INTERACTIVE MODEL

Penrose’s proposed lifetime

Adjust the controls, inspect the calculated response and use the reading links to place the model in its physical context.

Interactive model: Penrose’s proposed lifetime. Enable JavaScript to adjust its controls.

τ ≈ ℏ / E_G

Hypothesis explorer. E_G is an entered gravitational self-energy of a mass-density difference. This is not a complete collapse model or a verified universal law.

What this model assumes

Hypothesis explorer. E_G is an entered gravitational self-energy of a mass-density difference. This is not a complete collapse model or a verified universal law.

How to explore it

Begin with the default values. Change one control at a time and watch both the graph and the readouts. Then reset the model and change another parameter. This isolates which input produces the effect you are seeing.

The plotted values are generated from the displayed equation. Downloading the calculated data lets you inspect the numerical series or compare it with a calculation of your own. The data are synthetic model outputs, not observations from an apparatus.

Before carrying a prediction into an experiment, match the model’s assumptions to the actual system: the relevant degrees of freedom, boundary conditions, noise, losses and measurement convention. The linked articles explain which comparison is physically meaningful.

Penrose’s proposed lifetime

Calculated model curves. Hypothesis explorer. E_G is an entered gravitational self-energy of a mass-density difference. This is not a complete collapse model or a verified universal law. Default control values are used in this fixed figure.

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Penrose and gravitational objective reduction