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THE INTERNATIONAL SERIES OF MONOGRAPHS ON PHYSICS ...

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28 MICROSCOPIC <strong>PHYSICS</strong><br />

Thus there are two principal factors distinguishing liquid 4 He (or liquid 3 He)<br />

from the weakly interacting gases. Liquid 4 He and 3 He can be in equilibrium at<br />

zero pressure, and their chemical potentials at T = 0 are negative.<br />

3.3.2 Model liquid state<br />

Using our intuitive understanding of the liquid state, let us try to construct<br />

a simple model of the quantum liquid. The model energy density describing<br />

a stable isolated liquid at T = 0 must satisfy the following conditions: (i) it<br />

must be attractive (negative) at small n and repulsive (positive) at large n to<br />

provide equilibrium density of liquid; (ii) the chemical potential must be negative<br />

to prevent evaporation; (iii) the liquid must be locally stable, i.e. either the<br />

eigenfrequencies of collective modes must be real, or their imaginary part must<br />

be negative. All these conditions can be satisfied if we modify eqn (3.23) for<br />

a weakly interacting gas in the following way. Let us change the sign of the<br />

first term describing interaction and leave the second term coming from vacuum<br />

fluctuations intact, assuming that it is valid even at high density of particles. Due<br />

to the attractive interaction at low density the Bose gas collapses forming the<br />

liquid state. Of course, this is a rather artificial construction, but it qualitatively<br />

describes the liquid state. So we have the following model:<br />

ɛ(n) =− 1<br />

2 αn2 + 2<br />

5 βn5/2 , (3.32)<br />

where α>0 and β>0 are fitting parameters. In principle, one can use the<br />

exponents of n as other fitting parameters.<br />

Now we can use the equilibrium condition to obtain the equilibrium particle<br />

density n0(µ) as a function of the chemical potential:<br />

dɛ<br />

dn = µ → −αn0 + βn 3/2<br />

0 = µ. (3.33)<br />

From the equation of state one finds the pressure as a function of the equilibrium<br />

density:<br />

P (n0) =−˜ɛ(n0) =µn0(µ) − ɛ(n0(µ)) = − 1<br />

2 αn20 + 3<br />

5 βn5/2 0 . (3.34)<br />

The two contributions to the vacuum pressure cancel each other for the following<br />

value of the particle density:<br />

2 5α<br />

n0(P =0)= . (3.35)<br />

6β<br />

A droplet of the liquid with such a density will be in complete equilibrium in<br />

empty space if µ 0. These conditions are satisfied since the chemical<br />

potential and speed of sound are<br />

µ(P =0)=− 1<br />

6 n0α , (3.36)

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