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Program - Brookhaven National Laboratory

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CALIFA, a Calorimeter for the R3B/FAIR experiment<br />

D. Cortina-Gil, for the R3B collaboration<br />

Universidad de Santiago de Compostela<br />

The R3B experiment (Reactions with Relativistic Radioactive Beams) at FAIR (Facility for Antiproton and<br />

Ion Research) is a versatile setup dedicated to the study of reactions induced by high-energy radioactive<br />

beams. It will provide kinematically complete measurements with high efficiency, acceptance and resolution,<br />

making possible a broad physics program with rare-isotopes that addreses very relevant questions<br />

such as the structure of the atomic nucleus at the extreme of nuclear stability or reactions of astrophysics<br />

interest. CALIFA (CALorimeter for In-Fligth emitted pArticles), is a complex detector based on scintillation<br />

crystals, that will surround the target of the R3B experiment. CALIFA will act as total absorption<br />

gamma-calorimeter and spectrometer, as well as identifier of charged particles from target residues. This<br />

versatility is its most challenging requirement, demanding a huge dynamic range, to cover from low energy<br />

gamma-rays up to 300 MeV protons. This fact, along with the high-energy of the beams determine the<br />

conceptual design of the detector that will be presented in this paper together with the technical solutions<br />

proposed for its construction.<br />

HF 7 5:30 PM<br />

Atomic Number Determination of Fission Products by Digital Techniques<br />

J. Matarranz, I. Tsekhanovich<br />

Universite de Bordeaux-1/CENBG, 33175 Gradignan Cedex, France<br />

A.G. Smith, J.A. Dare, L. Murray, A.J. Pollitt<br />

Department of Physics and Astronomy, The University of Manchester, M13 9PL Manchester, UK<br />

T. Soldner, U. Koster<br />

Institut Laue-Langevin, 6 rue J. Horowitz, 38042 Grenoble, France<br />

D.C. Biswas<br />

Bhabha Atomic Research Centre, Trombay, 400085 Mumbai, India<br />

Determination of atomic numbers of non-accelerated fission products by non-radiative methods is a longstanding<br />

experimental problem. Correct fragment identification (i.e., by mass and atomic number) is<br />

relevant to the production probability (yield) of nuclei in low-energy fission reactions and is of interest to<br />

different domains of research incuding nuclear data for industry and spectroscopic studies of exotic nuclei.<br />

The difficulty in atomic number assignment is determined by the difference in the energy lost in a detector<br />

by fragments with adjacent nuclear charges. This difference is small and comparable to the detector<br />

energy resolution, whereas the range of nuclei to identify is relatively wide. An additional complication<br />

comes also from the fact that these subtle changes in the loss of energy between nuclei do not remain the<br />

same over the range of kinetic energies with which nuclei are produced in fission. Therefore assignment<br />

of atomic numbers to fission products is possible only if thorough care is given to the collection of the<br />

ionisation produced in the detector and to the consequent electronic treatment of signals. This approach<br />

is implemented in the design of the two-arm spectrometer of fission products (STEFF) recently built at<br />

the Manchester University. In addition to the identification of masses, by the double energy / double<br />

velocity measurement, the spectrometer is capable of delivering information on nuclear charges of fission<br />

products, on the event-by-event basis. This is achieved from the analysis of the fragments’ pulse shapes and<br />

ranges in gaseous detectors, both obtained using digital electronics in conjunction with specially developped<br />

algorithms. The technique has been optimised with beams of fission products with known kinetic energy<br />

and isobaric composition, as well as tested in the 235 U(nth, f) experiment at the ILL in France. The details<br />

of the method will be presented and explained, results on the identification of atomic numbers in the light<br />

group of fission products will be demonstrated and the perspectives discussed.<br />

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