1
The PLL consists of a phase frequency detector (PFD), a charge pump, a low pass filter, a voltage controlled oscillator (VCO), and a divider (divide by 16). An LVDS receiver and a CML driver are used as the input and output interface. The divider consists of a CML divider (divide by 2), a CML to CMOS converter, and a CMOS divider (divide by 8). The LVDS receiver, the phase frequency detector (PFD), the charge pump, the pass filter, the CMOS divider, and the CML driver are shared with the 5 Gbps 16:1 serializer. For details of these design blocks please see the poster “A 16:1 serializer for data transmission at 5 Gbps ” presented by Dr. Datao Gong. The bandwidth of the low pass filter and the current of charge pump are programmable to suit different applications. The phase margin of the PLL is larger than 46°. VCO Type LC-based VCO Ring- oscillator based VCO Power Consumption Low High Frequency High Low Phase noise/jitter performance Good Bad Radiation sensitivity Small Large Tuning range Narrow Wide Chip area Large Small VCO A NMOS or PMOS transistor with its source and drain tied together serves a varactor with monotonic C-V curve and large tuning range (Cmax/Cmin > 2). The tuning range is 3.79 – 5.01 GHz at the typical corner and room temperature and varies less than 8% in all corners and temperature range. The CML divider can work up to 5.1 GHz at all corners and from -40 °C to 85 °C. Present Upgrade Data rate per front-end board (FEB) (Gbps) 1.6 100 Power consumption per Gbps (mW) 1188 90 Cross-coupled transistors provides negative resistance, compensating the energy loss in the LC tank Operation frequency: 4 ~ 5 GHz for data rate 8 ~ 10 Gbps Random jitter < 1 ps (RMS) Power consumption < 100 mW High speed, low power, high quality inductors, no latch-up The radiation tolerance of a commercial 0.25 µm SoS CMOS technology has been evaluated in the previous study PLL block diagram 1.4 mm x 1.7 mm The PLL tracks the input frequenc y after 9 µs. The jitter after 9 µs is less than 2 ps (peak-peak). The phase noise of the VCO in the worst case Fabrication: submitted on August 3, 2009; Chip delivery: November 17, 2009 Test: in lab test: December 15, 2009; Radiation test: February 15, 2010 Plan: apply this LC-based PLL and design a multi-channel 16:1 serializer with each channel working around 10 Gbps in 2011 Tuning range (GHz) 3.8 – 5.1 Power consumption of core PLL (mW) 104 Area (mm 2 ) 1.4 x 1.7 Random Jitter from VCO (RMS, ps) < 1 Deterministic jitter (peak- peak, ps) 2 Acquisition time (μs) 9 Conclusion Introduction Design Performances Grant: US-ATLAS R&D program for the upgrade of the LHC and the US Department of Energy grant DE-FG02-04ER41299. Peter Clarke, Jay Clementson, Yi Kang, Francis M. Rotella, John Sung, and Gary Wu from Peregrine Semiconductor Corporation for technical assistance. Justin Ross at Southern Methodist University for setting up and maintaining the software environment. Jasoslav Ban, Mauro Citterio, Christine Hu, Sachin Junnarkar, Valentino Liberali, Paulo Rodrigues Simoes Moreira, Mitch Newcomer, Quan Sun, Fukun Tang, and Carla Vacchi for technical assistance and reviewing of this design. Acknowledgments On-chip spiral inductors with a peak frequency of 5.1 GHz. The Q factor is simulated to be 21.2 at 5 GHz. Reference current source Start-up circuit Decoupling capacitors are used to improve the noise performance Silicon-on-Sapphire (SoS) CMOS technology Design Goals Application Background: ATLAS Liquid Argon Calorimeter Optical Link Upgrade The Design of a Low-Power High-Speed Phase Locked Loop PLL Layout CML Divider Acquisition Time Deterministic Jitter Random Jitter Simulated results of the PLL Status and Plan Tiankuan Liu 1 , Datao Gong 1 , Suen Hou 2 , Zhihua Liang 1 , Chonghan Liu 1 , Da-Shung Su 2 , Ping-Kun Teng 2 , Annie C. Xiang 1 , Jingbo Ye 1 1 Department of Physics, Southern Methodist University, Dallas TX 75275, U.S.A. 2 Institute of Physics, Academia Sinica, Nangang 11529, Taipei, Taiwan [email protected] The random jitter due to the VCO’s phase noise, the dominant noise source, is less than 1 ps (RMS) from 10 kHz to 100 MHz.

The PLL consists of a phase frequency detector (PFD), a charge pump, a low pass filter, a voltage controlled oscillator (VCO), and a divider (divide by

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Page 1: The PLL consists of a phase frequency detector (PFD), a charge pump, a low pass filter, a voltage controlled oscillator (VCO), and a divider (divide by

• The PLL consists of a phase frequency detector (PFD), a charge pump, a low pass filter, a voltage controlled oscillator (VCO), and a divider (divide by 16). An LVDS receiver and a CML driver are used as the input and output interface. The divider consists of a CML divider (divide by 2), a CML to CMOS converter, and a CMOS divider (divide by 8).

• The LVDS receiver, the phase frequency detector (PFD), the charge pump, the pass filter, the CMOS divider, and the CML driver are shared with the 5 Gbps 16:1 serializer. For details of these design blocks please see the poster “A 16:1 serializer for data transmission at 5 Gbps ” presented by Dr. Datao Gong.

• The bandwidth of the low pass filter and the current of charge pump are programmable to suit different applications. The phase margin of the PLL is larger than 46°.

VCO Type LC-based VCO Ring-oscillator based VCO

Power Consumption Low High

Frequency High Low

Phase noise/jitter performance Good Bad

Radiation sensitivity Small Large

Tuning range Narrow Wide

Chip area Large Small

VCO

A NMOS or PMOS transistor with its source and drain tied together serves a varactor with monotonic C-V curve and large tuning range (Cmax/Cmin > 2).

The tuning range is 3.79 – 5.01 GHz at the typical corner and room temperature and varies less than 8% in all corners and temperature range.

The CML divider can work up to 5.1 GHz at all corners and from -40 °C to 85 °C.

Present Upgrade

Data rate per front-end board (FEB) (Gbps) 1.6 100

Power consumption per Gbps (mW) 1188 90

Cross-coupled transistors provides negative resistance, compensating the energy loss in the LC tank

• Operation frequency: 4 ~ 5 GHz for data rate 8 ~ 10 Gbps

• Random jitter < 1 ps (RMS)

• Power consumption < 100 mW

• High speed, low power, high quality inductors, no latch-up• The radiation tolerance of a commercial 0.25 µm SoS

CMOS technology has been evaluated in the previous study

PLL block diagram

1.4 mm x 1.7 mm

The PLL tracks the input frequency after 9 µs.

The jitter after 9 µs is less than 2 ps (peak-peak).

The phase noise of the VCO in the worst case

• Fabrication: submitted on August 3, 2009; Chip delivery: November 17, 2009

• Test: in lab test: December 15, 2009; Radiation test: February 15, 2010

• Plan: apply this LC-based PLL and design a multi-channel 16:1 serializer with each channel working around 10 Gbps in 2011

Tuning range (GHz) 3.8 – 5.1

Power consumption of core PLL (mW) 104

Area (mm2) 1.4 x 1.7

Random Jitter from VCO (RMS, ps) < 1

Deterministic jitter (peak-peak, ps) 2

Acquisition time (μs) 9

Conclusion

Introduction

Design

Performances

• Grant: US-ATLAS R&D program for the upgrade of the LHC and the US Department of Energy grant DE-FG02-04ER41299.

• Peter Clarke, Jay Clementson, Yi Kang, Francis M. Rotella, John Sung, and Gary Wu from Peregrine Semiconductor Corporation for technical assistance.

• Justin Ross at Southern Methodist University for setting up and maintaining the software environment.

• Jasoslav Ban, Mauro Citterio, Christine Hu, Sachin Junnarkar, Valentino Liberali, Paulo Rodrigues Simoes Moreira, Mitch Newcomer, Quan Sun, Fukun Tang, and Carla Vacchi for technical assistance and reviewing of this design.

Acknowledgments

On-chip spiral inductors with a peak frequency of 5.1 GHz. The Q factor is simulated to be 21.2 at 5 GHz.

Reference current sourceStart-up circuit

Decoupling capacitors are used to improve the noise performance

Silicon-on-Sapphire (SoS) CMOS technology Design GoalsApplication Background: ATLAS Liquid Argon

Calorimeter Optical Link Upgrade

The Design of a Low-Power High-Speed Phase Locked Loop

PLL Layout

CML Divider

Acquisition Time Deterministic Jitter Random Jitter

Simulated results of the PLL Status and Plan

Tiankuan Liu1, Datao Gong1, Suen Hou2, Zhihua Liang1, Chonghan Liu1, Da-Shung Su2, Ping-Kun Teng2, Annie C. Xiang1, Jingbo Ye1

1 Department of Physics, Southern Methodist University, Dallas TX 75275, U.S.A.2 Institute of Physics, Academia Sinica, Nangang 11529, Taipei, Taiwan

[email protected]

The random jitter due to the VCO’s phase noise, the dominant noise source, is less than 1 ps (RMS) from 10 kHz to 100 MHz.