A variational approach to relativistic superfluid vortex elasticity
Creators
- 1. Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton SO17 1BJ (United Kingdom)
- 2. Department of Physics, Saint Louis University, St. Louis, MO 63156-0907 (United States)
Description
It is well known that a superfluid rotates by forming an array of quantized vortices. A relativistic formulation for superfluid vortex dynamics is required for a range of problems in astrophysics and cosmology, from neutron star interiors and radio pulsar glitches to possible dark matter condensates on galactic scales. This paper develops a formalism for such systems, extending the well-established variational approach to relativistic fluids to account for the presence of a collection of quantized vortices. The model is firmly anchored in the geometry of the problem (drawing on aspects from basic string dynamics) and accounts for elastic aspects associated with a vortex array, providing a precise foundation for applications which have so far been based on somewhat ad hoc phenomenology. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1361-6382/ab79d7Additional details
Identifiers
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 37
- Journal Issue
- 8
- Journal Page Range
- [24 p.]
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52060575
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; CONDENSATES; COSMOLOGY; ELASTICITY; FLUIDS; GEOMETRY; NEUTRON STARS; NONLUMINOUS MATTER; PULSARS; RELATIVISTIC RANGE; SUPERFLUIDITY; VARIATIONAL METHODS; VORTICES
- Descriptors DEC
- CALCULATION METHODS; COSMIC RADIO SOURCES; ENERGY RANGE; MATHEMATICS; MATTER; MECHANICAL PROPERTIES; PHYSICS; STARS