andrey alexandrov (infn-napoli) on behalf of the news ... · system, a. alexandrov et al., 2014...

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The Dark Matter (DM) existence is one of the most open and discussed questions nowadays. The best candidates are so-called Weakly Interactive Massive Particles (WIMPs) with mass ranging from few GeV to a few TeV that interact with ordinary matter with cross sections typical or smaller than that of the weak processes. The motion of the Sun inside the galaxy causes an anisotropy in direction of WIMP-induced nuclear recoils, and, as it has never been observed, its evidence would unambiguously prove the existence of WIMP particles as DM constituents, which makes the directional DM search an extremely interesting and important issue from the point of view of fundamental science. Nuclear emulsion is a perfect choice for a detector for directional DM search because of its high density and the best position accuracy. The track length of recoil nuclei in emulsion is of the order of 100 nm, making the resolution of conventional optical microscopes insufficient to resolve them. Here we report about the R&D on a super-resolution optical microscope to be used in a future directional DM search experiment with nuclear emulsion as a detector media. The microscope will be fully automatic, will use novel image acquisition and analysis techniques, will achieve the spatial resolution of the order of few tens of nm and will be capable of reconstructing recoil tracks with the length of at least 100 nm with high angular resolution. ABSTRACT SCANNING SYSTEM TEST WITH C-ION BEAM 13th Pisa Meeting on Advanced Detectors, La Biodola, Isola d'Elba (Italy), May 24 - 30, 2015 Andrey Alexandrov (INFN-Napoli) on behalf of the NEWS collaboration E-mail: [email protected] ELLIPTICITY ANALYSIS POLARIZATION ANALYSIS Nuclear emulsion Target nuclei DM DM Direction of solar system (230km/sec) earth@summer earth@winter Dark matter wind DM Detection of recoiled nuclei as tracks Direction sensitive Detector How long is the recoil in emulsion? Nikon Oil Objective 100x, 1.45 N.A., Plan Apo Magnifying lens, Nikon VM C-2.5x Bonito CL/CMC-4000 CMOS Camera 4 Mpix UV LED λ=406 nm Optical resolution: 207 nm Dig. resolution: 27 nm/pixel View Size: 65 x 48 µm Rotatable Polarizer DIRECTIONAL SIGNATURE Ag 100 nm spherical no polarizing property Ag 100 nm spheroidal polarizing property H.Tamaru et al ., Applied Phys Letters 80, 1826 (2002) Scattering spectrum depends on the grain shape 171 nm 1.1 μm Elli 1.48 281 nm 1.1 μm Elli 1.68 gap Angular difference Angular resolution = 235 mrad = 13° L W ϕ X,Y Elliptical Fit Parameters Silver grains in emulsion are nanoparticles Grains tend to have spheroidal shape The reflected light is polarized Polarization angle depends on grain orientation Grain orientation is random With the analysis of the reflected light polarization it is possible to isolate individual grains With polarization analysis reconstruction of tracks with the length of 100 nm becomes possible Additional studies are in progress to push recoil length limit to below 100 nm The sequence of several grains making a track of a few hundred nm appears as a single cluster A cluster made of several grains tends to have an elliptical shape with the major axis coincident with the direction of the trajectory A cluster produced by a single grain tends to have a spherical shape With cluster ellipticity analysis it is possible to locate sub-resolution tracks and determine their direction Y axis σ = 10.51 nm X axis σ = 10.24 nm Position accuracy = 10.5 nm Sample irradiated with 80 keV Carbon ions = Ellipticity cut efficiency 1 kg – 50 nm 10 kg – 50 nm 1 kg – 100nm 10 kg – 100 nm 1 kg – 200nm 10 kg – 200 nm Sensitivity with a small detector *-X *-Y Displacement of the cluster mass center with change of polarization angle *-X *-Y Fog grain Track The microscope operation, DAQ and analysis is performed by the LASSO (Large Angle Scanning System, A. Alexandrov et al., 2014 JINST 9 C02034) Implemented a dedicated module to perform a 3D track reconstruction and ellipticity analysis Work on integration of a rotatable polarizer and implementation of a module for polarization analysis is in progress

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  • The Dark Matter (DM) existence is one of the most open and discussed questionsnowadays. The best candidates are so-called Weakly Interactive Massive Particles(WIMPs) with mass ranging from few GeV to a few TeV that interact with ordinarymatter with cross sections typical or smaller than that of the weak processes. Themotion of the Sun inside the galaxy causes an anisotropy in direction of WIMP-inducednuclear recoils, and, as it has never been observed, its evidence would unambiguouslyprove the existence of WIMP particles as DM constituents, which makes the directionalDM search an extremely interesting and important issue from the point of view offundamental science. Nuclear emulsion is a perfect choice for a detector for directionalDM search because of its high density and the best position accuracy. The track length ofrecoil nuclei in emulsion is of the order of 100 nm, making the resolution of conventionaloptical microscopes insufficient to resolve them. Here we report about the R&D on asuper-resolution optical microscope to be used in a future directional DM searchexperiment with nuclear emulsion as a detector media. The microscope will be fullyautomatic, will use novel image acquisition and analysis techniques, will achieve thespatial resolution of the order of few tens of nm and will be capable of reconstructingrecoil tracks with the length of at least 100 nm with high angular resolution.

    ABSTRACT

    SCANNING SYSTEMTEST WITH C-ION BEAM

    13th Pisa Meeting on Advanced Detectors, La Biodola, Isola d'Elba (Italy), May 24 - 30, 2015

    Andrey Alexandrov (INFN-Napoli) on behalf of the NEWS collaboration

    E-mail: [email protected]

    ELLIPTICITY ANALYSIS POLARIZATION ANALYSIS

    Nuclear emulsion

    Target nuclei

    DM

    DM

    Direction of solar system(230km/sec)

    earth@summer

    earth@winter

    Dark

    matter

    wind

    DM

    Detection of recoiled nuclei as tracks Direction sensitive Detector

    How long is the recoilin emulsion?

    Nikon Oil Objective100x, 1.45 N.A., Plan Apo

    Magnifying lens,Nikon VM C-2.5x

    Bonito CL/CMC-4000CMOS Camera4 Mpix

    UV LED λ=406 nm

    Optical resolution: 207 nmDig. resolution: 27 nm/pixelView Size: 65 x 48 µm

    Rotatable Polarizer

    DIRECTIONAL SIGNATURE

    Ag 100 nm sphericalno polarizing property

    Ag 100 nm spheroidal polarizing property

    H.Tamaru et al ., Applied Phys Letters 80, 1826 (2002)

    Scattering spectrum depends on the grain shape

    171 nm

    1.1 μm

    Elli 1.48

    281 nm

    1.1 μm

    Elli 1.68

    gap

    Angular difference

    Angular resolution = 235 mrad = 13°

    L

    W

    ϕ

    X,Y

    Elliptical Fit Parameters

    • Silver grains in emulsion are nanoparticles• Grains tend to have spheroidal shape• The reflected light is polarized• Polarization angle depends on grain orientation• Grain orientation is random• With the analysis of the reflected light polarization

    it is possible to isolate individual grains• With polarization analysis reconstruction of tracks

    with the length of 100 nm becomes possible• Additional studies are in progress to push recoil

    length limit to below 100 nm

    • The sequence of several grains making a track of a fewhundred nm appears as a single cluster

    • A cluster made of several grains tends to have anelliptical shape with the major axis coincident with thedirection of the trajectory

    • A cluster produced by a single grain tends to have aspherical shape

    • With cluster ellipticity analysis it is possible to locatesub-resolution tracks and determine their direction

    Y axis σ = 10.51 nmX axis σ = 10.24 nm

    Position accuracy = 10.5 nm

    Sample irradiated with 80 keV Carbon ions

    𝐸𝑓𝑓 =𝑁𝑒𝑥𝑝𝑜𝑠𝑒𝑑 𝑎𝑟𝑒𝑎𝑎𝑓𝑡𝑒𝑟 𝑐𝑢𝑡

    −𝑁𝑚𝑎𝑠𝑘 𝑎𝑟𝑒𝑎𝑎𝑓𝑡𝑒𝑟 𝑐𝑢𝑡

    𝑁𝑒𝑥𝑝𝑜𝑠𝑒𝑑 𝑎𝑟𝑒𝑎𝑏𝑒𝑓𝑜𝑟𝑒 𝑐𝑢𝑡

    −𝑁𝑚𝑎𝑠𝑘 𝑎𝑟𝑒𝑎𝑏𝑒𝑓𝑜𝑟𝑒 𝑐𝑢𝑡

    Ellipticity cut efficiency

    1 kg – 50 nm10 kg – 50 nm

    1 kg – 100nm10 kg – 100 nm

    1 kg – 200nm10 kg – 200 nm

    Sensitivity with a small detector

    * - X

    * - Y

    Displacement of the cluster mass center with change of polarization angle

    * - X

    * - Y

    Fog grain

    Track

    • The microscope operation, DAQ and analysis isperformed by the LASSO (Large Angle ScanningSystem, A. Alexandrov et al., 2014 JINST 9 C02034)

    • Implemented a dedicated module to perform a 3Dtrack reconstruction and ellipticity analysis

    • Work on integration of a rotatable polarizer andimplementation of a module for polarizationanalysis is in progress