Dark Matter – Dark Energy

Is All Dark Matter-Energy at the core of planets, stars, and galaxies?*

Background of this Key Question: A series of peer-reviewed articles by Dr. Alexander Kusenko (Kavli Institute for the Physics and Mathematics of the Universe and the University of California, Los Angeles) and then a series of popular articles has led to renewed speculations about the very nature of blackholes. As well, the Kusenko work has raised questions about the start of the universe, yet it is used within this website as a pivot to planets, stars, and galaxies.

Quick Question: Why is an infinitely-hot start of the universe necessary when it gets hot enough with a very cold start in less than a second? Look at the numbers: http://81018.com/calculations/

Quick Answer: The Hawking model is not necessary.
1. Hypothesize that the Planck base units as the first instant of time.
2. Hypothesize that the units define a primordial sphere.
3. Hypothesize that base-2 captures the expansion of Planck’s numbers.
4. Doing the math. Hypothesize about 18.5 tredecillion spheres per second.
5. Hypothesize that this is a cosmological constant and the expansion of the universe.
6. Hypothesize that the dynamics of sphere stacking and cubic-close packing of equal spheres: https://81018.com/ccp/ It is natural inflation (doublings).
7. The first 64 doublings (aka notations) are below the thresholds of length measurement by CERN. The first measurement of a unit of time isn’t until the zeptosecond at notation 74-77 — https://81018.com/a84/ — at the Garching MPI.

8. Hypothesis: This is our dark energy and dark matter: https://81018.com/dark/

A Geometric Conjecture for the Dark Energy Fraction

* Sci-News, by the editors, Dec 28, 2020
Alexander Kusenko et al. 2020. Exploring Primordial Black Holes from the Multiverse with Optical Telescopes. Phys. Rev. Lett 125 (18): 181304; doi: 10.1103, 30 October 2020 ArXiv, 2020
The LUX-ZEPLIN (LZ) collaboration is leading experimental dark matter detection, while institutions like the Vera C. Rubin Observatory and NASA are driving major research into both dark matter and dark energy. NASA Science Managed by the Sanford Underground Research Facility in South Dakota, this deep-underground experiment recently captured an intriguing single-particle interaction that physicists are studying as a potential first glimpse of a Weakly Interacting Massive Particle (WIMP). Located in Chile and partnered with institutions like SLAC National Accelerator Laboratory, researchers are utilizing the Legacy Survey of Space and Time (LSST) to map weak gravitational lensing and track how dark matter and dark energy shape the cosmos.
NASA Space Telescopes: NASA uses tools like the Hubble Space Telescope, the Fermi Gamma-ray Space Telescope, and the Nancy Grace Roman Space Telescope to map invisible matter via gravitational lensing and high-energy particle signatures. NASA Science (
The Dark Energy Survey (DES): Spearheaded by institutions including Argonne National Laboratory, DES maps galaxy clusters and cosmic expansion with extreme precision to understand if dark energy behaves as a steady force. Argonne National Laboratory (.gov)
“We can perform this study independently with a blind analysis to validate or invalidate LZ’s claim,” Elena Aprile, a physicist at Columbia University and spokesperson for the XENON experiment, told Science.

Read a report on the recent LZ underground signal from Science News.
Check out cosmological survey updates at SLAC National Accelerator Laboratory. SLAC National Accelerator Laboratory. Review space-based observation goals at NASA Science. NASA Science (.gov)

Matthew Kapust/Sanford Underground Research Facility/published by Frank Landymore, Futurism. 6 September 2026

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