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DTSTAMP:20260413T101721
DTSTART:20160311T113000
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URL:https://murmitoyen.com/events/vanille/udem/detail/642615
LOCATION:Université de Montréal - Pavillon Roger-Gaudry\, 2900\, chemin d
 e la Tour\, Montréal\, QC\, Canada\, H3T 1J6
SUMMARY:Probing the Hubble Sequence through Numerical Simulations - Paul To
 rrey (MIT Kavli Institute)
DESCRIPTION:Probing the Hubble Sequence through Numerical Simulations
\nPau
 l Torrey (MIT Kavli Institute)
\nIn astrophysics\, numerical simulations a
 re among the most powerful tools  available to probe the non-linear regim
 e of cosmic structure formation. They also provide one of the most powerf
 ul test-beds for understanding the  impact that hydrodynamics and physica
 l feedback processes have on the  evolution of galaxies.  In my talk\, I
  will present galaxy formation  simulations that couple a novel moving me
 sh hydrodynamical approach with  explicit baryon feedback prescriptions.
  This results in galaxy formation  models that reproduce a wide range of
  observable constrains including the  galaxy stellar mass function\, cosm
 ic star formation rate\, and galaxy  morphological diversity.  I will di
 scuss the numerical methods that we¹ve  employed\, how they vary from tr
 aditional methods\, why this matters for our  understanding of galaxy for
 mation\, and what we have learned from these  large numerical experiments
 . 
\nCette conférence s'adresse à tous\, y compris les professeurs\, le
 s chercheurs et les étudiants des trois cycles. Le café est servi à par
 tir de 11h30.
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