2013:groups:np:effectivedm
Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision | ||
|
2013:groups:np:effectivedm [2013/06/18 11:43] kiel.howe [Exploring other signal channels for simplest UV completions of effective operators] |
2013:groups:np:effectivedm [2013/06/20 12:24] (current) balazs.csaba |
||
|---|---|---|---|
| Line 15: | Line 15: | ||
| ^Name ^ e-mail ^ | ^Name ^ e-mail ^ | ||
| | Kiel Howe | howek@stanford.edu | | | Kiel Howe | howek@stanford.edu | | ||
| + | | Brian Shuve | bshuve@perimeterinstitute.ca | | ||
| + | | Gordan Krnjaic | gkrnjaic@perimeterinstitute.ca | | ||
| + | | Andreas Goudelis | andreas.goudelis@lapth.cnrs.fr | | ||
| + | | Csaba Balazs | csaba.balazs@monash.edu | | ||
| + | | Yun Jiang | yunjiang@ucdavis.edu | | ||
| + | | Alex Arbey | alexandre.arbey@ens-lyon.fr | | ||
| + | | Fawzi Boudjema| boudjema@lapth.cnrs.fr| | ||
| ==== Improving sensitivity of monojet-like searches ==== | ==== Improving sensitivity of monojet-like searches ==== | ||
| - | Goal - determine the best set of cuts to study ISR + MET final states for single insertions of effective Dark Matter operators (for example, the Harnik et. al. applied razor analysis) | + | Goal - determine the best set of cuts to study ISR + MET final states for single insertions of effective Dark Matter operators (for example, the Harnik et. al. razor recast) |
| Interested people: | Interested people: | ||
| ^Name ^ e-mail ^ | ^Name ^ e-mail ^ | ||
| - | | | | | + | | Marija Marjanovic | marija.marjanovic@cern.ch | |
| ==== Exploring other signal channels for simplest UV completions of effective operators ==== | ==== Exploring other signal channels for simplest UV completions of effective operators ==== | ||
| Line 32: | Line 39: | ||
| * Di-top resonance or di-vector-like-quark resonance for gluon operator | * Di-top resonance or di-vector-like-quark resonance for gluon operator | ||
| - | Should we tie this in with paired resonances project? | + | Should we tie this in with paired resonances working group? |
| Interested people: | Interested people: | ||
| ^Name ^ e-mail ^ | ^Name ^ e-mail ^ | ||
| | Kiel Howe | howek@stanford.edu | | | Kiel Howe | howek@stanford.edu | | ||
| + | | Brian Shuve | bshuve@perimeterinstitute.ca | | ||
| + | | Andreas Goudelis | andreas.goudelis@lapth.cnrs.fr | | ||
| + | | Aoife Bharucha | aoife.bharucha@desy.de | | ||
| + | | Gordan Krnjaic | gkrnjaic@perimeterinstitute.ca| | ||
| + | ==== Interpretation of the LHC monojet searches in terms of indirect detection and relic density ==== | ||
| + | Goal - the monojet searches at the LHC are currently reinterpreted (in a simple effective model with one mediator and one DM particle) in terms of dark matter scattering cross-sections with matter, as in direct detection experiments. Can we set also limits on indirect detection (gamma, proton, anti-proton spectra)? And can we deduce a lower limit on the relic density? Additional questions: | ||
| + | * which effective models are the most strongly constrained? | ||
| + | * what if more than one mediator/operator is present? | ||
| + | * which models are interesting? | ||
| + | * can we reinterpret the DM direct search results in terms of LHC cross-section? | ||
| + | Interested people: | ||
| + | ^Name ^ e-mail ^ | ||
| + | | Alex Arbey | alexandre.arbey@ens-lyon.fr | | ||
| + | | Genevieve Belanger | belanger@lapth.cnrs.fr | | ||
| + | | Andreas Goudelis | andreas.goudelis@lapth.cnrs.fr | | ||
| + | | Nazila Mahmoudi | nazila@cern.ch | | ||
| + | | Sacha Pukhov | pukhov@lapth.cnrs.fr | | ||
| + | | Yun Jiang | yunjiang@ucdavis.edu | | ||
| + | | Csaba Balazs | csaba.balazs@monash.edu | | ||
| + | | Fawzi Boudjema| boudjema@lapth.cnrs.fr| | ||
| ---- | ---- | ||
| Line 67: | Line 94: | ||
| * Tait et. al. http://arxiv.org/abs/1108.1196 | * Tait et. al. http://arxiv.org/abs/1108.1196 | ||
| * ... | * ... | ||
| + | |||
| + | Mediator production: | ||
| + | * Dijet resonances: An et al. http://arxiv.org/abs/1202.2894v1 | ||
| + | * Associated production: An et al. http://arxiv.org/abs/1212.2221 | ||
| + | * and references therein | ||
| ===== Beyond Effective dark matter ===== | ===== Beyond Effective dark matter ===== | ||
2013/groups/np/effectivedm.1371548615.txt.gz · Last modified: 2013/06/18 11:43 by kiel.howe
Page Tools
Except where otherwise noted, content on this wiki is licensed under the following license: Public Domain
