A Hypothetical Approach to Cosmic Inflation Incorporating Binary Entropy

The current paper presents an alternative hypothesis for the termination of cosmic inflation based on Huang’s model of spacetime involving the movement of a superfluid through a random resistor network. Using this model, we previously derived a mathematical relationship between the velocity of a reference frame and the probability that a random bond is intact. As an extension of this finding, the permutations of open and closed bonds are now shown to represent potential microstates, thus providing a means of relating motion within the network to binary entropy. Applying this concept to cosmic inflation, termination of this process is an expected consequence of the changes in binary entropy associated with the increasing velocity of expansion.

The Application of Fluid Dynamics to Probability States in Superfluid Spacetime

The possibility that spacetime has the characteristics of a superfluid suggests that the relationship between velocity and time may be modeled in terms of percolation theory, where time dilation corresponds to increasing fluid viscosity. By equating superfluid percolation through a porous medium to conductance in a random resistor network, it was previously shown that the Lorentz factor corresponds to a probability function describing a phase transition to normal fluid. The current paper discusses how this novel linkage of momentum, time, and probability may provide a means of resolving conflicts between quantum mechanics and relativity theory.

Is the Lorentz Factor a Probability Function in Superfluid Spacetime?

<p class="1Body">A number of studies indicate that spacetime may have properties resembling that of a superfluid, suggesting that percolation theory may provide a useful approach to studying the relationship between velocity and time. By hypothesizing that the effect described by the Lorentz factor may represent an increase in the viscosity of spacetime, it was possible to model time dilation in terms of the movement of a fluid through porous media. Using a random resistor network to equate superfluid percolation with conductance, it is shown that the Lorentz factor corresponds to a probability function involving the phase transition of the superfluid to a normal fluid with insulating properties.</p>