The formation of a bubble of true vacuum within a false vacuum, which then expands.Bubble nucleation is the process by which a new phase of matter forms from a metastable state, starting with the creation of a tiny bubble of the stable phase. In cosmology, this concept is central to the theory of false vacuum decay, where the entire universe could transition from a 'false' vacuum state to a 'true' lower-energy state. This transition would begin with the quantum nucleation of a bubble of true vacuum, which then expands at nearly the speed of light, potentially rewriting the laws of physics as it sweeps through space.
The concept of vacuum decay was introduced in the 1970s by Sidney Coleman and Frank De Luccia, who applied the mathematics of bubble nucleation from statistical mechanics to quantum field theory.
In a metastable state, the system is in a local energy minimum but not the global minimum. Quantum fluctuations or thermal energy can occasionally create a small region of the true vacuum. If this bubble is large enough, it will grow, because the energy gained from the volume of true vacuum outweighs the energy cost of the bubble's surface. This critical size is determined by the balance between volume energy and surface tension. Once a bubble exceeds this size, it expands irreversibly, converting the surrounding false vacuum.
Bubble nucleation is used to understand phase transitions in materials, such as boiling and cavitation, and it is a key concept in the search for new physics beyond the Standard Model, where the Higgs field's stability is analyzed.
The Large Hadron Collider at CERN has not created a vacuum bubble, and calculations show that cosmic rays hitting Earth are far more energetic than anything we can produce, yet the universe remains stable.






















