TITLE:
The Planck Particle Higgs Condensate Model Revisited: Limits on the Net Vacuum Pressure = Net Vacuum Energy Density for Higgs Binding
AUTHORS:
Christopher Pilot
KEYWORDS:
Higgs Condensate, Planck Particles, Winterberg Model, Vacuum Pressure, Vacuum Energy Density, Discrete Space, BEC Stability
JOURNAL NAME:
Journal of High Energy Physics, Gravitation and Cosmology,
Vol.12 No.4,
October
23,
2026
ABSTRACT: We revisit our model of a Higgs field as a
〈
ψ
+
ψ
−
〉
condensate, where
ψ
+
and
ψ
−
are the Planck Particle wave functions of Winterberg. Winterberg’s version of space deals with a two-component superfluid model, made up of material particles, which have positive and negative Planck mass,
m
p
=±
hc/
2πG
=±2.176E−8 kg
. According to Winterberg, 3-D space is literally made up of a vast assembly (sea) of such particles. Because the superfluid forces keeping these particles in place are very strong, and thus anchor the particles spatially in position, the particles are effectively bound, and box quantization conditions apply. We believe that space is discrete and has a graininess of the order,
L=5.028E−19 meters
, as shown in previous work. If we accept the notion that space is made up of discrete, tessellated cells, consisting of
ψ
+
and
ψ
−
particles, each occupying a fixed volume, and if the Higgs condensate is, indeed, a bound
〈
ψ
+
ψ
−
〉
structure, then we can prove that the Higgs condensate can only exist if the (net vacuum Planck Particle pressure) = (net vacuum Planck Particle energy density) lies within certain bounds, not too high, nor too low. Outside of these bounds, the BEC structure collapses, and no Higgs condensate state can exist. We’ll establish those bounds for a cubic cell construction.