Difference: SPheRIO (1 vs. 18)

Revision 182013-08-03 - WlQian

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META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 94 to 94
 

Contact

Changed:
<
<
Yogiro Hama, Takeshi Kodama, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
>
>
Yogiro Hama, Takeshi Kodama, Sandra Padula, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
  -- WlQian - 03 August 2013

Revision 172013-08-03 - WlQian

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Added:
>
>
 
Changed:
<
<
SPheRIO is the name of a numerical implementation of hydrodynamic model of nucleus-nucleus collisions based on Smoothed Particle Hydrodynamics (SPH) method. The code has been investigated and developed within the São Paulo - Rio de Janeiro Collaboration. SPheRIO is the shorthand of Smoothed Particle hydrodynamical evolution of Relativistic heavy-IOn collisions.
>
>
SPheRIO is the name of a numerical implementation of hydrodynamic model of nucleus-nucleus collisions based on Smoothed Particle Hydrodynamics (SPH) method. The code has been investigated and developed within the São Paulo - Rio de Janeiro Collaboration. SPheRIO is the shorthand of Smoothed Particle hydrodynamical evolution of Relativistic heavy-IOn collisions.
 

Presentation and history

Introduction

What is the Smoothed Particle Hydrodynamics (SPH)?

Changed:
<
<
The SPH algorithm was first introduced for astrophysical applications, and later the method was extended to heavy ion collisions by the use of the variational approach. The main references for the SPH method in heavy ion collisions are
>
>
The SPH algorithm was first introduced for astrophysical applications, and later the method was extended to heavy ion collisions by the use of the variational approach. The main references for the SPH method in heavy ion collisions are
 
Changed:
<
<
The method parameterizes the matter flow in terms of discrete Lagrangian coordinates, called SPH particles. In terms of SPH degrees of freedom, the equations of motion can be derived by using the variational principle. The main advantage of the method is that it is rather robust to deal with any kind of geometrical structure and violent dynamics. For example, shock wave phenomena can be treated without numerical difficulty, provided the size of SPH particles is appropriately chosen.
>
>
The method parameterizes the matter flow in terms of discrete Lagrangian coordinates, called SPH particles. In terms of SPH degrees of freedom, the equations of motion can be derived by using the variational principle. The main advantage of the method is that it is rather robust to deal with any kind of geometrical structure and violent dynamics. For example, shock wave phenomena can be treated without numerical difficulty, provided the size of SPH particles is appropriately chosen.
 

What is SPheRIO?

Line: 31 to 25
 

Initial conditions (IC)

Changed:
<
<
Hydrodynamic models employ the hypothesis that hot and dense matter created in collisions reaches at a certain instant a local thermal equilibrium, after which it expands and cools down before particle emission takes place. Such a local thermal equilibrium is usually characterized by some IC, which can be expressed in terms of distributions of the fluid velocity and of thermodynamical quantities for a given time-like parameter.
>
>
Hydrodynamic models employ the hypothesis that hot and dense matter created in collisions reaches at a certain instant a local thermal equilibrium, after which it expands and cools down before particle emission takes place. Such a local thermal equilibrium is usually characterized by some IC, which can be expressed in terms of distributions of the fluid velocity and of thermodynamical quantities for a given time-like parameter.
 
Changed:
<
<
In SPheRIO, one may employ different types of IC, such as Glauber type IC, which are based on a parameterization determined by single particle distributions, or on an event generator derived from some microscopic model.
>
>
In SPheRIO, one may employ different types of IC, such as Glauber type IC, which are based on a parameterization determined by single particle distributions, or on an event generator derived from some microscopic model.
 

What is the NeXus+SPheRIO?

Line: 44 to 35
 

Equation of state (EOS)

Changed:
<
<
In order to close the system of hydrodynamic equations, one also needs the EOS of the fluid, which describes the thermodynamic property of the fluid. In SPheRIO, several sets of pre-defined EOS are at disposal. The first set of EOS makes use of hadronic resonance model with finite volume corrections to describe the matter on the hadronic side, and MIT bag model for quark gluon plasma (QGP) phase. The main part of observed resonances in Particle Data Tables are included in the hadronic phase. Others include EOS inspired by lattice QCD data and EOS taking into account local strangeness neutrality. Also some simple EOS are provided for testing purposes, for instance, a set of analytic EOS which assumes a massless pion gas in the hadronic phase and the MIT bag model in the QGP phase.
>
>
In order to close the system of hydrodynamic equations, one also needs the EOS of the fluid, which describes the thermodynamic property of the fluid. In SPheRIO, several sets of pre-defined EOS are at disposal. The first set of EOS makes use of hadronic resonance model with finite volume corrections to describe the matter on the hadronic side, and MIT bag model for quark gluon plasma (QGP) phase. The main part of observed resonances in Particle Data Tables are included in the hadronic phase. Others include EOS with a fit to reproduce the lattice QCD data by Pasi Huovinen, EOS with a phenomenological critical point inspired by lattice QCD data and EOS taking into account local strangeness neutrality. Also some simple EOS are provided for testing purposes, for instance, a set of analytic EOS which assumes a massless pion gas in the hadronic phase and the MIT bag model in the QGP phase.
 

Freeze out

Changed:
<
<
With the system expanding and cooling down, the constituent particles will eventually reach the stage where they do not interact with each other, until they reach the detectors. This is the decoupling stage of the hydrodynamic model. SPheRIO can be configured to adopt three different freeze-out scenarios, namely, thermal freeze-out, thermal and chemical freeze-out, and a continuous emission (CE).
>
>
With the system expanding and cooling down, the constituent particles will eventually reach the stage where they do not interact with each other, until they reach the detectors. This is the decoupling stage of the hydrodynamic model. SPheRIO can be configured to adopt three different freeze-out scenarios, namely, thermal freeze-out, thermal and chemical freeze-out, and a continuous emission (CE).
 

ThermInAtor

Line: 62 to 47
 

History

Added:
>
>
  • Version 3.1
    • EOS with a phenomenological critical point inspired by lattice QCD data
    • EOS fit to lattice QCD data by Pasi Huovinen
    • Calculation of HBT radii
 
  • Version 3.0
    • Standalone build
    • EOS with local strangeness neutrality
Line: 69 to 58
 
    • Connection with TermInAtor
  • Version 2.0
    • EOS taking into account main part of observed resonances in Particle Data Tables
Deleted:
<
<
    • EOS Lattice QCD inspired
 
    • Continuous emission
  • Version 1.0
    • The main functionality
Line: 84 to 72
 

Download

Changed:
<
<
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (with EOS 1st order phase transition with strangeness)
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (without EOS tables)
>
>
  • Version 3.1 (FORTRAN) Version 3.1 of SPheRIO (update files only)
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (with EOS 1st order phase transition with strangeness)
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (without EOS tables)
 
<--   * Version 2.0 (FORTRAN) NeXus+SPheRIO (with EOS tables) -->
Changed:
<
<
>
>
 

Manual of SPheRIO

Line: 105 to 94
 

Contact

Deleted:
<
<
 Yogiro Hama, Takeshi Kodama, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
Changed:
<
<
-- WlQian - 16 Feb 2012

>
>
-- WlQian - 03 August 2013
 
META FILEATTACHMENT attachment="JPhysG_27-2001-75.pdf" attr="h" comment="" date="1280362885" name="JPhysG_27-2001-75.pdf" path="JPhysG_27-2001-75.pdf" size="1830125" stream="JPhysG_27-2001-75.pdf" user="Main.SandraPadula" version="1"
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Revision 162012-02-16 - WlQian

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META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 88 to 88
 
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (without EOS tables)
<--   * Version 2.0 (FORTRAN) NeXus+SPheRIO (with EOS tables) -->
Added:
>
>
 
Line: 108 to 109
 Yogiro Hama, Takeshi Kodama, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
Changed:
<
<
-- WlQian - 29 Jul 2010
>
>
-- WlQian - 16 Feb 2012
 

META FILEATTACHMENT attachment="JPhysG_27-2001-75.pdf" attr="h" comment="" date="1280362885" name="JPhysG_27-2001-75.pdf" path="JPhysG_27-2001-75.pdf" size="1830125" stream="JPhysG_27-2001-75.pdf" user="Main.SandraPadula" version="1"

Revision 152010-11-22 - WlQian

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 88 to 88
 
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (without EOS tables)
<--   * Version 2.0 (FORTRAN) NeXus+SPheRIO (with EOS tables) -->
Changed:
<
<
>
>
 

Manual of SPheRIO

Revision 142010-11-20 - WlQian

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META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 78 to 78
 

Main contributors

Deleted:
<
<

Download

 

Instruction and examples on Installation

See Installation instruction for more information.

Added:
>
>

Download

  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (with EOS 1st order phase transition with strangeness)
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO (without EOS tables)
<--   * Version 2.0 (FORTRAN) NeXus+SPheRIO (with EOS tables) -->
 

Manual of SPheRIO

Changed:
<
<
The present manual of SPheRIO version 3.0 can be found here.
>
>
The present manual of SPheRIO version 3.0 can be found here.
 

Useful Links

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<
<
>
>
 
Line: 116 to 115
 
META FILEATTACHMENT attachment="JPhysG_27-2001-557.pdf" attr="h" comment="" date="1280363266" name="JPhysG_27-2001-557.pdf" path="JPhysG_27-2001-557.pdf" size="722747" stream="JPhysG_27-2001-557.pdf" user="Main.SandraPadula" version="1"
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META FILEATTACHMENT attachment="spherio_manual_v2.pdf" attr="h" comment="" date="1280454398" name="spherio_manual_v2.pdf" path="spherio_manual_v2.pdf" size="242324" stream="spherio_manual_v2.pdf" user="Main.SandraPadula" version="1"
Added:
>
>
META FILEATTACHMENT attachment="spherio_manual_v201.pdf" attr="h" comment="" date="1290283517" name="spherio_manual_v201.pdf" path="spherio_manual_v201.pdf" size="293157" stream="spherio_manual_v201.pdf" user="Main.WlQian" version="1"

Revision 132010-07-30 - SandraPadula

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 27 to 27
  SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the São Paulo - Rio de Janeiro Collaboration. A general overview of SPheRIO can be found in
Changed:
<
<
>
>
 

Initial conditions (IC)

Line: 35 to 35
 and cools down before particle emission takes place. Such a local thermal equilibrium is usually characterized by some IC, which can be expressed in terms of distributions of the fluid velocity and of thermodynamical quantities for a given time-like parameter.
Changed:
<
<
In SPheRIO, one may employ different types of IC, such as Glauber type IC which are based on parameterization determined by single particle distributions, or event generator which is derived from some microscopic model.
>
>
In SPheRIO, one may employ different types of IC, such as Glauber type IC, which are based on a parameterization determined by single particle distributions, or on an event generator derived from some microscopic model.
 

What is the NeXus+SPheRIO?

Line: 48 to 48
 In SPheRIO, several sets of pre-defined EOS are at disposal. The first set of EOS makes use of hadronic resonance model with finite volume corrections to describe the matter on the hadronic side, and MIT bag model for quark gluon plasma (QGP) phase. The main part of observed resonances in Particle Data Tables are included in the hadronic phase. Others include EOS inspired by lattice QCD data and EOS taking into account local strangeness neutrality.
Changed:
<
<
Also some simple EOS are provided for test purpose, for instance, a set of analytic EOS with uses massless pion gas for hadronic phase and MIT bag model for QGP phase.
>
>
Also some simple EOS are provided for testing purposes, for instance, a set of analytic EOS which assumes a massless pion gas in the hadronic phase and the MIT bag model in the QGP phase.
 

Freeze out

Changed:
<
<
As the system expanding and cooling down, the constituent particles will finally reach the stage where they do not interact with each other, until they reach the detectors. This is the decoupling stage of hydrodynamic model. SPheRIO can be configured to adopt three different freeze-out scenarios, namely, thermal freeze-out, thermal and chemical freeze-out, continuous emission (CE).
>
>
With the system expanding and cooling down, the constituent particles will eventually reach the stage where they do not interact with each other, until they reach the detectors. This is the decoupling stage of the hydrodynamic model. SPheRIO can be configured to adopt three different freeze-out scenarios, namely, thermal freeze-out, thermal and chemical freeze-out, and a continuous emission (CE).
 

ThermInAtor

Changed:
<
<
A modified version of ThermInAtor is employed to handle hadron decay.
>
>
A modified version of ThermInAtor is employed to handle hadronic decay.
 

History

Line: 109 to 109
 Yogiro Hama, Takeshi Kodama, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
Changed:
<
<
<--  
-->

-- WlQian - 28 Jul 2010

>
>
-- WlQian - 29 Jul 2010
 

META FILEATTACHMENT attachment="JPhysG_27-2001-75.pdf" attr="h" comment="" date="1280362885" name="JPhysG_27-2001-75.pdf" path="JPhysG_27-2001-75.pdf" size="1830125" stream="JPhysG_27-2001-75.pdf" user="Main.SandraPadula" version="1"
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Changed:
<
<
META FILEATTACHMENT attachment="spherio_manual_v2.pdf" attr="" comment="" date="1280429067" name="spherio_manual_v2.pdf" path="spherio_manual_v2.pdf" size="242323" stream="spherio_manual_v2.pdf" user="Main.WlQian" version="1"
>
>
META FILEATTACHMENT attachment="spherio_manual_v2.pdf" attr="h" comment="" date="1280454398" name="spherio_manual_v2.pdf" path="spherio_manual_v2.pdf" size="242324" stream="spherio_manual_v2.pdf" user="Main.SandraPadula" version="1"

Revision 122010-07-29 - SandraPadula

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 29 to 29
 
Changed:
<
<

Inicitial conditions (IC)

>
>

Initial conditions (IC)

  Hydrodynamic models employ the hypothesis that hot and dense matter created in collisions reaches at a certain instant a local thermal equilibrium, after which it expands and cools down before particle emission takes place. Such a local thermal equilibrium is usually characterized by some IC, which can be expressed in terms of distributions of
Line: 106 to 106
 

Contact

Changed:
<
<
Yogiro Hama, Takeshi Kodama, Frederique Grassi,Otavio Socalowski Jr.,Wei-Liang Qian
>
>
Yogiro Hama, Takeshi Kodama, Frédérique Grassi,Otávio Socolowski Jr.,Wei-Liang Qian
 

Revision 112010-07-29 - WlQian

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 62 to 62
 

History

Changed:
<
<
  • Version 3.0 EOS taking into local strangeness neutrality, chemical freeze-out, standalone version, connection with terminator.
  • Version 2.0 EOS taking into account main part of observed resonances in Particle Data Tables, continuous emission.
  • Version 1.0 The main functionality, Equation of Motion (EOM), thermal freeze-out.
>
>
  • Version 3.0
    • Standalone build
    • EOS with local strangeness neutrality
    • Chemical freeze-out
    • Connection with TermInAtor
  • Version 2.0
    • EOS taking into account main part of observed resonances in Particle Data Tables
    • EOS Lattice QCD inspired
    • Continuous emission
  • Version 1.0
    • The main functionality
    • Equation of Motion (EOM) and List-Linked-Method
    • Thermal freeze-out
 

Main contributors

Line: 69 to 79
 

Main contributors

Deleted:
<
<
 

Download

Changed:
<
<
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO
  • Version 2.0 (FORTRAN) NeXus+SPheRIO
>
>
 

Instruction and examples on Installation

Changed:
<
<
See Installation and
>
>
See Installation instruction for more information.
 

Manual of SPheRIO

Changed:
<
<
The present manual of SPheRIO version 3.0 can be found here.
>
>
The present manual of SPheRIO version 3.0 can be found here.
 

Useful Links

Changed:
<
<
  • Home page of [[http://root.cern.ch/drupal/][ROOT]
>
>
 

Contact

Changed:
<
<
Wei-Liang Qian, Yogiro Hama, Takeshi Kodama, Frederique Grassi
>
>
Yogiro Hama, Takeshi Kodama, Frederique Grassi,Otavio Socalowski Jr.,Wei-Liang Qian
 
Line: 108 to 120
 
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Added:
>
>
META FILEATTACHMENT attachment="spherio_manual_v2.pdf" attr="" comment="" date="1280429067" name="spherio_manual_v2.pdf" path="spherio_manual_v2.pdf" size="242323" stream="spherio_manual_v2.pdf" user="Main.WlQian" version="1"

Revision 92010-07-29 - WlQian

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 85 to 85
 

Useful Links

Changed:
<
<
Home page of NeXus Home page of ThermInAtor Home page of RooT Home page of Pythia Home page of
>
>
  • Home page of NeXus
  • Home page of Epos
  • Home page of ThermInAtor
  • Home page of [[http://root.cern.ch/drupal/][ROOT]
  • Home page of Pythia
 

Contact

Revision 82010-07-29 - WlQian

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Added:
>
>
SPheRIO is the name of a numerical implementation of hydrodynamic model of nucleus-nucleus collisions based on Smoothed Particle Hydrodynamics (SPH) method. The code has been investigated and developed within the São Paulo - Rio de Janeiro Collaboration. SPheRIO is the shorthand of Smoothed Particle hydrodynamical evolution of Relativistic heavy-IOn collisions.
 

Presentation and history

Introduction

Line: 11 to 16
 The SPH algorithm was first introduced for astrophysical applications, and later the method was extended to heavy ion collisions by the use of the variational approach. The main references for the SPH method in heavy ion collisions are
Deleted:
<
<
<-- C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557. -->
 
Added:
>
>
The method parameterizes the matter flow in terms of discrete Lagrangian coordinates, called SPH particles. In terms of SPH degrees of freedom, the equations of motion can be derived by using the variational principle. The main advantage of the method is that it is rather robust to deal with any kind of geometrical structure and violent dynamics. For example, shock wave phenomena can be treated without numerical difficulty, provided the size of SPH particles is appropriately chosen.
 

What is SPheRIO?

Changed:
<
<
SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the S˜ao Paulo - Rio de Janeiro Collaboration. A general overview of SPheRIO can be found in
>
>
SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the São Paulo - Rio de Janeiro Collaboration. A general overview of SPheRIO can be found in
 
Added:
>
>

Inicitial conditions (IC)

Hydrodynamic models employ the hypothesis that hot and dense matter created in collisions reaches at a certain instant a local thermal equilibrium, after which it expands and cools down before particle emission takes place. Such a local thermal equilibrium is usually characterized by some IC, which can be expressed in terms of distributions of the fluid velocity and of thermodynamical quantities for a given time-like parameter.

In SPheRIO, one may employ different types of IC, such as Glauber type IC which are based on parameterization determined by single particle distributions, or event generator which is derived from some microscopic model.

What is the NeXus+SPheRIO?

It is a conjunction of NeXus and SPheRIO. NeXus provides the IC, and SPheRIO deals with hydrodynamic evolution part.

 
Deleted:
<
<

What is the NeXus+SPheRIO?

 

Equation of state (EOS)

Added:
>
>
In order to close the system of hydrodynamic equations, one also needs the EOS of the fluid, which describes the thermodynamic property of the fluid. In SPheRIO, several sets of pre-defined EOS are at disposal. The first set of EOS makes use of hadronic resonance model with finite volume corrections to describe the matter on the hadronic side, and MIT bag model for quark gluon plasma (QGP) phase. The main part of observed resonances in Particle Data Tables are included in the hadronic phase. Others include EOS inspired by lattice QCD data and EOS taking into account local strangeness neutrality. Also some simple EOS are provided for test purpose, for instance, a set of analytic EOS with uses massless pion gas for hadronic phase and MIT bag model for QGP phase.
 

Freeze out

Changed:
<
<

Therminator

>
>
As the system expanding and cooling down, the constituent particles will finally reach the stage where they do not interact with each other, until they reach the detectors. This is the decoupling stage of hydrodynamic model. SPheRIO can be configured to adopt three different freeze-out scenarios, namely, thermal freeze-out, thermal and chemical freeze-out, continuous emission (CE).

ThermInAtor

A modified version of ThermInAtor is employed to handle hadron decay.

 

History

Added:
>
>
  • Version 3.0 EOS taking into local strangeness neutrality, chemical freeze-out, standalone version, connection with terminator.
  • Version 2.0 EOS taking into account main part of observed resonances in Particle Data Tables, continuous emission.
  • Version 1.0 The main functionality, Equation of Motion (EOM), thermal freeze-out.
 

Main contributors

Added:
>
>
 

Download

Added:
>
>
  • Version 3.0 (FORTRAN) Standalone version of SPheRIO
  • Version 2.0 (FORTRAN) NeXus+SPheRIO
 

Instruction and examples on Installation

Added:
>
>
See Installation and
 

Manual of SPheRIO

Added:
>
>
The present manual of SPheRIO version 3.0 can be found here.
 

Useful Links

Added:
>
>
Home page of NeXus Home page of ThermInAtor Home page of RooT Home page of Pythia Home page of
 

Contact

Revision 72010-07-29 - SandraPadula

Line: 1 to 1
 
META TOPICPARENT name="HeavyIon"

SPheRIO

Line: 9 to 9
 

What is the Smoothed Particle Hydrodynamics (SPH)?

The SPH algorithm was first introduced for astrophysical applications, and later the method was extended to heavy ion collisions by the use of the

Changed:
<
<
variational approach. The reference for SPH method in heavy ion collisions is
>
>
variational approach. The main references for the SPH method in heavy ion collisions are
 
Changed:
<
<
C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557.
>
>
<-- C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557. -->
 
Changed:
<
<
* C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, JPhysG_27-2001-75.pdf

* T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27-2001-557

>
>
 

What is SPheRIO?

Changed:
<
<
SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the S˜ao Paulo - Rio de Janeiro Collaboration
>
>
SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the S˜ao Paulo - Rio de Janeiro Collaboration. A general overview of SPheRIO can be found in

 

What is the NeXus+SPheRIO?

Equation of state (EOS)

Line: 52 to 52
  -- WlQian - 28 Jul 2010

Deleted:
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META FILEATTACHMENT attachment="JPhysG_27-2001-557.pdf" attr="h" comment="" date="1280363266" name="JPhysG_27-2001-557.pdf" path="JPhysG_27-2001-557.pdf" size="722747" stream="JPhysG_27-2001-557.pdf" user="Main.SandraPadula" version="1"
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SPheRIO

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 * C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, JPhysG_27-2001-75.pdf
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* T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, !JPhysG_27-2001-557.pdf: JPhysG_27-2001-557.pdf
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* T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27-2001-557
 

What is SPheRIO?

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SPheRIO

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  C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557.
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* C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, JPhysG_27-2001-75.pdf

* T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, !JPhysG_27-2001-557.pdf: JPhysG_27-2001-557.pdf

 

What is SPheRIO?

SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the S˜ao Paulo - Rio de Janeiro

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-- WlQian - 28 Jul 2010 \ No newline at end of file

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META FILEATTACHMENT attachment="JPhysG_27-2001-75.pdf" attr="h" comment="" date="1280362885" name="JPhysG_27-2001-75.pdf" path="JPhysG_27-2001-75.pdf" size="1830125" stream="JPhysG_27-2001-75.pdf" user="Main.SandraPadula" version="1"
META FILEATTACHMENT attachment="JPhysG_27-2001-557.pdf" attr="h" comment="" date="1280363266" name="JPhysG_27-2001-557.pdf" path="JPhysG_27-2001-557.pdf" size="722747" stream="JPhysG_27-2001-557.pdf" user="Main.SandraPadula" version="1"

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SPheRIO

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Presentation and history

Introduction

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What is the Smoothed Particle Hydrodynamics?

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What is the Smoothed Particle Hydrodynamics (SPH)?

 
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The SPH algorithm was first introduced for astrophysical applications [??] [??] In C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557., we extended this numerical method to heavy-ion collisions by the use of the variational approach discussed in the preceding subsection.
>
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The SPH algorithm was first introduced for astrophysical applications, and later the method was extended to heavy ion collisions by the use of the variational approach. The reference for SPH method in heavy ion collisions is

C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557.

 

What is SPheRIO?

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>
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SPheRIO is the code which implements the entropy representation of the SPH model for relativistic high-energy collisions. It has investigated and developed within the S˜ao Paulo - Rio de Janeiro Collaboration
 

What is the NeXus+SPheRIO?

Equation of state (EOS)

Freeze out

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Contact

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Yogiro Hama
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Yogiro Hama, Takeshi Kodama, Frederique Grassi
 

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SPheRIO

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-- WlQian - 28 Jul 2010

Revision 12010-07-28 - WlQian

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Added:
>
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META TOPICPARENT name="HeavyIon"

SPheRIO

Presentation and history

Introduction

What is the Smoothed Particle Hydrodynamics?

The SPH algorithm was first introduced for astrophysical applications [??] [??] In C.E. Aguiar, T. Kodama, T. Osada and Y. Hama, J. Phys. G 27 (2001) 75; T. Kodama, C.E. Aguiar, T. Osada and Y. Hama, J. Phys. G 27 (2001) 557., we extended this numerical method to heavy-ion collisions by the use of the variational approach discussed in the preceding subsection.

What is SPheRIO?

What is the NeXus+SPheRIO?

Equation of state (EOS)

Freeze out

Therminator

History

Main contributors

Download

Instruction and examples on Installation

Manual of SPheRIO

Useful Links

Contact

hama@fma.if.usp.br

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