Talk:PlanetPhysics/Functorial Algebraic Geometry

Original TeX Content from PlanetPhysics Archive

edit
%%% This file is part of PlanetPhysics snapshot of 2011-09-01
%%% Primary Title: Functorial Algebraic Geometry and Physics
%%% Primary Category Code: 00.
%%% Filename: FunctorialAlgebraicGeometry.tex
%%% Version: 26
%%% Owner: bci1
%%% Author(s): bci1
%%% PlanetPhysics is released under the GNU Free Documentation License.
%%% You should have received a file called fdl.txt along with this file.        
%%% If not, please write to gnu@gnu.org.
\documentclass[12pt]{article}
\pagestyle{empty}
\setlength{\paperwidth}{8.5in}
\setlength{\paperheight}{11in}

\setlength{\topmargin}{0.00in}
\setlength{\headsep}{0.00in}
\setlength{\headheight}{0.00in}
\setlength{\evensidemargin}{0.00in}
\setlength{\oddsidemargin}{0.00in}
\setlength{\textwidth}{6.5in}
\setlength{\textheight}{9.00in}
\setlength{\voffset}{0.00in}
\setlength{\hoffset}{0.00in}
\setlength{\marginparwidth}{0.00in}
\setlength{\marginparsep}{0.00in}
\setlength{\parindent}{0.00in}
\setlength{\parskip}{0.15in}

\usepackage{html}

% this is the default PlanetPhysics preamble. as your 

\usepackage{amsmath, amssymb, amsfonts, amsthm, amscd, latexsym, enumerate}
\usepackage{xypic, xspace}
\usepackage[mathscr]{eucal}
\usepackage[dvips]{graphicx}
\usepackage[curve]{xy}

% define commands here
\theoremstyle{plain}
\newtheorem{lemma}{Lemma}[section]
\newtheorem{proposition}{Proposition}[section]
\newtheorem{theorem}{Theorem}[section]
\newtheorem{corollary}{Corollary}[section]
\theoremstyle{definition}
\newtheorem{definition}{Definition}[section]
\newtheorem{example}{Example}[section]
%\theoremstyle{remark}
\newtheorem{remark}{Remark}[section]
\newtheorem*{notation}{Notation}
\newtheorem*{claim}{Claim}
\renewcommand{\thefootnote}{\ensuremath{\fnsymbol{footnote}}}
\numberwithin{equation}{section}
\newcommand{\Ad}{{\rm Ad}}
\newcommand{\Aut}{{\rm Aut}}
\newcommand{\Cl}{{\rm Cl}}
\newcommand{\Co}{{\rm Co}}
\newcommand{\DES}{{\rm DES}}
\newcommand{\Diff}{{\rm Diff}}
\newcommand{\Dom}{{\rm Dom}}
\newcommand{\Hol}{{\rm Hol}}
\newcommand{\Mon}{{\rm Mon}}
\newcommand{\Hom}{{\rm Hom}}
\newcommand{\Ker}{{\rm Ker}}
\newcommand{\Ind}{{\rm Ind}}
\newcommand{\IM}{{\rm Im}}
\newcommand{\Is}{{\rm Is}}
\newcommand{\ID}{{\rm id}}
\newcommand{\grpL}{{\rm GL}}
\newcommand{\Iso}{{\rm Iso}}
\newcommand{\rO}{{\rm O}}
\newcommand{\Sem}{{\rm Sem}}
\newcommand{\SL}{{\rm Sl}}
\newcommand{\St}{{\rm St}}
\newcommand{\Sym}{{\rm Sym}}
\newcommand{\Symb}{{\rm Symb}}
\newcommand{\SU}{{\rm SU}}
\newcommand{\Tor}{{\rm Tor}}
\newcommand{\U}{{\rm U}}
\newcommand{\A}{\mathcal A}
\newcommand{\Ce}{\mathcal C}
\newcommand{\D}{\mathcal D}
\newcommand{\E}{\mathcal E}
\newcommand{\F}{\mathcal F}
%\newcommand{\grp}{\mathcal G}
\renewcommand{\H}{\mathcal H}
\renewcommand{\cL}{\mathcal L}
\newcommand{\Q}{\mathcal Q}
\newcommand{\R}{\mathcal R}
\newcommand{\cS}{\mathcal S}
\newcommand{\cU}{\mathcal U}
\newcommand{\W}{\mathcal W}
\newcommand{\bA}{\mathbb{A}}
\newcommand{\bB}{\mathbb{B}}
\newcommand{\bC}{\mathbb{C}}
\newcommand{\bD}{\mathbb{D}}
\newcommand{\bE}{\mathbb{E}}
\newcommand{\bF}{\mathbb{F}}
\newcommand{\bG}{\mathbb{G}}
\newcommand{\bK}{\mathbb{K}}
\newcommand{\bM}{\mathbb{M}}
\newcommand{\bN}{\mathbb{N}}
\newcommand{\bO}{\mathbb{O}}
\newcommand{\bP}{\mathbb{P}}
\newcommand{\bR}{\mathbb{R}}
\newcommand{\bV}{\mathbb{V}}
\newcommand{\bZ}{\mathbb{Z}}
\newcommand{\bfE}{\mathbf{E}}
\newcommand{\bfX}{\mathbf{X}}
\newcommand{\bfY}{\mathbf{Y}}
\newcommand{\bfZ}{\mathbf{Z}}
\renewcommand{\O}{\Omega}
\renewcommand{\o}{\omega}
\newcommand{\vp}{\varphi}
\newcommand{\vep}{\varepsilon}
\newcommand{\diag}{{\rm diag}}
\newcommand{\grp}{{\mathsf{G}}}
\newcommand{\dgrp}{{\mathsf{D}}}
\newcommand{\desp}{{\mathsf{D}^{\rm{es}}}}
\newcommand{\grpeod}{{\rm Geod}}
%\newcommand{\grpeod}{{\rm geod}}
\newcommand{\hgr}{{\mathsf{H}}}
\newcommand{\mgr}{{\mathsf{M}}}
\newcommand{\ob}{{\rm Ob}}
\newcommand{\obg}{{\rm Ob(\mathsf{G)}}}
\newcommand{\obgp}{{\rm Ob(\mathsf{G}')}}
\newcommand{\obh}{{\rm Ob(\mathsf{H})}}
\newcommand{\Osmooth}{{\Omega^{\infty}(X,*)}}
\newcommand{\grphomotop}{{\rho_2^{\square}}}
\newcommand{\grpcalp}{{\mathsf{G}(\mathcal P)}}
\newcommand{\rf}{{R_{\mathcal F}}}
\newcommand{\grplob}{{\rm glob}}
\newcommand{\loc}{{\rm loc}}
\newcommand{\TOP}{{\rm TOP}}
\newcommand{\wti}{\widetilde}
\newcommand{\what}{\widehat}
\renewcommand{\a}{\alpha}
\newcommand{\be}{\beta}
\newcommand{\grpa}{\grpamma}
%\newcommand{\grpa}{\grpamma}
\newcommand{\de}{\delta}
\newcommand{\del}{\partial}
\newcommand{\ka}{\kappa}
\newcommand{\si}{\sigma}
\newcommand{\ta}{\tau}
\newcommand{\lra}{{\longrightarrow}}
\newcommand{\ra}{{\rightarrow}}
\newcommand{\rat}{{\rightarrowtail}}
\newcommand{\ovset}[1]{\overset {#1}{\ra}}
\newcommand{\ovsetl}[1]{\overset {#1}{\lra}}
\newcommand{\hr}{{\hookrightarrow}}
\newcommand{\<}{{\langle}}
%\newcommand{\>}{{\rangle}}
%\usepackage{geometry, amsmath,amssymb,latexsym,enumerate}
%\usepackage{xypic}
\def\baselinestretch{1.1}
\hyphenation{prod-ucts}
%\grpeometry{textwidth= 16 cm, textheight=21 cm}
\newcommand{\sqdiagram}[9]{$$ \diagram #1 \rto^{#2} \dto_{#4}&
#3 \dto^{#5} \\ #6 \rto_{#7} & #8 \enddiagram
\eqno{\mbox{#9}}$$ }

\def\C{C^{\ast}}

\newcommand{\labto}[1]{\stackrel{#1}{\longrightarrow}}

%\newenvironment{proof}{\noindent {\bf Proof} }{ \hfill $\Box$
%{\mbox{}}

\newcommand{\quadr}[4]
{\begin{pmatrix} & #1& \\[-1.1ex] #2 & & #3\\[-1.1ex]& #4&
\end{pmatrix}}
\def\D{\mathsf{D}}

\begin{document}

 The following is a contributed topic on functorial algebraic geometry and physics:

\htmladdnormallink{``Functorial Algebraic Geometry: An Introduction'' -by Alexander Grothendieck}{http://www.math.jussieu.fr/~leila/grothendieckcircle/FuncAlg.pdf}

\subsubsection{Vol.1: Affine Algebraic Geometry}

(Following the Notes typewritten in English and edited by P. Gaeta,
without implying the approval by A. Grothendieck of these notes.)

A century ago \htmladdnormallink{algebraic}{http://planetphysics.us/encyclopedia/CoIntersections.html} Geometry could be contained in Klein's book (1880; Dover publs. 1963) : ``On Riemann's theory of Algebraic Functions and Their Integrals''. Furthermore, ``{\em the distinction between pure and applied mathematics was then to a large extent artificial and unimportant}'' (viz. P. Gaeta). For example in Klein's book cited above ``the study of Riemann surfaces was introduced by considering the practical physical problem of laminar flow in a plane or arbitrary surface. He even quotes Maxwell's treatise on page one.
The natural continuation of such a `transcedental approach' in our times is the study of {\em complex algebraic manifolds}...''
In contrast with Algebraic Geometry, the popular beliefs regarding \htmladdnormallink{Differential Geometry}{http://planetphysics.us/encyclopedia/DifferentialGeometry.html} are totally different: the latter never lost its \htmladdnormallink{flavor}{http://planetphysics.us/encyclopedia/QuarkAntiquarkPair.html} of applicability; such practical examples of differentiable \htmladdnormallink{manifolds}{http://planetphysics.us/encyclopedia/NoncommutativeGeometry4.html} are natural examples of {\em locally ringed spaces}. ``Thus, if a reader is familiar with differentiable manifolds, Grothendieck's {\em schemes} cannot look so terribly abstract...; we do not assume knowledge of differentiable manifolds as a
logical pre-requisite for this course, but a student interested in applications
should be interested in differentiable manifolds. The purpose of this informal Introduction is to develop an analogy between these new mathematical objects
introduced by Grothendieck (that is, in Algebraic Geometry) and certain objects within the structure of Mathematical Physics...'' Consider the `configuration space' $V_n$ or the `phase space' $W_{2n}$ of a holonomic \htmladdnormallink{dynamical system}{http://planetphysics.us/encyclopedia/ContinuousGroupoidHomomorphism.html} `with
n-degrees of freedom'; for any problems concerning $V_n$ one should only consider local \htmladdnormallink{functions}{http://planetphysics.us/encyclopedia/Bijective.html} $ f: U \to R$ defined within an open set
$U \subset V_n$. As an example, a \htmladdnormallink{Lagrangian}{http://planetphysics.us/encyclopedia/LagrangesEquations.html} coordinate function $ q_i$
(with $i= 1,2,..., n$) is only defined locally for a certain coordinate chart.
The \htmladdnormallink{Lagrange equations}{http://planetphysics.us/encyclopedia/LagrangesEquations.html} of \htmladdnormallink{motion}{http://planetphysics.us/encyclopedia/CosmologicalConstant2.html}:

\begin{equation}
\frac{d}{dt} \left ( \frac{\partial L}{\partial \dot{q_i}} \right ) - \frac{\partial L}{\partial q_i} = 0
\end{equation}

are valid only in a certain local coordinate system $(q_1, ..., q_n)$. In order to examine the behavior of the \htmladdnormallink{dynamic system}{http://planetphysics.us/encyclopedia/GenericityInOpenSystems.html} globally one must piece together local functions corresponding to different sets $U$, and this is achieved by verifying first that the set of functions $[f: U \to \mathbb{R}| U \subset V_n]$ form a {\em commutative ring with unit} $\Gamma (U)$ under pointwise addition and multiplication for such $U$. If $ V \subset U$, then there is a natural {\em restriction map} $r^U_V : \Gamma(U) \to \Gamma(V)$ which assigns to every
$\phi: U \to \mathbb{R}$ its restriction map with respect to $V$, that is,
$r^U_V = \phi|V : V \to \mathbb{R}$. This also means--in other words--that the local $C^{\infty}$- differentiable functions on $U$ form , or define, a
`{\em presheaf}' (viz. Ch.III).

Next one must consider the ``{\em germ}'' of $f: U \to \mathbb{R}$ at any point $x \in U$. Thus, let $f: U \to \mathbb{R}$ and $g: V \to \mathbb{R}$
be two such local functions; one then notes that $f$ and $g$ are equivalent
functions, $f \cong g$, if they agree on $W \subset U \cap V| x \, not \,  in\,  \subset U \cap V$.
The germ of $f$ at the point $x \in W$ denoted by $\widetilde{x}$ is the equivalence class of functions determined by this $\cong$ \htmladdnormallink{relation}{http://planetphysics.us/encyclopedia/Bijective.html}. One notes that this definition appears in elementary `complex analysis' in one variable. One can readily check that the germs $\widetilde{x}$ for all $x \in W$ form a {\em local ring}
(in the modern sense of the \htmladdnormallink{concept}{http://planetphysics.us/encyclopedia/PreciseIdea.html}). Henceforth, with the addition of several
\htmladdnormallink{topological}{http://planetphysics.us/encyclopedia/CoIntersections.html} properties, one can define a `{\em sheaf of germs of local
$C^{\infty}$-differentiable functions of $M$}' denoted by $\Theta_M$. $\Theta_X$
in the case when $X$ is a topological space can be then defined as the disjoint
sum $\cup_{x \in M} \Theta_{M,x}$ of the local rings $\Theta_{M,x}$ for every
point of $X$. Therefore, the differentiable manifold $V_n$ or $W_{2n}$ of \htmladdnormallink{classical mechanics}{http://planetphysics.us/encyclopedia/MathematicalFoundationsOfQuantumTheories.html} (or indeed, any differential manifold) is
an example of a locally ringed space $(X, \Theta_x)$, that is a topological space $X$ with a structure sheaf $\Theta_X$. Grothendieck's {\em schemes} are
also {\bf locally ringed spaces} $(X, \Theta_X)$.

Thus, sheaves were introduced to provide a transition from \emph{local to global} properties. Therefore, ``the global study of curves which solve the classical equations of motion--which is a difficult problem--has been simplified by the introduction of sheaves''.

Following Dieudonn\'e 's and Grothendieck's famous ``\'Elements de G\'eometrie Alg\'ebrique'', and Dieudonn\'e 's ``Algebraic Geometry'' and ``Fondements de la G\'eometrie Alg\'ebrique.'' Adv. in Math. (1969), \htmladdnormallink{Alexander Grothendieck}{http://planetphysics.us/encyclopedia/AlexanderGrothendieck.html} presented in 1973 a Buffalo Summer Course entitled:
``Survey on the functorial approach to affine algebraic groups''.
This was preceded by a lecture introducing the functorial `language' approach
(\htmladdnormallink{Introduction au Langage Fonctoriel}{http://www.math.jussieu.fr/~karoubi/Grothendieck.Alger.pdf})

Grothendieck also organized and presented most of the four famous \htmladdnormallink{SGA}{http://planetphysics.us/encyclopedia/SGA4.html} seminars (SGA-1 to SGA-4), ``S\'eminaires de G\'eometrie Alg\'ebrique'' (Seminars of Algebraic Geometry.) . Other relevant references were:
K\"ahler's ``Geometria arithmetica'' (1958), S. MacLane's ``Homology'' (1963),
Manin's ``Lectures on Algebraic Geometry'', Mumford's ``Introduction to Algebraic Geometry'', and J.P. Serre's ``Faisceaux alg\'ebrique coh\'erents."
(Coherent Algebraic Sheaves). In 1968 was also published by North-Holland the
book ``Dix expos\'es sur la cohomologie des sch\'emes'' (Ten expositions on the cohomology of schemes) by J. Giraud and Alexander Grothendieck.

\end{document}
Return to "PlanetPhysics/Functorial Algebraic Geometry" page.