Dynamic spin-response function of the high-temperature Bi2 Sr2 Ca Cu2 O8+δ superconductor from angle-resolved photoemission spectra

Physical Review B - Condensed Matter and Materials Physics

Volumn 75, Issue 17, 2007, Pages

  Chatterjee, U ^a,b   Morr, D K ^a   Norman, M R ^b   Randeria, M ^c   Kanigel, A ^a   Shi, M ^a,d   Rossi, E ^a   Kaminski, A ^e   Fretwell, H M ^e   Rosenkranz, S ^b   Kadowaki, K ^f   Campuzano, J C ^a,b  

^a UNIVERSITY OF ILLINOIS AT CHICAGO   (United States)

^b ARGONNE NATIONAL LABORATORY   (United States)

^c OHIO STATE UNIVERSITY   (United States)

^d PAUL SCHERRER INSTITUTE   (Switzerland)

^e IOWA STATE UNIVERSITY   (United States)

^f UNIVERSITY OF TSUKUBA   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 34347225129     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.75.172504     Document Type: Article

References (32)

1. A. Damascelli, Z. Hussain, and Z.-X. Shen, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.75.473 75, 473 (2003);
2. J. C. Campuzano, M. R. Norman, and M. Randeria, in The Physics of Superconductors, edited by, K. H. Bennemann, and, J. B. Ketterson, (Springer, Berlin, 2004), Vol. 2, p. 167.
3. J. Rossat-Mignod, Physica C PHYCE6 0921-4534 10.1016/0921-4534(91)91955-4 185, 86 (1991);
4. H. F. Fong, B. Keimer, P. W. Anderson, D. Reznik, F. Dogan, and I. A. Aksay, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.75.316 75, 316 (1995);
5. P. Dai, H. A. Mook, R. D. Hunt, and F. Dogan, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.63.054525 63, 054525 (2001).
6. J. Brinckmann and P. A. Lee, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.82.2915 82, 2915 (1999);
7. Y.-J. Kao, Q. Si, and K. Levin, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.61.R11898 61, R11898 (2000);
8. M. R. Norman, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.61.14751 61, 14751 (2000);
9. M. R. Norman, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.63.092509 63, 092509 (2001);
10. F. Onufrieva and P. Pfeuty, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.65.054515 65, 054515 (2002).
11. See, e.g., C.-H. Pao and N. E. Bickers, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.51.16310 51, 16310 (1994);
12. E. Demler and S.-C. Zhang, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.75.4126 75, 4126 (1995);
13. N. Bulut and D. J. Scalapino, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.53.5149 53, 5149 (1996).
14. M. Vojta and T. Ulbricht, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.93.127002 93, 127002 (2004);
15. G. S. Uhrig, K. P. Schmidt, and M. Gruninger, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.93.267003 93, 267003 (2004);
16. C. D. Batista, G. Ortiz, and A. V. Balatsky, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.64.172508 64, 172508 (2001).
17. H. F. Fong, Nature (London) NATUAS 0028-0836 10.1038/19255 398, 588 (1999).
18. M. Arai, T. Nishijima, Y. Endoh, T. Egami, S. Tajima, K. Tomimoto, Y. Shiohara, M. Takahashi, A Garrett, and S. M. Bennington, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83.608 83, 608 (1999).
19. S. M. Hayden, Nature (London) NATUAS 0028-0836 10.1038/nature02576 429, 531 (2004).
20. B. Fauque, arXiv:cond-mat/0701052 (unpublished).
21. A. Kaminski, M. Randeria, J. C. Campuzano, M. R. Norman, H. Fretwell, J. Mesot, T. Sato, T. Takahashi, and K. Kadowaki, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.86.1070 86, 1070 (2001).
22. U. Chatterjee, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.96. 107006 96, 107006 (2006).
23. G. D. Mahan, Many-Particle Physics (Plenum, New York, 1990).
24. J. R. Schrieffer, Theory of Superconductivity (Benjamin Cummings, Reading, MA, 1964).
25. M. Randeria, H. Ding, J. C. Campuzano, A. Bellman, G. Jennings, T. Yokoya, T. Takahashi, H. Katayama-yoshida, T. Mochiku, and K. Kadowaki, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.74.4951 74, 4951 (1995).
26. A. Kaminski, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.69.212509 69, 212509 (2004).
27. ARPES data are also affected by finite energy and momentum resolutions which, in principle, can be deconvolved from the data but, in practice, have been found not to have a significant effect on Im G. See M. R. Norman, H. Ding, H. Fretwell, M. Randeria, and J. C. Campuzano, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.60.7585 60, 7585 (1999).
28. See, e.g., N. Miyakawa, J. F. Zasadzinski, L. Ozyuzer, P. Guptasarma, D. G. Hinks, C. Kendziora, and K. E. Gray, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.83.1018 83, 1018 (1999);
29. S. H. Pan, Nature (London) NATUAS 0028-0836 10.1038/35095012 413, 282 (2001).
30. M. R. Norman, M. Randeria, H. Ding, and J. C. Campuzano, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.52.615 52, 615 (1995).
31. S. Pailhes, Y. Sidis, P. Bourges, Y. Hinkov, A. Ivanov, C. Ulrich, L. P. Regnault, and B. Keimer, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett. 93.167001 93, 167001 (2004).
32. I. Eremin, D. K. Morr, A. V. Chubukov, K. Bennemann, and M. R. Norman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.94.147001 94, 147001 (2005).