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Grant: Discovery Grants Program - Individual

Wilfrid Laurier University

$12,000.00

Mathematical Methods in Classical and Celestial Mechanics

EF 2014-15

Résumé
One important aspect of classical and celestial mechanics is the study of N-body problems. The most classical of the N-body problems is the Newtonian N-body problem, namely the analysis of the motion of N point particles in a setting where the dynamics are dictated by Newton's gravitational law. The study of N-body problems now includes just about any dynamical system that remotely resembles the Newtonian N-body problem. The most relevant for this proposal, besides the Newtonian N-body problem, include the full-body problems, the N-body problem on constant curvature spaces and the N-vortex problem. The vortex problem can be viewed as a N-body problem since, in an ideal fluid, one can study how vortices (i.e. points in a fluid where the fluid is spinning) interact without reference to the background fluid. Of particular interest in the planar Newtonian N-body problem and in the planar N-vortex problem are solutions that appear fixed when viewed in a uniformly rotating frame. Such solutions are called relative equilibria and the special configurations that are allowed in such motions are called relative equilibria configurations. I am interested in studying properties of relative equilibria and the configurations they define. The study of such configurations is important because they play a major role in understanding N-body behavior: they characterize the dynamical behavior of collisions and expansions and play a key role in the topology of the integral manifolds of the N-body problem. Another class of problems that I would like to study are the Full-body problems. Full body problems are concerned with the dynamical interaction of two or more distributed bodies. This is a fascinating class of problems that has many open questions and touches on numerous important issues in science and engineering, as for example binary asteroids, the dynamics of the Earth-Moon system, reaction and ionization of molecules, and stability and control of underwater vehicles. Additionally, I am interested in analyzing several aspects of the N-body problem on spaces of constant curvature. Some of the mathematical phenomena discovered in this area are so new and surprising that they need to be better understood.
Programme
Discovery Grants Program - Individual
Emplacement
Ontario, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data

Tel que publié

Application id
341836-2012
Name nom
Santoprete, Manuele
Department département
Mathematics
Organization id
35
Institution établissement
Wilfrid Laurier University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2014
Competition year année de concours
2012
Award amount
12000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1508
Committee name en
Mathematics and Statistics
Committee name fr
Mathématiques et statistique
Area of application code
1205
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Mathematical sciences
Area of application fr
Sciences mathématiques
Research subject code
2952
Research subject group en
Applied mathematics
Research subject group fr
Mathématiques appliquées
Research subject en
Linear and non-linear systems
Research subject fr
Systèmes linéaires et non linéaires
Partie
3
Nb partie
5
Application title
Mathematical Methods in Classical and Celestial Mechanics
Keyword
NSERC
Application summary
One important aspect of classical and celestial mechanics is the study of N-body problems. The most classical of the N-body problems is the Newtonian N-body problem, namely the analysis of the motion of N point particles in a setting where the dynamics are dictated by Newton's gravitational law. The study of N-body problems now includes just about any dynamical system that remotely resembles the Newtonian N-body problem. The most relevant for this proposal, besides the Newtonian N-body problem, include the full-body problems, the N-body problem on constant curvature spaces and the N-vortex problem. The vortex problem can be viewed as a N-body problem since, in an ideal fluid, one can study how vortices (i.e. points in a fluid where the fluid is spinning) interact without reference to the background fluid. Of particular interest in the planar Newtonian N-body problem and in the planar N-vortex problem are solutions that appear fixed when viewed in a uniformly rotating frame. Such solutions are called relative equilibria and the special configurations that are allowed in such motions are called relative equilibria configurations. I am interested in studying properties of relative equilibria and the configurations they define. The study of such configurations is important because they play a major role in understanding N-body behavior: they characterize the dynamical behavior of collisions and expansions and play a key role in the topology of the integral manifolds of the N-body problem. Another class of problems that I would like to study are the Full-body problems. Full body problems are concerned with the dynamical interaction of two or more distributed bodies. This is a fascinating class of problems that has many open questions and touches on numerous important issues in science and engineering, as for example binary asteroids, the dynamics of the Earth-Moon system, reaction and ionization of molecules, and stability and control of underwater vehicles. Additionally, I am interested in analyzing several aspects of the N-body problem on spaces of constant curvature. Some of the mathematical phenomena discovered in this area are so new and surprising that they need to be better understood.