# Wheeler's It from Bit Proposal in Loop Quantum Gravity

## TL;DR

This paper models spacetime in loop quantum gravity with punctures representing yes-no questions, deriving black hole entropy and predicting a cosmic phase transition in the early Universe.

## Contribution

It introduces a simplified spin network model with only two quantum states per puncture, linking quantum bits to spacetime geometry and cosmological phenomena.

## Key findings

- Derived an explicit partition function for spacetime with horizons.
- Reproduced the Bekenstein-Hawking entropy law for black holes.
- Predicted a cosmic phase transition with a decreasing cosmological constant.

## Abstract

As an attempt to realize Wheeler's "it-from-bit proposal" that physics should be reduced to simple yes-no questions we consider a model of loop quantum gravity, where the only allowed values of the quantum numbers $j_p$ at the punctures of the spin network on the spacelike two-surfaces of spacetime are $0$ and $\frac{1}{2}$. When $j_p=0$, the puncture is in the vacuum, and it does not contribute to the area of the two-surface, whereas when $j_p=\frac{1}{2}$, the puncture is in an excited state, and the allowed values of the associated quantum number $m_p$ are $-\frac{1}{2}$ and $+\frac{1}{2}$. As a consequence, the spin network used as a model of spacetime is analogous to a system of particles with spin $\frac{1}{2}$, and every puncture carries exactly one bit of information. When applied to spacetimes with horizon our model enables us to find an explicit expression for the partition function of spacetime. Using this partition function we may, among other things, obtain the Bekenstein-Hawking entropy law for black holes. When applied to cosmological models with horizon the partition function predicts a cosmic phase transition in the early Universe, where the cosmological constant went through a dramatic decrease and the matter of the Universe was created out of the vacuum.