@InProceedings{RochaMariMalhLudw:2019:ExGrAp,
author = "Rocha, Fl{\'a}via and Marinho J{\'u}nior, Rubens and Malheiro,
Manuel and Ludwig, Gerson Otto",
affiliation = "{Instituto Tecnol{\'o}gico da Aeron{\'a}utica (ITA)} and
{Instituto Tecnol{\'o}gico da Aeron{\'a}utica (ITA)} and
{Instituto Tecnol{\'o}gico da Aeron{\'a}utica (ITA)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Extended gravitomagnetism applied to mercury perihelium advance
and bending of light",
year = "2019",
organization = "Encontro naiconal de F{\'{\i}}sica de Part{\'{\i}}culas e
Campos, 40.",
abstract = "The gravitoelectromagnetic (GEM) equations were developed in 1928
by Joseph Lense and Hans Thirring, which used the linearized
Einstein field equations valid for a weak field scheme along with
a low velocity approximation. From this linearization it is
possible to define four equations analogous to Maxwells equations,
in which the mass is the perfect analogue of the electric charge.
This leads to a new concept in which a current of mass can
generate a gravitomagnetic field similar to the magnetic field
induced by a charge current in electromagnetism. In the Newtonian
limit terms of 1/c3 are neglected, while in the of gravitomagnetic
approximation the terms of order 1/c4 are neglected and for static
sources this theory reduces to the Newtonian case which does not
gives the correct value for the perihelion advance. However, in
this work will be presented corrections up to 1/c4 and within this
approximation we get 4/3 of the correct value for the Mercurys
perihelion advance and the exact value for the deflection of
light, thus showing that higher order corrections approach the
general relativistic result. We called the expansion up to order
1/c4 of extended gravitomagnetism.",
conference-location = "Campos do Jord{\~a}o, SP",
conference-year = "01-05 set.",
language = "en",
urlaccessdate = "23 maio 2024"
}