Anodic bonding

Anodic bonding is a wafer bonding procedure without any intermediate layer. This bonding technique, also known as field assisted bonding or electrostatic sealing,[1] is mostly used for connecting silicon/glass and metal/glass through electric fields. The requirements for anodic bonding are clean and even wafer surfaces and atomic contact between the bonding substrates through a sufficiently powerful electrostatic field. Also necessary is the use of borosilicate glass containing a high concentration of alkali ions. The coefficient of thermal expansion (CTE) of the processed glass needs to be similar to those of the bonding partner.[2]

Anodic bonding can be applied with glass wafers at temperatures of 250 to 400 °C or with sputtered glass at 400 °C.[3]

This procedure is mostly used for hermetic encapsulation of micro-mechanical silicon elements. The glass substrate encapsulation protects from environmental influences, e.g. humidity or contamination.[2] Further, other materials are used for anodic bonding with silicon, i.e. low-temperature cofired ceramics (LTCC).[4]

Contents

Overview

Anodic bonding on silicon substrates is divided into bonding using a glass wafer or a glass layer. The glass wafer is often sodium containing Borofloat or Pyrex glasses. With an intermediate glass layer, it is also possible to connect two silicon wafers.[5] Those glass layers are deposited by sputtering, spin-on of a glass solution or vapor deposition upon the processed silicon wafer.[3] The thickness of these layers is typically a few micrometer but at least 2 µm contrary to spin-on glasses whereas the thickness is about 1 µm or less.[5]

Also hermetic seals of silicon to glass bonds using an aluminium layer with thickness of 50 to 100 nm are achieved, reaching strengths of 18.0 MPa. This method enables burying electrically isolated conductors in the interface.[6]

Further, bonding of thermally oxidized wafers without a glass layer is possible. The procedural steps of anodic bonding are divided into the following:[2]

  1. Contact substrates
  2. Heating up substrates
  3. Bonding by the application of an electrostatic field
  4. Cooling down the wafer stack

The major drawback of anodic bonding is the different coefficients of thermal expansion for the used materials, silicon and glass. This mismatch can harm the bond through intrinsic material tensions within the used materials and cause disruptions in the bonding materials. The use of sodium containing glasses, e.g. Borofloat or Pyrex, supports to prevent this mismatch. Those glasses have a similar CTE in a specific range of applied temperature commonly up to 400 °C.[7]

The anodic bonding process is characterized by following variables:[8]

The typical bond strength is between 10 and 20 MPa and according to pull tests higher than the fracture strength of glass.

History

Anodic bonding is first mentioned by Wallis and Pomerantz in 1969.[1] It is applied as bonding of silicon wafers to sodium containing glass wafers under the influence of an applied electric field. This method is used up to date as encapsulation of sensors with electrically conducted glasses.[9]

Procedural steps of anodic bonding

Pretreatment of the substrates

The anodic bonding procedure is able to bond hydrophilic and hydrophobic silicon surfaces equally effective. The roughness of the surface should be less than 10 nm and free of contamination on the surface.[8] Even though anodic bonding is relatively tolerant to contaminations, a wide established cleaning procedure RCA takes place to remove those surface impurities.

The glass wafer can also be chemically etched or sand blasted for creating small cavities, where MEMS devices can be accommodated.[10]

Further mechanisms supporting the bonding process of not completely inert anodic materials can be the planarization or polishing of surfaces and the ablation of the surface layer by electrochemical etching.[8]

Contact the substrates

The wafers that meet the requirements are put into atomic contact. As soon the first contact is established, the bonding process starts close to the cathode, spreading in fronts to the edge. This bonding process takes several minutes.[11] The anodic bonding procedure is based on a glass wafer that is usually placed above a silicon wafer. An electrode is in contact with the glass wafer either through a needle or a full area cathode electrode.

If using a needle electrode, the bond spreads radially to the outside which makes it impossible to trap air between the surfaces. The radius of the bonded area equals approximately the radical of the passed time. Below temperatures of 350 to 400 °C and a bond voltage of 500 to 1000 V, this method is not very effective nor reliable.[12]

The use of a full area cathode electrode shows bond reactions all over the interface after powering up the potential.[8] This results from creating a homogeneous electric field distribution at temperatures of around 300 °C and bond voltage of 250 V.[12]

Heating and bonding by application of electrostatic field

The wafers are placed between the chuck and the top tool used as bond electrode at temperatures between 200 and 500 °C (compare to image "scheme of anodic bonding procedure") but below the softening point of glass (glass transition temperature).[10] The higher the temperature the better is the mobility of positive ions in glass.

The applied electrical potential between is set to a voltage of several 100 V.[8] This causes a diffusion of sodium ions (Na+) out of the bond interface to the backside of the glass to the cathode. That results, combined with humidity in formation of NaOH. High voltage helps to support the drifting of the positive ions in glass to the cathode. The diffusion is according to the Boltzmann distribution exponentially related to the temperature. The glass (NaO2) with its remaining oxygen ions (O2-) is negatively volume charged at the bonding surface compared to the silicon (compare to figure "ion drifting in bond glass" (1)). This is based on the depletion of Na+ ions.

Silicon is unlike, e.g. aluminium, an inert anode. In result no ions drift out of the silicon into the glass during the bond process. This affects a positive volume charge in the silicon wafer on the opposite side.[11] As a result a few micrometer thick high-impedance depletion region is developed at the bond barrier in the glass wafer. In the gap between silicon and glass the bond voltage drops. The bond process as a combination of electrostatic and electrochemical process starts.

The electrical field intensity in the depletion region is so high that the oxygen ions drift to the bond interface and pass out to react with the silicon to form SiO2 (compare to figure "ion drifting in bond glass" (2)). Based on the high field intensity in the depletion region or in the gap at the interface, both wafer surfaces are pressed together at a specific bond voltage and bond temperature. The process is realized at temperatures from 200 - 500 °C for about 5 to 20 min. Typically, the bonding or sealing time becomes longer when temperature and voltage are reduced.[13] The pressure is applied to create intimate contact between the surfaces to ensure good electrical conduction across the wafer pair.[14] This ensures intimate contact for the surfaces of the bonding partners. The thin formed oxide layer between the bond surfaces, siloxane (Si-O-Si), ensures the irreversible connection between the bonding partners.[8]

If using thermally oxidized wafers without a glass layer, the diffusion of OH- and H+ ions instead of Na+ ions leads to the bonding.[11]

Cooling down the substrate

After the bonding process a cooling for several minutes has to take place. This can be supported by purging an inert gas. The cooling time depends on the difference of CTE for the bonded materials. The higher the CTE difference is the slower the cooling down should be proceeded.

Technical specifications

Materials
  • Si-Si
  • Si-glass
  • Si-LTCC
  • Si-glass-PZT ceramics
  • Metal-glass (Al, Cu, Kovar, Mo, Ni, Invar, ...)
Temperature
  • Si-glass: > 250 °C
  • Si-Si (w. intermediate glass layer): > 300 °C
  • Metal-glass: 200 - 450 °C
Voltage
  • Si-glass: 300 - 500 V (max. < 2000 V)
  • Metal-glass: 50 - 1500 V
Advantages
  • easy technological processes
  • generation of stable bonds
  • generation of hermetic bonds
  • bonding below  450 °C
  • low restrictions for Si surface
Drawbacks
  • CTE differences for used materials
Researches
  • manufacturing process integration
  • Si-LTCC

See also

References

  1. ^ a b G. Wallis and D. I. Pomerantz (1969). "Field Assisted Glass-Metal Sealing". Journal of Applied Physics 40 (10): pp. 3946-3949. http://link.aip.org/link/?JAP/40/3946/1. 
  2. ^ a b c M. Wiemer and J. Frömel and T. Gessner (2003). "Trends der Technologieentwicklung im Bereich Waferbonden". In W. Dötzel. 6. Chemnitzer Fachtagung Mikromechanik & Mikroelektronik. 6. Technische Universität Chemnitz. pp. 178-188. 
  3. ^ a b A. Gerlach and D. Maas and D. Seidel and H. Bartuch and S. Schundau and K. Kaschlik (1999). "Low-temperature anodic bonding of silicon to silicon wafers by means of intermediate glass layers". Microsystem Technologies 5 (3): pp. 144-149. doi:10.1007/s005420050154. 
  4. ^ M.F. Khan and F.A. Ghavanini and S. Haasl and L. Löfgren and K. Persson and C. Rusu and K. Schjølberg-Henriksen and P. Enoksson (2010). "Methods for characterization of wafer-level encapsulation applied on silicon to LTCC anodic bonding". Journal of Micromechanics and Microengineering 20 (6): pp. 064020. http://stacks.iop.org/0960-1317/20/i=6/a=064020. 
  5. ^ a b H. J. Quenzer and C. Dell and B. Wagner (February 1996). "Silicon-silicon anodic-bonding with intermediate glass layers using spin-on glasses". Micro Electro Mechanical Systems, 1996 (MEMS '96) Proceedings. 'An Investigation of Micro Structures, Sensors, Actuators, Machines and Systems'.. 272-276. doi:10.1109/MEMSYS.1996.493993. 
  6. ^ K. Schjølberg-Henriksen and E. Poppe and S. Moe and P. Storås and M. M. V. Taklo and D. T. Wang and H. Jakobsen (2006). "Anodic bonding of glass to aluminium". Microsyst. Technol. 12 (5): pp. 441-449. doi:10.1007/s00542-005-0040-8. 
  7. ^ T. Gessner and T. Otto and M. Wiemer and J. Frömel (2005). "Wafer bonding in micro mechanics and microelectronics - an overview". The World of Electronic Packaging and System Integration. pp. 307-313. http://www.izm.fraunhofer.de/publi_download/papers/reichl_tagungsband/wafer_level_integration/206gessner.jsp. 
  8. ^ a b c d e f g S. Mack (1997). Eine vergleichende Untersuchung der physikalisch-chemischen Prozesse an der Grenzschicht direkt und anodischer verbundener Festkörper (Report). VDI. ISBN 3-18-343602-7. 
  9. ^ A. Plössl and G. Kräuter (1999). "Wafer direct bonding: tailoring adhesion between brittle materials". Materials Science and Engineering 25 (1-2): pp. 1-88. http://www.sciencedirect.com/science/article/B6TXH-3W48J3B-1/2/4a698948f4384db57b6ea3af7fdf29c3. 
  10. ^ a b M. Chiao (2008). "Packaging (and Wire Bonding)". Springer Science+Business Media, LLC.. 
  11. ^ a b c G. Gerlach and W. Dötzel (2008). Ronald Pething. ed. Introduction to Microsystem Technology: A Guide for Students (Wiley Microsystem and Nanotechnology). Wiley Publishing. doi:978-0-470-05861-9. 
  12. ^ a b P. Nitzsche and K. Klange and B. Schmidt and s. Grigull and U. Kreissig and B. Thoms and K. Herzog (1998). "Ion Drift Processes in Pyrex Type Alkali-Borosilicate Glass during Anodic Bonding". Electrochemical Society 145 (5): pp. 1755-1762. doi:10.1002/chin.199830293. 
  13. ^ G. Wallis (1975). "Field Assisted Glass Sealing". ElectroComponent Science and Technology 2 (1): pp. 45-53. doi:10.1155/APEC.2.45. 
  14. ^ S. Farrens and S. Sood (2008). "Wafer Level Packaging: Balancing Device Requirements and Materials Properties". IMAPS. International Microelectronics and Packaging Society. 

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