Exact ground states of rotating Bose gases close to a Feshbach resonance

Physical Review Letters

Volumn 92, Issue 22, 2004, Pages

  Cooper, N R ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

HALL EFFECT; HAMILTONIANS; KINETIC ENERGY; MATHEMATICAL MODELS; MOLECULES; QUANTUM THEORY; RESONANCE; SCATTERING;

ATOMIC GASES; FESHBACH RESONANCE; MASS RATIO; WAVE SCATTERING;

GROUND STATE;

EID: 3042838575     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.92.220405     Document Type: Article

References (19)

1. N. K. Wilkin, J. M. F. Gunn, and R. A. Smith, Phys. Rev. Lett. 80, 2265 (1998).
2. R. B. Laughlin, Phys. Rev. Lett. 50, 1395 (1983).
3. N. K. Wilkin and J. M. F. Gunn, Phys. Rev. Lett. 84, 6 (2000); N. R. Cooper and N. K. Wilkin, Phys. Rev. B 60, R16279 (1999).
4. N. K. Wilkin and J. M. F. Gunn, Phys. Rev. Lett. 84, 6 (2000); N. R. Cooper and N. K. Wilkin, Phys. Rev. B 60, R16279 (1999).
5. N. R. Cooper, N. K. Wilkin, and J. M. F. Gunn, Phys. Rev. Lett. 87, 120405 (2001).
6. N. Regnault and Th. Jolicoeur, Phys. Rev. Lett. 91, 030402 (2003).
7. S. G. Bhongale, J. N. Milstein, and M. J. Holland, Phys. Rev. A 69, 053603 (2004).
8. E. Timmermans et al., Phys. Rev. Lett. 83, 2691 (1999).
9. M. Holland, J. Park, and R. Walser, Phys. Rev. Lett. 86, 1915 (2001).
10. U. R. Fischer, P. O. Fedichev, and A. Recati, J. Phys. B 37, S301 (2004).
11. G. Moore and N. Read, Nucl. Phys. B 360, 362 (1991).
12. N. Read and E. H. Rezayi, Phys. Rev. B 59, 8084 (1999).
13. In terms of the detuning ε, defined in [7], Δ (≡ - ℏω⊥ - ℏω∥/2).
14. 1/2.
15. B. I. Halperin, Helv. Phys. Acta 56, 75 (1983); F.D.M. Haldane and E. H. Rezayi, Phys. Rev. Lett. 60, 956 (1988).
16. B. I. Halperin, Helv. Phys. Acta 56, 75 (1983); F.D.M. Haldane and E. H. Rezayi, Phys. Rev. Lett. 60, 956 (1988).
17. We exclude the uninteresting case g = 0, so that β ≠ O and α/β is finite.
18. M. Greiter, X. G. Wen, and F. Wilczek, Phys. Rev. Lett. 66, 3205 (1991).
19. k=3〉 remain the ground states.