6–10 Sept 2021
Varenna, Villa Monastero
Europe/Rome timezone

Short_Oral_25: Conceptual design of a Cherenkov based gamma-ray diagnostic for measurement of 17 MeV gamma rays from T(D, γ)5He in magnetic confinement fusion plasmas

9 Sept 2021, 17:20
10m
Villa Monastero (Varenna, Villa Monastero)

Villa Monastero

Varenna, Villa Monastero

Short oral in replacement of poster

Speaker

Oscar Putignano (Istituto Nazionale di Fisica Nucleare)

Description

At present, the only method for assessing the fusion power throughput of a reactor relies on the absolute measurement of 14 MeV neutrons produced in the D-T nuclear reaction. [1]
For ITER and DEMO, however, at least another independent measurement of the fusion power is required.
The 5He nucleus produced in the D-T fusion reaction has two de-excitation channels. The most likely is its disintegration in a particle and a neutron, D+T→5He→α+n, by means of the nuclear force. There is however also an electromagnetic channel, with a branching ratio ~10-5, which leads to the emission of a 17 MeV gamma-ray, i.e. D+T→5He*→ 5He+γ. [2] The detection of this gamma-ray emission could serve as an independent method to determine the fusion power.
In order to enable 17 MeV gamma-ray measurements, there is need for a detector with some coarse energy discrimination and, most importantly, capable to work in a neutron rich environment.
Conventional inorganic scintillators, such as LaBr3(Ce), have comparable efficiencies to neutrons and gamma rays and they cannot be used for 17 MeV gamma-ray measurements without significant neutron shielding.
In order to overcome this limitation, we here propose the conceptual design of a gamma ray counter with a variable energy threshold based on the Cherenkov effect and designed to operate in intense neutron fields.
The detector geometry has been optimized using Geant4 so to achieve a gamma-ray to neutron efficiency ratio better than 105. The design is based on a gas Cherenkov detector and uses a CsI coated scintillating GEM (Gas Electron Multiplier) as photon pre-amplifier, together with a wavelength shifter to minimize the sensitivity to neutrons.
Photons produced in the GEM are collected by an optical window and a bundle of optical fibers, which guides them towards an array of silicon photomultipliers (SiPMs) located further away from the plasma, in a region at low nuclear radiation.

References
[1] L. Bertalot et al., "Fusion Power Measurement at ITER," in IEEE Transactions on Nuclear Science, vol. 63, no. 3, pp. 1682-1687, June 2016, doi: 10.1109/TNS.2016.2553125.
[2] F. E. Cecil et al, “Measurement and application of DDγ, DTγ and D3Heγ reactions at low energy.” Netherlands: N. p., 1985. Web.
[3] S. Agostinelli er al. “Geant4—a simulation toolkit”, Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment,V 506, Issue 3, 2003, 250-303.

Primary authors

Oscar Putignano (Istituto Nazionale di Fisica Nucleare) Gabriele Croci Andrea Muraro (IFP-CNR) Ms Stephanie Cancelli (Unimib) Luca Giacomelli (ISTP-CNR) Giuseppe Gorini (Universita' degli Studi di Milano-Bicocca) Dr Giovanni Grosso (Consiglio Nazionale delle Ricerche, Istituto per la Scienza e Tecnologia dei Plasmi, Milano ) Matteo Hakeem Kushoro (Università degli Studi Milano Bicocca) Ms Marcer Giulia (UNIMIB) Massimo Nocente (Dipartimento di Fisica - Università di Milano-Bicocca) Enrico Perelli Cippo (Istituto per la Scienza e Tecnologia dei Plasmi - CNR) Marica Rebai (MIB) Marco Tardocchi (Istituto di Fisica del Plasma "Piero Caldirola",CNR) Marco Tardocchi (Istituto di Fisica del Plasma "Piero Caldirola",CNR)

Presentation materials