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| title = An Equilibrium Orbital Electron
| title = An Equilibrium Orbital Electron
| author = [[Adam R Brute]]
| author = [[Adam R Brute]]
| keywords = electron, electromagnetic radiation, orbit
| published = 1997
| published = 1997
| journal = [[Galilean Electrodynamics]]
| journal = [[Galilean Electrodynamics]]
| volume = [[8]]
| volume = 8
| number = [[6]]
| number = 6
| pages = 113-115
| pages = 113-115
}}
}}
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==Abstract==
==Abstract==


A novel solution is here suggested for the problem of how a point-like electron particle can orbit an atomic nucleus and yet not emit electromagnetic radiation.  The argument begins with inspection of the physical similarities and differences between straight-line and curved-orbit motion.  A novel innovation is then suggested whereby an atomic orbital electron could be in a physical state equivalent to straight-line motion, and so not suffer radiative decay.[[Category:Scientific Paper]]
A novel solution is here suggested for the problem of how a point-like electron particle can orbit an atomic nucleus and yet not emit electromagnetic radiation.  The argument begins with inspection of the physical similarities and differences between straight-line and curved-orbit motion.  A novel innovation is then suggested whereby an atomic orbital electron could be in a physical state equivalent to straight-line motion, and so not suffer radiative decay.
 
[[Category:Scientific Paper|equilibrium orbital electron]]

Latest revision as of 09:27, 21 July 2026

Scientific Paper
TitleAn Equilibrium Orbital Electron
Author(s)Adam R Brute
Keywordselectron, electromagnetic radiation, orbit
Published1997
JournalGalilean Electrodynamics
Volume8
Number6
Pages113-115

Abstract

A novel solution is here suggested for the problem of how a point-like electron particle can orbit an atomic nucleus and yet not emit electromagnetic radiation. The argument begins with inspection of the physical similarities and differences between straight-line and curved-orbit motion. A novel innovation is then suggested whereby an atomic orbital electron could be in a physical state equivalent to straight-line motion, and so not suffer radiative decay.