Published September 21, 2020 | Version v1
Publication Open

Precision Constraints for Three-Flavor Neutrino Oscillations from the Full <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>MINOS</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math> and MINOS Dataset

Creators

  • 1. Fermi National Accelerator Laboratory
  • 2. Iowa State University
  • 3. University of Cincinnati
  • 4. University of Oxford
  • 5. Lancaster University
  • 6. University of Cambridge
  • 7. The University of Texas at Austin
  • 8. Universidade Federal de Goiás
  • 9. University of Manchester
  • 10. Tufts University
  • 11. Harvard University
  • 12. University of Dallas
  • 13. University of Minnesota
  • 14. University College London
  • 15. Universidade de São Paulo
  • 16. University of Pittsburgh
  • 17. University of Warsaw
  • 18. University of Minnesota, Duluth
  • 19. University of Sussex
  • 20. University of Houston
  • 21. William & Mary
  • 22. Williams (United States)
  • 23. Los Alamos National Laboratory
  • 24. Stanford University
  • 25. Otterbein University
  • 26. Science and Technology Facilities Council
  • 27. Rutherford Appleton Laboratory

Description

We report the final measurement of the neutrino oscillation parameters $\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}$ and ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}$ using all data from the MINOS and $\mathrm{MINOS}+$ experiments. These data were collected using a total exposure of $23.76\ifmmode\times\else\texttimes\fi{}{10}^{20}$ protons on target producing ${\ensuremath{\nu}}_{\ensuremath{\mu}}$ and ${\overline{\ensuremath{\nu}}}_{\ensuremath{\mu}}$ beams and 60.75 kt yr exposure to atmospheric neutrinos. The measurement of the disappearance of ${\ensuremath{\nu}}_{\ensuremath{\mu}}$ and the appearance of ${\ensuremath{\nu}}_{e}$ events between the Near and Far detectors yields $|\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}|=2.4{0}_{\ensuremath{-}0.09}^{+0.08}(2.4{5}_{\ensuremath{-}0.08}^{+0.07})\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }{\mathrm{eV}}^{2}$ and ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}=0.4{3}_{\ensuremath{-}0.04}^{+0.20}(0.4{2}_{\ensuremath{-}0.03}^{+0.07})$ at 68% C.L. for normal (inverted) hierarchy.

⚠️ This is an automatic machine translation with an accuracy of 90-95%

Translated Description (Arabic)

نبلغ عن القياس النهائي لمعلمات تذبذب النيوترينو $\mathrm {\ ensuremath {\Delta }}{ m }_{ 32 }^{ 2 }$ و ${\ mathrm{sin }}^{ 2 }{\ensuremath {\ theta }}_{ 23 }$ باستخدام جميع البيانات من تجارب MINOS و $\mathrm{MINOS }+$. تم جمع هذه البيانات باستخدام تعرض إجمالي قدره $ 23.76\ ifmmode\ times\ else\ texttimes\fi {} {10}^ {20 }$ بروتونات على الهدف تنتج ${\ ensuremath {\ nu }}_{\ ensuremath {\mu }}$ و ${\ overline {\ ensuremath {\ nu }}}_{\ ensuremath {\ mu }}$ أشعة و 60.75 كيلو طن في السنة من التعرض للنيوترونات في الغلاف الجوي. إن قياس اختفاء ${\ ensuremath {\nu }}_{\ ensuremath {\ mu }}$ وظهور ${\ ensuremath {\ nu }}_{ e }$ الأحداث بين أجهزة الكشف القريبة والبعيدة ينتج عنه $|\ mathrm{\ ensuremath {\ Delta }}{ m }_{ 32 }^{ 2 }|= 2.4{0 }_{\ ensuremath {-} 0.09 }^{+0.08 }( 2.4{5 }_{\ ensuremath {-} 0.08 }^{+0.07})\ ifmmode\times\ else\ texttimes\ fi {}{ 10 }^{\ ensuremath {-} 3}\text {}\ text {}{\ mathrm{eV }}^{ 2 }$ و ${\ mathrm{sin }}^{ 2 }{\ ensuremath {\theta }}_{ 23 }=0.4{3 }_\ ensuremath {0.04 }^+20 }( 0.4_{ 2 }}}{\ ensuremath -{ 0.03-0 }^{ 0.07} في التسلسل الهرمي).

Translated Description (French)

Nous rapportons la mesure finale des paramètres d'oscillation des neutrinos $ \mathrm{\ ensuremath {\Delta}}{m}_{32}^{2}$ et ${\mathrm{sin}}^{2}{\ ensuremath {\theta}}_{23}$ en utilisant toutes les données des expériences MINOS et $ \mathrm{MINOS}+$ . Ces données ont été collectées en utilisant une exposition totale de 23,76 $ \ ifmmode\times\else\ texttimes\fi{}{10}^{20}$ protons sur la cible produisant des faisceaux ${\ ensuremath {\nu}}_{\ ensuremath {\mu}}$ et ${\overline{\ ensuremath {\nu}}}_{\ ensuremath {\mu}}$ et une exposition de 60,75 kt par an aux neutrinos atmosphériques. La mesure de la disparition de ${\ ensuremath {\nu}}_{\ ensuremath {\mu}}$ et l'apparition de ${\ ensuremath {\nu}}_{e}$ événements entre les détecteurs Proche et Loin donne $|\mathrm{\ ensuremath {\Delta}}{m}_{32}^{2}|=2,4{0}_{\ ensuremath {-}0,09}^{+0,08}(2,4{5}_{\ ensuremath {-}0,08}^{+0,07})\ ifmmode\times\ else\ texttimes\fi{}{10}^{\ ensuremath {-}3}\text{ }\text{ }{\mathrm{eV}}^{2}$ et ${\mathrm{sin}}^{2}{\ ensuremath {\theta}}_{23}=0,4{3}_{\ ensuremath {-}0,04}^{+0,20}(0,4{2}_{\ ensuremath {-}0,03}^{+0,07})$ à 68 % C.L. (inversé) pour la hiérarchie normale.

Translated Description (Spanish)

Informamos la medición final de los parámetros de oscilación de neutrinos $\mathrm{\ ensuremath {\Delta}}{m}_{32}^{2}$ y ${\mathrm{sin}}^{2}{\ ensuremath {\theta}}_{23}$ utilizando todos los datos de los experimentos de MINOS y $\mathrm{MINOS}+$. Estos datos se recopilaron utilizando una exposición total de $ 23.76\ ifmmode\times\else\ texttimes\fi{}{10}^{20}$ protones en el objetivo que producen ${\ ensuremath {\nu}}_{\ ensuremath {\mu}}$ y ${\overline{\ ensuremath {\nu}}_{\ ensuremath {\mu}}$ haces y 60.75 kt de exposición anual a neutrinos atmosféricos. La medición de la desaparición de ${\ ensuremath {\nu}}_{\ ensuremath {\mu}}$ y la aparición de ${\ ensuremath {\nu}}_{e}$ eventos entre los detectores Cercano y Lejano arroja $|\mathrm{\ ensuremath {\Delta}}{m}_{32}^{2}|=2.4{0}_{\ ensuremath {-}0.09}^{+0.08}(2.4{5}_{\ ensuremath {-}0.08}^{+0.07})\ ifmmode\times\else\\ texttimes\fi{}{10}^{\ ensuremath {-}3}\text{ }\text{ } {\mathrm{eV}}^{2}$ y ${\ mathmath {sin}}^{2} {\ ensuremath {\theta}}_{23}=0.4{3}_{\ ensuremath {-}0.04}^{+0.20}(0.4{2}_{\ ensuremath {-}0.03}^{+0.07}) a $ 68% C.L. (jerarquía normal).

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Additional details

Additional titles

Translated title (Arabic)
القيود الدقيقة لتذبذبات النيوترينو ثلاثية النكهات من مجموعة بيانات <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>MINOS</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math> و MINOS الكاملة
Translated title (French)
Contraintes de précision pour les oscillations de neutrinos à trois saveurs de l'ensemble de données complet <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>MINOS</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math> et MINOS
Translated title (Spanish)
Restricciones de precisión para las oscilaciones de neutrinos de tres sabores del conjunto de datos completo de <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>MINOS</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math> y MINOS

Identifiers

Other
https://openalex.org/W3037742165
DOI
10.1103/physrevlett.125.131802

Is supplement to
https://openalex.org/W4391272932 (Other)
https://openalex.org/W4298196783 (Other)
https://openalex.org/W4231437460 (Other)
https://openalex.org/W3125908676 (Other)
https://openalex.org/W2985687605 (Other)
https://openalex.org/W2166991428 (Other)
https://openalex.org/W2055591770 (Other)
https://openalex.org/W1993471123 (Other)
https://openalex.org/W1972632452 (Other)
https://openalex.org/W1581062067 (Other)

GreSIS Basics Section

Is Global South Knowledge
Yes
Country
Brazil

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