 147004 (2004).
20. Q. Yuan, F. Yuan, and C. S. Ting, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.72.054504 72, 054504 (2005).
21. K. Ishii, K. Tsutsui, Y. Endoh, T. Tohyama, S. Maekawa, M. Hoesch, K. Kuzushita, M. Tsubota, T. Inami, J. Mizuki, Y. Murakami, and K. Yamada, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94.207003 94, 207003 (2005).
22. N. P. Armitage, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.88. 257001 88, 257001 (2002).
23. P. K. Mang, O. P. Vajk, A. Arvanitaki, J. W. Lynn, and M. Greven, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.93.027002 93, 027002 (2004).
24. R. S. Markiewicz, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.70. 174518 70, 174518 (2004).
25. A. Zimmers, L. Shi, D. C. Schmadel, W. M. Fisher, R. L. Greene, H. D. Drew, M. Houseknecht, G. Acbas, M.-H. Kim, M.-H. Yang, J. Cerne, J. Lin, and A. Millis, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.76.064515 76, 064515 (2007).
26. J. W. Seo, K. Yang, D. W. Lee, Y. S. Roh, J. H. Kim, H. Eisaki, H. Ishii, I. Jarrige, Y. Q. Cai, D. L. Feng, and C. Kim, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.73.161104 73, 161104 (R) (2006).
27. Y. Tokura, S. Koshihara, T. Arima, H. Takagi, S. Ishibashi, T. Ido, and S. Uchida, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.41.11657 41, 11657 (1990).
28. The spectra were first smoothed with a Gaussian of 0.37 eV width to account for the resolution. The spectra were further smoothed via folding with a Lorentzian of 0.30 eV width to mimic what appears to be an intrinsic linewidth.
29. The branch near 4 eV is weak in the experimental data. Since this branch has a different symmetry than the 2 eV branch, it resonates at a different photon energy (near 8.894 eV), as evident from the raw data profile in Fig. 1.
30. The experimental spectra for energy transfers beyond about 6 eV contain significant contributions from bands beyond the three-band model we considered for this work.
31. K. Penc and W. Stephan, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.62.12707 62, 12707 (2000).