Email: mikko.i.laitinen@jyu.fi Large area transition-edge sensor array for particle induced X-ray emission spectroscopy M Palosaari1, K Kinnunen1, I Maasilta1,

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email: mikko.i.laitinen@jyu.fi Large area transition-edge sensor array for particle induced X-ray emission spectroscopy M Palosaari1, K Kinnunen1, I Maasilta1, C Reintsema2, D Schmidt2, J Fowler2, R Doriese2, J Ullom2, M Käyhkö1, J Julin1, Mikko Laitinen1, T Sajavaara1 1Department of Physics, University of Jyväskylä, P.O. Box 35, Jyväskylä 40014, Finland 2National Institute of Standards and Technology, Boulder CO 80305, United States email: mikko.i.laitinen@jyu.fi

INTRODUCTION to TES Superconducting Transition-Edge Sensor

Transition-Edge Sensor (TES) TES as a calorimeter Measures the energy of incident radiation Schematics of a calorimeter Typical pulse from a calorimeter

Superconducting state TES Operation Operates between superconducting and normal state Extremely sensitive R(T) Excellent energy resolution Wide energy range Detects radiation, in our case X-rays Particles also possible Normal state transition edge Superconducting state Typical transition of a TES

TES basics TES thin film device is made of normal metal - superconducting metal bilayer. The absorber details depend on the desired energy range. TESs are usually fabricated on thin SiN membranes to limit the thermal conductivity G. In typical TES array, all pixels different -> automated calibration essential Photograph of a 256 pixel TES array made in VTT, Finland.

PIXE-TES SETUP IN JYVÄSKYLÄ

PIXE-TES Setup in Jyväskylä

Details inside the instrument ~15 mm ~300 mm

Jyväskylä TES specifications 160 pixels from NIST, upgradable to 256 (from VTT) Total area with 160 pixels ~16 mm2 Single pixel count rate limited to <20 Hz, typical value 10 Hz 2 mm thick Bi absorber with Mo/Cu superconducting juction Detection efficiencies with 100 um of Be: 80 % at 5 keV, 20 % at 10 keV, 5 % at 30 keV Low energies limited by MeV particle absorber, probably not needed

PIXE-TES MEASUREMENTS From a single pixel to many…

PIXE-TES results from Jyväskylä Roughly one year ago: 12 pixels Mn Kα from Fe-55 source Best pixel Instrumental resolution for the best pixel with 55Fe source was 3.06 eV

PIXE-TES results from Jyväskylä Now: 160 pixels… But, Computer interface and I/O cards cannot handle all pixels simultaneously I/O card + PC update coming from NIST to finally secure the function of all 256 possible channels, simultaneously. This month: data with Fe-55 source Resolution around 5 eV for combined 40 pixels, Improvement seen by better data analysis

PIXE-TES results from Jyväskylä SRM-611, trace elements in glass All TES data shown was analyzed last week, 1 eV / bin Analysis resolution for all of these plots ~10 eV

PIXE-TES results from Jyväskylä SRM-611, trace elements in glass

PIXE-TES results from Jyväskylä SRM-611, trace elements in glass Differences between pixels which are not only statistics

PIXE-TES results from Jyväskylä SRM-1157, speciality tool steel No Si escape peak Bi escape peaks Single measurement, wide energy range

PIXE-TES results from Jyväskylä SRM-1157, speciality tool steel V, Cr, Mn, Fe separated

In the Near Future Read-out upgraded to full scale. Modification of PIXE setup to be able to measure samples in atmosphere. Study art samples in a project that just started X-ray measurements with our own detector array fabricated by VTT. Study the satellite peaks with different ions and energies. ->> Chemical information from wide energy/elemental range ???

Conclusions Instrumental resolution of 3 eV demonstrated Combined pixel resolution of ~5 eV looks realistic Wide energy scale (“0” to tens of keV) Reasonable count rates available (10 Hz/pixel, 256 pixels) Active detector area about 16 mm2 No liquid He needed for ADR cryo cooler Largish instrument: ~5 cm sample-to-detector Data handling and analysis: automation necessary Is the chemical information achievable, after all ?

Acknowledgements

t 3-8. July, 2016, in Jyväskylä, Finland

Pixel calibration Single pixel shows Si peaks nicely but without good calibration, sum spectrum useless Sample: SRM-611 No/bad calibration regime good calibration

TES-PIXE data calibration Raw pulse height data where sample was changed. Sample 1 Sample 2 Eenergy scale Substrate was Si for both samples Measurement time/duration

TES-PIXE data Making selection to single (example) emission line Before liner fit Straight line to guide the eye

Straight line to guide the eye TES-PIXE data After linear fit Si Si Straight line to guide the eye

Nitride hits

PIXE Mn vs. 55Fe What is the origin of the hump? Mn Kα from Fe55 source same pixel What is the origin of the hump?

Detector performance: PIXE Mn vs. 55Fe source Instrumental resolution for the best pixel with 55Fe source was 3.06 eV. For 2 MeV protons and Mn sample resolution was 4.20 eV. M. Palosaari et. al J. Low Temp. DOI 201310.1007/s10909-013-1004-5

PIXE applications Traditional PIXE applications Archaeology Geology Filters in industry Old paintings Rev. Sci. Instrum. 78, 073105 (2007) J. Hasegawa et. al With better detectors one could see the chemical environment of the sample.

TES vs. SDD Impurities in the Cu sample resolved better with TES detector

Stainless steel example

PIXE Mn vs. 55Fe FWHM broadens less than 1eV. Mn Kα from Fe55 source same pixel FWHM broadens less than 1eV.

TES vs. SDD

TES circuit diagram

Example: Thin film with high mass element Atomic layer deposited Ru film on HF cleaned Si Scattered beam, 35Cl, used for Ru deph profile Monte Carlo simulations needed for getting reliable values for light impurities at the middle of the film Ru SiO2 Si Metallic films have traditionally been difficult to deposit with ALD. This is one example of ongoing analysis of these Ru thin films. Scattered 35Cl is used for Ru depth profile, recoiled Ru suffers too much from multiple scattering. Poor E resolution Low energy heavy ion ERDA – See posters!

Example: Diamond-like carbon films 2.3 µm thick diamond-like-carbon film on Si, measured with 9 MeV 35Cl All isotopes can be determined for light masses Light elements can be well quantified (N content 0.05±0.02 at.%) Menetelmä soveltuu bulk-näytteiden mittaamiseen. Low energy heavy ion ERDA

ALD 8.6 nm Al2O3/Si Atomic layer deposited Al2O3 film on silicon (Prof. Ritala, U. of Helsinki) Density of 2.9 g/cm3 and thickness of 8.6 nm determined with XRR (Ritala) Elemental concentrations in the film bulk as determined with TOF ERDA are O 60±3 at.%, Al 35±2 at.%, H 4±1 at.%. and C 0.5±0.2 at.% Parhaimmillaan menetelmä on ohutkalvotutkimuksessa. hiili eroaa pinnassa ja rajapinnassa (surface and interface).

10 nm CNx on silicon TOF-ERDA results from sputter deposited 10 nm thick CNx hard coating on Si. Measured with 6 MeV 35Cl beam and extreme glancing angle of 3° A density of 2.0 g/cm3 was used in converting areal densities to nm Tavalliset jorinat, kehutaan syvyysresoluutiota. Mainitaan kalvossa näkyvän aikaismman kasvatuksen jäljiltä fluoria sekä kromia + sputteroinnista johtuen argonia. 38

Effect of stripper gas pressure 13.6 MeV 63Cu7+ CaPO (hydroxyapatite)

Gas ionization detector Thin (~100 nm) SiN window Electrons for T2 timing signal emitted from the membrane Myös etusironneita elektroneja: paikkaherkkään anodiin 40

Future improvements: Gas ionization detector 30 mm Massaerotuskyky raskaammille massoille paranee huomattavasti, huomaa mm Si:n isotoopit TOF-E results from ETH Zürich Incident ion 12 MeV 127I and borosilicate glass target 200 nm thick SiN membrane from Aalto University, Finland, on 100 mm wafer Nucl. Instr. and Meth. B 248 (2006) 155-162

Gas ionization detector to replace Si-energy detector Why try to fix a well working system? Greatly improved energy resolution for low energy heavy ions → heavier masses can be resolved Gas detector is 1D position sensitive by nature → possibility for kinematic correction and therefore larger solid angles possible Gas detector does not suffer from ion bombardment Recoil ranges in isobutane 10.2 MeV 79Br 8.5 MeV 35Cl Gas ionization detector develoment – See posters!