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Introduction to Teichmüller theory, old and new, II

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<strong>Introduction</strong> <strong>to</strong> <strong>Teichmüller</strong> <strong>theory</strong>, <strong>old</strong> <strong>and</strong> <strong>new</strong>, <strong>II</strong> 27<br />

In what follows, “projective” means “complex projective”.<br />

Since the projective transformations of the sphere are holomorphic, a projective<br />

structure on a surface has an underlying conformal structure. In other words, there is a<br />

forgetful map π : P (S) → T (S) from the space of marked projective structures on S<br />

<strong>to</strong> the <strong>Teichmüller</strong> space T (S) of S. This map makes the space P (S) a fiber bundle<br />

over <strong>Teichmüller</strong> space.<br />

As it is the case for hyperbolic structures, projective structures, through their holonomy<br />

representation, can be studied in the context of the representation <strong>theory</strong> of the<br />

fundamental group of the surface S in the group PSL(2, C). There is a complex structure<br />

on the space P (S), <strong>and</strong> from works of Hejhal, Earle <strong>and</strong> Hubbard, it follows that<br />

the holonomy map from the space P (S) <strong>to</strong> the character variety of representations<br />

of π1(S) in PSL(2, C) is a local biholomorphism. Chapter 12 contains a review of<br />

basic properties of holonomy maps of projective structure, as well as a discussion of<br />

other issues of representation <strong>theory</strong> (discreteness, degeneration, etc.) that have been<br />

studied in depth by various authors, in particular by D. Dumas.<br />

There are several ways of parameterizing projective structures on surfaces, <strong>and</strong> one<br />

classical way uses Schwarzian derivatives. The Schwarzian derivative is a differential<br />

opera<strong>to</strong>r which is invariant under Möbius transformations. It was already studied in<br />

the nineteenth century, in relation with the Schwarzian differential equation w ′′ (z) +<br />

1<br />

2<br />

q(z)w(z) = 0, where z varies in a domain of the Riemann sphere <strong>and</strong> where q is a<br />

holomorphic function.<br />

We recall that the Schwarzian derivative of a Möbius transformation is zero, <strong>and</strong><br />

that, in some sense, the Schwarzian derivative of a conformal map is a measure of how<br />

far this map is from being a Möbius transformation. The Schwarzian derivative can<br />

also be considered as a measure of the difference between two projective structures.<br />

There is an intimate relationship between Schwarzian derivatives <strong>and</strong> quadratic<br />

differentials, the latter being certainly more familiar <strong>to</strong> <strong>Teichmüller</strong> theorists. The<br />

Schwarzian derivative Sf of a holomorphic function f of one complex variable is<br />

defined by the formula<br />

(Sf )(z) = f ′′′ (z)<br />

f ′ (z)<br />

<br />

3 f ′′ (z)<br />

−<br />

2 f ′ 2 (z)<br />

(the formula is not important for what follows). A quadratic differential appears<br />

from a projective structure on a surface by taking the Schwarzian derivative of a<br />

developing map of that structure. Using this fact, Schwarzian derivatives establish<br />

a correspondence between projective structures on a given surface with the space<br />

of holomorphic quadratic differentials on that surface. In this correspondence, each<br />

fiber π −1 (X) of the map π : P (S) → T (S) over a point X in T (S) is identified<br />

with the vec<strong>to</strong>r space of holomorphic quadratic differentials on a Riemann surface<br />

representing X. Since the vec<strong>to</strong>r space of holomorphic quadratic differentials over a<br />

surface is also the cotangent space <strong>to</strong> <strong>Teichmüller</strong> space at the corresponding point, the<br />

<strong>theory</strong> of the Schwarzian derivative makes an identification between the space P (S)<br />

<strong>and</strong> the cotangent bundle T ∗ T (S) of <strong>Teichmüller</strong> space.

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