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2017:groups:np:llpsm [2017/07/25 16:05] nishita.desai [Task List] |
2017:groups:np:llpsm [2017/07/25 16:13] nishita.desai |
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People interested: Nishita Desai, Stefania Gori, Andreas Goudelis, Sabine Kraml, Andre Lessa, Matthew McCullough, Dipan Sengupta, Benjamin Fuks, Eric Conte, Amit Chakraborty, Abhishek Iyer, Daniele Barducci, José Zurita, Jose Miguel No, Biplob Bhattacherjee, Shankha Banerjee, Haiying Cai, Sezen Sekmen, Gabriel Facini, Andy Buckley | People interested: Nishita Desai, Stefania Gori, Andreas Goudelis, Sabine Kraml, Andre Lessa, Matthew McCullough, Dipan Sengupta, Benjamin Fuks, Eric Conte, Amit Chakraborty, Abhishek Iyer, Daniele Barducci, José Zurita, Jose Miguel No, Biplob Bhattacherjee, Shankha Banerjee, Haiying Cai, Sezen Sekmen, Gabriel Facini, Andy Buckley | ||
- | Discussions: | + | We now have a mailing list: leshouches-llp-recast AT cern.ch |
- | * Friday (June 16) 10.00-12.00, Library | + | |
- | * Friday (June 16) 14.30-16.00, Auditorium | + | |
Topics: | Topics: | ||
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=== What do we want from this exercise? === | === What do we want from this exercise? === | ||
- | * One document listing validation (or lack of it) for each category | + | * One document showing validation (or lack of it) for each category |
- | * A list of models people are interested in re-interpreting these searches for. Is there anything that changes that cannot be smoothly interpolated? e.g. number of tracks? Anything else? | + | * A list of models people are interested in re-interpreting these searches for. Is there anything that changes that cannot be smoothly interpolated? e.g. number of tracks? Anything else? |
===== Simplified models definitions ===== | ===== Simplified models definitions ===== | ||
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* Displaced tops: SUSY models with stop NLSP, simplified models (emerged from discussion as most interesting candidate model). See [[disptop|here]], | * Displaced tops: SUSY models with stop NLSP, simplified models (emerged from discussion as most interesting candidate model). See [[disptop|here]], | ||
* Disappearing R-hadrons: SUSY models with coloured NLSP and small mass splittings (probably not the most interesting scenario to explore for now). | * Disappearing R-hadrons: SUSY models with coloured NLSP and small mass splittings (probably not the most interesting scenario to explore for now). | ||
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