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1 A. Dbeyssi, le 17/05/2011 o Radiative correction : emission of photon (soft hard and virtual) in initial and final state . o PandaRoot : Generators and transport models. o Effect of the PHOTOS package of PANDAROOT : Simulation with radiative correction. o Monte Carlo Simulations of in PANDAROOT: Study of energy and angular distribution of electrons and positrons . e e p p RADIATIVE CORRECTIONS TO IN PANDAROOT e e p p

RADIATIVE CORRECTIONS TO IN PANDAROOT

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RADIATIVE CORRECTIONS TO IN PANDAROOT. Radiative correction : emission of photon (soft hard and virtual ) in initial and final state . PandaRoot : Generators and transport models . - PowerPoint PPT Presentation

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Page 1: RADIATIVE CORRECTIONS  TO                        IN  PANDAROOT

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A. Dbeyssi, le 17/05/2011

o Radiative correction : emission of photon (soft hard and virtual) in initial and final state .

o PandaRoot : Generators and transport models.

o Effect of the PHOTOS package of PANDAROOT : Simulation with radiative correction.

o Monte Carlo Simulations of in PANDAROOT: Study of energy

and angular distribution of electrons and positrons .

eeppRADIATIVE CORRECTIONS TO IN PANDAROOT

eepp

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RADIATIVE CORRECTIONS

Virtual and soft photon emission (Born approximation) :

Hard photon emission :

eeppA. Dbeyssi, le 17/05/2011

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• Framework of simulation and analysis for the PANDA experiment.

• Extension of FairRoot framework developped at GSI.• Based on Root and Virtual Monte-Carlo (transport

model : Geant3, Geant 4 and Fluka) .

RADIATIVE CORRECTIONS IN PANDAROOT

• EvtGen generator: handle complex decay channels.• DPM (Dual Parton Model) generator : generation and

studies of background events.• UrQMD (Ultra-relativistic Quantum Molecular Dynamic

Model) : used to study collision.

PandaRoot

Event generators of PandaRoot

A. Dbeyssi, le 17/05/2011

Ap

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• The radiative correction are implemented in Pandaratoot with the package PHOTOS :

Emisson of photons as initial and final state radiation (soft and virtual photons) .

• Simulation with\without Photos , analysis and comparison of the obtained spectra for energy and angular distribution of the emitted particles.

• generation of 10 000 events.• Using the Macro : run_sim-tpccombi.C • EvtGen generator : EvtElectronPositron.hh. (M.

GUMBERIDZE)• Geant3 transport model.

RADIATIVE CORRECTIONS IN PANDAROOT

PHOTOS

A. Dbeyssi, le 17/05/2011

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noPhotos

Decay pbarpSystem 1.0 e+ e- ElectronPositron 1;

Enddecay End

RADIATIVE CORRECTIONS IN PANDAROOT

Decay file (.DEC):

A. Dbeyssi, le 17/05/2011

•Proton form factor : R=1 (GE=GM).

•2 values of antiproton momentum : p=1.7 and 10 GeV/c.•analysis of Monte-Carlo in 4π = no detector acceptance.

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RADIATIVE CORRECTIONS IN PANDAROOTA. Dbeyssi, le 17/05/2011

noPhotos Photos

GeVpp 7.1

GeVs

16.12

GeVEe

16.1

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RADIATIVE CORRECTIONS IN PANDAROOT

Electron-positron energy in the laboratory frame at 1.7 GeV:

A. Dbeyssi, le 17/05/2011

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ANGULAR DISTRIBUTION OF THE ELECTRON

Angular distribution of the electron at 1.7 GeV :

A. Dbeyssi, le 17/05/2011

Small difference -> necessary to decrease the widh of the bin.

PhotosnoPhotos

00987.0

0362.0

A

A

00984.0

01435.0

A

A

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PROBABILITY OF PHOTON EMMISION A. Dbeyssi, le 17/05/2011

Probability of photon emmision in PHOTOS

• no γ : 75 %• 1 γ : 21 %• 2 γ : 4 %

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RADIATIVE CORRECTIONS IN PANDAROOTA. Dbeyssi, le 17/05/2011

Energy of emitted photons in the laboratory frame

P = 1.7 GeV/cP =10 GeV/c

Mostly soft photon emission

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RADIATIVE CORRECTIONS IN PANDAROOTA. Dbeyssi, le 17/05/2011

Angular distribution of emitted photons in the laboratory frame

Forward emission of photons

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• Simulation for the channel .

started

• First tests of the Photos have been done

• This work can be extended to : Tracking and reconstruction of the generated

particles inside the detectors. Radiative corrections for the other reactions like

the muon productions. Generator for the hard photon emission :

Thank you

SUMMARY A. Dbeyssi, le 17/05/2011

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eepp

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RADIATIVE CORRECTIONS IN PANDAROOT

Positron and electron energy distribution in the centre of masse at 1.7 GeV.

A. Dbeyssi, le 17/05/2011