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A high-flux upgrade for the BRISP spectrometer at ILL.
Zanatta, M; Barocchi, F; De Francesco, A; Farhi, E; Formisano, F; Guarini, E; Laloni, A; Orecchini, A; Paciaroni, A; Petrillo, C; Pilgrim, W-C; Suck, J-B; Sacchetti, F.
Affiliation
  • Zanatta M; Dipartimento di Informatica, Università di Verona, I-37134 Verona, Italy.
  • Barocchi F; Dipartimento di Fisica e Astronomia, Università di Firenze, I-50019 Sesto Fiorentino, Italy.
  • De Francesco A; IOM-CNR, Operative Group in Grenoble (OGG), c/o Institut Laue Langevin, F-38042 Grenoble, France.
  • Farhi E; Institut Laue Langevin, F-38042 Grenoble, France.
  • Formisano F; IOM-CNR, Operative Group in Grenoble (OGG), c/o Institut Laue Langevin, F-38042 Grenoble, France.
  • Guarini E; Dipartimento di Fisica e Astronomia, Università di Firenze, I-50019 Sesto Fiorentino, Italy.
  • Laloni A; IOM-CNR, Operative Group in Grenoble (OGG), c/o Institut Laue Langevin, F-38042 Grenoble, France.
  • Orecchini A; Dipartimento di Fisica e Geologia, Università di Perugia, I-06123 Perugia, Italy.
  • Paciaroni A; IOM-CNR, c/o Dipartimento di Fisica e Geologia, Università di Perugia, I-06123 Perugia, Italy.
  • Petrillo C; Dipartimento di Fisica e Geologia, Università di Perugia, I-06123 Perugia, Italy.
  • Pilgrim WC; Physikalische Chemie, Philipps Universität Marburg, D-35032 Marburg, Germany.
  • Suck JB; Institute of Physics, Technische Universität Chemnitz, D-09107 Chemnitz, Germany.
  • Sacchetti F; Dipartimento di Fisica e Geologia, Università di Perugia, I-06123 Perugia, Italy.
Rev Sci Instrum ; 88(5): 053905, 2017 May.
Article in En | MEDLINE | ID: mdl-28571465
ABSTRACT
To date, the BRISP spectrometer represents the state-of-the-art for every instrument aiming to perform Brillouin neutron scattering. Exploiting accurate ray-tracing McStas simulations, we investigate an improved configuration of the BRISP primary spectrometer to provide a higher flux at the sample position, while preserving all the present capabilities of the instrument. This configuration is based on a neutron guide system and is designed to fit the instrument platform with no modifications of the secondary spectrometer. These evaluations show that this setup can achieve a flux gain factor ranging from 3 to 6, depending on the wavelength. This can expand the experimental possibilities of BRISP towards smaller samples, possibly using also complex sample environments.

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2017 Document type: Article Affiliation country: Italy

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2017 Document type: Article Affiliation country: Italy
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