General Construction of Tubular Geometry
arXiv:1608.07506
Abstract
We consider the problem of locally describing tubular geometry around a submanifold embedded in a (pseudo)Riemannian manifold in its general form. Given the geometry of ambient space in an arbitrary coordinate system and equations determining the submanifold in the same system, we compute the tubular expansion coefficients in terms of this {\it a priori data}. This is done by using an indirect method that crucially applies the tubular expansion theorem for vielbein previously derived. With an explicit construction involving the relevant coordinate and non-coordinate frames we verify consistency of the whole method up to quadratic order in vielbein expansion. Furthermore, we perform certain (long and tedious) higher order computation which verifies the first non-trivial spin connection term in the expansion for the first time. Earlier a similar method was used to compute tubular geometry in loop space. We explain this work in the light of our general construction.
arXiv comment40 pages
References in corpus (11)
- The large D limit of General Relativity
- Large D gravity and low D strings
- Fermi Coordinates for Weak Gravitational Fields
- Black hole tidal problem in the Fermi normal coordinates
- A membrane paradigm at large D
- Universal quasinormal modes of large D black holes
- Explicit Fermi Coordinates and Tidal Dynamics in de Sitter and Goedel Spacetimes
- Effective Hamiltonians for Constrained Quantum Systems
- The Energy-Level Shifts of a Stationary Hydrogen Atom in Static External Gravitational Field with Schwarzschild Geometry
- A Statistical Mechanical Problem in Schwarzschild Spacetime
- Fermi coordinates in Schwarzschild spacetime: closed form expressions