How should spin-weighted spherical functions be defined?

Abstract

Spin-weighted spherical functions provide a useful tool for analyzing tensor-valued functions on the sphere. A tensor field can be decomposed into complex-valued functions by taking contractions with tangent vectors on the sphere and the normal to the sphere. These component functions are usually presented as functions on the sphere itself, but this requires an implicit choice of distinguished tangent vectors with which to contract. Thus, we may more accurately say that spin-weighted spherical functions are functions of both a point on the sphere and a choice of frame in the tangent space at that point. The distinction becomes extremely important when transforming the coordinates in which these functions are expressed, because the implicit choice of frame will also transform. Here, it is proposed that spin-weighted spherical functions should be treated as functions on the spin group. This approach more cleanly reflects the geometry involved, and allows for a more elegant description of the behavior of spin-weighted functions. In this form, the spin-weighted spherical harmonics have simple expressions as elements of the Wigner $\mathfrak{D}$ representations, and transformations under rotation are simple. Two variants of the angular-momentum operator are defined directly in terms of the spin group; one is the standard angular-momentum operator $\mathbf{L}$, while the other is shown to be related to the spin-raising operator $ð$. Computer code is also included, providing an explicit implementation of the spin-weighted spherical harmonics in this form.

This version corrects a typo in the definition of $K_{\pm }$ above Eq. (44a). All other equations remain unchanged, including Eqs. (45b) and (46)

References in corpus (3)

• Fast and Exact Spin-s Spherical Harmonic Transforms
• Gravitational-wave modes from precessing black-hole binaries
• Geometry of the Hopf Bundle and spin-weighted Harmonics

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