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SUMMARY:Solving the Boltzmann Equation for Neutrino Transport in Relativist
	ic Astrophysics
DTSTAMP:20260330T195000Z
DTSTART;VALUE=DATE:20240708
DTEND;VALUE=DATE:20240712
DESCRIPTION:The spectacular observation of gravitational waves from a binar
	y neutron star merger by the LIGO-Virgo Collaboration (GW170817)\, and a s
	uccessful follow-up campaign by nearly every electromagnetic telescope ush
	ered in this new era of multi-messenger astrophysics. Much of the understa
	nding of such events arises from numerical modeling. An important part of 
	this modeling is the inclusion in simulations of neutrino transport\, as d
	escribed by Boltzmann's equation. Because of inherent computational resour
	ce limits and given the high cost of the transport equations and the compl
	exity of neutrino-matter interactions\, there is a trade-off between compu
	tational cost and physical realism in all simulations. This workshop cover
	s various approaches to solving the neutrino transport problem in compact 
	object mergers and core-collapse supernovae\, including Monte Carlo method
	s\, moment truncation schemes\, and other techniques.
URL:https://icerm.brown.edu/topical_workshops/tw-24-sbe/
LOCATION:Providence\, RI\, USA
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