Download A Comprehensive Introduction to Differential Geometry by Michael Spivak PDF

By Michael Spivak

Booklet by way of Michael Spivak, Spivak, Michael

Show description

Read Online or Download A Comprehensive Introduction to Differential Geometry PDF

Similar differential geometry books

A Comprehensive Introduction to Differential Geometry

Ebook by way of Michael Spivak, Spivak, Michael

Differential Geometry in the Large: Seminar Lectures New York University 1946 and Stanford University 1956

Those notes include components: chosen in York 1) Geometry, New 1946, issues college Notes Peter Lax. through Differential within the 2) Lectures on Stanford Geometry huge, 1956, Notes J. W. college by means of grey. are the following without crucial They reproduced switch. Heinz was once a mathematician who mathema- Hopf famous vital tical principles and new mathematical instances.

Extra info for A Comprehensive Introduction to Differential Geometry

Sample text

Then ∇X Y = (XY k + X i Y j Γkij )Ek . Proof. Just use the defining rules for a connection and compute: ∇X Y = ∇X (Y j Ej ) = (XY j )Ej + Y j ∇X i Ei Ej = (XY j )Ej + X i Y j ∇Ei Ej = XY j Ej + X i Y j Γkij Ek . 3). 3) 52 4. Connections Existence of Connections So far, we have studied properties of connections, but have not produced any, so you might be wondering if they are plentiful or rare. In fact, they are quite plentiful, as we will show shortly. Let’s begin with a trivial example: on Rn , define the Euclidean connection by ∇X Y j ∂j = (XY j )∂j .

2). More generally, if V is any n-dimensional vector space endowed with an inner product, we can set g(X, Y ) = X, Y for any X, Y ∈ Tp V = V . Choosing an orthonormal basis (E1 , . . , En ) for V defines a map from Rn to V by sending (x1 , . . , xn ) to xi Ei ; this is easily seen to be an isometry of (V, g) with (Rn , g¯). Spheres Our second model space is the sphere of radius R in Rn+1 , denoted SnR , ◦ with the metric g R induced from the Euclidean metric on Rn+1 , which we call the round metric of radius R.

We can immediately write down a large group of isometries of SnR by observing that the linear action of the orthogonal group O(n + 1) on Rn+1 preserves SnR and the Euclidean metric, so its restriction to SnR acts by isometries of the sphere. 3. O(n + 1) acts transitively on orthonormal bases on SnR . More precisely, given any two points p, p˜ ∈ SnR , and orthonormal bases {Ei } 34 3. 2. Transitivity of O(n + 1) on orthonormal bases. ˜i } for Tp˜Sn , there exists ϕ ∈ O(n + 1) such that ϕ(p) = p˜ for Tp SnR and {E R ˜ and ϕ∗ Ei = Ei .

Download PDF sample

Rated 4.05 of 5 – based on 15 votes