Wednesday
22 Jun/22
16:30 - 18:30 (Europe/Zurich)

Utilizing the causal spectrum of gravitational waves

Where:  

4/3-006 at CERN

The low frequency part of the gravitational wave spectrum generated by local physics, such as a phase transition, is largely fixed by causality, offering a clean window into the early Universe.
Due to the difference between sub-horizon and super-horizon physics, a distinct spectral feature can allow for the direct measurement of the conformal Hubble rate at which the phase transition occurred. As an example, free-streaming particles present during the phase transition affect the production of super-horizon modes. This leads to a steeper decrease in the spectrum at low frequencies as compared to the well-known causal k³ scaling. If the universe was not radiation dominated when the waves were generated, a similar feature is also present. As a surprising consequence, one can see that a period of matter domination following the production of gravitational waves actually increases their power spectrum at low frequencies.
I will also discuss the observability of this primordial signal at a future detector like LISA, accounting for the presence of astrophysical foregrounds.