Probing the scale of grand unification with gravitational waves
APA
Domcke, V. (2021). Probing the scale of grand unification with gravitational waves. Perimeter Institute. https://pirsa.org/21060001
MLA
Domcke, Valerie. Probing the scale of grand unification with gravitational waves. Perimeter Institute, Jun. 22, 2021, https://pirsa.org/21060001
BibTex
@misc{ pirsa_PIRSA:21060001, doi = {10.48660/21060001}, url = {https://pirsa.org/21060001}, author = {Domcke, Valerie}, keywords = {Particle Physics}, language = {en}, title = {Probing the scale of grand unification with gravitational waves}, publisher = {Perimeter Institute}, year = {2021}, month = {jun}, note = {PIRSA:21060001 see, \url{https://pirsa.org}} }
Cosmic strings arise as remnants of phase transitions in the early Universe, often related to theories of grand unification (GUTs). If such a phase transitions occurs at high energies, the resulting cosmic string network generates a sizable amount of gravitational waves. Most work so far has focused on the gravitational wave signal from topologically stable cosmic strings. In this talk I will introduce metastable cosmic strings, which are a generic consequence of many GUTs. I will discuss how this idea can be probed in various ongoing and upcoming gravitational wave experiments, from pulsar timing arrays to space- and ground-based interferometers. In the final part of my talk I will discuss a recent proposal on using the radio telescopes to probe this and other sources of ultra high frequency gravitational waves.