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Large scale computing at INFN

13 February 2017
Dipartimento di Fisica Sapienza Univ. di Roma
Europe/Rome timezone

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Session

Il calcolo ad alte prestazioni nella fisica teorica INFN

13 Feb 2017, 10:00
aula "Careri" primo piano edificio "Marconi" (Dipartimento di Fisica Sapienza Univ. di Roma)

aula "Careri" primo piano edificio "Marconi"

Dipartimento di Fisica Sapienza Univ. di Roma

Conveners

Il calcolo ad alte prestazioni nella fisica teorica INFN

  • Raffaele Tripiccione (FE)

Presentation materials

There are no materials yet.

  1. 0. Introduzione
    Leonardo Cosmai (BA)
    13/02/2017, 10:00
    Introduzione
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  2. 1. BIOPHYS (1)
    Mario Nicodemi (NA)
    13/02/2017, 10:15
    Computer simulations of polymer physics and the 3D structure of the human genome Chromosomes in mammalian cells have a complex spatial organization serving vital functional purposes. We are showing that their 3D structure can be derived with high accuracy, and its molecular determinants identified, by use of polymer physics combined with advanced, massive computer simulations and...
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  3. 5. BIOPHYS (2)
    Francesco Stellato (ROMA2)
    13/02/2017, 10:20
    presentazione BIOPHYS (seconda parte)
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  4. 9. FBS
    Michele Viviani (PI)
    13/02/2017, 10:25
    presentazione FBS
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  5. 7. FIELDTURB
    Guido Boffetta (TO)
    13/02/2017, 10:35
    presentazione FLDTURB
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  6. 13. LQCD123
    Silvano Simula (ROMA3)
    13/02/2017, 10:45
    i.s. LQCD123
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  7. 10. MANYBODY
    Francesco Pederiva (TIFP)
    13/02/2017, 10:55
    presentazione MANYBODY
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  8. 6. NEMESYS
    Antonio Sindona (C)
    13/02/2017, 11:05
    presentazione NEMESYS
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  9. 14. NPQCD
    Massimo D'Elia (PI)
    13/02/2017, 11:15
    i.s. NPQCD
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  10. 11. QCDLAT
    Leonardo Giusti (MIB)
    13/02/2017, 11:25
    presentazione QCDLAT
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  11. 2. QFT_HEP
    Pietro Colangelo (BA)
    13/02/2017, 11:35
    I will present the foreseen activity and the computational needs of Iniziativa Specifica QFT-HEP (LNF node, Maria Paola Lombardo). The research includes: 1) A quantitative study of the quark gluon plasma up to temperatures \simeq 1 Gev with a realistic matter content (two almost physical light flavors, and a strange and a charm quark). The main observables will be the Equation of State...
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  12. 12. SFT
    Michele Caselle (TO)
    13/02/2017, 11:45
    presentazione SFT
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  13. 8. STRENGTH
    Nunzio Itaco (NA)
    13/02/2017, 11:55
    pesentazione STRENGTH
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  14. 3. TEONGRAV
    Roberto De Pietri (PR)
    13/02/2017, 12:05
    presentazione TEONGRAV
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  15. 16. Neutron Star Matter (NeuMatt)
    Alessandro Drago (FE)
    13/02/2017, 12:15
    The detection of GWs associated with the merger of two neutron stars offers a new important tool to test the Equation of State of matter at very high densities. Preliminary studies have indicated the possibility of discriminating among the various theoretically possible EoSs by analysing the GW signal before and after the merger. Morever, the merger of two neutron stars is supposed to be at...
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  16. 17. Cosmological computing with InDark
    Paolo Natoli (FE)
    13/02/2017, 12:20
    The goal of InDark is to investigate crucial aspects of the standard cosmological model and their connection with particle physics. The project focuses on inflation in the early Universe, the nature of dark matter and the nature of dark energy, also in terms of scenarios of modified gravity, as well as on neutrino cosmology. Particular emphasis is given to the present-day and future...
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  17. 15. La macchina sperimentale
    Piero Vicini (ROMA1)
    13/02/2017, 12:30
  18. 18. High-Resolution Simulation of Biological Neural Networks
    Pier Stanislao Paolucci (ROMA1)
    13/02/2017, 12:40
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