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Development of DC-DC converter ASICs S.Michelis 1,3, B.Allongue 1, G.Blanchot 1, F.Faccio 1, C.Fuentes 1,2, S.Orlandi 1, S.Saggini 4 1 CERN – PH-ESE 2.

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Presentation on theme: "Development of DC-DC converter ASICs S.Michelis 1,3, B.Allongue 1, G.Blanchot 1, F.Faccio 1, C.Fuentes 1,2, S.Orlandi 1, S.Saggini 4 1 CERN – PH-ESE 2."— Presentation transcript:

1 Development of DC-DC converter ASICs S.Michelis 1,3, B.Allongue 1, G.Blanchot 1, F.Faccio 1, C.Fuentes 1,2, S.Orlandi 1, S.Saggini 4 1 CERN – PH-ESE 2 UTFSM, Valparaiso, Chile 3 EPFL, Lausanne 4 University of Udine ATLAS–CMS Power Working Group 31/03/2010

2 Outline S.Michelis CERN/PH 2  AMIS2 New results with AMIS2 Proton irradiation Efficiency in QFN32 package  ASIC designed in IHP technology Features From IHP1 to IHP2 Overcurrent protection Bandgap Schedule 2

3 AMIS2 prototype ATLAS–CMS Power Working Group 31/03/2010 S.Michelis CERN/PH 3  Internal oscillator  Internal voltage reference  Programmable delay between gate signals  Integrated feedback loop with bandwidth of 20Khz  TID radiation tolerance up to 300Mrad  Already used and tested in Aachen and Fermilab Details presented at TWEPP09 (http://indico.cern.ch/contributionDisplay.py?contribId=97&sessionId=42&confId=49682) Annealing 3 days Annealing 7 days Pre rad

4 AMIS2 proton irradiation  AMIS2 has been irradiated with proton at the CERN “irrad1” facility (24 GeV/c proton beam from PS). Two different different proton fluences have been reached: 2 10 15 p/cm 2 and 5 10 15 p/cm 2 Therefore we have a prototype in the backup technology that is fully functional with TID up to 300Mrd and proton fluence up to 5 10 15 p/cm 2 S.Michelis CERN/PH 4ATLAS–CMS Power Working Group 31/03/2010 Please note that the pre-rad results are taken with different bonding setup. These results are shown only to compare the efficiency trend

5 S.Michelis CERN/PH 5ATLAS–CMS Power Working Group 31/03/2010 AMIS2 package 5 7 mm Package QFN48 5 mm Package QFN32

6 AMIS2 QFN32 efficiency S.Michelis CERN/PH 6ATLAS–CMS Power Working Group 31/03/2010 Efficiency with new board and new package has been extracted. Higher efficiency is measured in comparison with QFN48 in particular for higher load

7 IHP1 prototype ATLAS–CMS Power Working Group 31/03/2010 S.Michelis CERN/PH 7  First prototype in the IHP SGB25VGOD technology – main technology chosen after radiation tests of LDMOS (high-V) transistors  Design included in MPW run of May09  Features integrated in the prototype: oscillator (with sawtooth) and reliable soft start procedure Improved and safer handling of dead times during commutation (with adaptive logic monitoring the output node). Higher efficiency and softer commutations proven More reliable mechanism for power transistor turn- off to prevent possible multiple commutations in a cycle  External components needed Regulated voltage supplies bandgap reference Compensation network  Packaged in QFN48 2.5mm 2.8mm

8 Measurement vs Estimate ATLAS–CMS Power Working Group 31/03/2010 S.Michelis CERN/PH 8 Vin=10V, Vout=2.5V, Iout=2A Estimated Efficiency

9 Using estimate to choose L, f ATLAS–CMS Power Working Group 31/03/2010 S.Michelis CERN/PH 9  Example of the choice of conditions (L, frequency) for the following requirements: Vin=10V, Iout=1 and 2 A, Vout=2.5 to 0.9V  Each point obtained setting L and frequency such that the evaluated efficiency is the highest

10 10 IHP2 prototype  Second prototype in the IHP SGB25VGOD technology  Design included in MPW run of Jan10 Expected back in May 2010  Additional features integrated in the prototype: Linear regulators Bandgap Overcurrent protection Improvement in the adaptive logic Triplication and logic against SEU Enablers Complete circuit Over current protection Dimension of the power transistors  External components needed Compensation network 3mm 2.9mm ATLAS–CMS Power Working Group 31/03/2010 S.Michelis CERN/PH Half power transistor switched off

11 Moving from IHP1 to IHP2 ATLAS–CMS Power Working Group 31/03/2010 11 S.Michelis CERN/PH

12 Adaptive logic Pmos on Nmos on Pmos on Nmos on Phase C out L Vout Nmos Pmos ILIL Phase ILIL Diode Conduction Almost zero diode conduction Negative comp Low side comp High side comp Adaptive logic allows reducing the dead time. This optimizes the switching operation and improves the efficiency ATLAS–CMS Power Working Group 31/03/2010 12 S.Michelis CERN/PH

13 Overcurrent protection Pmos on Nmos on Pmos on C out L Vout Nmos Pmos ILIL Phase ILIL Over current sensing 2 possible cases: Current limiter during startup Converter restart after startup Turn off Pmos Over current limit ATLAS–CMS Power Working Group 31/03/2010 13 S.Michelis CERN/PH

14 Bandgap circuit S.Michelis CERN/PH 14ATLAS–CMS Power Working Group 31/03/2010 The sensitive part of this design and in this technology is the diode. Different diode layouts with enclosed design, additional guard rings and different current density need to be investigated Bandgap voltage Vs TID with normal diode

15 Bandgap circuit  Different bandgap version in IHP technology has been designed and submitted in October 2009. Expected back this week  Target is high stability of the bandgap voltage over variation of temperature, Vdd, TID and displacement damage.  Results will be presented soon ATLAS–CMS Power Working Group 31/03/2010 15 S.Michelis CERN/PH

16 Schedule IHP2  Mid May 2010 20 Chip expected back in package QFN48  May-June 2010 Extensive functional and radiation tests  July-August 2010 Order of 100 naked chip Decision of necessary control pins and packaging in QFN32 IHP3  Next submission Investigating bump bonding Reduction of resistance of on chip metal and bondings Smaller size if direct bondend on pcb (~3x3 mm) ATLAS–CMS Power Working Group 31/03/2010 16 S.Michelis CERN/PH

17 Conclusion  AMIS2 is a prototype in the backup technology that is fully functional with TID up to 300Mrd proton fluence up to 5 10 15 p/cm 2 efficiency between 70 and 80% Excellent noise performances of AMIS2, mounted on optimized PCB, will be presented by Georges  ASIC designed in IHP technology has better performances (efficiency between 80 and 85%). A complete design with protection is expected back in May 2010 S.Michelis CERN/PH 17ATLAS–CMS Power Working Group 31/03/2010


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