Cristiano Bozza - Research activities

 

Cristiano Bozza has mainly been working on neutrino oscillations; he is in the OPERA Collaboration (long-baseline appearance experiment in the CNGS beam, with the detector located at the LNGS).

Current activities

Several Italian and European physicists are involved in the OPERA experiment, trying to detect the appearance of ντ in a pure beam of νμ. The CNGS beam, almost purely made of muon neutrinos, is produced at CERN towards the Laboratori Nazionali del Gran Sasso. During their travelling length (732 km) some muon neutrinos are expected to "transform" into tau neutrinos (neutrino oscillation). The OPERA detector, using lead as a target and nuclear emulsions as tracking devices, is expected to signal tau neutrino appearance.
It is the first time worldwide, and in particular in High Energy Physics, that nuclear emulsion are used on such a large scale.


Right: sketch of the CNGS beam line from CERN to Gran Sasso

OPERA is optimized to show the signal in the oscillation parameter region pointed at by the SuperKamiokande experiment. Cristiano Bozza is among the first proposers of OPERA to the SPSC. The OPERA discovery potential is extremely high, è estremamente elevato, thanks to the very low physical and instrumental background achieved through nuclear emulsions. In the SuperK favoured oscillation parameter region, OPERA is almost certain to observe oscillation signal; if not so, a vast oscillation parameter region would be excluded.

Right: probability to observe tau neutrinos, and exclusion plot in case of no appearance detection

Cristiano Bozza is the European Contactperson for the data-taking software of the European Scanning System (ESS), used in the OPERA experiment by all European labs to take data from nuclear emulsions.
The ESS (European Scanning System) uses high technology commercial components to set the world record in scanning speed on nuclear emulsions at 20 cm2/h/side with angular acceptance for microtracks up to tanθ=1.
The camera is a Mikrotron MC1310 with 1280x1024 pixel resolution in a 8-bit greyscale, operated at 376 fps (frames per second), with a data flux as large as 471 MB/s.
The mechanics have been developed by Micos in joint work with the European Emulsion Group, of which the Salerno Emulsion Group is part, and reaches a precision of 0.1 μm.
The optics has been developed byNikon in
joint work with the European Emulsion Group, of which the Salerno Emulsion Group is part, and provides corrected images on a field of view as large as 400 μm.
The motion controller is a National Instruments FlexMotion PCI 7344 card.
The image preprocessor, mainly used for 2D filtering, is a Matrox Odyssey XCL Pro.
The control workstation is a Dell Precision 650.

Right: one of the automatic microscopes running the ESS in the laboratory of the Salerno Emulsion Group

SySal, the ESS software, is mainly developed in Salerno by the Salerno Emulsion Group.
It is a flexible imaging system, developed with the commitment to be hardware-independent, and designed to adapt to very diverse real working conditions, able to work 24 hours per day without human assistance.
The system has been programmed mostly in C++ for the parts that directly interact with the microscope (although critical code sections have been written in Assembler), with an extensive use of COM/ActiveX. High level code (strategy control, decisions, etc.) have been written in C# using the .NET framework.
The software recognizes 3D microtracks in both thin and thick emulsion layers in realtime and with sustained flux.

Right: SySal snapshot

Cristiano Bozza is the Main Developer for the "OPERA Scanning Database" (the database that hosts OPERA emulsion data) and leads the development and management team, which involves scientists from several countries.
TheOPERA Scanning DB is a unique example in High Energy Physics of fully relational DB without external file
data sources. Real implementations of this DB can accept data at a rate between 30 and 60 MIph (Million INSERTs per hour), and the final size of the data set at the end of OPERA is foreseen to be between 30 and 100 TB.
The DB has an automatic data replication structure that makes data worldwide data sharing efficient while ensuring redundancy and data safety.

Right: data sharing schema among the various local sites

Cristiano Bozza has been measuring and analyzing interactions in nuclear emulsions from pion, muon and neutrino beams.
Several steps are needed for such activities:

  • data taking by the automatic microscope;
  • microtracks linking between either emulsion sides;
  • alignment and connection of tracks from originally stacked plates;
  • volume track reconstruction;
  • vertex reconstruction;
  • momentum/energy estimation and particle identification for event tracks;
  • kinematical reconstruction events;
  • physical interpretation.
Right: computer reconstruction of a pion interaction event in an OPERA ECC exposed to a pion beam at CERN (total length about 8 mm); data have been taken in the laboratory of the Salerno Emulsion Group

More information about OPERA are found by clicking on the experiment logo:

More information about Nuclear Emulsions


In the past Cristiano Bozza took part in the CHORUS experiment (short-baseline appearance for neutrino oscillations in the WBNB beam, with a detector located at CERN). He developed the SySal (System of Salerno) system on large inspection area Nikon microscopes, and he performed data analysis. The Salerno Emulsion Group contributed about 5% of the final statistics of CHORUS, and was deeply involved in studies about charm physics in emulsion. Click on the experiment logo to get more information.


 

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