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VERSION:2.0
PRODID:-//RLASKEY//CALENDEROUS//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20261018T123019Z
LAST-MODIFIED:20190422T184901Z
DTSTART:20190424T190000Z
DTEND:20190424T200000Z
UID:event2113@bu.edu
URL:http://physics.bu.edu/internal/events/show/2113
SUMMARY:New Probes of Old Structure: Cosmology with 21cm Intensity Mapping 
	and the Cosmic Microwave Background
DESCRIPTION:Featuring Laura Newburgh\, Yale University\nHosted by: Indara S
	uarez\n\nPart of the HEE Seminar Series.\n\nCurrent cosmological measuremen
	ts have left us with deep questions about our Universe: What caused the exp
	ansion of the Universe at the earliest times? How did structure form? What 
	is Dark Energy and does it evolve with time? New experiments like CHIME\, H
	IRAX\, and ACTPol are poised to address these questions through 3-dimension
	al maps of structure and measurements of the polarized Cosmic Microwave Bac
	kground. In this talk\, I will describe how we will use 21cm intensity meas
	urements from CHIME and HIRAX to place sensitive constraints on Dark Energy
	 between redshifts 0.8 -- 2.5\, a poorly probed era corresponding to when D
	ark Energy began to impact the expansion history of the Universe. I will al
	so discuss how we will use data from new CMB instruments to constrain cosmo
	logical parameters like the total neutrino mass and probe structure at late
	 times.
LOCATION:PRB 595\, 3 Cummington Mall\, 02215
STATUS:CONFIRMED
CLASS:PUBLIC
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