Probing strong dynamics with cosmic neutrinos
- Autores
- Anchordoqui, Luis A.; Garcia Canal, Carlos Alberto; Soriano, Jorge F.
- Año de publicación
- 2019
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- IceCube has observed 80 astrophysical neutrino candidates in the energy range 0.02 Eν/PeV2. Deep inelastic scattering of these neutrinos with nucleons on Antarctic ice sheet probe center-of-mass energies s∼1 TeV. By comparing the rates for two classes of observable events, any departure from the benchmark (perturbative QCD) neutrino-nucleon cross section can be constrained. Using the projected sensitivity of South Pole next-generation neutrino telescope we show that this facility will provide a unique probe of strong interaction dynamics. In particular, we demonstrate that the high-energy high-statistics data sample to be recorded by IceCube-Gen2 in the very near future will deliver a direct measurement of the neutrino-nucleon cross section at s∼1 TeV, with a precision comparable to perturbative QCD informed by HERA data. We also use IceCube data to extract the neutrino-nucleon cross section at s∼1 TeV through a likelihood analysis, considering (for the first time) both the charged-current and neutral-current contributions as free parameters of the likelihood function.
Fil: Anchordoqui, Luis A.. American Museum of Natural History; Estados Unidos. City University of New York; Estados Unidos
Fil: Garcia Canal, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Soriano, Jorge F.. City University of New York; Estados Unidos - Materia
-
strong dynamics
neutrinos - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/130316
Ver los metadatos del registro completo
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Probing strong dynamics with cosmic neutrinosAnchordoqui, Luis A.Garcia Canal, Carlos AlbertoSoriano, Jorge F.strong dynamicsneutrinoshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1IceCube has observed 80 astrophysical neutrino candidates in the energy range 0.02 Eν/PeV2. Deep inelastic scattering of these neutrinos with nucleons on Antarctic ice sheet probe center-of-mass energies s∼1 TeV. By comparing the rates for two classes of observable events, any departure from the benchmark (perturbative QCD) neutrino-nucleon cross section can be constrained. Using the projected sensitivity of South Pole next-generation neutrino telescope we show that this facility will provide a unique probe of strong interaction dynamics. In particular, we demonstrate that the high-energy high-statistics data sample to be recorded by IceCube-Gen2 in the very near future will deliver a direct measurement of the neutrino-nucleon cross section at s∼1 TeV, with a precision comparable to perturbative QCD informed by HERA data. We also use IceCube data to extract the neutrino-nucleon cross section at s∼1 TeV through a likelihood analysis, considering (for the first time) both the charged-current and neutral-current contributions as free parameters of the likelihood function.Fil: Anchordoqui, Luis A.. American Museum of Natural History; Estados Unidos. City University of New York; Estados UnidosFil: Garcia Canal, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Soriano, Jorge F.. City University of New York; Estados UnidosAmerican Physical Society2019-11-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/130316Anchordoqui, Luis A.; Garcia Canal, Carlos Alberto; Soriano, Jorge F.; Probing strong dynamics with cosmic neutrinos; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 100; 103001; 1-11-2019; 1-122470-00102470-0029CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.100.103001info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.100.103001info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-11-26T09:06:21Zoai:ri.conicet.gov.ar:11336/130316instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-11-26 09:06:22.257CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Probing strong dynamics with cosmic neutrinos |
| title |
Probing strong dynamics with cosmic neutrinos |
| spellingShingle |
Probing strong dynamics with cosmic neutrinos Anchordoqui, Luis A. strong dynamics neutrinos |
| title_short |
Probing strong dynamics with cosmic neutrinos |
| title_full |
Probing strong dynamics with cosmic neutrinos |
| title_fullStr |
Probing strong dynamics with cosmic neutrinos |
| title_full_unstemmed |
Probing strong dynamics with cosmic neutrinos |
| title_sort |
Probing strong dynamics with cosmic neutrinos |
| dc.creator.none.fl_str_mv |
Anchordoqui, Luis A. Garcia Canal, Carlos Alberto Soriano, Jorge F. |
| author |
Anchordoqui, Luis A. |
| author_facet |
Anchordoqui, Luis A. Garcia Canal, Carlos Alberto Soriano, Jorge F. |
| author_role |
author |
| author2 |
Garcia Canal, Carlos Alberto Soriano, Jorge F. |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
strong dynamics neutrinos |
| topic |
strong dynamics neutrinos |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
IceCube has observed 80 astrophysical neutrino candidates in the energy range 0.02 Eν/PeV2. Deep inelastic scattering of these neutrinos with nucleons on Antarctic ice sheet probe center-of-mass energies s∼1 TeV. By comparing the rates for two classes of observable events, any departure from the benchmark (perturbative QCD) neutrino-nucleon cross section can be constrained. Using the projected sensitivity of South Pole next-generation neutrino telescope we show that this facility will provide a unique probe of strong interaction dynamics. In particular, we demonstrate that the high-energy high-statistics data sample to be recorded by IceCube-Gen2 in the very near future will deliver a direct measurement of the neutrino-nucleon cross section at s∼1 TeV, with a precision comparable to perturbative QCD informed by HERA data. We also use IceCube data to extract the neutrino-nucleon cross section at s∼1 TeV through a likelihood analysis, considering (for the first time) both the charged-current and neutral-current contributions as free parameters of the likelihood function. Fil: Anchordoqui, Luis A.. American Museum of Natural History; Estados Unidos. City University of New York; Estados Unidos Fil: Garcia Canal, Carlos Alberto. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Soriano, Jorge F.. City University of New York; Estados Unidos |
| description |
IceCube has observed 80 astrophysical neutrino candidates in the energy range 0.02 Eν/PeV2. Deep inelastic scattering of these neutrinos with nucleons on Antarctic ice sheet probe center-of-mass energies s∼1 TeV. By comparing the rates for two classes of observable events, any departure from the benchmark (perturbative QCD) neutrino-nucleon cross section can be constrained. Using the projected sensitivity of South Pole next-generation neutrino telescope we show that this facility will provide a unique probe of strong interaction dynamics. In particular, we demonstrate that the high-energy high-statistics data sample to be recorded by IceCube-Gen2 in the very near future will deliver a direct measurement of the neutrino-nucleon cross section at s∼1 TeV, with a precision comparable to perturbative QCD informed by HERA data. We also use IceCube data to extract the neutrino-nucleon cross section at s∼1 TeV through a likelihood analysis, considering (for the first time) both the charged-current and neutral-current contributions as free parameters of the likelihood function. |
| publishDate |
2019 |
| dc.date.none.fl_str_mv |
2019-11-01 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/130316 Anchordoqui, Luis A.; Garcia Canal, Carlos Alberto; Soriano, Jorge F.; Probing strong dynamics with cosmic neutrinos; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 100; 103001; 1-11-2019; 1-12 2470-0010 2470-0029 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/130316 |
| identifier_str_mv |
Anchordoqui, Luis A.; Garcia Canal, Carlos Alberto; Soriano, Jorge F.; Probing strong dynamics with cosmic neutrinos; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 100; 103001; 1-11-2019; 1-12 2470-0010 2470-0029 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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