Probing for heavy neutral leptons at DUNE and ICARUS
The Standard Model has for a long time been successful in describing the world around, that is, until the discovery of neutrino oscillations. This led to the understand- ing that neutrinos were not massless as originally thought, and requires physics beyond the Standard Model. A possible solution...
محفوظ في:
المؤلف الرئيسي: | |
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مؤلفون آخرون: | |
التنسيق: | Final Year Project |
اللغة: | English |
منشور في: |
Nanyang Technological University
2024
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الموضوعات: | |
الوصول للمادة أونلاين: | https://hdl.handle.net/10356/175662 |
الوسوم: |
إضافة وسم
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المؤسسة: | Nanyang Technological University |
اللغة: | English |
الملخص: | The Standard Model has for a long time been successful in describing the world
around, that is, until the discovery of neutrino oscillations. This led to the understand-
ing that neutrinos were not massless as originally thought, and requires physics beyond
the Standard Model. A possible solution to this problem is the proposal of the existence
of so called Heavy Neutral Leptons. These Heavy Neutral Leptons are proposed to
mix with the Standard Model neutrino flavours, but they are much heavier than them.
To fully test this theory and discover the behaviour of such new objects, methods to
produce and detect them are needed. These methods allow physicists to probe into
uncharted waters upon finding the Heavy Neutral Leptons, that can possibly solve
more unanswered questions by the Standard Model such as why is there more matter
than antimatter in the Universe? Or what is dark matter which is found abundantly
in the Universe? This thesis presents contributions to the current simulations that are
done at the DUNE and ICARUS experiments, by performing the sensitivity analysis
of the detectors in probing for these new particles. For DUNE, the current simulations
are developed further to enable adding additional features leading to a more accurate
version that goes more in line with recent theoretical developments. For ICARUS, the
actual background data obtained from cosmic muons, acting as noise are used to obtain
the most realistic estimations of the sensitivity. |
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