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TH Theory Conference Room (CERN)
TH Theory Conference Room
CERN
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Description
**EVO** All sessions and meetings will be broadcasted in the Universe community ("LHC2FC")
Registration: due to the large number of registrants, it won't be possible to accommodate any new participant. Please contact us by email if you desperately want to attend the workshop.
Goals of this TH Institute will be (i) to discuss recent physics developments, (ii) to anticipate near-term capabilities of Tevatron, LHC and other experiments, and (iii) to have discussions on the most effective ways to be prepared for giving science input to plans of the post-LHC era.
In particular, we want to address the following points:
-- Physics progress and results prior to LHC collisions
-- Physics goals and prospects for 2009/2010
-- Physics goals and prospects beyond 2010 and beyond the first LHC upgrade already approved for 2013
To answer the last two questions, we need to know what we can expect from the LHC with a certain luminosity, e.g. 10 fb^-1, in different scenarios of the TeV-scale physics and which strategy for the future one would adopt in each case. Discussing things in terms of signatures suggests our efforts be organized into four broad categories of possible signatures in the early LHC data: (i) a Higgs candidate (+anything else), (ii) no Higgs candidate (+anything else), (iii) missing energy, (iv) some more exotic signal(s) of new physics. Four discussion groups will study in details these different scenarios.
** Format ** The schedule will in general contain a few talks or planned discussions in the morning hours, followed by informal discussions and work in the afternoon hours. An overview of the programme is given here. The program also includes a Future Colliders Overview sub-series where the cases for different colliders (Tevatron, (s)LHC, ILC, LHeC, CLIC and Muon collider) will be presented.
** Working Groups **Four discussion groups will be focused on the different scenarios
of signatures observed in the initial LHC runs. See here for details.
**EVO** All sessions and meetings will be broadcasted in the Universe community ("LHC2FC")
Support
Participants
Adam Martin
Agnieszka Luszczak
Albert De Roeck
Alejandro Jenkins
Andrey Korytov
Arnd Meyer
Aurelio Juste
Barbara Mele
Bryan Webber
Chiara Mariotti
christophe Grojean
Daniel Froidevaux
David Morrissey
Dirk Zerwas
Dmitry Bardin
Durgaprasad Roy
Elzbieta Richter-Was
Emi Kou
Erkcan Ozcan
Farvah Nazila Mahmoudi
Fawzi Boudjema
Fernando Febres Cordero
Francesco Sannino
Francois RICHARD
Georg Weiglein
George W.S. Hou
Georges Azuelos
Gino Isidori
Gordon Kane
Graham W. Wilson
Gregory Moreau
Grigorios Chachamis
Gudrid Moortgat-Pick
Guillelmo Gomez-Ceballos
Gustavo C, Branco
Helenka Przysiezniak Frey
Herbert Dreiner
Hiroshi Yokoya
Ilya Ginzburg
James Stirling
James Wells
Jamie Tattersall
Jan Kalinowski
Jernej Fesel Kamenik
JoAnne Hewett
John Gunion
Kai-Feng Chen
Karl Jakobs
Ketevi Assamagan
Kiwoon Choi
Klaus Desch
Klaus Moenig
Krzysztof Rolbiecki
Laura Reina
Leszek Roszkowski
Lidia Kalinovskaya
Marcela Carena
Marco Pieri
Margarete Muehlleitner
Margarida Nesbitt Rebelo
Maria Krawczyk
Mark Lancaster
Markus Schumacher
Masahiro Yamaguchi
Meltem Serin
Michele Caffo
Mikolaj MISIAK
Motoi ENDO
Oliver Buchmueller
Orlando Panella
Osamu JINNOUCHI
Peter Uwer
Philip Bechtle
Pierre Savard
Pietro Govoni
Radja Boughezal
Robert Palmer
Rohini Godbole
Sabine Kraml
Sabine Riemann
Sally Dawson
Sebastian Grab
Sezen Sekmen
Shoji Asai
Shrihari Gopalakrishna
Stefan Ask
Stefan Pokorski
Stefania De Curtis
Sven Heinemeyer
Tahmasib Aliyev
Takeo Moroi
Tania Robens
Tao Han
Thomas G. Rizzo
Thomas LeCompte
Tilman Plehn
Tobias Hurth
Wieslaw Placzek
Wolfgang Hollik
Yasuhiro Shimizu
Yukinari Sumino
Yves Sirois
