On the tension between the latest NOνA and T2K data
The latest data from the T2K and NO ν A experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combi...
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Published in | The European physical journal. C, Particles and fields Vol. 82; no. 10 |
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Main Authors | , |
Format | Journal Article |
Language | English |
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13.10.2022
Springer Nature B.V |
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Abstract | The latest data from the T2K and NO
ν
A experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combined) shows that the tension arises primarily from the
ν
e
appearance data, and is compounded by the
ν
¯
μ
disappearance data. We provide an explanation for the tension based on parameter degeneracies. Apart from the analysis with the standard matter effect, we also analyse the data with the vacuum oscillation hypothesis. We find that vacuum oscillations fit the data as well as matter effects do; and also reduce the tension between the two experiments. We have also done a study of the future run of NO
ν
A, T2K and DUNE in the context of establishing this tension with higher statistical significance. |
---|---|
AbstractList | Abstract The latest data from the T2K and NO $$\nu $$ ν A experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combined) shows that the tension arises primarily from the $$\nu _e$$ ν e appearance data, and is compounded by the $$\bar{\nu }_\mu $$ ν ¯ μ disappearance data. We provide an explanation for the tension based on parameter degeneracies. Apart from the analysis with the standard matter effect, we also analyse the data with the vacuum oscillation hypothesis. We find that vacuum oscillations fit the data as well as matter effects do; and also reduce the tension between the two experiments. We have also done a study of the future run of NO $$\nu $$ ν A, T2K and DUNE in the context of establishing this tension with higher statistical significance. The latest data from the T2K and NO ν A experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combined) shows that the tension arises primarily from the ν e appearance data, and is compounded by the ν ¯ μ disappearance data. We provide an explanation for the tension based on parameter degeneracies. Apart from the analysis with the standard matter effect, we also analyse the data with the vacuum oscillation hypothesis. We find that vacuum oscillations fit the data as well as matter effects do; and also reduce the tension between the two experiments. We have also done a study of the future run of NO ν A, T2K and DUNE in the context of establishing this tension with higher statistical significance. The latest data from the T2K and NOνA experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the source of the tension between the data from these two experiments. An analysis of their data from various channels (individually, and combined) shows that the tension arises primarily from the νe appearance data, and is compounded by the ν¯μ disappearance data. We provide an explanation for the tension based on parameter degeneracies. Apart from the analysis with the standard matter effect, we also analyse the data with the vacuum oscillation hypothesis. We find that vacuum oscillations fit the data as well as matter effects do; and also reduce the tension between the two experiments. We have also done a study of the future run of NOνA, T2K and DUNE in the context of establishing this tension with higher statistical significance. |
ArticleNumber | 910 |
Author | Rahaman, Ushak Raut, Sushant K. |
Author_xml | – sequence: 1 givenname: Ushak orcidid: 0000-0003-0419-2970 surname: Rahaman fullname: Rahaman, Ushak email: ushakr@uj.ac.za organization: Centre for Astro-Particle Physics (CAPP) and Department of Physics, University of Johannesburg, IFIC - Instituto de Física Corpuscular (Univ. de Valéncia — CSIC) Catedrático José Beltrán – sequence: 2 givenname: Sushant K. surname: Raut fullname: Raut, Sushant K. organization: Division of Sciences, Krea University |
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Snippet | The latest data from the T2K and NO
ν
A experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify... Abstract The latest data from the T2K and NO $$\nu $$ ν A experiments show a tension in their preferred values of the oscillation parameters. In this work, we... The latest data from the T2K and NOνA experiments show a tension in their preferred values of the oscillation parameters. In this work, we try to identify the... |
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SubjectTerms | Astronomy Astrophysics and Cosmology Data analysis Elementary Particles Experiments Hadrons Heavy Ions Measurement Science and Instrumentation Nuclear Energy Nuclear Physics Parameter identification Particle physics Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article - Theoretical Physics String Theory |
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Title | On the tension between the latest NOνA and T2K data |
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