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4
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0000049039
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W. A. Moeur, P. K. Day, F.-C. Liu, S. T. P. Boyd, M. J. Adriaans, and R. V. Duncan, Phys. Rev. Lett. 78, 2421 (1997).
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Phys. Rev. Lett.
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Moeur, W.A.1
Day, P.K.2
Liu, F.-C.3
Boyd, S.T.P.4
Adriaans, M.J.5
Duncan, R.V.6
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5
-
-
4243339968
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-
See, e.g., N. Giordano, P. Muzikar, and S. S. C. Burnett, Phys. Rev. B 36, 667 (1987); P. Muzikar and N. Giordano, Physica A 157, 742 (1989).
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(1987)
Phys. Rev. B
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, pp. 667
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-
Giordano, N.1
Muzikar, P.2
Burnett, S.S.C.3
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6
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-
0007137224
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-
See, e.g., N. Giordano, P. Muzikar, and S. S. C. Burnett, Phys. Rev. B 36, 667 (1987); P. Muzikar and N. Giordano, Physica A 157, 742 (1989).
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(1989)
Physica A
, vol.157
, pp. 742
-
-
Muzikar, P.1
Giordano, N.2
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8
-
-
25744453446
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-
W. Y. Tam and G. Ahlers, Phys. Rev. B 32, 5932 (1985); 33, 183 (1986).
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(1986)
Phys. Rev. B
, vol.33
, pp. 183
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-
-
13
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-
4243420258
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-
R. Haussmann and V. Dohm, Phys. Rev. Lett. 72, 3060 (1994); Z. Phys. B 87, 229 (1992).
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(1992)
Z. Phys. B
, vol.87
, pp. 229
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-
-
14
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-
0007119322
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-
P. B. Weichman, A. Prasad, R. Mukhopadhyay, and J. Miller, Phys. Rev. Lett. 80, 4923 (1998).
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(1998)
Phys. Rev. Lett.
, vol.80
, pp. 4923
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-
Weichman, P.B.1
Prasad, A.2
Mukhopadhyay, R.3
Miller, J.4
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15
-
-
0043048285
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-
9, Q > 0 this state has a finite coherence length (though, like all superfluid states, it has an infinite thermal conductivity), and is therefore noncritical, hence our preferred notation
-
9, Q > 0 this state has a finite coherence length (though, like all superfluid states, it has an infinite thermal conductivity), and is therefore noncritical, hence our preferred notation.
-
-
-
-
16
-
-
0043048346
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-
∞(Q) is well defined
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∞(Q) is well defined.
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-
-
-
17
-
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0002286105
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-
J. A. Lipa, D. R. Swansson, J. A. Nissen, T. C. P. Chui, and U. E. Israelson, Phys. Rev. Lett. 76, 944 (1996).
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(1996)
Phys. Rev. Lett.
, vol.76
, pp. 944
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-
Lipa, J.A.1
Swansson, D.R.2
Nissen, J.A.3
Chui, T.C.P.4
Israelson, U.E.5
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18
-
-
0001483141
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-
J. Machta, D. Candela, and R. B. Hallock, Phys. Rev. B 47, 4581 (1993); G. Ahlers and F.-C. Liu, J. Low Temp. Phys. 105, 255 (1996).
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(1993)
Phys. Rev. B
, vol.47
, pp. 4581
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-
Machta, J.1
Candela, D.2
Hallock, R.B.3
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19
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-
0030264525
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J. Machta, D. Candela, and R. B. Hallock, Phys. Rev. B 47, 4581 (1993); G. Ahlers and F.-C. Liu, J. Low Temp. Phys. 105, 255 (1996).
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(1996)
J. low Temp. Phys.
, vol.105
, pp. 255
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-
Ahlers, G.1
Liu, F.-C.2
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20
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85087226443
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0 indeed lies nearly on top of the equilibrium lambda line
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0 indeed lies nearly on top of the equilibrium lambda line.
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-
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22
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0042547397
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-
note
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- malization group theory of the SOC state. This theory improves on our mean field results in one important respect: it accounts approximately for renormalization of universal properties due to critical fluctuations. However, since vortices and phase slips exist only for n = 1, the dynamics of the large-n SOC state will be very different from the true dynamics (in particular, there is no persistent superflow for n > 1), and is therefore missing important physics that the mean field approximation treats correctly. At present the two approaches should be viewed as complementary, each containing a distinct subset of the key ingredients required for a full theory.
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-
-
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23
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12044252828
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An anonymous referee has pointed out that a more general class of periodic pattern forming systems with an Eckhaus instability [see, e.g., P. C. Hohenberg and M. C. Cross, Rev. Mod. Phys. 65, 851 (1993) for a review] might also show self-organization of this same kind.
-
(1993)
Rev. Mod. Phys.
, vol.65
, pp. 851
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-
Hohenberg, P.C.1
Cross, M.C.2
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25
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-
0042547398
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-
private communication
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David Goodstein, private communication.
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-
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Goodstein, D.1
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27
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0041545317
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-
An equivalent condition was obtained by Onuki in Ref. 17
-
An equivalent condition was obtained by Onuki in Ref. 17.
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-
-
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28
-
-
0041545314
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-
If the pressure were not static, one would have to include here also thermal expansion effects (Talso Chui, private communication). Thus, to obtain a closed system of equations one also requires separate hydrodynamic equations for the pressure (or density) and for the local fluid velocity. In addition to the heat diffusion mode, these equations would also contain the ordinary (first) sound mode. When temperature varies on time scales long compared to relevant first sound frequencies, the isobaric assumption is correct and the single closed equation (11) for the temperature emerges
-
If the pressure were not static, one would have to include here also thermal expansion effects (Talso Chui, private communication). Thus, to obtain a closed system of equations one also requires separate hydrodynamic equations for the pressure (or density) and for the local fluid velocity. In addition to the heat diffusion mode, these equations would also contain the ordinary (first) sound mode. When temperature varies on time scales long compared to relevant first sound frequencies, the isobaric assumption is correct and the single closed equation (11) for the temperature emerges.
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-
-
-
29
-
-
0043048343
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p. This is presumably tied to the existence in this case of solutions with an oscillating component
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p. This is presumably tied to the existence in this case of solutions with an oscillating component.
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-
-
-
30
-
-
0042046596
-
-
0 = 0, the first of equations (30) is non-dissipative, and in fact identical in form to the Gross-Pitaevski equation for the order parameter field 〈Ψ〈 at zero temperature, the linearized solution to which contains a sound mode with a Bogoliubov-type spectrum. However, because the normal fluid density vanishes at T = 0, this mode corresponds to first sound, not second sound. The Gross-Pitaevski equation therefore has a very different interpretation from the Model F equation, and the latter should not be thought of as some finite temperature correction to the former
-
0 = 0, the first of equations (30) is non-dissipative, and in fact identical in form to the Gross-Pitaevski equation for the order parameter field 〈Ψ〈 at zero temperature, the linearized solution to which contains a sound mode with a Bogoliubov-type spectrum. However, because the normal fluid density vanishes at T = 0, this mode corresponds to first sound, not second sound. The Gross-Pitaevski equation therefore has a very different interpretation from the Model F equation, and the latter should not be thought of as some finite temperature correction to the former.
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-
-
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32
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-
0041545318
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-
note
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∞ will presumably be metastable to an interface state, so that in principle the interface should grow continuously out of the boundary as the superfluid is heated in a quasistatic fashion (consistent with the theory presented in Ref. 18). However in any real experiment where the heating takes place at a finite rate, hysteresis effects should occur with a finite "superheating" of the superfluid state. The magnitude of the superheating will be very sensitive to boundary nucleation effects, and it remains to be seen whether it is experimentally observable.
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-
-
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34
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0041545251
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The experimental observability of this effect is limited by the same metastability issues described in footnote 28 above
-
The experimental observability of this effect is limited by the same metastability issues described in footnote 28 above.
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-
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35
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0042547395
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This is completely analogous to the behavior of a spin system in a magnetic field gradient: different spins will precess at different rates
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This is completely analogous to the behavior of a spin system in a magnetic field gradient: different spins will precess at different rates.
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-
-
-
36
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0042547394
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-
private communication
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R. V. Duncan, private communication.
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-
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Duncan, R.V.1
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37
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0041545252
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1) slightly smaller than unity
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1) slightly smaller than unity.
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