Copyright © 2007 Elsevier B.V. All rights reserved.
The nylon scintillator containment vessels for the Borexino solar neutrino experiment
Received 13 August 2007;
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Abstract
Borexino is a solar neutrino experiment designed to observe the 0.86 MeV neutrinos emitted in the pp cycle of the sun. Neutrinos will be detected by their elastic scattering on electrons in 100 ton of liquid scintillator. The neutrino event rate in the scintillator is expected to be low (
0.35 events per day per ton), and the signals will be at energies below 1.5 MeV, where background from natural radioactivity is prominent. Scintillation light produced by the recoil electrons is observed by an array of 2240 photomultiplier tubes. Because of the intrinsic radioactive contaminants in these PMTs, the liquid scintillator is shielded from them by a thick barrier of buffer fluid. A spherical vessel made of thin nylon film contains the scintillator, separating it from the surrounding buffer. The buffer region itself is divided into two concentric shells by a second nylon vessel in order to prevent inward diffusion of radon atoms. The radioactive background requirements for Borexino are challenging to meet, especially for the scintillator and these nylon vessels. Besides meeting requirements for low radioactivity, the nylon vessels must also satisfy requirements for mechanical, optical, and chemical properties. The present paper describes the research and development, construction, and installation of the nylon vessels for the Borexino experiment.
Keywords: Borexino; Solar neutrinos; Nylon; Organic scintillator; Low-background
PACS classification codes: 29.40.Mc; 26.65.+t; 81.05.Lg
Article Outline
- 1. Introduction and overview of the Borexino experiment
- 2. The design requirements for the vessels
- 3. Production and selection of nylon film
- 3.1. Production of the nylon film
- 3.1.1. Radiopurity levels of the nylon pellets
- 3.1.2. The nylon film extrusion process
- 3.1.3. Pre-cleaning of the nylon film
- 3.2. Selection of the nylon film
- 3.2.1. Chemical compatibility
- 3.2.2. Mechanical measurements
- 3.2.3. Optical measurements
- 3.2.4. Radioactivity requirements and measurements
- 3.2.5. Film selection summary
- 4. Fabrication of the nylon vessels
- 4.1. Clean room design and control of radon exposure
- 4.2. Fabrication of the nylon envelopes
- 4.3. The polar region design and tube assemblies
- 4.4. The ropes
- 4.5. Instrumentation
- 4.5.1. Temperature sensors
- 4.5.2. Load cells
- 4.5.3. Calibration light sources and optical fibers
- 4.5.4. Feed-through connections
- 4.5.5. Radioactivity measurements for instrumentation elements
- 4.6. Leak tightness specifications and leak checking
- 4.7. Calculated stresses on the nylon film
- 5. Shipping and installation in Gran Sasso
- 5.1. Packaging and shipping
- 5.2. Installation of the nylon vessels
- 5.3. Inflation with synthetic air
- 5.3.1. Radon limits on synthetic air
- 5.3.2. Leak rate tests
- 5.4. Pressure control and DCS in filling stations
- 5.5. Purging with nitrogen
- 6. Summary of radiopurity
- 6.1. Gamma backgrounds
- 6.2. Radon diffusion through nylon
- 6.2.1. Permeability of nylon to radon
- 6.2.2. Radon emanation from nylon
- 6.2.3. Principle of the OV barrier
- 7. Conclusions
- Acknowledgements
- References






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100 ton), consistent with predictions of Standard Solar Models and neutrino oscillations with LMA-MSW parameters.





