Working Group on Radiative Corrections and Generators for Low Energy Hadronic Cross Section and Luminosity

Name: Working Group on Radiative Corrections and Generators for Low Energy Hadronic Cross Section and Luminosity
Start: 2010-04-19T14:30:00+02:00
End: 2010-04-20T14:30:00+02:00
Location: Laboratori Nazionali di Frascati

19–20 Apr 2010

Laboratori Nazionali di Frascati

Europe/Rome timezone

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rita.bertelli@lnf.infn.it

How much can we learn about (gamma* gamma* -> pi0) from KLOE-2: studies with EKHARA Monte Carlo generator

20 Apr 2010, 09:30

30m

Aula Seminari (Laboratori Nazionali di Frascati)

Aula Seminari

Laboratori Nazionali di Frascati

Via Enrico Fermi, 40 I-00044 Frascati

FSR and Gamma Gamma physics (2)

Sergiy Ivashyn (University of Silesia)

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Working Group on Radiative Corrections and Generators for Low Energy Hadronic Cross Section and Luminosity

Support

How much can we learn about (gamma* gamma* -> pi0) from KLOE-2: studies with EKHARA Monte Carlo generator

Aula Seminari

Laboratori Nazionali di Frascati

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