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CLARO Requirements 30 April 2013 CERN g.pessina -1- CLARO Paolo Carniti INFN & University of Milano Bicocca Lorenzo Cassina INFN & University of Milano Bicocca Angelo Cotta Ramusino INFN and University of Ferrara Massimiliano Fiorini INFN and University of Ferrara Andrea Giachero INFN & University of Milano Bicocca Claudio Gotti INFN & University of Milano Bicocca Matteo Maino INFN & University of Milano Bicocca Roberto Malaguti INFN and University of Ferrara Gianluigi Pessina INFN & University of Milano Bicocca CLARO supporters: Marta Calvi INFN & University of Milano Bicocca Clara Matteuzzi INFN & University of Milano Bicocca

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  • CLARO Requirements 30 April 2013 CERN g.pessina -1-

    CLARO

    Paolo Carniti INFN & University of Milano Bicocca

    Lorenzo Cassina INFN & University of Milano Bicocca

    Angelo Cotta Ramusino INFN and University of Ferrara

    Massimiliano Fiorini INFN and University of Ferrara

    Andrea Giachero INFN & University of Milano Bicocca

    Claudio Gotti INFN & University of Milano Bicocca

    Matteo Maino INFN & University of Milano Bicocca

    Roberto Malaguti INFN and University of Ferrara

    Gianluigi Pessina INFN & University of Milano Bicocca

    CLARO supporters:

    Marta Calvi INFN & University of Milano Bicocca

    Clara Matteuzzi INFN & University of Milano Bicocca

  • CLARO Requirements 30 April 2013 CERN g.pessina -2-

    Summary

    • Requirements from the upgrade;

    • Spillover;

    • Cross-talk;

    • CLARO vs MAROC3;

    • CLARO vs NINO;

    • Resources;

    • Plans.

  • CLARO Requirements 30 April 2013 CERN g.pessina -3-

    Requirements

    1. Capability to work up to 25 ns bunch crossing rate with no spillover

    (see next);

    2. Gain tuning to the pixel spread (factor of 3 maximum);

    3. Binary output with adjustable threshold;

    4. Small power consumption (programmable as a function of the

    occupancy, connected to 1. and se next);

    5. Cross-talk threshold below 5% (see why next and Claudio talk);

    6. RadHard proved up to 81013 n/cm2 (next week we will know and

    see Angelo talk).

  • CLARO Requirements 30 April 2013 CERN g.pessina -4-

    Spillover requirements (1)

    From Sajan simulations the maximum occupancy is expected between

    22% and 31%, but only in the central region of the detector.

  • CLARO Requirements 30 April 2013 CERN g.pessina -5-

    Spillover requirements (2)

    According to statistics the level of occupancy foreseen asks for no spillover, or

    a marginal amount of it.

    In addition the larger part of the detector region has a very low level of

    occupancy. Therefore there the requirements of speed can be relaxed and

    power consumption can be adjusted accordingly.

  • CLARO Requirements 30 April 2013 CERN g.pessina -6-

    Spillover requirements (3)

    CLARO recovery time is within 25 ns and spillover is not present at all.

    Power dissipation can be set remotely (new feature) in low power mode and high

    power mode.

    In low power mode signal is recovered anyway 25 ns and can be applied in the

    lower occupancy parts of the detector.

    CLARO measured signals from a few

    hundreds of PMT e- up to more than 3 Me-.

  • CLARO Requirements 30 April 2013 CERN g.pessina -7-

    Cross-talk (1)

    From the PMT characterization it

    seems that triggering below 35-

    40% of the single-photon peaking

    falls into noise.

    We face 2 scenarios.

    We suppose to have single-photon hits. The photon signals extend up to about the

    double of the peak. If we ask that these signals do not trigger the neighbor

    channels by cross-talk they should stay within 35%, or 17% with respect to the

    peak.

    Add 5% of additional margin we arrive at 12% (take care: 12% is not statistical is

    the fraction of charge lost in the nearby channel via stray capacitance).

    But…

  • CLARO Requirements 30 April 2013 CERN g.pessina -8-

    Cross-talk (2)

    So we have to add a constraint. One possible choice is that the maximum signal

    that can be lost must be less than 20%, which means that 5% is the maximum

    acceptable cross-talk.

    Concerning single photon only we could consider acceptable a maximum

    cross-talk level of 5%, limited by 20% of signal loss.

    Q(1-4)

    Q

    Cxt

    Cxt

    Cxt Cxt

    Q from pixel

    Q

    Q

    Q

    The fraction of the signal, , in the nearby

    channels is 4 times that of the single channel. If

    we do not care about it, the risk is that neither of

    the 5 channels will trigger at all. For instance,

    12%4=48%>35% threshold set!

    (this is true as far as the time scale of the cross-

    talk signal is comparable to that of the shaping

    time, example Ri=100 and Cxt=2 pF 8 ns).

  • CLARO Requirements 30 April 2013 CERN g.pessina -9-

    Cross-talk (3)

    According to Sajan simulation, an

    occupancy of about 25% lead to a

    probability of double hit of about 6%.

    If we would like to avoid cross-talk from this situation we have to ask for a factor of

    2 smaller threshold, from which subtract again 5% of margin obtaining 4% of

    acceptable cross-talk.

    In case of double-photon signal we could consider acceptable a maximum

    cross-talk level of 4-5%, or ¼ of the threshold, whichever is smaller.

  • CLARO Requirements 30 April 2013 CERN g.pessina -10-

    Cross-talk (4)

    In summary:

    So we could consider:

    Maximum cross-talk: 5%

    • Single photon 5% of maximum acceptable cross-talk

    • Double-photon 4-5% of maximum acceptable cross-

    talk

  • CLARO Requirements 30 April 2013 CERN g.pessina -11-

    Summary of the characteristics

    Power consumption in ‘low power’ mode 0.7 mW/ch a low rate, 1.9 mW/ch @ 10 MHz event rate

    Power consumption in ‘timing’ mode 1.5 mW/ch at low rate, 2.3 mW/ch @ 10 MHz event rate

    Power consumption Remotely settable in the new chip, hardwired settable in the present

    Input noise @ Ci=3.3 pF 6 ke- RMS

    Gain setting 3 bits

    Threshold setting 5 bits

    Programming interface SPI (addressable SPI in the new version, Angelo’s talk)

    Threshold step at max gain 150 ke-

    Peaking time

  • CLARO Requirements 30 April 2013 CERN g.pessina -12-

    Competitor comparison: MAROC (1)

    CLARO MAROC (*)

    Power (save a factor of 5) 0.7 mW/ch 3.5 mW/ch

    Input noise 6 ke- RMS 6.5 ke- RMS

    Gain setting 3 bits 8 bits

    Threshold setting 5 bits Common to all channels, 10 bit DAC.

    Programming interface SPI (addressable SPI in the new version)

    SPI standard

    Threshold step at max gain 150 ke- Do not know

    Pulse width (narrower pulse width, 4 to 5 times)

    5 ns to 25 ns Peaking time from 20 to 25 ns for fast shaping, 100 ns to 125 ns pulse width, 30 ns to 150 ns, tunable, pulse width from 150n s to 600 ns

    Crosstalk 0% on chip 0.25% on chip, slow shaper 1% on chip for fast shaper (2-3% measured on previous versions)

    Rad Hard We will see next week Do not know, expected similar to the present CLARO design

    Rad hard strategy Triple redundancy in the register, addressable SPI protocol which simplify the logic (see Angelo’s talk)

    No strategy (as far we know)

    Time over threshold Available Not Available

    (*) Source of characteristics: MAROC3 datasheet

  • CLARO Requirements 30 April 2013 CERN g.pessina -13-

    Competitor comparison: MAROC (2)

    0 25 50 75 100 125 150 175 2000

    0.1

    0.2

    0.3

    0.4

    0.5

    0.6

    0.7

    0.8

    0.9

    11

    Time (ns)

    Arb

    . U

    n.

    MAROC3

    CLARO

    Effect of shaping time on signal:

    spillover B

    unch

    -3

    Bunch

    -5

    Bu

    nch

    -4

    Bu

    nch

    -2

    Bu

    nch

    -1

    Bu

    nch

    -6

    Bunch

    -7

  • CLARO Requirements 30 April 2013 CERN g.pessina -14-

    Competitor comparison: NINO (1)

    CLARO NINO (*)

    Power (50 times smaller) 0.7 mW/ch (0.18 W per module) 35 mW/ch (9 W per module)

    Input noise 6 ke- RMS 5 ke- RMS

    Gain setting 3 bits Fixed

    Threshold setting 5 bits Only in hd, not programmable

    Programming interface SPI (addressable SPI in the new version)

    Not present

    Threshold step at max gain 150 ke- Do not know

    Pulse width 5 ns to 25 ns Do not know

    Crosstalk 0% on chip Donot know

    Rad Hard We will see next week Do not know, expected a bit better to the present CLARO design (0.25 vs 0.35 CMOS)

    Rad hard strategy Triple redundancy in the register, addressable SPI protocol which simplify the logic (see Angelo’s talk)

    No strategy (as far we know)

    Time over threshold Available Available: the output is only digital, not proportional to the input charge in amplitude, but in wildness.

    Jitter 10 ps RMS, single photon 10 ps RMS, single photon.

    (*) Source of characteristics: NIMA 533, 183, 2004, IEEE TNS 51, 1974, 2004.

  • CLARO Requirements 30 April 2013 CERN g.pessina -15-

    Common attribute

    CLARO, MAROC3 and NINO have all the input impedance declared between

    50 and 100 .

    This means that the expected level of cross-talk is expected quite similar in all

    cases.

  • CLARO Requirements 30 April 2013 CERN g.pessina -16-

    Resources

    Recently MIB and FE joined some resources in this project.

    In the next years we can dedicate time to both the PMT and the electronics.

    In addition Genova will contribute also to both items.

    We will have a meeting after tomorrow about this.

  • CLARO Requirements 30 April 2013 CERN g.pessina -17-

    Plans

    • Module prototype with the present CLARO version (80 chips on the

    way, 4 PMTs and spare);

    • New 8 channels CLARO (Rad Hard, gain, threshold, etc.)