Continuous Monitoring of Rabi Oscillations in a Josephson Flux Qubit

Physical Review Letters

Volumn 91, Issue 9, 2003, Pages 979061-979064

  Il'ichev, E ^a   Oukhanski, N ^a   Izmalkov, A ^a,b   Wagner, Th ^a   Grajcar, M ^c,d   Meyer, H G ^a   Smirnov, A Yu ^e   Maassen van den Brink, Alec ^e   Amin, M H S ^e   Zagoskin, A M ^e,f  

^a LEIBNIZ INSTITUTE OF PHOTONIC TECHNOLOGY   (Germany)

^b NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPHI   (Russian Federation)

^c Comenius University ^*  (Slovakia)

^d FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

^e D WAVE SYSTEMS INC   (Canada)

^f UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FLUX; OSCILLATIONS; SPECTROSCOPIC ANALYSIS; SUPERCONDUCTING DEVICES;

JOSEPHSON FLUX QUBITS;

ATOMIC PHYSICS;

EID: 0142025354     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (23)

1. Y. Makhlin, G. Schön, and A. Shnirman, Rev. Mod. Phys. 73, 357 (2001).
2. Y. Nakamura, Yu. A. Pashkin, and J. S. Tsai., Phys. Rev. Lett. 87, 246601 (2001).
3. D. Vion, A. Aassime, A. Cottet, P. Joyez, H. Pothier, C. Urbina, D. Esteve, and M. H. Devoret, Science 296, 886 (2002).
4. J. M. Martinis, S. Nam, J. Aumentado, and C. Urbina, Phys. Rev. Lett. 89, 117901 (2002).
5. I. Chiorescu, Y. Nakamura, C. J. P. M. Harmans, and J. E. Mooij, Science 299, 1869 (2003).
6. R here is the angular frequency of probability oscillations. After one resonant oscillation, the wave function has changed its sign. In cases where this is relevant, defining the Rabi frequency twice as small is advantageous - e.g., M. H. S. Amin, A.Yu. Smirnov, and A. Maassen van den Brink, Phys. Rev. B 67, 100508(R) (2003).
7. A. Yu. Smirnov, cond-mat/0306004.
8. C. H. van der Wal, A. C. J. ter Haar, F. K. Wilhelm, R. N. Scheuten, C. J. P. M. Harmans, T. P. Orlando, S. Lloyd, and J. E. Mooij, Science 290, 773 (2000).
9. J. E. Mooij, T. P. Orlando, L. Levitov, L. Tian, C. H. van der Wal, and S. Lloyd, Science 285, 1036 (1999).
10. E. Il'ichev et al., Rev. Sci. Instrum. 72, 1882 (2001).
11. J. M. Raimond, M. Brune, and S. Haroche, Rev. Mod. Phys. 73, 565 (2001).
12. A. N. Korotkov and D. V Averin, Phys. Rev. B 64, 165310 (2001).
13. A. H. Silver and J. E. Zimmerman, Phys. Rev. 157, 317 (1967).
14. Ya. S. Greenberg, A. Izmalkov, M. Grajcar, E. Il'ichev, W. Krech, H.-G. Meyer, M. H. S. Amin, and A. Maassen van den Brink, Phys. Rev. B 66, 214525 (2002).
15. Ya. S. Greenberg, A. Izmalkov, M. Grajcar, E. Il'ichev, W. Krech, and H.-G. Meyer, Phys. Rev. B 66, 224511 (2002).
16. E. Il'ichev et al., Appl. Phys. Lett. 80, 4184 (2002).
17. N. Oukhanski, M. Grajcar, E. Il'ichev, and H.-G. Meyer, Rev. Sci, Instrum. 74, 1145 (2003).
18. b.
19. T.
20. Rabi. Compare the concluding remarks in [5].
21. F. Plastina and G. Falci, Phys. Rev. B 67, 224514 (2003); A. Blais, A. Maassen van den Brink, and A. M. Zagoskin, Phys. Rev. Lett 90, 127901 (2003); A.Yu. Smirnov and A. M. Zagoskin, cond-mat/0207214.
22. F. Plastina and G. Falci, Phys. Rev. B 67, 224514 (2003); A. Blais, A. Maassen van den Brink, and A. M. Zagoskin, Phys. Rev. Lett 90, 127901 (2003); A.Yu. Smirnov and A. M. Zagoskin, cond-mat/0207214.
23. F. Plastina and G. Falci, Phys. Rev. B 67, 224514 (2003); A. Blais, A. Maassen van den Brink, and A. M. Zagoskin, Phys. Rev. Lett 90, 127901 (2003); A.Yu. Smirnov and A. M. Zagoskin, cond-mat/0207214.