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VERSION:2.0
PRODID:-//linuxsoftware.nz//NONSGML Joyous v1.4//EN
BEGIN:VEVENT
SUMMARY:Simulating Binary Neutron Star Mergers: Implications for Multimess
 enger Astronomy and Dark Matter Searches
DTSTART:20230504T143000Z
DTEND:20230504T160000Z
DTSTAMP:20260730T195017Z
UID:d7794afd-c1fb-4773-b19d-d7c1028c636a
SEQUENCE:1
CREATED:20230502T081744Z
DESCRIPTION: ABSTRACT: Throughout the Universe\, many high-energy\, catacl
 ysmic astrophysical collisions of neutron stars are continuously occurring
 . These collisions provide an excellent testbed to probe the properties of
  supranuclear-dense matter\, to study the production of heavy elements\, t
 o allow for an independent measurement of the expansion rate of our Univer
 se\, and to perform an indirect search for dark matter. Essential for such
  studies are reliable models describing the merger dynamics. Keeping this 
 in mind\, numerical-relativity simulations can be seen as a prerequisite f
 or a reliable interpretation of multi-messenger events\, and to further de
 velop gravitational-wave and electromagnetic transient models. We show som
 e of our most recent results and identify how simulation can be used for m
 ulti-messenger studies and how simulations including dark matter admixed s
 tars will open the door to identify the presence of dark matter in binary 
 neutron star mergers. 
LAST-MODIFIED:20230502T081744Z
LOCATION:Centro de Congressos ( -2 Floor of Civil Building)
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/simulating-binary-neutron-
 star-mergers-implications-for-multimessenger-astronomy-and-dark-matter-sea
 rches/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="vc368"> ABSTRACT: Througho
 ut the Universe\, many high-energy\, cataclysmic astrophysical collisions 
 of neutron stars are continuously occurring. These collisions provide an e
 xcellent testbed to probe the properties of supranuclear-dense matter\, to
  study the production of heavy elements\, to allow for an independent meas
 urement of the expansion rate of our Universe\, and to perform an indirect
  search for dark matter. <br/><br/>Essential for such studies are reliable
  models describing the merger dynamics. Keeping this in mind\, numerical-r
 elativity simulations can be seen as a prerequisite for a reliable interpr
 etation of multi-messenger events\, and to further develop gravitational-w
 ave and electromagnetic transient models. <br/><br/>We show some of our mo
 st recent results and identify how simulation can be used for multi-messen
 ger studies and how simulations including dark matter admixed stars will o
 pen the door to identify the presence of dark matter in binary neutron sta
 r mergers. </p>
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