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Contents

   



(Top)
 


1 Superfluidity of liquid helium  





2 Ultracold atomic gases  





3 Superfluids in astrophysics  





4 In high-energy physics and quantum gravity  





5 See also  





6 References  





7 Further reading  





8 External links  














Superfluidity






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From Wikipedia, the free encyclopedia
 


Helium II will "creep" along surfaces in order to find its own level—after a short while, the levels in the two containers will equalize. The Rollin film also covers the interior of the larger container; if it were not sealed, the helium II would creep out and escape.
The liquid helium is in the superfluid phase. A thin invisible film creeps up the inside wall of the bowl and down on the outside. A drop forms. It will fall off into the liquid helium below. This will repeat until the cup is empty—provided the liquid remains superfluid.

Superfluidity is the characteristic property of a fluid with zero viscosity which therefore flows without any loss of kinetic energy. When stirred, a superfluid forms vortices that continue to rotate indefinitely. Superfluidity occurs in two isotopesofhelium (helium-3 and helium-4) when they are liquefied by cooling to cryogenic temperatures. It is also a property of various other exotic states of matter theorized to exist in astrophysics, high-energy physics, and theories of quantum gravity.[1] The theory of superfluidity was developed by Soviet theoretical physicists Lev Landau and Isaak Khalatnikov.

Superfluidity often co-occurs with Bose–Einstein condensation, but neither phenomenon is directly related to the other; not all Bose–Einstein condensates can be regarded as superfluids, and not all superfluids are Bose–Einstein condensates.[citation needed] Superfluids have some potential practical uses, such as dissolving substances in a quantum solvent.

Superfluidity of liquid helium[edit]

Superfluidity was discovered in helium-4byPyotr Kapitsa[2] and independently by John F. Allen and Don Misener[3] in 1937. Onnes possibly observed the superfluid phase transition on August 2 1911, the same day that he observed superconductivity in mercury.[4] It has since been described through phenomenology and microscopic theories.

In liquid helium-4, the superfluidity occurs at far higher temperatures than it does in helium-3. Each atom of helium-4 is a boson particle, by virtue of its integer spin. A helium-3 atom is a fermion particle; it can form bosons only by pairing with another particle like itself, which occurs at much lower temperatures. The discovery of superfluidity in helium-3 was the basis for the award of the 1996 Nobel Prize in Physics.[1] This process is similar to the electron pairinginsuperconductivity.

Ultracold atomic gases[edit]

Superfluidity in an ultracold fermionic gas was experimentally proven by Wolfgang Ketterle and his team who observed quantum vorticesinlithium-6 at a temperature of 50 nK at MIT in April 2005.[5][6] Such vortices had previously been observed in an ultracold bosonic gas using rubidium-87 in 2000,[7] and more recently in two-dimensional gases.[8] As early as 1999, Lene Hau created such a condensate using sodium atoms[9] for the purpose of slowing light, and later stopping it completely.[10] Her team subsequently used this system of compressed light[11] to generate the superfluid analogue of shock waves and tornadoes:[12]

These dramatic excitations result in the formation of solitons that in turn decay into quantized vortices—created far out of equilibrium, in pairs of opposite circulation—revealing directly the process of superfluid breakdown in Bose–Einstein condensates. With a double light-roadblock setup, we can generate controlled collisions between shock waves resulting in completely unexpected, nonlinear excitations. We have observed hybrid structures consisting of vortex rings embedded in dark solitonic shells. The vortex rings act as 'phantom propellers' leading to very rich excitation dynamics.

— Lene Hau, SIAM Conference on Nonlinear Waves and Coherent Structures

Superfluids in astrophysics[edit]

The idea that superfluidity exists inside neutron stars was first proposed by Arkady Migdal.[13][14] By analogy with electrons inside superconductors forming Cooper pairs because of electron–lattice interaction, it is expected that nucleons in a neutron star at sufficiently high density and low temperature can also form Cooper pairs because of the long-range attractive nuclear force and lead to superfluidity and superconductivity.[15]

In high-energy physics and quantum gravity[edit]

Superfluid vacuum theory (SVT) is an approach in theoretical physics and quantum mechanics where the physical vacuum is viewed as superfluid.[citation needed]

The ultimate goal of the approach is to develop scientific models that unify quantum mechanics (describing three of the four known fundamental interactions) with gravity. This makes SVT a candidate for the theory of quantum gravity and an extension of the Standard Model.[citation needed]

It is hoped that development of such a theory would unify into a single consistent model of all fundamental interactions, and to describe all known interactions and elementary particles as different manifestations of the same entity, superfluid vacuum.[citation needed]

On the macro-scale a larger similar phenomenon has been suggested as happening in the murmurationsofstarlings. The rapidity of change in flight patterns mimics the phase change leading to superfluidity in some liquid states.[16]

Light behaves like a superfluid in various applications such as Poisson's Spot. As the liquid helium shown above, light will travel along the surface of an obstacle before continuing along its trajectory. Since light is not affected by local gravity its "level" becomes its own trajectory and velocity. Another example is how a beam of light travels through the hole of an aperture and along its backside before diffraction.[citation needed]

See also[edit]

References[edit]

  1. ^ a b "The Nobel Prize in Physics 1996 – Advanced Information". www.nobelprize.org. Retrieved 2017-02-10.
  • ^ Kapitza, P. (1938). "Viscosity of Liquid Helium Below the λ-Point". Nature. 141 (3558): 74. Bibcode:1938Natur.141...74K. doi:10.1038/141074a0. S2CID 3997900.
  • ^ Allen, J. F.; Misener, A. D. (1938). "Flow of Liquid Helium II". Nature. 142 (3597): 643. Bibcode:1938Natur.142..643A. doi:10.1038/142643a0. S2CID 4135906.
  • ^ van Delft, Dirk; Kes, Peter (2010-09-01). "The discovery of superconductivity". Physics Today. 63 (9): 38–43. Bibcode:2010PhT....63i..38V. doi:10.1063/1.3490499. ISSN 0031-9228.
  • ^ "MIT physicists create new form of matter". mit.edu. 22 June 2005. Retrieved November 22, 2010.
  • ^ Grimm, R. (2005). "Low-temperature physics: A quantum revolution". Nature. 435 (7045): 1035–1036. Bibcode:2005Natur.435.1035G. doi:10.1038/4351035a. PMID 15973388. S2CID 7262637.
  • ^ Madison, K.; Chevy, F.; Wohlleben, W.; Dalibard, J. (2000). "Vortex Formation in a Stirred Bose–Einstein Condensate". Physical Review Letters. 84 (5): 806–809. arXiv:cond-mat/9912015. Bibcode:2000PhRvL..84..806M. doi:10.1103/PhysRevLett.84.806. PMID 11017378. S2CID 9128694.
  • ^ Burnett, K. (2007). "Atomic physics: Cold gases venture into Flatland". Nature Physics. 3 (9): 589. Bibcode:2007NatPh...3..589B. doi:10.1038/nphys704.
  • ^ Hau, L. V.; Harris, S. E.; Dutton, Z.; Behroozi, C. H. (1999). "Light speed reduction to 17 metres per second in an ultracold atomic gas". Nature. 397 (6720): 594–598. Bibcode:1999Natur.397..594V. doi:10.1038/17561. S2CID 4423307.
  • ^ "Lene Hau". Physicscentral.com. Retrieved 2013-02-10.
  • ^ Hau, Lene Vestergaard (2003). "Frozen Light" (PDF). Scientific American: 44–51.
  • ^ Hau, Lene (September 9–12, 2006). "Shocking Bose–Einstein Condensates with Slow Light". SIAM.org. Society for Industrial and Applied Mathematics.
  • ^ A. B. Migdal (1959). "Superfluidity and the moments of inertia of nuclei". Nucl. Phys. 13 (5): 655–674. Bibcode:1959NucPh..13..655M. doi:10.1016/0029-5582(59)90264-0.
  • ^ A. B. Migdal (1960). "Superfluidity and the Moments of Inertia of Nuclei". Soviet Phys. JETP. 10 (5): 176. Bibcode:1959NucPh..13..655M. doi:10.1016/0029-5582(59)90264-0.
  • ^ U. Lombardo & H.-J. Schulze (2001). "Superfluidity in Neutron Star Matter". Physics of Neutron Star Interiors. Lecture Notes in Physics. Vol. 578. pp. 30–53. arXiv:astro-ph/0012209. doi:10.1007/3-540-44578-1_2. ISBN 978-3-540-42340-9. S2CID 586149.
  • ^ Attanasi, A.; Cavagna, A.; Del Castello, L.; Giardina, I.; Grigera, T. S.; Jelić, A.; Melillo, S.; Parisi, L.; Pohl, O.; Shen, E.; Viale, M. (2014). "Information transfer and behavioural inertia in starling flocks". Nature Physics. 10 (9): 615–698. arXiv:1303.7097. Bibcode:2014NatPh..10..691A. doi:10.1038/nphys3035. PMC 4173114. PMID 25264452.
  • Further reading[edit]

    External links[edit]


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