Pomeranchuk Instability and Bose Condensation of Scalar Quanta in A

Pomeranchuk Instability and Bose Condensation of Scalar Quanta in A

Pomeranchuk instability and Bose condensation of scalar quanta in a Fermi liquid E. E. Kolomeitsev1 and D. N. Voskresensky2 1Matej Bel University, SK-97401 Banska Bystrica, Slovakia 2 National Research Nuclear University (MEPhI), 115409 Moscow, Russia (Dated: October 14, 2018) We study excitations in a normal Fermi liquid with a local scalar interaction. Spectrum of bosonic scalar-mode excitations is investigated for various values and momentum dependence of the scalar Landau parameter f0 in the particle-hole channel. For f0 > 0 the conditions are found when the phase velocity on the spectrum of the zero sound acquires a minimum at a non-zero momentum. For −1 < f0 < 0 there are only damped excitations, and for f0 < −1 the spectrum becomes unstable against a growth of scalar-mode excitations (a Pomeranchuk instability). An effective Lagrangian for the scalar excitation modes is derived after performing a bosonization procedure. We demonstrate that the Pomeranchuk instability may be tamed by the formation of a static Bose condensate of the scalar modes. The condensation may occur in a homogeneous or inhomogeneous state relying on the momentum dependence of the scalar Landau parameter. Then we consider a possibility of the condensation of the zero-sound-like excitations in a state with a non-zero momentum in Fermi liquids moving with overcritical velocities, provided an appropriate momentum dependence of the Landau parameter f0(k) > 0. PACS numbers: 21.65.-f, 71.10.Ay, 71.45.-d Keywords: Nuclear matter, Fermi liquid, sound-like excitations, Pomeranchuk instability, Bose condensation I. INTRODUCTION density fluctuations. In hydrodynamic terms the condi- tion f < 1 implies that the speed of the first sound 0 − The theory of normal Fermi liquids was built up by becomes imaginary. This would lead to an exponential growth of the aerosol-like mixture of droplets and bub- Landau [1], see in textbooks [2–4]. The Fermi liquid ap- proach to the description of nuclear systems was devel- bles (spinodal instability). In a one-component Fermi liq- uid spinodal instability results in a mixed liquid-gas like oped by Migdal [5, 6]. In the Fermi liquid theory the low- lying excitations are described by several phenomeno- stationary state determined by the Maxwell construction logical Landau parameters. Pomeranchuk has shown in if the pressure has a van der Waals form as a function Ref. [7] that Fermi liquids are stable only if some inequal- of the volume. In the isospin symmetric nuclear matter ities on the values of the Landau parameters are fulfilled. (if the Coulomb interaction is neglected) the liquid-gas phase transition might occur [16, 17] for the baryon den- In this work we study low-lying scalar excitation modes < < sities 0.3n0 ∼ n ∼ 0.7n0, where n0 is the nuclear satura- (density-density fluctuations) in the cold normal Fermi tion density. In a many-component system a mechanical liquids for various values and momentum behavior of the instability is accompanied by a chemical instability, see scalar Landau parameter f0 in the particle-hole channel. Ref. [18]. The inclusion of the Coulomb interaction, see We assume that an interaction in the particle-particle Refs. [19, 20], leads to a possibility of the pasta phase in channel is repulsive and the system is, therefore, stable the neutron star crusts for densities 0.3n < n < 0.7n . against pairing in an s-wave state. An induced p-wave 0 ∼ ∼ 0 pairing to be possible at very low temperatures T <Tc,p, The key point of this work is that we suggest an al- see Refs. [8], can be precluded by the assumption that ternative description of unstable zero-sound-like modes which might be realized at certain conditions. We arXiv:1505.03884v1 [nucl-th] 14 May 2015 the temperature of the system is small but above Tc,p. demonstrate that for f0 < 1 instability may result in For f0 > 0 the conditions will be found when the − phase velocity of the spectrum possesses a minimum at an accumulation of a static Bose condensate of the scalar a non-zero momentum. This means that the spectrum field. The condensate amplitude is stabilized by the re- satisfies the Landau necessary condition for superfluid- pulsive self-interaction. The condensation may occur in ity. As a consequence this may lead to a condensation the homogeneous either in inhomogeneous state depend- of zero-sound-like excitations with a non-zero momentum ing on the momentum dependence of the Landau param- in moving Fermi liquids with the velocity above the Lan- eter f0(k). In the presence of the condensate the Fermi dau critical velocity [9]. Similar phenomena may occur liquid proves to be stable. in moving He-II, cold atomic gases, and other moving The work is organized as follows. In Sect. II we study media, like rotating neutron stars, cf. Refs. [10–15]. For spectrum of excitations in a one-component Fermi liquid 1 < f0 < 0 excitations are damped, for f0 < 1 the in the scalar channel in dependence on f0(k). In Sect. III spectrum− is unstable against the growth of zero-sound-− we bosonize the local interaction and suggest an effec- like modes and hydrodynamic modes. Up to now it was tive Lagrangian for the self-interacting scalar modes. In thought that for f0 < 1 the mechanical stability condi- Sect. IV we study Pomeranchuk instability for f0 < 1 tion is violated that results− in exponential buildup of the and suggest a novel possibility of the occurrence of the− 2 static Bose-condensate which leads to a stabilization of in Eq. (5) can be expressed in terms of dimensionless the system. In Sect. V we consider condensation of scalar scalar and spin Landau parameters excitations in moving Fermi liquids with repulsive inter- ˜ ′ 2 ω ′ actions. Concluding remarks are formulated in Sect. VI. f(~n , ~n)= a N0Γ0 (~n , ~n) , ′ 2 ω ′ g˜(~n , ~n)= a N0Γ1 (~n , ~n) , (6) II. EXCITATIONS IN A FERMI LIQUID where the normalization constant is chosen as in applica- tions to atomic nuclei [6, 21, 22] with the density of states A. Landau particle-hole amplitude. at the Fermi surface, N0 = N(n = n0), taken at the nu- ∗ mF(n) pF(n) clear saturation density n0 and N(n)= π2 . Such Consider the simplest case of a one-component Fermi a normalization is at variance with that used, e.g., in liquid of non-relativistic fermions. As discussed in the Refs. [1–4]. Their parameters are related to ours defined Introduction, we assume that the system is stable against in Eq. (6) as f = N f/N˜ 0 and g = N g/N˜ 0. pairing. The particle-hole scattering amplitude on the The Landau parameters can be expanded in terms of Fermi surface obeys the equation [2–4, 6] the Legendre polynomials P (~n ~n ′), l · ′ ω ′ ′ ′ Tph(~n , ~n; q)= Γ (~n , ~n) f˜(~n , ~n)= f˜ P (~n ~n ) , (7) l l · ω ′ ′′ ′′ ′′ Xl b + Γ (~n , ~n b) ph(~n ; q) Tph(~n , ~n; q) ~n ′′ , (1) h L i and the similar expression exists for the parameterg ˜. where ~n andb ~n ′ are directions of fermionb momenta before The Landau parameters f˜ ,g ˜ can be directly related and after scattering and q = (ω,~k) is the momentum 0,1 0,1 to observables [4]. For instance, the effective quasiparti- transferred in the particle-hole channel. The brackets cle mass is given by [2, 3] stand for averaging over the momentum direction ~n ∗ mF 2 1 dΩ~n =1+ a N Γ0(cos θ)cos θ =1+ f1 , (8) ... ~n = ... , (2) m 3 h i Z 4 π F where the bar denotes the averaging over the azimuthal and the particle-hole propagator is and polar angles. The positiveness of the effective mass +∞ +∞ is assured by fulfillment of the Pomeranchuk condition 2 dǫ dpp f1 > 3. Note that the traditional normalization of the ph(~n; q)= G(pF+) G(pF−) , (3) − L Z 2πi Z π2 Landau parameters (6) depends explicitly on the effective −∞ 0 mass m∗ through the density of states N. Therefore, it is instructive to rewrite Eq. (8) using the definition in ~ where we denoted pF± = (ǫ ω/2,pF ~n k/2) and pF Eq. (6) stands for the Fermi momentum.± The quasiparticle± con- tribution to the full Green’s function is given by m∗ 1 F = . (9) 1 mF mF 1 ∗ f˜ 2 2 3 m (n0) 1 a p pF − F G(ǫ, ~p)= , ξ~p = − ∗ . (4) ǫ ξ~p + i 0 signǫ 2 mF − From this relation we obtain the constraint f˜1 < ∗ ∗ 3 m (n0)/mF for the effective mass to remain positive Here mF is the effective fermion mass, and the param- F eter a determines a quasiparticle weight in the fermion and finite; otherwise the effective mass tends to infinity ˜ ∗ spectral density, 0 < a 1, which is expressed through in the point where f1 =3 mF(n0)/mF. Thus, for the sys- ≤ R −1 tems where one expects a strong increase of the effective the retarded fermion self-energy ΣF (ǫ,p) as a = 1 R − mass, the normalization (6) of the Landau parameters (∂ Σ /∂ǫ)0. The full Green’s function contains also a ℜ F would be preferable. A large increase of the effective regular background part Greg, which is encoded in the fermion mass may be a sign of a quantum phase transi- renormalized particle-hole interaction Γˆω in Eq. (1). tion dubbed in Refs. [23, 24] as a fermion condensation. The interaction in the particle-hole channel can be The latter is connected with the appearance of multi- written as connected Fermi surfaces.

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    12 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us