Interpolating Between Hyperbolic and Sol Geometry

A smooth one-parameter family connecting two Thurston geometries.

This short note gives a metric on R3\mathbb{R}^3 which in some sense interpolates between 3-dimensional hyperbolic space and Sol geometry.

Hyperbolic Metric: Upper Half Space

Let H={(x,y,z)R3z>0}\mathcal{H}=\{(x,y,z)\in\mathbb{R}^3\mid z>0\} be the upper half space of R3\mathbb{R}^3, and the metric

g=dx2+dy2+dz2z2g =\frac{dx^2+dy^2+dz^2}{z^2}

Sol Metric

Sol geometry is given by the space R3\RR^3 together with the metric g=e2zdx2+e2zdy2+dz2g= e^{-2z}dx^2+e^{2z}dy^2+dz^2

The Log Model of the Hyperoblic Plane

The first step is to build a new model of the hyperbolic plane on all of R3\RR^3, by taking the logarithm of the zz coordinate. Precisely, let L,EL,E be the pair of homeomorphisms HR3\mathcal{H}\leftrightarrow \RR^3 given by L(x,y,z)=(x,y,logz)L(x,y,z)=(x,y,\log z), E(x,y,z)=(x,y,ez)E(x,y,z)=(x,y,e^z). We have the hyperbolic metric written on H\mathcal{H}, so we can use EE to pull it back to R3\RR^3.

PICTURE

To make the calculation clear, we will temporarily use X,Y,ZX,Y,Z as the coordinates on H\mathcal{H} and x,y,zx,y,z the coordinates on R3\RR^3. The metric on R3\RR^3 is determined by all the pairwise dot-products of the coordinate basis fields x,y,z\partial_x,\partial_y,\partial_z, which can be computed via pullback after understanding the action of EE at a point (x,y,z)(x,y,z):

Ex=XEy=YEz=ezZE_\ast \partial_x = \partial_X\hspace{1cm}E_\ast \partial_y =\partial_Y\hspace{1cm}E_\ast\partial_z=e^z\partial_Z

For mixed dot products, note that EE does not change the angles between basis directions so x,y,z\partial_x,\partial_y,\partial_z are pairwise orthogonal under pullback just as X,Y,Z\partial_X,\partial_Y,\partial_Z are on H\mathcal{H}. This leaves only the diagonal terms to compute:

x,x(x,y,z)=Ex,ExE(x,y,z)=X,X(x,y,ez)=1(ez)2(XX)=1e2z\begin{align} \langle \partial_x,\partial_x\rangle_{(x,y,z)}&=\langle E_\ast \partial_x,E_\ast \partial_x\rangle_{E(x,y,z)}\\ &= \langle \partial_X,\partial_X\rangle_{(x,y,e^z)}\\ &=\frac{1}{(e^z)^2}\left(\partial_X\cdot\partial_X\right)\\ &=\frac{1}{e^{2z}} \end{align}

Where in the last line we used the metric on H\mathcal{H} is the Euclidean metric divided by the square of the zz coordinate. The same reasoning holds for y,y\langle \partial_y,\partial_y\rangle giving an identical answer. This leaves only the zz component:

z,z(x,y,z)=Ez,EzE(x,y,z)=ezZ,ezz(x,y,ez)=1(ez)2(ezZezz)=(ez)2(ez)2(ZZ)=1\begin{align} \langle \partial_z,\partial_z\rangle_{(x,y,z)}&=\langle E_\ast \partial_z,E_\ast \partial_z\rangle_{E(x,y,z)}\\ &= \langle e^z\partial_Z,e^z\partial_z\rangle_{(x,y,e^z)}\\ &=\frac{1}{(e^z)^2} \left(e^z\partial_Z\cdot e^z\partial_z\right)\\ &=\frac{(e^z)^2}{(e^z)^2}(\partial_Z\cdot \partial_Z)\\ &= 1 \end{align}

Thus the metric tensor in coordinates (x,y,z)(x,y,z) on R3\RR^3 is

g=e2zdx2+e2zdy2+dz2g = e^{-2z}dx^2+e^{-2z}dy^2+dz^2

This metric has the factors in front of the zz coordinate exponentially decreasing as zz increases: it will be more convenient to ‘flip’ this behavior, and pull back the metric once more under the reflection (x,y,z)(x,y,z)(x,y,z)\mapsto(x,y,-z). The result is simply to flip the sign of the exponents:

Log-Hyperbolic Model

The log model of hyperbolic space is given by R3\RR^3 together with the metric g=e2zdx2+e2zdy2+dz2g = e^{2z}dx^2+e^{2z}dy^2+dz^2

The Interopolating Metric

The log-hyperbolic model looks very similar to Sol geometry: they have the same coordinate domain and the metric form is identical save a crucial difference: in H3\mathbb{H}^3 the sign of the exponentials is both the same, and in Sol the exponential factors prefixing the xx and yy coordinate directions are opposite. A natural idea is to change the prefactor on dx2dx^2 to a different function of zz,

g=f(z)dx2+e2zdy2+dz2g= f(z)dx^2+e^{2z}dy^2+dz^2

Where f(z)e2zf(z)\approx e^{2z} for z>>0z>>0 and f(z)e2zf(z)\approx e^{-2z} for z<<0z << 0. This would produce a geometry which looks much like H3\mathbb{H}^3 for z>>0z>>0 and much like Sol for z<<0z << 0. The obvious choice of such a function is some sort of hyperbolic cosine, as this is built directly from these two exponentials. Writing things down explicitly, one sees that 2cosh(2z)2\cosh(2z) is the correct form:

g=2cosh(2z)dx2+e2zdy2+dz2=(e2z+e2z)dx2+e2zdy2+dz2\begin{align} g &= 2\cosh(2z) dx^2+e^{2z}dy^2+dz^2\\ &= \left(e^{2z}+e^{-2z}\right)dx^2+e^{2z}dy^2+dz^2 \end{align}

More work needs to be done to understand this geometry: in particular, it remains to be quantified exactly how similar the geometries on each side of z=0z=0 approach hyperbolic and sol.

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