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1
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36949051230
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NATUAS 0028-0836 10.1038/248030a0
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S. W. Hawking, Nature (London) NATUAS 0028-0836 10.1038/248030a0 248, 30 (1974).
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Hawking, S.W.1
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2
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0033246313
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RMPHAT 0034-6861 10.1103/RevModPhys.71.463
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F. Dafolvo, S. Giorgini, L. P. Pitaevskii, and S. Stringari, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.71.463 71, 463 (1999).
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Dafolvo, F.1
Giorgini, S.2
Pitaevskii, L.P.3
Stringari, S.4
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3
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84925126367
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edited by C. J. Pethick and H. Smith (Cambridge University Press, Cambridge
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Bose-Einstein Condensation in Dilute Gases, edited by, C. J. Pethick, and, H. Smith, (Cambridge University Press, Cambridge, 2002).
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(2002)
Bose-Einstein Condensation in Dilute Gases
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5
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36149004969
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PHRVAO 0031-899X 10.1103/PhysRev.106.1135
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T. D. Lee, K. Huang, and C. N. Yang, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.106.1135 106, 1135 (1957).
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Lee, T.D.1
Huang, K.2
Yang, C.N.3
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6
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0037930223
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See, e.g., edited by L. P. Pitaevskii and S. Stringari (Clarendon Press, Oxford
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See, e.g., Bose-Einstein Condensation, edited by, L. P. Pitaevskii, and, S. Stringari, (Clarendon Press, Oxford, 2003).
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(2003)
Bose-Einstein Condensation
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7
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0000703952
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PLRAAN 1050-2947 10.1103/PhysRevA.56.3840
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F. Dalfovo, S. Giorgini, M. Guilleumas, L. Pitaevskii, and S. Stringari, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.56.3840 56, 3840 (1997).
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Phys. Rev. A
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Dalfovo, F.1
Giorgini, S.2
Guilleumas, M.3
Pitaevskii, L.4
Stringari, S.5
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8
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0001053337
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PLRAAN 1050-2947 10.1103/PhysRevA.57.3008
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Y. Castin and R. Dum, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.57. 3008 57, 3008 (1998).
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Castin, Y.1
Dum, R.2
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9
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0000935910
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PLRAAN 1050-2947 10.1103/PhysRevA.56.1414
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C. W. Gardiner, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.56.1414 56, 1414 (1997).
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Phys. Rev. A
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Gardiner, C.W.1
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10
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34247884975
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We thank I. Carusotto for kindly pointing this out to our attention.
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We thank I. Carusotto for kindly pointing this out to our attention.
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11
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34247856481
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The linear phonon dispersion relation, characteristic of a massless relativistic free field would lead (after renormalization) to a vanishing quantum depletion.
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The linear phonon dispersion relation, characteristic of a massless relativistic free field would lead (after renormalization) to a vanishing quantum depletion.
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13
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0034317499
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PRLTAO 0031-9007 10.1103/PhysRevLett.85.4643
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L. J. Garay, J. R. Anglin, J. I. Cirac, and P. Zoller, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.85.4643 85, 4643 (2000);
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Garay, L.J.1
Anglin, J.R.2
Cirac, J.I.3
Zoller, P.4
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17
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0003407449
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See, e.g., edited by V. P. Frolov and I. D. Novikov (Kluwer, Dordrecht, The Netherlands
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See, e.g., Black Hole Physics: Basic Concepts and New Developments, edited by, V. P. Frolov, and, I. D. Novikov, (Kluwer, Dordrecht, The Netherlands, 1997).
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(1997)
Black Hole Physics: Basic Concepts and New Developments
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18
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34247886562
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For this estimation μ2 g1 2 n0 3 2 m3 2 1.
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For this estimation μ2 g1 2 n0 3 2 m3 2 1.
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19
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0001755020
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Note that the order of magnitude of these terms confirms the prediction of PLRAAN 1050-2947 10.1103/PhysRevA.55.3645
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Note that the order of magnitude of these terms confirms the prediction of E. Timmermans, P. Tommasini, and K. Huang, Phys. Rev. A PLRAAN 1050-2947 10.1103/PhysRevA.55.3645 55, 3645 (1997).
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(1997)
Phys. Rev. A
, vol.55
, pp. 3645
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Timmermans, E.1
Tommasini, P.2
Huang, K.3
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20
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34247867046
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To realize this kind of configurations, it is necessary to add source (well) terms in the continuity Eq. 9 in order to conserve the mass. However, the presence of these terms do not invalidate our treatment since Eqs. 12 13 remain unchanged.
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To realize this kind of configurations, it is necessary to add source (well) terms in the continuity Eq. 9 in order to conserve the mass. However, the presence of these terms do not invalidate our treatment since Eqs. 12 13 remain unchanged.
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21
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33645143654
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See e.g., RNUCAC 0035-5917
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See e.g., R. Balbinot, A. Fabbri, S. Fagnocchi, and R. Parentani, Riv. Nuovo Cimento RNUCAC 0035-5917 28, 1 (2005).
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(2005)
Riv. Nuovo Cimento
, vol.28
, pp. 1
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Balbinot, R.1
Fabbri, A.2
Fagnocchi, S.3
Parentani, R.4
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