Can you describe the metric on the space of positive definite quadratic forms?

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SUMMARY

The metric on the space of positive definite quadratic forms on R2 is represented as GL(2, R)/O(2), which is equivalent to H x R+, where H denotes the hyperbolic plane. The left-invariant metric on GL(2, R) is defined as ds2 = (1/2) Tr[(M-1 dM)(M-1 dM)T], leading to the expression ds2 = (dr/r)2 + (1/y2)(dx2 + dy2). This formulation is consistent with the decomposition of GL(n, R) matrices and highlights the relationship between the determinant of matrices and the structure of the space.

PREREQUISITES
  • Understanding of GL(2, R) and O(2) groups
  • Familiarity with hyperbolic geometry and the Poincaré disk model
  • Knowledge of differential geometry concepts, particularly metrics
  • Basic understanding of quadratic forms and their properties
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  • Study the properties of the Poincaré disk model in hyperbolic geometry
  • Explore the implications of the Maurer-Cartan form in Lie group theory
  • Investigate the relationship between positive definite quadratic forms and their geometric representations
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Mathematicians, particularly those specializing in differential geometry, algebraic geometry, and Lie group theory, will benefit from this discussion. It is also relevant for researchers exploring the geometric properties of quadratic forms and their applications in theoretical physics.

lavinia
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I am told that the set of positive definite quadratic forms on R^2 has a metric that turns it into

H x R where H is the hyperbolic plane. Can you describe this metric?

* As a space the forms are viewed as GL(2,R)/O(2).
 
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Let's note that there's a Gauss-type decomposition of GL(n,\mathbb{R}) matrices as

\mathcal{M} = U D \mathcal{O},

where U is upper-triangular (with 1s on the diagonal), D is diagonal (with \det{D}>0) and \mathcal{O} is orthogonal (in O(n)). I claim that

M = \begin{pmatrix} 1 & \sqrt{2} x \\ 0 & 1 \end{pmatrix} \begin{pmatrix} r y & 0\\ 0 & r/y \end{pmatrix},

is the general element of the coset GL(2,\mathbb{R})/O(2) provided that r,y>0.

We can place the usual left-invariant metric on GL(2,\mathbb{R}), which will induce the metric

ds^2 = \frac{1}{2} \text{Tr} \left[ (M^{-1} dM) (M^{-1} dM) ^T\right],

= \left( \frac{dr}{r}\right)^2 + \frac{1}{y^2} \left( dx^2 + dy^2 \right)

on the coset. The space is therefore GL(2,\mathbb{R})/O(2) = H \times \mathbb{R}^+. Note that this is consistent with H = SL(2,\mathbb{R})/SO(2) and \mathbb{R}^+ = \mathbb{R}/\{ 1,-1\}.
 
fzero said:
Let's note that there's a Gauss-type decomposition of GL(n,\mathbb{R}) matrices as

\mathcal{M} = U D \mathcal{O},

where U is upper-triangular (with 1s on the diagonal), D is diagonal (with \det{D}>0) and \mathcal{O} is orthogonal (in O(n)). I claim that

M = \begin{pmatrix} 1 & \sqrt{2} x \\ 0 & 1 \end{pmatrix} \begin{pmatrix} r y & 0\\ 0 & r/y \end{pmatrix},

is the general element of the coset GL(2,\mathbb{R})/O(2) provided that r,y>0.

We can place the usual left-invariant metric on GL(2,\mathbb{R}), which will induce the metric

ds^2 = \frac{1}{2} \text{Tr} \left[ (M^{-1} dM) (M^{-1} dM) ^T\right],

= \left( \frac{dr}{r}\right)^2 + \frac{1}{y^2} \left( dx^2 + dy^2 \right)

on the coset. The space is therefore GL(2,\mathbb{R})/O(2) = H \times \mathbb{R}^+. Note that this is consistent with H = SL(2,\mathbb{R})/SO(2) and \mathbb{R}^+ = \mathbb{R}/\{ 1,-1\}.

what is the usual left invariant metric on GL(2,\mathbb{R})?
 
lavinia said:
what is the usual left invariant metric on GL(2,\mathbb{R})?

It's

<br /> ds^2 = \frac{1}{2} \text{Tr} \left[ (\mathcal{M}^{-1} d\mathcal{M}) (\mathcal{M}^{-1} d\mathcal{M}) ^T\right].<br />

The normalization is put in for convenience. \mathcal{M}^{-1} d\mathcal{M} is the Maurer-Cartan form.
 
fzero said:
It's

<br /> ds^2 = \frac{1}{2} \text{Tr} \left[ (\mathcal{M}^{-1} d\mathcal{M}) (\mathcal{M}^{-1} d\mathcal{M}) ^T\right].<br />

The normalization is put in for convenience. \mathcal{M}^{-1} d\mathcal{M} is the Maurer-Cartan form.

Thanks. I will do some reading about this.

Do you have a simple geometric picture of this metric? Start with an ellipse centered at the origin of R^2. Map it onto the Poincare disk somehow. Then maybe the factor of R comes from uniformly scaling the ellipses.
 
Last edited:
lavinia said:
Thanks. I will do some reading about this.

Do you have a simple geometric picture of this metric? Start with an ellipse centered at the origin of R^2, map it onto the Poincare disk somehow. Then maybe the factor of R comes from uniformly scaling the ellipses.

The factor of \mathbb{R}^+ corresponds to the determinant of a matrix in the component GL(n,\mathbb{R})^+ connected to the identity. The metric we found is consistent with the well known fact that GL(n,\mathbb{R})^+=SL(n,\mathbb{R})\times \mathbb{R}^+.
 
fzero said:
The factor of \mathbb{R}^+ corresponds to the determinant of a matrix in the component GL(n,\mathbb{R})^+ connected to the identity. The metric we found is consistent with the well known fact that GL(n,\mathbb{R})^+=SL(n,\mathbb{R})\times \mathbb{R}^+.

Ok. This is helpful.

Does this picture work?

Each positive definite quadratic form determines an ellipse, its ellipse of unit vectors.

An ellipse has three parameters, the lengths of its two axes and its angle of tilt to the xy-coordinate axes.
The subset that are rotations of ellipses with tilt angle zero and fixed x-axis length, (They are rotations of ellipses with equation, x^2 + y^2/b^2 = K) form a two parameter family.
(By convention, angles of rotation can be chosen to be between 0 and pi (the interval, [0,pi), and the first axis can be chosen to be the one that lines up with the x-axis when the rotation is undone. )

For each ellipse in this 2 parameter family, map it to the point in the Poincare disk whose angle is twice the tilt angle and whose Euclidean distance to the origin is |k1 - k2|/k1 + k2 where k1 and k2 are the lengths of its axes.

This two parameter family looks like the Poincare disk under this mapping. As the x-axis length is varied to account for all positive definite quadratic forms, the entire set looks like the Cartesian product of the Poincare disk with the open half line of positive real numbers.

Is this the correct picture?

What is the importance of this metric for understanding the space of positive definite quadratic forms?
 
Last edited:
I would identify your K with \mathbb{R}^+ in the coset, then the ratio of axis lengths b and tilt angle form the UHP. I think you're still mapping the ratio and tilt angle to the Poincare disk, so you might find that the metric on your space is in the same conformal class as the one on the UHP.

As far as the importance of the metric, I have no specific applications in mind for doing geometry on the space of positive definite quadratic forms. That is not to say that there aren't any. I just happened to be aware of some Lie group geometry that could shed some light on your original question.
 

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