Video URL
https://pirsa.org/21110044Friendship in the Axiverse
APA
Cyncynates, D. (2021). Friendship in the Axiverse . Perimeter Institute for Theoretical Physics. https://pirsa.org/21110044
MLA
Cyncynates, David. Friendship in the Axiverse . Perimeter Institute for Theoretical Physics, Nov. 30, 2021, https://pirsa.org/21110044
BibTex
@misc{ scivideos_PIRSA:21110044, doi = {10.48660/21110044}, url = {https://pirsa.org/21110044}, author = {Cyncynates, David}, keywords = {Particle Physics}, language = {en}, title = {Friendship in the Axiverse }, publisher = {Perimeter Institute for Theoretical Physics}, year = {2021}, month = {nov}, note = {PIRSA:21110044 see, \url{https://scivideos.org/pirsa/21110044}} }
David Cyncynates University of Washington
Abstract
A generic low-energy prediction of string theory is the existence of a large collection of axions, commonly known as a string axiverse. String axions can be distributed over many orders of magnitude in mass, and are expected to interact with one another through their joint potential. In this talk, I will show how non-linearities in this potential lead to a new type of resonant energy transfer between axions with nearby masses. This resonance generically transfers energy from axions with larger decay constants to those with smaller decay constants, leading to a multitude of signatures. These include enhanced direct detection prospects for a resonant pair comprising even a small subcomponent of dark matter, and boosted small-scale structure if the pair is the majority of DM. Near-future iterations of experiments such as ADMX and DM Radio will be sensitive to this scenario, as will astrophysical probes of DM substructure.