2019
DOI: 10.48550/arxiv.1912.00843
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On the interaction constant measurement of polarized fermions via sound wave spectra obtained from hydrodynamics with the pressure evolution equation

Pavel A. Andreev

Abstract: Usually, hydrodynamic equations are restricted by the continuity and Euler equations. However, the account of the higher moments of the distribution function gives better description of the kinetic properties. Therefore, the pressure tensor evolution equation (PTEE) is derived for spin polarized degenerate fermions. Moreover, it is found that the pressure tensor enters the interaction term generalizing the p-wave interaction in the Euler equation. Hence, the PTEE allows to give a more accurate description of t… Show more

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Cited by 13 publications
(22 citation statements)
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References 26 publications
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“…(3) The microscopic distribution of spin-1 bosons in the physical space can be obtained by the projection of the distribution in the configurational space [8], [10], [12], [41], [42], [43]…”
Section: Hydrodynamic Equationsmentioning
confidence: 99%
“…(3) The microscopic distribution of spin-1 bosons in the physical space can be obtained by the projection of the distribution in the configurational space [8], [10], [12], [41], [42], [43]…”
Section: Hydrodynamic Equationsmentioning
confidence: 99%
“…The pressure of the normal fluid is dropped in equation (46). Equations ( 45), ( 46) correspond to equations 127-129 given in Ref.…”
Section: Nonlinear Schrodinger Equationsmentioning
confidence: 99%
“…Therefore, the account of the pressure evolution together with the pressure flux evolution gives the generalization of the model presented with the nonlinear Schrodinger equations ( 45), (46). Necessity of additional equations is demonstrated in Refs.…”
Section: Nonlinear Schrodinger Equationsmentioning
confidence: 99%
“…Unpolarized fermions are mostly discussed in literature regime for fermions [21], [22], [23]. If we have system of spin-1/2 Fermi atoms with equal population of the spinup state and the spin-down state we can observe interesting phases of matter.…”
Section: Introductionmentioning
confidence: 99%