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Hydrosim meeting

2–4 Feb 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
    02/02/2015, 09:30
  2. 1. Gadget3 Data Structures and Tree Walk: standard version vs. modifications
    Antonio Ragagnin
    02/02/2015, 09:40
  3. 2. An improved hydrodynamical scheme as the core of a new production code
    Alexander Beck
    02/02/2015, 10:05
  4. 3. The mass accretion rate of galaxy clusters: a measurable quantity
    Cristiano De Boni
    02/02/2015, 10:30
  5. 4. Pseudo phase space density with Dianoga
    Emiliano Munari
    02/02/2015, 11:25
  6. 5. Temperature Structure and high-z clusters
    Elena Rasia
    02/02/2015, 11:50
  7. 6. SZ scaling relations in Dianoga simulations
    Dunjia Fabian
    02/02/2015, 12:15
  8. 7. Pressure of the hot gas in simulations of galaxy clusters
    Susana Planelles
    02/02/2015, 12:40
  9. 30. About the impact of baryons on the cluster mass function: Fitting formula and cosmological implications
    Alex Saro
    02/02/2015, 14:30
  10. 8. Anisotropic thermal conduction in galaxy clusters
    Alexander Arth
    02/02/2015, 14:55
  11. 9. Music and Music-AGN clusters
    Gustavo Yepes
    02/02/2015, 15:20
  12. 10. The nIFTy comparison project
    Federico Sembolini
    02/02/2015, 15:45
  13. 11. Chaotic cold accretion onto SMBHs: the role of rotation
    Massimo Gaspari
    02/02/2015, 16:10
    AGN
  14. 12. Radio-mode AGN activity via kinetic feedback in galaxy clusters
    Paramita Barai
    02/02/2015, 17:05
    AGN
  15. 13. Connection between AGN and their host galaxies
    Lisa Steinborn-Bachmann
    02/02/2015, 17:30
    AGN
  16. 14. New degrees of freedom in the Dark Sector: fifth forces, momentum exchange and dark energy clustering
    Marco Baldi
    02/02/2015, 17:50
  17. 16. Magneticum: To big to fail
    Klaus Dolag
    03/02/2015, 09:30
  18. 17. CLUES toward the formation of the Local Universe
    Jenny Sorce
    03/02/2015, 09:55
  19. 18. Simulating primordial structures
    Umberto Maio
    03/02/2015, 10:20
  20. 19. Realistic distributions of HI without running expensive radiative transfer post-processing codes
    Francisco Navarro-Villaescusa
    03/02/2015, 11:15
  21. 20. Formation of disk galaxies with MUPPI
    Pierluigi Monaco
    03/02/2015, 11:40
  22. 21. Angular momentum in galactic halos
    Adelheid Teklu
    03/02/2015, 12:05
  23. 22. Towards next generations of HPC systems
    Claudio Gheller
    03/02/2015, 14:30
  24. 23. Towards porting the GADGET code to the MIC architecture
    Luigi Iapichino
    03/02/2015, 15:20
  25. 31. The importance of HPC for high precision, direct N-Body simulations
    Mario Spera
    03/02/2015, 15:45
  26. 24. Gas angular momentum and BH accretion: flash update
    Juan Carmona-Loiza
    04/02/2015, 09:30
  27. 26. MUPPI: current development: flash update
    David Goz
    04/02/2015, 09:40
  28. 29. MUPPI: new hydro scheme and AGN
    Giuseppe Murante
    04/02/2015, 09:50
  29. 25. Comparison of old and new AGN and hydro schemes in the Dianoga cluster set: flash update
    Cinthia Ragone-Figueroa
    04/02/2015, 10:00
  30. 27. primo
  31. 28. secondo
    Giovanni Vladilo
  32. 15. TBD
    Lauro Moscardini