The Mare Nostrum Universe The biggest SPH simulation up to now
The Mare Nostrum Universe The biggest SPH simulation up to now The Mare Nostrum Universe The biggest SPH simulation up to now
Halo Mass function • 4063 clusters with M > 10 14 h -1 Msun • 58167 groups+clusters with M >10 13 h -1 Msun • 506000 objects with M > 10 12 h -1 Msun • More than 1 million objects with more than 100 particles
Spin parameter Dark halos λ = 0.023 for all overdensities no hint that substructures have a different spin distribution “gas” halos λ ~ 0.05
- Page 1 and 2: The Mare Nostrum Universe Gustavo Y
- Page 3 and 4: What is Mare Nostrum? • IBM JS20
- Page 6 and 7: The MareNostrum Universe TREEPM+SPH
- Page 8 and 9: Moore`s Law: Law Capacity of profes
- Page 10 and 11: Collaborators: • S. Gottlober (AI
- Page 14 and 15: Shapes of halos Shape of the dark m
- Page 16 and 17: Shape of dark matter halos at Viria
- Page 18 and 19: Dark Halos Dark matter particles Ba
- Page 20 and 21: Baryon phase space diagram
- Page 22 and 23: Baryon phase space diagram
- Page 24 and 25: Evolution of baryon phases (T > 10
- Page 26 and 27: Clusters of galaxies Most massive c
- Page 28 and 29: X-ray Temperature function
- Page 30 and 31: Comparison of Lx for two versions o
- Page 32 and 33: Evolution of scaling relations
- Page 34 and 35: Evolution of scaling relations
- Page 36 and 37: Strong Lensing • Arcs from our mo
- Page 38: Thank you -gustavo.yepes@uam.es - s
Spin parameter<br />
Dark halos<br />
λ = 0.023 for all overdensities<br />
no hint that substructures have a different<br />
spin distribution<br />
“gas” halos<br />
λ ~ 0.05
Change language