Download Variations on a Theme by Kepler by Victor W. Guillemin and Shlomo Sternberg PDF

By Victor W. Guillemin and Shlomo Sternberg

This publication is predicated at the Colloquium Lectures offered via Shlomo Sternberg in 1990. The authors delve into the mysterious position that teams, specifically Lie teams, play in revealing the legislation of nature through concentrating on the standard instance of Kepler movement: the movement of a planet lower than the appeal of the solar in line with Kepler's legislation. Newton discovered that Kepler's moment law--that equivalent components are swept out in equivalent times--has to do with the truth that the strength is directed radially to the solar. Kepler's moment legislations is de facto the statement of the conservation of angular momentum, reflecting the rotational symmetry of the approach in regards to the foundation of the strength. In latest language, we'd say that the crowd $O(3)$ (the orthogonal crew in 3 dimensions) is liable for Kepler's moment legislation. via the top of the 19th century, the inverse sq. legislations of allure was once visible to have $O(4)$ symmetry (where $O(4)$ acts on a section of the six-dimensional part area of the planet). Even greater teams have on account that been chanced on to be interested by Kepler movement. In quantum mechanics, the instance of Kepler movement manifests itself because the hydrogen atom. Exploring this circle of rules, the 1st a part of the e-book was once written with the final mathematical reader in brain. the rest of the ebook is geared toward experts. It starts off with an indication that the Kepler challenge and the hydrogen atom show $O(4)$ symmetry and that the shape of this symmetry determines the inverse sq. legislation in classical mechanics and the spectrum of the hydrogen atom in quantum mechanics. the gap of regularized elliptical motions of the Kepler challenge (also often called the Kepler manifold) performs a crucial position during this e-book. The final component to the booklet reviews some of the cosmological versions during this related conformal classification (and having various isometry teams) from the perspective of projective geometry. The computation of the hydrogen spectrum presents a demonstration of the main that enlarging the section house can simplify the equations of movement within the classical atmosphere and reduction within the quantization challenge within the quantum atmosphere. The authors offer a brief precis of the homological quantization of constraints and an inventory of contemporary purposes to many fascinating finite-dimensional settings. The publication closes with an summary of Kostant's conception, within which a unitary illustration is linked to the minimum nilpotent orbit of $SO(4,4)$ and during which electromagnetism and gravitation are unified in a Kaluza-Klein-type thought in six dimensions.

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The null geodesics for this metric on Sl x S3 are clearly the product of Sl with a great circle of S3 . A cross section in 'Y to the forward null geodesics is clearly given by e = O. The restriction of the symplectic form of T* M to this cross section is exactly the symplectic form of T* S (under the identification of this cross section with T+ S by projection). This proves that ~ is symplectically equivalent to T+ S . 9. The groups SO(2, 4) and SU(2, 2) We have already mentioned that the space M can be regarded as the conformal completion of Minkowski space, and the group SO(2, 4) acts as a double cover of the group of all conformal transformations of M.

They give the geodesic flow with unit velocity for the sphere, but described in the stereographically projected coordinates. Now comes the crucial step. Observe that on the region where II~II =f. 0 we have 1 II~II-l J = H + 1 where IIwl12 H(w,~) = -2- - mr 1 which is our old Kepler Hamiltonian except that the position and momentum variables have been interchanged. ) So we must understand the effect on the vector fields of the replacement f(w, ~) = II~II. On the hypersurface H = - 1' which corresponds to dJ = fd(H J = 0, we clearly have + 1) so ~J = f~lI' Multiplying a vector field ~ by a function f can be thought of as replacing the independent variable t by the independent variable s related to t by dtjds = f.

So the stereographic projection is a diffeomorphism of S N with Rn and hence induces a diffeomorphism of T* S N with T* R n which carries the canonical one-form fJ:<; = ,. dz of T* S onto the canonical one-form fJRn = ~ . dw of T*Rn. In this last expression for fJ R" we have identified T*Rn with R n ffi R n so ~ E Rn. In the expression for fJ s we are regarding T* S as the submanifold of T*Rn+l = Rn+ 1 ffi Rn+ 1 consisting of all pairs (z, 0 satisfying IIzl12 = 1 and ,. z = O. Thus fJs is the restriction to T* S of the canonical one-form of T* R n+ 1 .

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