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Third-body perturbation in the case of elliptic orbits for the disturbing body
(2008-12-01)
In the present work it is presented a semi-analytical and a numerical study of the perturbation caused in a spacecraft by a third body using a double averaged analytical model with the disturbing function expanded in ...
Third-body perturbation in the case of elliptic orbits for the disturbing body
(2008-12-01)
In the present work it is presented a semi-analytical and a numerical study of the perturbation caused in a spacecraft by a third body using a double averaged analytical model with the disturbing function expanded in ...
Perturbation analysis of second-order cone programming problems
(SPRINGER, 2005-11)
We discuss first and second order optimality conditions for nonlinear second-order cone programming problems, and their relation with semidefinite programming problems. For doing this we extend in an abstract setting the ...
Some orbital characteristics of lunar artificial satellites
(Springer, 2010-12-01)
In this paper we present an analytical theory with numerical simulations to study the orbital motion of lunar artificial satellites. We consider the problem of an artificial satellite perturbed by the non-uniform distribution ...
Some orbital characteristics of lunar artificial satellites
(Springer, 2010-12-01)
In this paper we present an analytical theory with numerical simulations to study the orbital motion of lunar artificial satellites. We consider the problem of an artificial satellite perturbed by the non-uniform distribution ...
Studying the lifetime of orbits around Moons in elliptic motion
(2016-10-01)
The main goal of the present paper is to study the lifetime of orbits around moons that are in elliptic motion around their parent planet. The lifetime of the orbits is defined as the time the orbit stays in orbit around ...
Generation of inflationary perturbations in the continuous spontaneous localization model: The second order power spectrum
(American Physical Society, 2020-08)
Cosmic inflation, which describes an accelerated expansion of the early Universe, yields the most successful predictions regarding temperature anisotropies in the cosmic microwave background (CMB). Nevertheless, the precise ...