Visualization Study of Counterflow in Superfluid 4He using Metastable Helium Molecules
- 1. Physics Department, Yale University, New Haven, Connecticut 06515 (United States)
- 2. School of Physics and Astronomy, University of Birmingham, Birmingham B15 2TT (United Kingdom)
Description
Heat is transferred in superfluid 4He via a process known as thermal counterflow. It has been known for many years that above a critical heat current the superfluid component in this counterflow becomes turbulent. It has been suspected that the normal-fluid component may become turbulent as well, but experimental verification is difficult without a technique for visualizing the flow. Here we report a series of visualization studies on the normal-fluid component in a thermal counterflow performed by imaging the motion of seeded metastable helium molecules using a laser-induced-fluorescence technique. We present evidence that the flow of the normal fluid is indeed turbulent at relatively large velocities. Thermal counterflow in which both components are turbulent presents us with a theoretically challenging type of turbulent behavior that is new to physics.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.105.045301;
- arXiv
- arXiv:1004.2545v1;
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 105
- Journal Issue
- 4
- Journal Page Range
- p. 045301-045301.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42004101
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- FLOW VISUALIZATION; FLUORESCENCE; HEAT TRANSFER; HELIUM; HELIUM 4; LASER RADIATION; METASTABLE STATES; MOLECULES; SUPERFLUIDITY
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ELEMENTS; EMISSION; ENERGY LEVELS; ENERGY TRANSFER; EVEN-EVEN NUCLEI; EXCITED STATES; FLUIDS; GASES; HELIUM ISOTOPES; ISOTOPES; LIGHT NUCLEI; LUMINESCENCE; NONMETALS; NUCLEI; PHOTON EMISSION; RADIATIONS; RARE GASES; STABLE ISOTOPES
Optional Information
- Notes
- (c) 2010 The American Physical Society