Brunetti, Giulia
(2011)
Neutrino velocity measurement with the OPERA experiment in the CNGS beam, [Dissertation thesis], Alma Mater Studiorum Università di Bologna.
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Abstract
In the thesis is presented the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam, a muon neutrino beam produced at CERN. The OPERA detector observes muon neutrinos 730 km away from the source.
Previous measurements of the neutrino velocity have been performed by other experiments.
Since the OPERA experiment aims the direct observation of muon neutrinos oscillations into tau neutrinos, a higher energy beam is employed. This characteristic together with the higher number of interactions in the detector allows for a measurement with a much smaller statistical uncertainty.
Moreover, a much more sophisticated timing system (composed by cesium clocks and GPS receivers operating in “common view mode”), and a Fast Waveform Digitizer (installed at CERN and able to measure the internal time structure of the proton pulses used for the CNGS beam), allows for a new measurement with a smaller systematic error.
Theoretical models on Lorentz violating effects can be investigated by neutrino velocity measurements with terrestrial beams.
The analysis has been carried out with blind method in order to guarantee the internal consistency and the goodness of each calibration measurement.
The performed measurement is the most precise one done with a terrestrial neutrino beam, the statistical accuracy achieved by the OPERA measurement is about 10 ns and the systematic error is about 20 ns.
Abstract
In the thesis is presented the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam, a muon neutrino beam produced at CERN. The OPERA detector observes muon neutrinos 730 km away from the source.
Previous measurements of the neutrino velocity have been performed by other experiments.
Since the OPERA experiment aims the direct observation of muon neutrinos oscillations into tau neutrinos, a higher energy beam is employed. This characteristic together with the higher number of interactions in the detector allows for a measurement with a much smaller statistical uncertainty.
Moreover, a much more sophisticated timing system (composed by cesium clocks and GPS receivers operating in “common view mode”), and a Fast Waveform Digitizer (installed at CERN and able to measure the internal time structure of the proton pulses used for the CNGS beam), allows for a new measurement with a smaller systematic error.
Theoretical models on Lorentz violating effects can be investigated by neutrino velocity measurements with terrestrial beams.
The analysis has been carried out with blind method in order to guarantee the internal consistency and the goodness of each calibration measurement.
The performed measurement is the most precise one done with a terrestrial neutrino beam, the statistical accuracy achieved by the OPERA measurement is about 10 ns and the systematic error is about 20 ns.
Tipologia del documento
Tesi di dottorato
Autore
Brunetti, Giulia
Supervisore
Dottorato di ricerca
Scuola di dottorato
Scienze matematiche, fisiche ed astronomiche
Ciclo
23
Coordinatore
Settore disciplinare
URN:NBN
Data di discussione
20 Maggio 2011
URI
Altri metadati
Tipologia del documento
Tesi di dottorato
Autore
Brunetti, Giulia
Supervisore
Dottorato di ricerca
Scuola di dottorato
Scienze matematiche, fisiche ed astronomiche
Ciclo
23
Coordinatore
Settore disciplinare
URN:NBN
Data di discussione
20 Maggio 2011
URI
Gestione del documento: