Post on 29-May-2020
Guilhem Lavaux
Workshop "Deciphering the Dynamic Universe"
Statistical reconstruction and simulation of the initial conditions of our Local Universe
(PLUS project)
November 27th 2014
Institut d'Astrophysique de Paris / CNRS
Collaboration: J. Jasche, S. Peirani, PLUS collaboration
Motivation
● Galaxy catalogues static picture of the Universe
● Large scale structurenon-trivial statistical properties
● Initial conditions trivial (and a test is interesting per se)
● Foreground/selection effects must be taken care of
complementary observationsConstrained simulations
A static picture of Local Universe
2M++, Lavaux & Hudson (2011)
Completeness at K=11.5 Completeness at K=12.5
Galaxy distribution
The 2M++ galaxy redshift catalogLavaux & Hudson (2011, MNRAS)
Local Universe simulation (PLUS)
Aim: Biggest and most accurate simulation of the Local Universe
Current observational base: 2M++ (Lavaux & Hudson 2012)
BORG(Jasche & Wandelt 2013)
2M++ dataset SFI++/Taipan/6dFLarger surveys (2MPZ...)
SuperVelMod(Lavaux 2014)
Small scale improvements (10-15 Mpc/h subbox, enforce distances)
Local Group + Local Sheet simulation
Large scale Initial conditions(600 Mpc/h, 2563 phases, extended to 10243)
Dark MatterBaryon physics
Fine bias calibration
DONE TO DO NEW TECHNOLOGY
The BORG data model
−logP (δ ,α ,~n )=A+∑i
~n R i(1+δNL ,i [δ ])α−N iα log (1+δNL, i [δ ])+∑k
| δ̂k |2
2 Pk
Field derived from Cloud-In-Cell + 2LPT dynamicsδNL [δ]
Linear response operator (mask, radial selection)
« Mean » density of tracers
NGP binned data
Poisson probabilityGaussian prior
bias
sampled using Hamiltonian Monte Carlo algorithmδ
Parameter exploration using HMC
Evolve system with Hamiltonian dynamics
Pump and dump energy in the system by varying
Create an Hamiltonian :
Assimilate the posterior to a potential energy :
Compute acceptance :
Generate a MC sample dropping the state of
Parameter exploration using HMC
Evolve system with Hamiltonian dynamics
Pump and dump energy in the system by varying
Create an Hamiltonian :
Assimilate the posterior to a potential energy :
Compute acceptance :
Generate a MC sample dropping the state of
INVOLVE GRADIENT COMPUTATIONS !INVOLVE GRADIENT COMPUTATIONS !
Power spectrum / Phase convergence
0.1 1
10-6
10-5
10-4
10-3
10-2
10-1
Large scale structure detection and caracterization
Binned distribution of galaxies
Sloan Wall
Final dark matter density distribution
Sloan Wall
Dark matter density distribution (ARES view)
Sloan Wall Mpc/h
Mpc/h
Supergalactic plane
Shapley concentration
Coma
Pisces-Cetus
Perseus-Pisces
?
Another example: Tully's void
Thick 2M++ slice (± 20 Mpc/h), Density field in the galactic plane
Another example: Tully's void
Thin HIPASS slice (± 20 Mpc/h), Density field in the galactic plane
BORG/DIVA structure classification
Dynamically based structure classifier (DIVA, Lavaux & Wandelt 2010)
Only possible when displacement field is available
BORG !
MC Sample Displacement +Shear field
DIVA classification (Watershed + Eigenvalues)
Initial condition voxel marking
Lagrangian transport
Eulerian classification MC Map
Lavaux & Jasche (in prep.), Leclercq et al. (arxiv : 1410.0355)
Another example: Tully's void
Thin HIPASS slice (± 20 Mpc/h), Density field in the galactic plane
Void probability density in the galactic plane (DIVA criterion), HIPASS slice (± 10 Mpc/h)
Structure finding with BORG/DIVA
Full resimulation
Initial conditions
Sloan Wall
Local Universe Simulation
600 Mpc/h, 60 Mpc/h projection, 5123 dark matter PLUS collaboration
OTHER MOVIE
2M++ galaxy catalogue (Lavaux & Hudson 2012)
Local Universe Simulation
Large scales: BORG (Jasche & Wandelt)
600 Mpc/h, 200 Mpc/h projection, 10243 dark matter PLUS collaboration
2M++ galaxy catalogue (Lavaux & Hudson 2012)
Local Universe Simulation
Large scales: BORG (Jasche & Wandelt)
600 Mpc/h, 60 Mpc/h projection, 20483 dark matter, z=1 PLUS collaboration
Conclusion
Full resimulationStructure prediction
and/or classification
BORG
Galaxy surveys + Data model (selection, bias, completeness, ...)
Final density Initial density
Preliminary results 5123, 10243 (20483 to come)
Stable large scale structuration
PLUS project - redshift space distortion - Local Group dynamics - hydrodynamics
Available ensemble final density fields
Showcases for Tully's void and Sloan Wall