POLAR: Design of a novel X-ray polarimeter based on plastic scintillators and multi-anode photomultipliers
- 1. POLAR collaboration and Integral Science Data Centre, Universite de Geneve, 1290 Versoix (Switzerland)
- 2. DPNC, Universite de Geneve, 1211 Geneve 4 (Switzerland)
Description
POLAR [1] is a space-borne hard X-ray polarimeter whose design has been optimized to measure the level of linear polarization of gamma-ray bursts (GRB) in the energy range 50-500 keV. In POLAR, the GRB photons undergo Compton scattering in a target made out of 1600 plastic scintillator bars (6x6x200 mm3 each). The azimuthal distribution of the scattered photons inside the target provides the information on the GRB polarization. The target is divided into 5x5 units, each one consisting of 8x8 scintillator bars optically coupled with a 64 channel multi-anode photomultiplier (MAPM, Hamamatsu H8500). POLAR, thanks to its large modulation factor (μ100 40%), its large effective area (Aeff = 400 cm2), and its large field of view (around 1/3 of the sky) will be able to determine the degree and angle of polarization of a strong GRB of energy 10-5 erg cm-2 s1 with a minimum detectable polarization of less than 10% (3σ). To be able to measure polarization of photons with energy as low as 50 keV, an energy threshold for each single channel of maximum 5 keV is required. This introduces strong constraints in the photon collection efficiency. To improve it, detailed studies of the scintillator bar surfaces and the available wrapping materials have been performed using both Monte Carlo simulations (GEANT4) and laboratory measurements. At present, a POLAR demonstration model (2 of the 25 units of the final design) is being tested in the laboratory. The engineering-qualification model will be ready in 2010. Investigations conducted by the POLAR instrument will provide very valuable information on how the X and γ-rays are emitted in GRBs. This way, an important contribution to the explanation of the particle acceleration will be achieved. We will present the design and status of POLAR with the newest results acquired from Monte Carlo simulations and from the demonstration model laboratory measurements. (authors)
Additional details
Identifiers
Publishing Information
- Publisher
- Institute of Experimental Physics, Slovak Academy of Sciences
- Imprint Place
- Kosice (Slovakia)
- ISBN
- 978-80-968060-5-8
- Imprint Title
- Proceedings of the 21. European Cosmic Ray Symposium
- Imprint Pagination
- 634 p.
- Journal Page Range
- p. 605-610
- Report number
- INIS-SK--2010-040
Conference
- Title
- 21. European Cosmic Ray Symposium
- Dates
- 9-12 Sep 2008
- Place
- Kosice (Slovakia)
INIS
- Country of Publication
- Slovakia
- Country of Input or Organization
- Slovakia
- INIS RN
- 41124707
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- CHARGED PARTICLES; CHERENKOV COUNTERS; CHERENKOV RADIATION; COSMIC GAMMA BURSTS; COSMIC GAMMA SOURCES; COSMIC PHOTONS; ELEMENTARY PARTICLES; ENERGY DEPENDENCE; EQUATIONS; EXPERIMENTAL DATA; GAMMA ASTRONOMY; HIGH ENERGY PHYSICS; MONTE CARLO METHOD; NUCLEAR PHYSICS; PLASTIC SCINTILLATION DETECTORS; PRIMARY COSMIC RADIATION
- Descriptors DEC
- ASTRONOMY; BOSONS; CALCULATION METHODS; COSMIC RADIATION; COSMIC RAY SOURCES; DATA; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; INFORMATION; IONIZING RADIATIONS; MASSLESS PARTICLES; MEASURING INSTRUMENTS; NUMERICAL DATA; PHOTONS; PHYSICS; PRIMARY COSMIC RADIATION; RADIATION DETECTORS; RADIATIONS; SCINTILLATION COUNTERS; SOLID SCINTILLATION DETECTORS
Optional Information
- Notes
- 10 figs., 8 refs.