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DTSTART:19700308T020000
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DTSTART:19701101T020000
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DTSTAMP:20210916T132453Z
LOCATION:Lise Girardin
DTSTART;TZID=Europe/Stockholm:20210708T123000
DTEND;TZID=Europe/Stockholm:20210708T130000
UID:submissions.pasc-conference.org_PASC21_sess158_msa190@linklings.com
SUMMARY:Numerical Methods for Clustering Dark Energy Simulations
DESCRIPTION:Minisymposium\n\nNumerical Methods for Clustering Dark Energy 
 Simulations\n\nBlot, Corasaniti\n\nClustering dark energy is a class of mo
 dels in which the speed of propagation of the perturbations in the dark en
 ergy component is small compared to the speed of light, causing the pertur
 bations to collapse on scales inside the horizon and affecting the process
  of cosmic structure formation. In this talk, I will present a numerical a
 pproach to simulate such scenarios using the fluid description. The numeri
 cal solution is based on the Godunov scheme, coupled with a Riemann solver
 . I will show some preliminary results of the implementation of these meth
 ods in the cosmological simulation code RAMSES.\n\nDomain: Physics
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