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ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$

Searches for monojet plus missing transverse momentum signatures are sensitive to new phenomena involving invisible particles, such as the pair-production of dark matter, one particularly well motivated possibility. We report on the expected sensitivity to dark matter in monojet signatures at an upg...

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Detalles Bibliográficos
Autor principal: Schramm, S
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.nuclphysbps.2015.09.404
http://cds.cern.ch/record/1757485
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author Schramm, S
author_facet Schramm, S
author_sort Schramm, S
collection CERN
description Searches for monojet plus missing transverse momentum signatures are sensitive to new phenomena involving invisible particles, such as the pair-production of dark matter, one particularly well motivated possibility. We report on the expected sensitivity to dark matter in monojet signatures at an upgraded LHC with the ATLAS detector. The effective field theory models typically used for monojet dark matter interpretations have validity limitations. These are addressed both through applying additional constraints, and through a first look at the use of simplified models of dark matter pair-production.
id cern-1757485
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling cern-17574852022-08-10T12:38:05Zdoi:10.1016/j.nuclphysbps.2015.09.404http://cds.cern.ch/record/1757485engSchramm, SATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$Particle Physics - ExperimentSearches for monojet plus missing transverse momentum signatures are sensitive to new phenomena involving invisible particles, such as the pair-production of dark matter, one particularly well motivated possibility. We report on the expected sensitivity to dark matter in monojet signatures at an upgraded LHC with the ATLAS detector. The effective field theory models typically used for monojet dark matter interpretations have validity limitations. These are addressed both through applying additional constraints, and through a first look at the use of simplified models of dark matter pair-production.ATL-PHYS-PROC-2014-142oai:cds.cern.ch:17574852014-09-23
spellingShingle Particle Physics - Experiment
Schramm, S
ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title_full ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title_fullStr ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title_full_unstemmed ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title_short ATLAS Sensitivity to WIMP Dark Matter in the Monojet Topology at $\sqrt{s}=14\,\mathrm{TeV}$
title_sort atlas sensitivity to wimp dark matter in the monojet topology at $\sqrt{s}=14\,\mathrm{tev}$
topic Particle Physics - Experiment
url https://dx.doi.org/10.1016/j.nuclphysbps.2015.09.404
http://cds.cern.ch/record/1757485
work_keys_str_mv AT schramms atlassensitivitytowimpdarkmatterinthemonojettopologyatsqrts14mathrmtev