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VERSION:2.0
PRODID:-//RLASKEY//CALENDEROUS//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260920T225007Z
LAST-MODIFIED:20190913T143504Z
DTSTART:20190918T201500Z
DTEND:20190918T211500Z
UID:event2177@bu.edu
URL:http://physics.bu.edu/internal/events/show/2177
SUMMARY:Multi-Wavelength Observatories: New probes of GWs from the Center o
	f Galaxies 
DESCRIPTION:Featuring Razieh E. Meibody\, Harvard\n\nPart of the HET Semina
	r Series.\n\nGW Astronomy was ushered after the recent detection of GWs fro
	m Binary BHs (BBHs) in LIGO/Virgo collaboration. There are several outstand
	ing questions related to the GWs\, including the source of the BBHs\, their
	 distance and the frequency range associated with the binaries that are ess
	ential here. While LIGO is capable to answer some of these questions\, the 
	others are completely beyond the access of the ground based detectors. Mult
	i-Wavelength observatories is an excellent place to answer such questions. 
	\nIn this talk\, we discuss about the Multi-Wavelength observatories rangin
	g from 1e-6 to 1e3 Hz and with the capability of shedding light about the e
	volution of the BBHs much before their merger up to their merging time. Wit
	h an especial focus on Laser Interferometer Space Antenna (LISA)\, we will 
	also estimate the expected number of the GW events from the inspiral phase 
	of stellar mass BHs around the center of SgrA* and the impact of the dynami
	cal friction of the stellar cluster around SgrA* on the GW signal.
LOCATION:PRB 595\, 3 Cummington Mall\, 02215
STATUS:CONFIRMED
CLASS:PUBLIC
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