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Riemannian Approximation

Math - Heisenberg09

The fields on the Heisenberg group \mathbb H that gives it its sub-Riemannian and metric structure is given by

X = \frac{\partial}{\partial x} - \frac{1}{2}y \frac{\partial}{\partial t}, Y = \frac{\partial}{\partial y} + \frac{1}{2}x \frac{\partial}{\partial t}

These are declared orthonormal, and only lines whose velocities are given by aX + bY have a (finite) speed. One may view this setup as a degenerate Riemannian structure, where a third vector field (say, s \frac{\partial}{\partial t}) has degenerated as s was sent to zero.

The Riemannian approximation I find natural interpolates between Euclidean and Heisenberg geometries, and has not yet been explored. Here are the frame fields:

X_s = \frac{\partial}{\partial x} - \frac{s}{2} y \frac{\partial}{\partial t}, Y_s = \frac{\partial}{\partial y} + \frac{s}{2} x \frac{\partial}{\partial t}, T_s = (1-s) \frac{\partial}{\partial t}

At s=0, this is the standard Euclidean frame field, and at s=1 it degenerates to the Heisenberg structure. In between, it gives Riemannian structures on \mathbb R^3 with properties that degenerate as s goes to 1.

As with any Riemannian structure, geodesics through a given point with assigned direction exist and are unique. They can be found by solving the geodesic equation

\nabla_{\gamma\prime} \gamma\prime = 0

for the Levi-Civita connection corresponding to the orthonormal frame field. Given a curve \gamma = (x,y,z) and some calculations, the condition on \gamma becomes:

(1-s)^2 x\prime\prime + s y\prime ( z\prime + \frac{s}{2}( x\prime y - y\prime x) )=0 

(1-s)^2 y\prime \prime - s x\prime ( z\prime + \frac{s}{2}( x\prime y - y\prime x) )=0

 ( z\prime + \frac{s}{2}( x\prime y - y\prime x) )\prime =0

These equations are easily solved. The following animations show, as s changes, geodesics leaving the origin with fixed initial velocity. The length of the geodesics changes with s since otherwise they quickly become too small to see.

Last Updated ( Friday, 22 May 2009 11:36 )

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The Heisenberg 3-Sphere

Math - Heisenberg09

S^3 has a Lie group structure as a subset of the quaternions. Given a point p \in S^3, a choice of a two-dimensional subspace of T_p S^3 can be extended to a 2-dimensional distribution on the entire manifold. With an appropriate choice of stereographic projection, this corresponds to the sub-Riemannian distribution on the Heisenberg group. The restriction of the Euclidean inner product to T_pS^3 also extends to the other points, giving a sub-Riemannian structure and Carnot-Caratheodory (CC) metric on S^3.

As with the Heisenberg group, one might consider the metric properties of this space. What are the geodesics? Are they unique? What do the spheres look like?

The geodesics, it turns out come in two flavors: homeomorphic to \mathbb R and S^1. As with the Heisenberg group, there is a curvature \lambda to a geodesic, and if \frac{\lambda}{1-\lambda} is irrational, the geodesic is dense in a Clifford torus (see post on the Hopf Fibration):

 

Last Updated ( Thursday, 14 May 2009 20:14 )

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Mathematica Notebook: Horisontal, Hopf, Lens

Math - Heisenberg09
The images and animations in the previous four posts were made using Mathematica. Here is the notebook Horisontal Curves, Hopf Fibration, and Lens Spaces that contains commands for producing most of the images and animations I posted. Feel free to contact me with any questions or comments you have about it.

Last Updated ( Wednesday, 13 May 2009 11:13 )

Lens Space

Math - Heisenberg09

The Lens space L(p,q) is the quotient of S^3 by an action of \mathbb{Z}_p. The group acts on \mathbb{C}^2 by the p^{th} root of unity in the first coordinate and the q^{th} power of that in the second coordinate, and the action restricts to S^3. So why a "Lens" space, and how does one visualize it?

 I drew L(5,2) by drawing a lattice in S^3 invariant under the group action. Here's the picture (after stereographic projection):

Last Updated ( Tuesday, 12 May 2009 11:45 )

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Steak Herb Rub

Food - Grill

Ingredients:

2 Tbsp chopped fresh basil or 2 tsp dried
2 tsp chopped fresh thyme or 1 tsp dried
1 Tbsp chopped fresh rosemary or 2 tsp dried
1 Tbsp chopped fresh oregano or 2 tsp dried
1 Tbsp crushed fennel seeds
1 tsp ground coriander
2 tsp garlic powder or granulated garlic
2 Tbsp salt
2 tsp coarsely ground black pepper

found here

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