QCD at finite baryon density: Nucleon droplets and color superconductivity

Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

Volumn 422, Issue 1-4, 1998, Pages 247-256

  Alford, Mark ^a   Rajagopal, Krishna ^b   Wilczek, Frank ^a  

^a INSTITUTE FOR ADVANCED STUDY   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040633467     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0370-2693(98)00051-3     Document Type: Article

References (29)

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12. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
13. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
14. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
15. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
16. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
17. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
18. For reviews, see S.P. Klevansky, Rev. Mod. Phys. 64 (1992) 649; T. Hatsuda, T. Kunihiro, Phys. Rept. 247 (1994) 221; V. Bernard, U.-G. Meissner, I. Zahed, Phys. Rev. D 36 (1987) 819; T. Hatsuda, T. Kunihiro, Phys. Lett. B 198 (1987) 126; M. Asakawa, K. Yazaki, Nucl. Phys. A 504 (1989) 668; S. Klimt, M. Lutz, W. Weise, Phys. Lett. B 249 (1990) 386; M. Lutz, S. Klimt, W. Weise, Nucl. Phys. A 542 (1992) 521; D. Ebert et al., Int. J. Mod. Phys. A 8 (1993) 1295; S. Ying, Phys. Lett. B 283 (1992) 341.
19. For a review, see T. Schaefer, E.V. Shuryak, hepph/9610451. Extensions to finite density are considered in T. Schaefer, hep-ph/9708256, and in R. Rapp, T. Schaefer, E.V. Shuryak, M. Velkovsky, hep-ph/9711396.
20. For a review, see T. Schaefer, E.V. Shuryak, hepph/9610451. Extensions to finite density are considered in T. Schaefer, hep-ph/9708256, and in R. Rapp, T. Schaefer, E.V. Shuryak, M. Velkovsky, hep-ph/9711396.
21. For a review, see T. Schaefer, E.V. Shuryak, hepph/9610451. Extensions to finite density are considered in T. Schaefer, hep-ph/9708256, and in R. Rapp, T. Schaefer, E.V. Shuryak, M. Velkovsky, hep-ph/9711396.
22. M. Buballa, Nucl. Phys. A 609 (1996) 519.
23. J. Aichelin, private communication.
24. Percolation-based approaches to the chiral transition as a function of density include: G. Baym, Physica A 96 (1979) 131; T. Celik, F. Karsch, H. Satz, Phys. Lett. B 97 (1980) 128.
25. Percolation-based approaches to the chiral transition as a function of density include: G. Baym, Physica A 96 (1979) 131; T. Celik, F. Karsch, H. Satz, Phys. Lett. B 97 (1980) 128.
26. See, for example, J.M. Lattimer et al., Astrophys. J. 425 (1994) 425; C. Schaab et al., Astrophys. J. 480 (1997) L111; for a review of the observations, see H. Ögleman, in: M. Alpar et al., (Eds.), The Lives of the Neutron Stars, Kluwer, 1995, p. 101.
27. See, for example, J.M. Lattimer et al., Astrophys. J. 425 (1994) 425; C. Schaab et al., Astrophys. J. 480 (1997) L111; for a review of the observations, see H. Ögleman, in: M. Alpar et al., (Eds.), The Lives of the Neutron Stars, Kluwer, 1995, p. 101.
28. See, for example, J.M. Lattimer et al., Astrophys. J. 425 (1994) 425; C. Schaab et al., Astrophys. J. 480 (1997) L111; for a review of the observations, see H. Ögleman, in: M. Alpar et al., (Eds.), The Lives of the Neutron Stars, Kluwer, 1995, p. 101.
29. C. Schaab et al. in [13].