Radiative Corrections from medium to high energy experiments
Aula Leonardi
ECT*
Historically, radiative corrections were applied through correction factors to experimental data. Complicated modern experiments require implementing radiative processes in a full experimental simulation. The cross section for internal radiation depends strongly on the angles between photon and lepton lines, rising quickly over multiple orders when the photon is nearly collinear with a lepton. This presents challenges in the efficiency and numerical stability of MC simulations. Current, modern generators overcome this either via brute-force, averaging over small phase space elements to reduce the numerical instability, or by biasing the random number generation. A concerted effort by the community to author next-generation generators, addressing existing issues and incorporating the best available theoretical calculations, is required.
The workshop will give the community a guideline of the precision available now, and conversely inform the theoretical and computational community on future requirements.
adi ashkenazi
Adrian Signer
Andrei Afanasev
Ashot Gasparian
Axel Schmidt
Aymeric Proust
Baishan Hu
Balasubramaniam K M
Carlos Munoz Camacho
Clement Legris
Doris Jakubassa-Amundsen
Egle Tomasi-Gustafsson
Ethan Cline
Evangeline Downie
faiza saba
Franziska Hagelstein
Fred Myhrer
Gil Paz
Hubert Spiesberger
Igor Akushevich
Jan Bernauer
Jan Friedrich
Johannes Bluemlein
Jose Goity
Julia Tena Vidal
Kazuyoshi Kurita
Kyle Salamone
Kyo Tsukada
Lin Li
Marco Rocco
Masanori Wakasugi
Michael Kohl
Miha Mihovilovic
Mikhail Gorshteyn
Norbert Kaiser
Oleksandr Tomalak
Panos Stamoulis
Peter Blunden
Rachel Ratvasky
Ronald Gilman
Ryan Plestid
Steffen Strauch
Susan Schadmand
Taiga Goke
Tanvi Patel
Tomas Husek
Toshimi Suda
Vladimir Khachatryan
Vladimir Plekhanov
Vladyslava Sharkovska
William Briscoe
Win Lin
Xiaochao Zheng
Yannick Ulrich
Yuki HONDA