Neutrino Wakes
APA
Pen, U. (2014). Neutrino Wakes. Perimeter Institute. https://pirsa.org/14060041
MLA
Pen, Ue-Li. Neutrino Wakes. Perimeter Institute, Jun. 06, 2014, https://pirsa.org/14060041
BibTex
@misc{ pirsa_PIRSA:14060041, doi = {10.48660/14060041}, url = {https://pirsa.org/14060041}, author = {Pen, Ue-Li}, keywords = {Cosmology}, language = {en}, title = {Neutrino Wakes}, publisher = {Perimeter Institute}, year = {2014}, month = {jun}, note = {PIRSA:14060041 see, \url{https://pirsa.org}} }
Canadian Institute for Theoretical Astrophysics (CITA)
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Abstract
We identify a new non-linear neutrino wake effect, due to the streaming motions of neutrinos relative to dark matter, analogous to the Tseliakhovich-Hirata effect. We compute the effect in moving background perturbation theory, compare to direct n-body simulations, and forecast its observability in current and future surveys. Depending on neutrino mass, this effect could be observable in upcoming surveys through a cross correlation dipole in lensing and galaxies. Unlike previous cosmological neutrino effects, this depends primarily on neutrino mass, making it complementary to measurements that depend on neutrino density.