Speaker
Description
Gravitational waves can be produced from first order cosmological phase transitions that occur early in the Universe. Exciting recent results including a possible signal of a stochastic gravitational wave background from pulsar timing array experiments mean that we have now entered an era where robust predictions of the gravitational wave spectra from first order phase transitions are vital. Based on a recent invited review, Prog.Part.Nucl.Phys. 135 (2024) 104094 and several related works I will discuss various subtle issues in the prediction of gravitational wave spectra from first order phase transitions that can significantly impact the predictions and review the current status of predictions for gravitational waves from first order phase transitions. In particular I will discuss criteria for determining if a phase transition completes, and the dependence of gravitational wave predictions on the transition temperature and a variety of standard approximations.
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