From Quantum Turbulence to Classical Hydrodynamics
ORAL
Abstract
How well can coarse-grained quantum turbulence be described by hydrodynamic theories? Such a simplification is almost certainly needed to describe macroscopic phenomena such as pulsar glitches in neutron stars, but how well do they or can they actually work? In this talk I will discuss some ideas and present results about both bosonic and fermionic quantum turbulence that addresses this question.
*This material is based upon work supported by the National Science Foundation under Award No(s). Award Nos. 2012190 and 2309322. Any opinions, findings and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.
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Presenters
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Michael M Forbes
- Washington State University