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Low Noise Front-End for HEP Experiments: Low Noise Front-End for HEP Experiments:

Low Noise Front-End for HEP Experiments: - PowerPoint Presentation

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Low Noise Front-End for HEP Experiments: - PPT Presentation

from the Brookhaven Years to the Road Ahead In Memoriam of Franco Manfredi 19352015 Sergio Rescia Brookhaven National Laboratory Pavia 5 December 2016 2 Franco Manfredi the Brookhaven Days ID: 1031158

rescia noise detecting signals noise rescia signals detecting dec 2016 detector input voltage type franco manfredi high jfet physics

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1. Low Noise Front-End for HEP Experiments: from the Brookhaven Years to the Road AheadIn Memoriam of Franco Manfredi 1935-2015Sergio Rescia Brookhaven National LaboratoryPavia, 5 December 2016

2. 2Franco Manfredi: the Brookhaven DaysThe Supercollider Days and the Monolithic JFET Preamplifier Project… and its legacy… and the futureLow Noise Front-End for HEP Experiments: from the Brookhaven Years to the Road AheadA Symposium in Memoriam of Franco Manfredi Sergio Rescia rescia@bnl.govS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

3. Franco Manfredi3foto

4. 4Circa 1987-88 at BNL …S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

5. 5…. and in Milano.S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

6. Franco’s Philosohy:6Franco’s background was in physics.He had a keen interest both in device physics and detector physics.He was a strong believer in the Milano group’s (and Radeka’s Instrumentation Division) philosophy that the only real optimization is of the detector – readout electronics as a whole, starting from first principles and basic device/detector properties.S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

7. 7Superconducting Super ColliderFrom Wikipedia, the free encyclopediaS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

8. The Monolithic JFET Process Project8First we tried simply to work with Interfet to build larger JFETs (NJ450, NJ903, NJ1800, NJ3600)Based on our collective experience we soon thought to exploit the low noise properties, rad hardness, cryogenic capabilities of JFET to build a monolithic preamplifierInterfet (a spin-off of Texas Instruments) had access to Ti Simox material, and …. ODEtchIsolation OxideGrind-Lap-PolishPOLISHED SLICEPROCESSINGSilicon SubstratePatterned OxideORPatternOxideSiliconOxideSiliconOxidePolysiliconPolysiliconPolysilicon DepositionSiliconWaferFabricationS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

9. 9Dielectric isolation process devices. a): Devices built in adjacent tubs are connected by back to back diodes in series with a high value resistor due to the polysilicon bridge shown in b). If true isolation is needed, anisotropic etching can be employed to leave free standing “mesas” of silicon on a SiO2 floor.Dielectric Isolation ProcessS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

10. 1Starting wafer: 0.5 cm, N-type, (111) Silicon2Diffuse back-gate wells: 0.002 cm3Grow oxide: tox ~ 50 nm4Strip oxide, chemical clean and epi growth. tepi ~ 5-7 mRepi = 0.5 cm (L-type) and 1.5 cm (H-type)5Pattern and diffuse isolation ring (P-type)6Pattern gate and gate diffusion (P-type)7Pattern source and drain and diffusion (N-type)8Open contact window. Probe test structures. Gate targeting (by additional drive-in)9Nitride deposition (dielectric layer to isolate metal)10Evaporate and pattern metal (aluminum)11Nitride protective overcoatBURIED LAYER PROCESSS. Rescia "Detecting Signals into the Noise" 5 Dec. 201610

11. 11Temperature dependence of the transconductance gm before (white symbols) andafter (solid black symbols) a 55 Mrad g-ray irradiation for an implanted NJFET (W/L = 2500/5) in the saturation region (VDS = 2.5 V).TEMPERATURE DEPENDENCE (55Mrad)S. Rescia "Detecting Signals into the Noise"

12. 12Pinch-off voltage and drain current IDSS (VGS = 0) as a function of neutron fluence ata constant temperature of 95 K for devices of different channel resistivities. The curves have been normalized to the pre-irradiation values. The transistors have been irradiated and measured in the saturation region (VDS = 2.5 V) at T = 95 K.Neutron Damage: Vp and IDSSS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

13. 13Noise vs TemperatureS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

14. 14Noise vs g Irradiation (55Mrad)S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

15. 15Noise vs neutron irradiation (4E14n/cm2)S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

16. 16IPA3 Monolithic JFET PreamplifierS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

17. 17ParameterL-typeH-typeInput DeviceNJFET,W = 11400 m, L = 5 mOpen-loop input capacitance50 pF40 pFPower dissipation80 mWDC gain A0ZOUT = 10 k82 dB75 dBZOUT = 100 76 dB70 dBRise time (CD = 500 p, CF = 33 pF)15 nsNoise voltage /Hz](f > 1 kHz)T= 300 K0.60.7T = 120 K0.40.4Equivalent noise charge [e rms](RC)2 -(CR)2 bipolar shaping at tp = 50 nsENC = 1200 + 18 CDENC= 1100+ 21 CDIPA3 Monolithic JFET PreamplifierMeasured CharacteristicsS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

18. 18Time domain response of the output of the IO751 bi-linear preamplifier in the linear and non linear regions after the preamplifier (curves a, a’) and after shaping (curves b, b’) at tp = 50 ns. The input currents correspond to a LKr energy of 15 GeV (curves a and b) and 150 GeV (curves a’ and b’) and the vertical scales are also scaled by a factor of ten.Bi-linear transfer characteristics from LAr in to peak shaper out for the IO751 preamplifier. The break point is at 60 GeV, and the ratio of the two slopes is about 4.Bilinear CharacteristicsS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

19. 191993: Abrupt SSC CancellationThe R&D was quickly terminated.Yet to do:Monolithic ResistorsMonolithic CapacitorsDischarge Protection… but a rich heritage:Very low noise audio hearing aid Very large JFET DevelopmentProof of Principle of 10s of Mrad Radiation Hardness(one preamp was irradiated to 300Mrad, still working) S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

20. 20PHYSICS BASELELECTRONIC LAB MICHAEL STEINACHER KLINGELBERGSTR. 82 CH‐4056 BASEL SWITZERLANDLOW NOISE / HIGH STABILITY I TO V CONVERTERSP 983 WITH IF3602DATASHEET VERSION 1.2SEPTEMBER 2014FEATURESLow input voltage noise Typical input referred voltage noise: 2 nV/sqrt(Hz) @ 10 Hz1.2 nV/sqrt(Hz) @ 1 kHzStable and low drift input voltage Typical input voltage drift @25°C:±0.15 µV/KInput current noise level: 6.1 fA/sqrt(Hz) @10 Hz, 109 V/AFive decades of gain: 105…109 V/ABroadband (e.g. min. 20 kHz @ 108 V/A)Integrated low‐pass‐filter: 30 Hz…100 kHzRemote controllable gain and LP‐cutoffInput voltage can be shifted up to ±100 mV by an external offset voltageGreen LED indicates when input offset voltage is compensated and stableRed LED indicates overloaded conditionSMA input & output connectors / BNC‐adapters includedOverload protected current inputS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

21. 200pV/√Hz21x6 NJ3600Franco’s 200pV/√Hz amplifier:World Record?S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

22. LHC ATLAS Calorimeter (1990s-2000s)Challenging LHCHigh energy 14 TeVHigh collision rate : 40 MHzSmall branching ratios…Challenging calorimetryGood resolutionSmall constant term (<1%)Low dead materialChallenging electronicsLarge dynamic range (16 bits)Low noiseHigh speedHigh radiation hardnessChallenging scheduleBe ready for 1999 !S. Rescia "Detecting Signals into the Noise" 5 Dec. 201622

23. ATLAS @ LHCS. Rescia "Detecting Signals into the Noise" 23

24. DUNE neutrino Experiment (Lar)S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016LBNF/DUNEMuon neutrinos/antineutrinos from high-power proton beam 1.2 MW from day one (upgradeable)Large underground Liquid Argon Time Projection Chamber4 x 17 kton fiducial (useable) mass of >40 ktonNear detector to characterize the beamFDNDnmnm & ne1300 kmChicagoSouth Dakota

25. DUNE Design = Far detector: 70-kt LAr-TPC = 4 x 17 kt detectors140 mS. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

26. Dipartimento di Fisica dell’Università di Milano – Physics ColloquiaTHE LHC LUMINOSITY MONITORTHE CONCEPT WHICH UNDERLIES THE LUMINOSITY MONITOR FOR LHCProton-proton collisions at the Interaction Points (IP) of (LHC) will produce high fluxes of neutrons and photons that will be intercepted by the neutral absorbers located about 140m downstream the IP1 and IP5 collision points. The energy associated with the showers initiated by the neutral flux from the IPs is proportional to the charge of the colliding bunches and hence to the luminosity.The study was focused on a detector able to provide information on the shower population with response times compatible with the 40 MHz bunch collision frequency.The idea was to install it into a slot machined inside the copper core of the absorbers in order to monitor and optimize the LHC luminosity in a bunch-by- bunch operation.The first problem was identifying the detector type suitable for the purpose. The luminosity monitor is a nearly zero-angle detector and as such it will be exposed to an extremely high dose of radiation. It should stand, before a replacement is possible, up to 1 GGy, a dose exceeding by at least two orders of magnitude that expected for detectors in LHC experiments. Ordinary solid-state detectors were discarded as it was concluded that they wouldn’t survive long enough for the purpose. Polycrystalline CdTe was proven to be promising, but later it was abandoned because of technological difficulties in the realization of adequately large sensitive areas. The best solution was identified to be a multigap ionization chamber operating at a high pressure of the filling gas.P.F. Manfredi – Ionization-based detectors and related low-noise techniques 5026S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

27. Dipartimento di Fisica dell’Università di Milano – Physics ColloquiaP.F. Manfredi – Ionization-based detectors and related low-noise techniques 5127S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

28. 53Dipartimento di Fisica dell’Università di Milano – Physics ColloquiaDETECTOR EVOLUTIONFirst version (years 2000, 2001)NGAP = NSER x NPAR =60 xGAP = 0.5 mmdrift vel. = 3 cm/s (98% Ar + 2% N2)CDETECTOR = CGAP x NPAR / NSERSecond version (years 2003 e 2004)NGAP= NPAR =6xGAP = 1 mmdrift vel. = 4.5 cm/s (94% Ar + 6% N2) QGAP doubledCGAP halvedCDETECTOR = CGAP x NPARP.F. Manfredi – Ionization-based detectors and related low-noise techniques28S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

29. 29Remembering FrancoA wonderful, knowledgeable and patient teacher. A sad loss, for his family, his colleagues, his friends and the scientific community.“The end of an era…”Having studied with him, worked with him, had fun with him, he has enriched my life, the lives of all of us and set an example on how to balance life and career.S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

30. 30From Veljko Radeka:S. Rescia "Detecting Signals into the Noise" 5 Dec. 2016

31. Remembering Franco ….I met Franco a little more than half a century ago. This gave me a lasting feeling of the warmth of an extraordinary human being, whether when we got together , or only when exchanging brief messages.He succeeded in being magnanimous and supportive to others while having to deal with some untimely losses suffered by his family. His patience in life was also evident in the approach to his work, always a very careful and thorough analysis, and even in his lecture notes in his exceptionally neat handwriting …For many years I received a message from Franco for Thanksgiving Holiday. Last year there was no message ….I will always remember my dear friend, VeljkoFranco was fascinated by JFETsAbove: A precursor to MOS switched capacitor circuits …From: Alta Frequenza, Vol XI, 1971A small sample of Franco’s work:S. Rescia "Detecting Signals into the Noise" 5 Dec. 201631