Accelerator studies of neutrino oscillations

Ereditato, A.; Migliozzi, P.

doi:10.1007/bf03548892

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Hamiltonian and Perturbation Methods For Short-and Long-baseline Neutrino Oscillations1

Lorentz-violation Specific Signals In Neutrino Oscillations1

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2021

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“…Baselines are regarded as long or short based on their L/E ratio. L/E ∼ 0.01 = 10 km/GeV and L/E ∼ 100 = 10,000 km/GeV are taken as short and long baselines, respectively [153].…”

Section: Hamiltonian and Perturbation Methods For Short-and Long-baseline Neutrino Oscillationsmentioning

confidence: 99%

“…Here, ∆m 2 is the mass-squared difference between two oscillating neutrino flavors; there is an inverse proportionality to the first power of the energy and direct proportionality to the length of the baseline. Table 1 of Reference [153] is an example of a comparison of baseline and energy ranges for different settings. Neutrinos of nuclear reactions and solar neutrinos carry similar energies, while atmospheric and accelerator neutrinos have energies orders of magnitude higher.…”

Section: Lorentz-violation Specific Signals In Neutrino Oscillationsmentioning

confidence: 99%

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Astrophysical Neutrinos in Testing Lorentz Symmetry

Roberts

2021

Galaxies

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An overview of searches related to neutrinos of astronomical and astrophysical origin performed within the framework of the Standard-Model Extension is provided. For this effective field theory, key definitions, intriguing physical consequences, and the mathematical formalism are summarized within the neutrino sector to search for effects from a background that could lead to small deviations from Lorentz symmetry. After an introduction to the fundamental theory, examples of various experiments within the astronomical and astrophysical context are provided. Order-of-magnitude bounds of SME coefficients are shown illustratively for the tight constraints that this sector allows us to place on such violations.

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“…Baselines are regarded as long or short based on their L/E ratio. L/E ∼ 0.01 = 10 km/GeV and L/E ∼ 100 = 10,000 km/GeV are taken as short and long baselines, respectively [153].…”

Section: Hamiltonian and Perturbation Methods For Short-and Long-baseline Neutrino Oscillationsmentioning

confidence: 99%

Section: Lorentz-violation Specific Signals In Neutrino Oscillationsmentioning

confidence: 99%