2005
DOI: 10.1007/s10909-005-4730-5
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Cavitation of Electron Bubbles in Liquid Helium Below Saturation Pressure

Abstract: PACS 47.55.Bx, 64.60.Qb, 71.15.Mb

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Cited by 18 publications
(19 citation statements)
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“…We recall that ρ b is the bulk pH 2 density at such temperature. This type of interaction was already used for liquid 4 He [10], and the results obtained were found to be very similar to those obtained using the Hartree-type interaction term [11]. We have checked that the results obtained using both type of interactions are indeed very similar also in the case of pH 2 .…”
Section: Density Functional For Parahydrogensupporting
confidence: 74%
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“…We recall that ρ b is the bulk pH 2 density at such temperature. This type of interaction was already used for liquid 4 He [10], and the results obtained were found to be very similar to those obtained using the Hartree-type interaction term [11]. We have checked that the results obtained using both type of interactions are indeed very similar also in the case of pH 2 .…”
Section: Density Functional For Parahydrogensupporting
confidence: 74%
“…It can be seen that it leads to the unphysical result that P expl < P sp for T ≥ 28 K. Analogously to the helium case, this failure is related to the presence of a sizeable gas-like region within the electron bubble [11], which cannot be described within the simple capillary approximation. Any improvement in the method used to address cavitation induced by electrons calls for a more realistic description of the bubble-liquid interface, together with using an electron-pH 2 interaction that reproduces the energy barrier encountered by an electron entering liquid pH 2 , much along what has been done for liquid helium [10,11]. This is the aim of the next Section.…”
Section: Capillary Approximationmentioning
confidence: 96%
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“…5 Cavity formation around electrons in LHe has been studied extensively using various methods 12,13 including density function theory (DFT). [14][15][16][17] DFT methods specially developed for LHe provide good agreement with first principles methods for small helium clusters, 18 but have the disadvantage that they are restricted to zero Kelvin. Despite all these efforts, the precise prediction of the transition from gas-kinetic to hydrodynamic flow still remains a challenge for theory.…”
Section: Introductionmentioning
confidence: 99%