Cargando…
Pinning down the Invisible Sneutrino
For points in SUSY parameter space where the sneutrino is lighter than the lightest chargino and next-to-lightest neutralino, its direct mass determination from sneutrino pair production process at e+e- collider is impossible since it decays invisibly. In such a scenario the sneutrino can be discove...
Autores principales: | , , , , |
---|---|
Lenguaje: | eng |
Publicado: |
2008
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2008/10/090 http://cds.cern.ch/record/1128618 |
_version_ | 1780914884887707648 |
---|---|
author | Kalinowski, J. Kilian, W. Reuter, J. Robens, T. Rolbiecki, K. |
author_facet | Kalinowski, J. Kilian, W. Reuter, J. Robens, T. Rolbiecki, K. |
author_sort | Kalinowski, J. |
collection | CERN |
description | For points in SUSY parameter space where the sneutrino is lighter than the lightest chargino and next-to-lightest neutralino, its direct mass determination from sneutrino pair production process at e+e- collider is impossible since it decays invisibly. In such a scenario the sneutrino can be discovered and its mass determined from measurements of two-body decays of charginos produced in pairs at the ILC. Using the event generator WHIZARD we study the prospects of measuring sneutrino properties in a realistic ILC environment. In our analysis we include beamstrahlung, initial state radiation, a complete account of reducible backgrounds from SM and SUSY processes, and a complete matrix-element calculation of the SUSY signal which encompasses all irreducible background and interference contributions. We also simulate photon induced background processes using exact matrix elements. Radiation effects and the cuts to reduce background strongly modify the edges of the lepton energy spectra from which the sneutrino and chargino mass are determined. We discuss possible approaches to measure the sneutrino mass with optimal precision. |
id | cern-1128618 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
spelling | cern-11286182023-03-14T20:30:26Zdoi:10.1088/1126-6708/2008/10/090http://cds.cern.ch/record/1128618engKalinowski, J.Kilian, W.Reuter, J.Robens, T.Rolbiecki, K.Pinning down the Invisible SneutrinoParticle Physics - PhenomenologyFor points in SUSY parameter space where the sneutrino is lighter than the lightest chargino and next-to-lightest neutralino, its direct mass determination from sneutrino pair production process at e+e- collider is impossible since it decays invisibly. In such a scenario the sneutrino can be discovered and its mass determined from measurements of two-body decays of charginos produced in pairs at the ILC. Using the event generator WHIZARD we study the prospects of measuring sneutrino properties in a realistic ILC environment. In our analysis we include beamstrahlung, initial state radiation, a complete account of reducible backgrounds from SM and SUSY processes, and a complete matrix-element calculation of the SUSY signal which encompasses all irreducible background and interference contributions. We also simulate photon induced background processes using exact matrix elements. Radiation effects and the cuts to reduce background strongly modify the edges of the lepton energy spectra from which the sneutrino and chargino mass are determined. We discuss possible approaches to measure the sneutrino mass with optimal precision.For points in SUSY parameter space where the sneutrino is lighter than the lightest chargino and next-to-lightest neutralino, its direct mass determination from sneutrino pair production process at e+e- collider is impossible since it decays invisibly. In such a scenario the sneutrino can be discovered and its mass determined from measurements of two-body decays of charginos produced in pairs at the ILC. Using the event generator WHIZARD we study the prospects of measuring sneutrino properties in a realistic ILC environment. In our analysis we include beamstrahlung, initial state radiation, a complete account of reducible backgrounds from SM and SUSY processes, and a complete matrix-element calculation of the SUSY signal which encompasses all irreducible background and interference contributions. We also simulate photon induced background processes using exact matrix elements. Radiation effects and the cuts to reduce background strongly modify the edges of the lepton energy spectra from which the sneutrino and chargino mass are determined. We discuss possible approaches to measure the sneutrino mass with optimal precision.arXiv:0809.3997CERN-PH-TH-2008-199SI-HEP-2008-14PITHA-08-23SFB-CPP-08-68CERN-PH-TH-2008-199PITHA 08-23SFB-CPP-08-68SI-HEP-2008-14oai:cds.cern.ch:11286182008-09-24 |
spellingShingle | Particle Physics - Phenomenology Kalinowski, J. Kilian, W. Reuter, J. Robens, T. Rolbiecki, K. Pinning down the Invisible Sneutrino |
title | Pinning down the Invisible Sneutrino |
title_full | Pinning down the Invisible Sneutrino |
title_fullStr | Pinning down the Invisible Sneutrino |
title_full_unstemmed | Pinning down the Invisible Sneutrino |
title_short | Pinning down the Invisible Sneutrino |
title_sort | pinning down the invisible sneutrino |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/2008/10/090 http://cds.cern.ch/record/1128618 |
work_keys_str_mv | AT kalinowskij pinningdowntheinvisiblesneutrino AT kilianw pinningdowntheinvisiblesneutrino AT reuterj pinningdowntheinvisiblesneutrino AT robenst pinningdowntheinvisiblesneutrino AT rolbieckik pinningdowntheinvisiblesneutrino |