Direct dark matter detection around the corner? Prospects in the Constrained MSSM
We outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We find that 10(-10) pb less than or s...
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| Format: | Conference item |
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2007
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| _version_ | 1797051042150481920 |
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| author | Trotta, R Ruiz de Austri, R Roszkowski, L |
| author_facet | Trotta, R Ruiz de Austri, R Roszkowski, L |
| author_sort | Trotta, R |
| collection | OXFORD |
| description | We outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We find that 10(-10) pb less than or similar to sigma(SI)(p) less than or similar to 10(-8) pb for direct WIMP detection (with details slightly dependent on the assumptions made). We conclude that most of the 95% probability region for the cross section will be explored by future one-tonne detectors, that will therefore cover most of the currently favoured region of parameter space. |
| first_indexed | 2024-03-06T18:14:11Z |
| format | Conference item |
| id | oxford-uuid:040c060f-63bc-4686-9aee-bbda67abce2c |
| institution | University of Oxford |
| last_indexed | 2024-03-06T18:14:11Z |
| publishDate | 2007 |
| record_format | dspace |
| spelling | oxford-uuid:040c060f-63bc-4686-9aee-bbda67abce2c2022-03-26T08:49:45ZDirect dark matter detection around the corner? Prospects in the Constrained MSSMConference itemhttp://purl.org/coar/resource_type/c_5794uuid:040c060f-63bc-4686-9aee-bbda67abce2cSymplectic Elements at Oxford2007Trotta, RRuiz de Austri, RRoszkowski, LWe outline the WIMP dark matter parameter space in the Constrained MSSM by performing a comprehensive statistical analysis that compares with experimental data predicted superpartner masses and other collider observables as well as a cold dark matter abundance. We find that 10(-10) pb less than or similar to sigma(SI)(p) less than or similar to 10(-8) pb for direct WIMP detection (with details slightly dependent on the assumptions made). We conclude that most of the 95% probability region for the cross section will be explored by future one-tonne detectors, that will therefore cover most of the currently favoured region of parameter space. |
| spellingShingle | Trotta, R Ruiz de Austri, R Roszkowski, L Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title | Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title_full | Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title_fullStr | Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title_full_unstemmed | Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title_short | Direct dark matter detection around the corner? Prospects in the Constrained MSSM |
| title_sort | direct dark matter detection around the corner prospects in the constrained mssm |
| work_keys_str_mv | AT trottar directdarkmatterdetectionaroundthecornerprospectsintheconstrainedmssm AT ruizdeaustrir directdarkmatterdetectionaroundthecornerprospectsintheconstrainedmssm AT roszkowskil directdarkmatterdetectionaroundthecornerprospectsintheconstrainedmssm |