When:
Tuesday, March 31, 2015
4:00 PM - 5:00 PM CT
Where: Technological Institute, F160, 2145 Sheridan Road, Evanston, IL 60208 map it
Audience: Faculty/Staff - Student - Public
Contact:
Liz Lwanga
(847) 491-3645
Group: Physics and Astronomy Astrophysics Seminars
Category: Academic
Title: Cosmic Neutrinos and Large-scale Structure
Speaker: Marilena Loverde, The University of Chicago
Host: Claude-André Faucher-Giguère
Abstract: Cosmic background neutrinos are nearly as abundant as cosmic microwave background photons, but their mass, which determines the strength of their gravitational clustering, is unknown. Neutrino oscillation data gives a strict lower limit on neutrino mass, while cosmological datasets provide the most stringent upper limit. Even if the neutrino masses are the minimum required by oscillation data, their gravitational effects on structure formation will nevertheless be detectable in -- and in fact required to explain -- data within the next decade. I will discuss the physical effects of the cosmic neutrino background on structure formation and present a new signature that may be used to measure neutrino mass with large galaxy surveys.
Keywords: Physics, Astronomy, Astrophysics