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Hydrosim meeting

Feb 2 – 4, 2015
Villa Bazzoni, OATs
Europe/Rome timezone

Contribution List

32 out of 32 displayed
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  1. 0. Welcome and scope of the meeting
    Stefano Borgani
    2/2/15, 9:30 AM
  2. 1. Gadget3 Data Structures and Tree Walk: standard version vs. modifications
    Antonio Ragagnin
    2/2/15, 9:40 AM
  3. 2. An improved hydrodynamical scheme as the core of a new production code
    Alexander Beck
    2/2/15, 10:05 AM
  4. 3. The mass accretion rate of galaxy clusters: a measurable quantity
    Cristiano De Boni
    2/2/15, 10:30 AM
  5. 4. Pseudo phase space density with Dianoga
    Emiliano Munari
    2/2/15, 11:25 AM
  6. 5. Temperature Structure and high-z clusters
    Elena Rasia
    2/2/15, 11:50 AM
  7. 6. SZ scaling relations in Dianoga simulations
    Dunjia Fabian
    2/2/15, 12:15 PM
  8. 7. Pressure of the hot gas in simulations of galaxy clusters
    Susana Planelles
    2/2/15, 12:40 PM
  9. 30. About the impact of baryons on the cluster mass function: Fitting formula and cosmological implications
    Alex Saro
    2/2/15, 2:30 PM
  10. 8. Anisotropic thermal conduction in galaxy clusters
    Alexander Arth
    2/2/15, 2:55 PM
  11. 9. Music and Music-AGN clusters
    Gustavo Yepes
    2/2/15, 3:20 PM
  12. 10. The nIFTy comparison project
    Federico Sembolini
    2/2/15, 3:45 PM
  13. 11. Chaotic cold accretion onto SMBHs: the role of rotation
    Massimo Gaspari
    2/2/15, 4:10 PM
    AGN
  14. 12. Radio-mode AGN activity via kinetic feedback in galaxy clusters
    Paramita Barai
    2/2/15, 5:05 PM
    AGN
  15. 13. Connection between AGN and their host galaxies
    Lisa Steinborn-Bachmann
    2/2/15, 5:30 PM
    AGN
  16. 14. New degrees of freedom in the Dark Sector: fifth forces, momentum exchange and dark energy clustering
    Marco Baldi
    2/2/15, 5:50 PM
  17. 16. Magneticum: To big to fail
    Klaus Dolag
    2/3/15, 9:30 AM
  18. 17. CLUES toward the formation of the Local Universe
    Jenny Sorce
    2/3/15, 9:55 AM
  19. 18. Simulating primordial structures
    Umberto Maio
    2/3/15, 10:20 AM
  20. 19. Realistic distributions of HI without running expensive radiative transfer post-processing codes
    Francisco Navarro-Villaescusa
    2/3/15, 11:15 AM
  21. 20. Formation of disk galaxies with MUPPI
    Pierluigi Monaco
    2/3/15, 11:40 AM
  22. 21. Angular momentum in galactic halos
    Adelheid Teklu
    2/3/15, 12:05 PM
  23. 22. Towards next generations of HPC systems
    Claudio Gheller
    2/3/15, 2:30 PM
  24. 23. Towards porting the GADGET code to the MIC architecture
    Luigi Iapichino
    2/3/15, 3:20 PM
  25. 31. The importance of HPC for high precision, direct N-Body simulations
    Mario Spera
    2/3/15, 3:45 PM
  26. 24. Gas angular momentum and BH accretion: flash update
    Juan Carmona-Loiza
    2/4/15, 9:30 AM
  27. 26. MUPPI: current development: flash update
    David Goz
    2/4/15, 9:40 AM
  28. 29. MUPPI: new hydro scheme and AGN
    Giuseppe Murante
    2/4/15, 9:50 AM
  29. 25. Comparison of old and new AGN and hydro schemes in the Dianoga cluster set: flash update
    Cinthia Ragone-Figueroa
    2/4/15, 10:00 AM
  30. 27. primo
  31. 28. secondo
    Giovanni Vladilo
  32. 15. TBD
    Lauro Moscardini