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VERSION:2.0
PRODID:-//RLASKEY//CALENDEROUS//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20261021T085437Z
LAST-MODIFIED:20171020T191831Z
DTSTART:20171023T180000Z
DTEND:20171023T190000Z
UID:event1841@bu.edu
URL:http://physics.bu.edu/internal/events/show/1841
SUMMARY:Boosted Dark Matter at Super-Kamiokande
DESCRIPTION:Featuring Christopher Kachulis\n\nPart of the Departmental Semi
	nars.\n\nDissertation Committee:  Kearns\, Katz\, Sushkov\, Carey\, Grant\n
	\nAbstract:  \n\nThere has long been ample evidence for the existence of da
	rk matter.  Based on observation of the Cosmic Microwave Background\, dark 
	matter accounts for about 25% of the energy density of the Universe.  Beyon
	d this\, however\, little is known about the properties of dark matter.  Di
	rect and indirect detection searches\, as well as searches for dark matter 
	produced at particle accelerators\, have thus far all produced null results
	.  I will present a brief history of dark matter experimental results\, and
	 then discuss a class of dark matter models called "boosted" dark matter.  
	In these models\, some small fraction of dark matter is produced at late ti
	mes at relativistic energies\, thus the name "boosted".  I will then presen
	t the results of a search for boosted dark matter from the Galactic Center 
	and the Sun at Super-Kamiokande.
LOCATION:PRB 595\, 3 Cummington Mall\, 02215
STATUS:CONFIRMED
CLASS:PUBLIC
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