Quantum Bubbles as a New Source of Gravitational Waves express

Original: "The Role of Microstate Degeneracy in Phase Transitions: Gravitational Waves from Bubble Entanglement"
· Gia Dvali, Lucy Komisel
arXiv:2512.13947 · 2025-12-15 · CC BY 4.0 · 2 min
Bubbles that emerged after the Big Bang carry quantum complexity and, when they collide, produce unusual gravitational waves.

The early universe was an extremely hot and dense medium. In this medium, like bubbles of steam in boiling water, bubbles of a new state of space spontaneously emerged — regions where physical properties changed abruptly. Usually, such bubbles are considered relatively simple structures, but some of them carried a colossal number of hidden 'patterns'—microscopic states that physicists call entropy. Imagine a soap bubble: its thin film shimmers with a rainbow, but here the bubble's surface glows not with seven colors but with billions of different shades, each corresponding to a separate quantum variant.

This multiplicity of states ties the bubbles together through quantum entanglement: each bubble is born as a superposition of all its possible variants, forming a single nonlocal system.

When such bubbles collide and merge, their quantum entanglement does not vanish without a trace but significantly affects the dynamics of the merger. This influence leaves a characteristic imprint on gravitational waves — ripples in the fabric of spacetime that travel at the speed of light. Unlike the merger of black holes, where information about the internal structure, according to classical ideas, seems to be lost to an outside observer, quantum bubbles generously pass on their 'memories' through the gravitational-wave signal. In this signal, a clear quantum trace is preserved — an echo of their multiplicity, manifesting in subtle features of the waveform.

This phenomenon echoes Stephen Hawking's idea of the 'memory burden' of black holes, according to which information does not disappear but is encoded on the event horizon. However, bubbles, in contrast to black holes, actively share information via gravitational waves, making it potentially observable.

Future detectors, whose sensitivity continues to improve following the example of instruments built by Rainer Weiss (a pioneer of laser interferometry for detecting gravitational waves), could pick up these characteristic signals. Detecting such a quantum echo would allow us to glimpse the quantum 'personality' of space itself, revealing its fundamental nature at a level inaccessible to any other experiment.

Each bubble was born in all possible states at once, as if a tossed coin landed both heads and tails simultaneously. The bubble's complexity was astronomical: the number of its microstates exceeds the number of atoms in the observable universe.

Science fiction often plays with the theme of multiple universes, but here the 'bubble universes' are also quantum-entangled, as if they share a common memory of the moment of creation.

Scientists
Albert EinsteinBarry BarishKip ThorneRichard FeynmanRussell HulseHenri Poincaré
Concepts
bubble collision quantum bubble false vacuum decay gravitational entanglement nucleation primordial gravitational waves quantum classical transition degeneracy black hole merger temporal entanglement false vacuum direct waves black hole memory effect common envelope galaxy merger signatures turbulent coagulation galaxy formation condensation qubit decoherence starburst