We found a match
Your institution may have rights to this item. Sign in to continue.
- Title
Our Universe Through the Unruh Effect and Information Theory.
- Authors
Schweitzer, Mark
- Abstract
This article explores the implications of bridging quantum mechanics and general relativity when the Unruh effect is observed by a particle moving at escape velocity in a gravitational field. A quantum model is developed where the Unruh effect can produce a graviton particle which when added to the Universe would increase the information content of the Universe horizon by one bit of energy as per the holographic principle. A strange particle, s = 95 MeV/c², can produce a graviton via the Unruh effect in its gravitational field at a distance of its particle wavelength from its center of mass. If the smallest unit of information is one bit, the strange particle would be the smallest detector possible in our Universe, limiting the vacuum energy density to 10-9 J/m³. Observers at the strange particle wavelength would 26 1 observe a Rindler horizon at RH = 2$R = 10 m and would perceive the ratio of matter as -- = 0.309 of the Universe energy. A wavefunction can be used to represent membranes composed of wave packets of strange particle energy and these membranes made up of any quantized number of strange particles can be used to determine the limits of size and structure of mass-energy composition within our Universe along with providing a mechanism for the expansion of the Universe itself. The luminosity of stars, quasars, and galaxies can be predicted by this model. It is theorized that the Universe contains Q quanta of time, Q³ bits of information, and can be modeled with Q² strange particles. Finally, the Unruh effect from a group of Q particles will always stretch space by a strange particle wavelength and produce a new strange particle pair for each quantum of time, equivalent to the strong interaction.
- Subjects
STRANGE particles; UNRUH effect; CENTER of mass; GRAVITATIONAL fields; QUANTUM mechanics
- Publication
Journal of the Royal Astronomical Society of Canada, 2024, Vol 118, Issue 5, p202
- ISSN
0035-872X
- Publication type
Article