Edward A. Belbruno

Prof. Dr. Edward A. Belbruno

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Research Focus & Metrics

Academic Career Length

7Years (2020-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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4 January 2022 in Monthly Notices of the Royal Astronomical Society
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno
JGJames Green
James Green
A resultant gravitational force due to the current estimates of the virial mass of the Milky Way galaxy, dominated by dark matter, is estimated near the Sun and is described in two different analytical models yielding consistent results. One is a two step Hernquist model, the other is a Navarro–Frenk–White model. The effect of this force is estimated on trajectories for spacecraft sufficiently far from the Sun. The difficulty of detecting this force is studied. It is concluded that its effect should be considered for certain spacecraft missions. Its effect on the Pioneer and New Horizons spacecrafts is discussed. A future mission is discussed that may be able to detect this force. Implications of this force are discussed with its impact for problems in planetary astronomy and astrophysics.

1 January 2020 in Journal of Physics Communications
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno
It is shown that a class of approximate resonance solutions in the three-body problem under the Newtonian gravitational force are equivalent to quantized solutions of a modified Schrödinger equation for a wide range of masses that transition between energy states. In the macroscopic scale, the resonance solutions are shown to transition from one resonance type to another through weak capture at one of the bodies, while in the Schrödinger equation, one obtains quantized wave solutions transitioning between different energies. The resonance transition dynamics provides a classical model of a particle moving between different energy states in the Schrödinger equation. This methodology provides a connection between celestial and quantum mechanics.

15 February 2023 in Celestial Mechanics and Dynamical Astronomy
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno
MGMarian Gidea
Marian Gidea
WLWai-Ting Lam
Wai-Ting Lam

18 November 2024 in Celestial Mechanics and Dynamical Astronomy
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno

6 November 2024 in Celestial Mechanics and Dynamical Astronomy
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Journal Article
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno
JGJames Green
James Green

11 February 2020 in arXiv
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Edward A. BelbrunoEdward A. Belbruno
Edward A. Belbruno
It is shown that a class of approximate resonance solutions in the three-body problem under the Newtonian gravitational force are equivalent to quantized solutions of a modified Schr\"odinger equation for a wide range of masses that transition between energy states. In the macroscopic scale, the resonance solutions are shown to transition from one resonance type to another through weak capture at one of the bodies, while in the Schr\"odinger equation, one obtains quantized wave solutions transitioning between different energies. The resonance transition dynamics provides a classical model of a particle moving between different energy states in the Schr\"odinger equation. This methodology provides a connection between celestial and quantum mechanics.