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Cosmological constant
In Binary Pulse Theory: Cosmological Constant of the Null Vacuum
BPT explains itIn standard physics
Einstein's Λ, the energy density of empty space; its measured value is about 10¹²² times smaller than quantum theory suggests.
In Binary Pulse Theory
Λ is the Null Vacuum's density and follows a universe's harmonic level as its life does, so it is not tuned. Counting the vacuum on the horizon rather than through the volume answers the 10¹²² gap.
The BPT terms behind it
The Cosmological Constant of the Null Vacuum is Einstein's Λ read as the Null Vacuum's density in geometric units: the cosmological constant and the vacuum's energy are one quantity in two units.
One Dial is the book's reading of fine-tuning: the constants physics treats as separate dials are, in Binary Pulse Theory, all set by one number, the harmonic level.
The Holographic Vacuum Density is the vacuum a horizon of radius R◎ can hold: a vacuum's energy counted on its boundary rather than through its volume.
Also known as
lambda · Λ · cosmological constant problem
Related
The standard physics term is here to help you find your way in; the book itself writes in BPT's own terms. Read them in the lexicon, or start the book at Binary Pulse Theory.