1 / 10

Casimir forces, surface fluctuations, and thinning of superfluid films Mehran Kardar (MIT)

Casimir forces, surface fluctuations, and thinning of superfluid films Mehran Kardar (MIT). Roya Zandi Joseph Rudnick (UCLA). Phys. Rev. Lett. 93 , 155302 (2004). 4 He thin film experiments R. Garcia and M.H.W. Chan, Phys. Rev. Lett. 83, 1187 (1999). Superfluid transition. Superfluid.

freja
Download Presentation

Casimir forces, surface fluctuations, and thinning of superfluid films Mehran Kardar (MIT)

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Casimir forces, surface fluctuations, and thinning of superfluid filmsMehran Kardar (MIT) Roya Zandi Joseph Rudnick (UCLA) Phys. Rev. Lett. 93, 155302 (2004)

  2. 4He thin film experimentsR. Garcia and M.H.W. Chan, Phys. Rev. Lett. 83, 1187 (1999) Superfluid transition Superfluid Normal fluid The film is thinner at the transition, and in the superfluid phase Question:Why are films thinner in the superfluid state?

  3. Casimireffect Proc. K. Ned. Akad. Wet. 51, 793 (1948) Quantum fluctuations of the EM field between conducting plates in vacuum results in long-ranged forces • Normal modes of Electro-Magnetic field between plates: • The ground state energy of quantized normal modes: • An attractive force between plates:

  4. Finite-size effects at Criticality • Analogs in Statistical Mechanics • Phase diagrams: • Free energy of the long-wavelength fluctuations: M.E. Fisher and P.-G. de Gennes, C.R. Acad. Sci. Ser. B 287, 207 (1978) M.E. Fisher + P.-G. de Gennes, C. R. Acad. Sci.Ser. B 287, 207 (1978) C

  5. Superfluid Helium Pressure • Superfluid He has “massless” Goldstone modes (phonons) associated with the phase of the quantum condenstae. • The interaction resulting from (thermal) fluctuations of these modes is H. Li and M. Kardar, PRL 67, 3275 (1991); PRA 46, 6490 (1992) fluid C superfluid gas temp

  6. Wetting by a Superfluid film • R. Garcia and M.H.W. Chan, Phys. Rev. Lett. 83, 1187 (1999). • Question:What determines the thickness of the wetting layer? d He (vapor) He (liquid)

  7. Thinning of a Superfluid film d h He (vapor) • Thickness of the wetting film is obtained by minimizing • The film is thinner at the transition, and in the superfluid phase • The observed thinning of the film is larger than can be accounted by the Casimir forces associated with Goldstone modes. He (liquid) Goldstone modes + ? Critical

  8. Surface fluctuations • Normal fluid is clamped due to viscosity • Superfluid films have a velocity field associated with the superfluid phase • Kinetic energy • Free energy associated with superfluid flow • Dzyaloshinskii, Lifshitz, Pitaevskii (1961) • Mahale and Cole (1986) • Not a Helfrich interaction which is repulsive

  9. Thinning of a Superfluid film • Casimir force due to surface fluctuations • Total Casimirforce: M. Krech Ueno & Balibar (2004)

  10. Summary • Bulk Goldstone modes + surface fluctuations suffice to explain the excess thinning of the film in the superfluid region. Future work • Effect of surface fluctuations at--and especially immediately below--the superfluid transition

More Related