Quantifying uncertainties in the high-energy neutrino cross-section
The predictions for high-energy neutrino and antineutrino deep inelastic scattering cross-sections are compared within the conventional DGLAP formalism of next-to-leading order QCD, using the latest parton distribution functions (PDF) such as CT10, HERAPDF1.5 and MSTW08 and taking account of PDF unc...
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| Materialtyp: | Conference item |
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Springer
2012
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| _version_ | 1826282092814663680 |
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| author | Cooper-Sarkar, A Mertsch, P Sarkar, S |
| author_facet | Cooper-Sarkar, A Mertsch, P Sarkar, S |
| author_sort | Cooper-Sarkar, A |
| collection | OXFORD |
| description | The predictions for high-energy neutrino and antineutrino deep inelastic scattering cross-sections are compared within the conventional DGLAP formalism of next-to-leading order QCD, using the latest parton distribution functions (PDF) such as CT10, HERAPDF1.5 and MSTW08 and taking account of PDF uncertainties. From this, a benchmark cross-section and uncertainty are derived which is consistent with the results obtained earlier using the ZEUS-S PDFs. The use of this is advocated for analysing data from neutrino telescopes, in order to facilitate comparison between their results. |
| first_indexed | 2024-03-07T00:38:38Z |
| format | Conference item |
| id | oxford-uuid:8247a19e-cb18-4c0d-9c2d-ee5d08521a05 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T00:38:38Z |
| publishDate | 2012 |
| publisher | Springer |
| record_format | dspace |
| spelling | oxford-uuid:8247a19e-cb18-4c0d-9c2d-ee5d08521a052022-03-26T21:36:17ZQuantifying uncertainties in the high-energy neutrino cross-sectionConference itemhttp://purl.org/coar/resource_type/c_5794uuid:8247a19e-cb18-4c0d-9c2d-ee5d08521a05Symplectic Elements at OxfordSpringer2012Cooper-Sarkar, AMertsch, PSarkar, SThe predictions for high-energy neutrino and antineutrino deep inelastic scattering cross-sections are compared within the conventional DGLAP formalism of next-to-leading order QCD, using the latest parton distribution functions (PDF) such as CT10, HERAPDF1.5 and MSTW08 and taking account of PDF uncertainties. From this, a benchmark cross-section and uncertainty are derived which is consistent with the results obtained earlier using the ZEUS-S PDFs. The use of this is advocated for analysing data from neutrino telescopes, in order to facilitate comparison between their results. |
| spellingShingle | Cooper-Sarkar, A Mertsch, P Sarkar, S Quantifying uncertainties in the high-energy neutrino cross-section |
| title | Quantifying uncertainties in the high-energy neutrino cross-section |
| title_full | Quantifying uncertainties in the high-energy neutrino cross-section |
| title_fullStr | Quantifying uncertainties in the high-energy neutrino cross-section |
| title_full_unstemmed | Quantifying uncertainties in the high-energy neutrino cross-section |
| title_short | Quantifying uncertainties in the high-energy neutrino cross-section |
| title_sort | quantifying uncertainties in the high energy neutrino cross section |
| work_keys_str_mv | AT coopersarkara quantifyinguncertaintiesinthehighenergyneutrinocrosssection AT mertschp quantifyinguncertaintiesinthehighenergyneutrinocrosssection AT sarkars quantifyinguncertaintiesinthehighenergyneutrinocrosssection |