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SUMMARY:Data analysis strategy used for the detection of CNO solar neutrin
 os with Borexino
DTSTART;VALUE=DATE-TIME:20210830T171500Z
DTEND;VALUE=DATE-TIME:20210830T173000Z
DTSTAMP;VALUE=DATE-TIME:20261011T085037Z
UID:indico-contribution-15560@indico.ific.uv.es
DESCRIPTION:Speakers: Luca Pelicci (Forschungszentrum and RWTH University)
 \nBorexino is a large liquid scintillator experiment located at the underg
 round INFN Laboratori Nazionali del Gran Sasso\, in Italy. It was designed
  and built with the primary goal of real-time detection of low energy sola
 r neutrinos\, and in more than ten years of data taking it has measured al
 l the neutrino fluxes produced in the proton-proton-chain\, i.e. the main 
 fusion process accounting for ~99% of the energy production in the Sun. Re
 cently\, after improvements and developments in both hardware and software
 \, Borexino has provided the first observation of solar neutrinos emitted 
 from the subdominant Carbon-Nitrogen-Oxygen (CNO) fusion cycle. One of the
  key aspects of the analysis is the effectiveness and the performances of 
 the multivariate fitting technique adopted to disentangle the neutrino sig
 nals from the backgrounds present in the detector. All the crucial steps o
 f the analysis strategy adopted to extract the interaction rate of CNO neu
 trinos will be described in this poster.\n\nhttps://indico.ific.uv.es/even
 t/6178/contributions/15560/
LOCATION:
URL:https://indico.ific.uv.es/event/6178/contributions/15560/
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