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Energy-conserving methods for Hamiltonian boundary value problems and applications in astrodynamics

arXiv: 1309.2832 , http://arxiv.org/abs/1309.2832
handle: 2158/907932 , 11586/127969
We introduce new methods for the numerical solution of general Hamiltonian boundary value problems. The main feature of the new formulae is to produce numerical solutions along which the energy is precisely conserved, as is the case with the analytical solution. We apply the methods to locate periodic orbits in the circular restricted three body problem by using their energy value rather than their pe- riod as input data. We also use the methods for solving optimal transfer problems in astrodynamics.
22 pages, 4 figures
energy conservation, 65P10, 65L10 65L06, numerical solution, Energyng conserving Kutta methods; Hamiltonian value problems; Astrodynamics; optimal control, three body problem, Numerical Analysis (math.NA), Hamiltonian boundary value problems, FOS: Mathematics, Mathematics - Numerical Analysis
energy conservation, 65P10, 65L10 65L06, numerical solution, Energyng conserving Kutta methods; Hamiltonian value problems; Astrodynamics; optimal control, three body problem, Numerical Analysis (math.NA), Hamiltonian boundary value problems, FOS: Mathematics, Mathematics - Numerical Analysis
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).25 popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.Top 10% influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).Top 10% impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.Top 10%
