Upgrade Radiation Issues Christopher O’Grady For the DCH Electronics Upgrade Group Based on work by Jerry Va’vra.

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Presentation transcript:

Upgrade Radiation Issues Christopher O’Grady For the DCH Electronics Upgrade Group Based on work by Jerry Va’vra

Introduction In principle, we need to study SEU and radiation “death” issues of all new chips (FPGA and flash perhaps most worrisome). Worked on this in parallel with development. Had hoped we could do “back of the envelope” calculation saying all OK, but didn’t happen. Neutrons appear to be a problem This presentation will be “fuzzy”. Situation in flux.

Complications Only have guess for the neutron rate (depends on some assumptions) Only have guess for neutron spectrum Only have approximate answer for cross section for our device Only have approximate answer for number of configuration bits we rely on Rate scales with Luminosity!! (jerry believes radiative bhabhas slamming into beam wall).

Proton Cross Section Per Bit VirtexII Proton Cross Section from Xilinx Have read that neutrons>20MeV similar

Simulation of Neutron Production Alberto Fasso’s FLUKA simulation Iron Slab. Copper similar. 10% of neutrons > 20MeV

Va’vras Detection Method Uses a Boron detector, which detects “thermal” (low energy neutrons). Moderates “all” neutrons to be thermal using polyethylene wrapper (if anything, undercounts). Without polyethylene, no rate observed (good evidence he is really seeing neutrons). 1MeV neutrons act like a gas, fall off as 1/r**2 (not true for 20MeV neutrons). Assuming a single point source of 1MeV neutrons, can calculate position of source and then rates everywhere.

Rates from Va’vra’s Logbook Jerry says that KEK sees about 1kHz n/cm**2, not lumi dependent.

Neutron SEU Cross-Sections DeviceNeutron Energy (MeV) Cross Section Per Device (cm**2) XC4010E14<1.3E-11 XC4010E0-11<0.4E-11 XC4010E1004.0E-10 XC4036XLA>222.7E-9 XC3S1000>105.4E-8 (XILINX) XC3S1000Cosmic ray (LANSCE) 2.6E-8 (XILINX) XC3S1000Cosmic ray (LANSCE) 1E-7 (ATMEL) XC2V1000>108.8E-8 (XILINX) XC2V E-7 (ATMEL) { { { 4000 series Spartan3 series VirtexII series

SEU Estimates with XC3S1000 Xilinx claims to have study saying that only 2- 10% of configuration bits are used in a typical design. In addition, we are currently only using about 30% of CLBs. (2000n/cm**2/s)*(2.6E-8cm**2/device)*(48devices)*0.1= /s (XILINX number) (2000n/cm**2/s)*(1E-7cm**2/device)*(48devices)*0.1= /s (ATMEL number) Corresponds to about 1 SEU per hour. We’re using XC3S1500, which has factor 2 more configuration bits.

Are We Making Things Worse? Assume XC4010E bit cross-section is the same as XC3000 series bit cross-section. Coincidentally, XC4010E (178kbit) = 1*XC3190(64kbit)+3*XC3142(30kbit)+2*XC3120 (14kbit) i.e. one current box “equals” one XC4010E: (2000n/cm**2/s)*(4.0E-10cm**2/device)*(48devices)*0.1=3.8E-6/s (XILINX number) This is one SEU every 72 hours. We could be making things ~100 times worse.

Some Existing DCH Corruption Don’t think we see errors every 72 hours, but … See two sources of data corruption: 1. Elefant “lock” problem. Typically breaks in a whole quadrant 2. Illegal board addresses regularly. Not understood. Karl attempted to reproduce (1) using high rate 1MeV neutrons. No success in 1 week.

What should we do? If present, this problem affects more than just FPGAs: elefant, atom chip SRAM and configurations, for example. Seems like a bigger “experiment” problem. Configuration corruption is the worst. Perhaps move to ATMEL flash based FPGAs? (lower cross-sections by >100). Atmel downsides: not as much block RAM (matt), more difficult to synthesize (herbst) TMR+partial reconfiguration?

Other Ideas (that don’t fix problem) Monte-Carlo directionality of 20MeV neutrons (hard to really believe) Checksum FPGA every event Understand existing DCH corruption Work with Lockman/Bower on G4 neutron simulation (long time scale) Put a neutron detector in DCH electronics region Use SEUPI (xilinx tool) to understand how many critical configuration bits we have