Speaker
Ms
Alisha Marriott-Best
(University of Swansea)
Description
LISA and ET will operate in different frequency ranges but with comparable integrated sensitivities to a stochastic GW background (SGWB). We explore their synergies in detecting cosmological SGWBs with large amplitudes and broad frequency spectra, arising from sources such as cosmological phase transitions, cosmic strings, and primordial inflation. By combining measurements from both detectors, we can more effectively characterize the GW spectrum across different frequency scales.
