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2023

Model-Independent Radiative Symmetry Breaking and Gravitational Waves

Salvio, Alberto

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Models where symmetries are predominantly broken (and masses are then generated) through radiative corrections typically produce strong first-order phase transitions with a period of supercooling, when the temperature dropped by several orders of magnitude.

Here it is shown that a model-independent description of these phenomena and the consequent production of potentially observable gravitational waves is possible in terms of few parameters (which are computable once the model is specified) if enough supercooling occurred.
It is explicitly found how large the supercooling should be in terms of those parameters, in order for the model-independent description to be valid.
It is also explained how to systematically improve the accuracy of such description by computing higher-order corrections in an expansion in powers of a small quantity, which is a function of the above-mentioned parameters.

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