In mathematics, mathematical physics, and theoretical physics, the spin tensor is a quantity used to describe the rotational motion of particles in spacetime. The tensor has application in general relativity and special relativity, as well as quantum mechanics, relativistic quantum mechanics, and quantum field theory.
Background on Noether currents
The Noether current for translations in space is momentum, while the current for increments in time is energy. These two statements combine into one in spacetime: translations in spacetime, i.e. a displacement between two events, is generated by the four-momentum P. Conservation of four-momentum is given by the continuity equation:
where is the stress–energy tensor, and ∂ are partial derivatives that make up the four gradient (in non-Cartesian coordinates this must be replaced by the covariant derivative). Integrating over spacetime:
gives the four-momentum vector at time t.
The Noether current for a rotation about the point y is given by a tensor of 3rd order, denoted . Because of the Lie algebra relations
where the 0 subscript indicates the origin (unlike momentum, angular momentum depends on the origin), the integral:
gives the angular momentum tensor at time t.
The spin tensor is defined at a point x to be the value of the Noether current at x of a rotation about x,
The continuity equation
The quantity S is the density of spin angular momentum (spin in this case is not only for a point-like particle, but also for an extended body), and M is the density of orbital angular momentum. The total angular momentum is always the sum of spin and orbital contributions.
gives the torque density showing the rate of conversion between the orbital angular momentum and spin.
Examples of materials with a nonzero spin density are molecular fluids, the electromagnetic field and turbulent fluids. For molecular fluids, the individual molecules may be spinning. The electromagnetic field can have circularly polarized light. For turbulent fluids, we may arbitrarily make a distinction between long wavelength phenomena and short wavelength phenomena. A long wavelength vorticity may be converted via turbulence into tinier and tinier vortices transporting the angular momentum into smaller and smaller wavelengths while simultaneously reducing the vorticity. This can be approximated by the eddy viscosity.
- Poincaré group
- Lorentz group
- Relativistic angular momentum
- Center of mass (relativistic)
- Mathisson–Papapetrou–Dixon equations
- Pauli–Lubanski pseudovector
- A. K. Raychaudhuri; S. Banerji; A. Banerjee (2003). General Relativity, Astrophysics, and Cosmology. Astronomy and astrophysics library. Springer. pp. 66–67. ISBN 038-740-628-X.
- J.A. Wheeler; C. Misner; K.S. Thorne (1973). Gravitation. W.H. Freeman & Co. pp. 156–159, §5.11. ISBN 0-7167-0344-0.
- L. M. Butcher; A. Lasenby; M. Hobson (2012). "Localizing the Angular Momentum of Linear Gravity". Phys. Rev. D. arXiv: . Bibcode:2012PhRvD..86h4012B. doi:10.1103/PhysRevD.86.084012.
- T. Banks (2008). "Modern Quantum Field Theory: A Concise Introduction". Cambridge University Press. ISBN 113-947-389-1.
- S. Kopeikin, M.Efroimsky, G. Kaplan (2011). "Relativistic Celestial Mechanics of the Solar System". John Wiley & Sons. ISBN 352-763-457-6.
- W. F. Maher; J. D. Zund (1968). "A spinor approach to the Lanczos spin tensor". II Nuovo Cimento A. 10. 57 (4). Springer. pp. 638–648.
- von Jan Steinhoff. "Canonical Formulation of Spin in General Relativity (Dissertation)" (PDF). Retrieved 2013-10-27.