1. Field of the Invention
The present invention relates to hermetically sealed glass packages that are suitable to protect thin film devices that are sensitive to the ambient environment. Some examples of such devices are organic emitting light diode (OLED) displays, sensors, and other optical devices. The present invention is demonstrated using OLED displays as an example.
2. Description of Related Art
OLEDs have been the subject of a considerable amount of research in recent years because of their use and potential use in a wide variety of electroluminescent devices. For instance, a single OLED can be used in a discrete light emitting device or an array of OLEDs can be used in lighting applications or fiat-panel display applications (e.g., OLED displays). The traditional OLED displays are known as being very bright and having a good color contrast and wide viewing angle. However, the traditional OLED displays and in particular the electrodes and organic layers located therein are susceptible to degradation resulting from interaction with oxygen and moisture leaking into the OLED display from the ambient environment. It is well known that the life of the OLED display can be significantly increased if the electrodes and organic layers within the OLED display are hermetically sealed from the ambient environment, Unfortunately, in the past it was very difficult to develop a sealing process to hermetically seal the OLED display. Some of the factors that made it difficult to properly seal the OLED display are briefly mentioned below:
Today the most common way for sealing the OLED display is to use different types of epoxies, inorganic materials and/or organic materials that form the seal after they are cured by ultra-violet light. Vitex systems manufactures and sells a coating under the brand name of Batrix™ which is a composite based approach where alternate layers of inorganic materials and organic materials can be used to seal the OLED display. Although these types of seals usually provide good mechanical strength, they can be very expensive and there are many instances in which they have failed to prevent the diffusion of oxygen and moisture into the OLED display. Another common way for sealing the OLED display is to utilize metal welding or soldering, however, the resulting seal is not durable in a wide range of temperatures because of the substantial differences between the coefficients of thermal expansions (CTEs) of the glass plates and metal in the OLED display. Accordingly, there is a need to address the aforementioned problems and other shortcomings associated with the traditional seals and the traditional ways for sealing the OLED displays. These needs and other needs are satisfied by the hermetic sealing technology of the present invention.
The present invention includes a hermetically sealed OLED display and method for manufacturing the hermetically sealed OLED display. Basically, the hermetically sealed OLED display is manufactured by providing a first substrate plate and a second substrate plate and depositing a frit onto the second substrate plate. OLEDs are deposited on the first substrate plate. An irradiation source (e.g., laser, infrared light) is then used to heat the frit which melts and forms a hermetic seal that connects the first substrate plate to the second substrate plate and also protects the OLEDs. The frit is glass that was doped with at least one transition metal and possibly a CTE lowering filler such that when the irradiation source heats the frit, it softens and forms a bond. This enables the frit to melt and form the hermetic seal while avoiding thermal damage to the OLEDs.
A more complete understanding of the present invention may be obtained by reference to the following detailed description when taken in conjunction with the accompanying drawings wherein:
Referring to
Referring to
Referring to
At step 206, the OLEDs 104 and other circuitry are deposited onto the first substrate plate 102. The typical OLED 104 includes an anode electrode, one or more organic layers and a cathode electrode. However, it should be readily appreciated by those skilled in the art that any known OLED 104 or future OLED 104 can be used in the OLED display 100. Again, it should be appreciated that this step can be skipped if an OLED display 100 is not being made but instead a glass package is being made using the sealing process of the present invention.
At step 208, the frit 106 is deposited along the edges of the second substrate plate 107. For instance, the frit 106 can be placed approximately 1 mm away from the free edges of the second substrate plate 107. In the preferred embodiment, the frit 106 is a low temperature glass frit that contains one or more absorbing ions chosen from the group including iron, copper, vanadium, and neodymium (for example). The frit 106 may also be doped with a filler (e.g., inversion filler, additive filler) which lowers the coefficient of thermal expansion of the frit 106 so that it matches or substantially matches the coefficient of thermal expansions of the two substrate plates 102 and 107. The compositions of several exemplary frits 106 are provided below with respect to experiment #'s 1-5 and TABLES 2 and 3.
At step 210 (optional), the frit 106 can be pre-sintered to the second substrate plate 107. To accomplish this, the frit 106 which was deposited at step 208 onto the second substrate plate 107 is then heated so that it becomes attached to the second substrate plate 107. A more detailed discussion about the optional step 210 is provided below with respect to experiment #3.
At step 212, the frit 106 is heated by the irradiation source 110 (e.g., laser or infrared lamp) in a manner so that the frit 106 forms the hermetic seal 108 which connects and bonds the first substrate plate 102 to second substrate plate 107 (see
Described below are several experiments that were conducted by one or more of the inventors. Basically, the inventors have experimented with and used different types of irradiation sources 110 to heat different types of frits 106 in order to connect and bond together two Code 1737 glass plates 102 and 107. The different compositions of these exemplary frits 106 are provided below with respect to experiment #'s 1-5.
In this experiment, the irradiation source 110 was a laser 110a (e.g., 810 nm Ti:sapphire laser 110a) that emitted a laser beam 112a through a lens 114a and through the first substrate plate 102 which heated and softened the frit 106 (see
As mentioned above, to increase the absorption of the frit 106 it was necessary to dope the glass with one or more transition metals such as vanadium, iron, or neodymium (for example). This was done because the aforementioned transition metals have a large absorption cross-section around 800-nm as illustrated by the absorption spectrum graphs in
To demonstrate the feasibility of this approach two exemplary frits 106 were laser-heated using a 0.9 watt, 800 nm Ti:sapphire laser 110a the output of which was focused into the frit 106 by a 10 cm lens 114a. The exemplary frits 106 were placed between two 1 mm thick Code 1737 glass plates 102 and 107. The first frit 106 was made from glass containing iron, vanadium and phosphorus.
It should be readily appreciated that depending on the optical properties of the particular frit 106 and substrate plates 102 and 107 other types of lasers 110a can be used which operate at different powers, different speeds and different wavelengths. However, the laser wavelength should be within the band of high absorption in the particular frit 106. For instance, Ytterbium (900 nm<λ<1200 nm), Nd:YAG (λ=1064 nm), Nd:YALO (λ=1.08 μm), and erbium (λ≈1.5 μm) CW lasers can be used.
In this experiment, a CO2 laser 110a was used to locally heat a frit 106 dispersed along the edges of the substrates plates 102 and 107 without causing a significant temperature rise away from the sealed edges.
First, a thin layer of V2O5—Fe2O3—P2O5 preform frit 106 containing fillers to enable a CTE match to display glass was spread along the edge of one of the Code 1737 glass plates 102 and 107 (see
Another aspect of this experiment related to the placement of the preform vanadate iron phosphate glass frit 106 in between the Code 1737 glass substrate plates 102 and 107. Since flaws can be easily introduced along the edges of the Code 1737 glass plates 102 and 107 from prior processing steps such as cutting and handling, the probability of edge cracking at the interface of the frit 106 and plates 102 and 107 is increased for a given temperature gradient and CTE mismatch when the initial flaw size is greater. And, since the thermal stresses induced during lasing and subsequent cooling cycles are elastic in nature there is no relaxation of stresses. To address this concern, the preform vanadate iron phosphate glass frit 106 in this experiment was applied at a small distance away from the free edges of glass substrates 102 and 107 (see
In this experiment, the irradiation source 110 was a laser 110a (e.g., CO2 laser 110a) that emitted a laser beam 112a through a split-beam optics arrangement 500 which split the laser beam 112a into two laser beams 112a′ and 112a″ which where then directed towards the first and second Code 1737 glass plates 102 and 107 (see
In this experiment, an exemplary V2O5—ZnO—P2O5 (VZP) frit 106 and Code 1737 glass substrate plates 102 and 107 were chosen. The first step 210 of sealing, i.e. pre-sintering the VZP frit 106 to plate 107 was performed at 400° C. in furnace environment for 1 hour, and followed by furnace cooling to prevent cracking. Good wettability, and hence bonding, was observed at the interface of the VZP frit 106 and plate 107 without any indication of local delamination or non-adhered region. Then, the second step 212 of sealing followed by using a localized CO2 laser 110a. In particular, the edges of both surfaces of the substrate plates 102 and 107 were heated locally to the softening temperature of the VZP frit 106 by the CO2 laser 110a. The CO2 laser 110a emitted a single beam 112a which was split into two beams 112a′ and 112a″ that were focused onto the substrate plates 102 and 107 (see
In this experiment, the irradiation source 110 was a 1000 watt infrared lamp (not shown) that was controlled by a variable voltage controller. This particular infrared lamp emitted a light over a wavelength range of approximately 800 to 2000 nm. The samples that were sealed using the infrared lamp consisted of two 1″×1″ Code 1737 glass plates 102 and 107, where an exemplary frit 106 was applied as a thin strip along the 4 edges of one of the plates 102 and 107. The compositions of some exemplary frits 106 used in experiment #4 are provided in TABLE #1.
As mentioned earlier, it is important when infrared radiation is used to seal a frit 106 that the frit 106 absorbs heat in the infrared region. As described above, vanadium is a particularly strong infrared absorber in oxide glasses. As such, most of the initial calibration and sealing work in this experiment was done using frits 106 having blend 5801, which consisted of a mixture of a titano-vanadium frit and lithium alumino-silicate filler (see TABLE #1). The 5801 blend powder was first made into a paste using a suitable solvent/binder system such as amyl acetate/nitrocellulose, or pine oil, loaded into a syringe, and then hand-dispensed along the edges of one of the Code 1737 glass plates 102 or 107. After applying the 5801 blend frit 106, the two glass plates 102 and 107 were manually pressed over each other using mild hand pressure, and then placed in an oven at 100° C. to dry the 5801 blend frit 106.
The sample plates 102 and 107 were then placed about 40 mm under the infrared lamp (the approximate focal length of the lamp) and set on top of a piece of refractory cloth to serve as insulation. The sealing step 212 was carried out a single edge at a time. A refractory block made of alumina was placed over the entire surface area of the glass plates 102 and 107 to serve as an infrared mask with the exception of the actual seal edge that was to be sealed. The temperature in the sample glass plates 102 and 107 was monitored by a thermocouple placed in the center of the two plates 102 and 107 through a small hole drilled through the top plate 102. Once the masked glass plates 102 and 107 and thermocouple were placed under the IR lamp, the lamp controller was turned to 10% of maximum power, and the sample plates 102 and 107 were then oriented for actual sealing. The lamp controller was then turned off, final checks were made of the thermocouple, and then the power was turned immediately to the level used for sealing (typically 40-60% of maximum output).
During the operation of the infrared lamp, the seal edge was viewed with infrared-absorbing protective glasses. Once softening was observed in the 5801 blend frit 106, the power was immediately turned-off to the infrared lamp, and the lamp itself was moved away from the sample plates 102 and 107. The typical time to seal one edge was approximately 60 seconds.
In addition to the aforementioned 5801 and 5817 blend frits 106, infrared-sealing work was also carried out with the 5913 blend. Approximately half of the sealed sample plates 102 and 107 were tested and the seal was determined to be hermetic-using the criterion of not exhibiting any leak larger than 10−8 cm3/s in a He leak test.
It should be noted that a laser 110a has also been used to melt one of the frits 106 listed in TABLE #1. In particular, a 7 watt, 810-nm, continuous wave (CW) semiconductor laser 110a emitting a laser beam 112a focused onto a 2.5 mm spot and moved at a velocity of 0.5 mm/s was used to melt 5913 blend frit 106 (see
Before discussing the details of this experiment, one should remember that there are several considerations which should be kept in mind when designing a frit 106 that can be used to make a hermetically sealed OLED display 100. Following is a list of some of these considerations:
The requirement that frit-sealing be accompanied by at best only a minimal temperature rise in the adjacent OLEDs can be satisfied with a low temperature sealing frit 106. However, most low temperature oxide frits of reasonable durability have CTE values well above the CTEs of the substrates plates 102 and 107. As such, the high CTE of low temperature glass frits may require the use of filler additions, or inert phases that lower the CTE. These fillers may be “additive fillers” such as lithium alumino-silicate crystalline phases which have an intrinsically-lower CTE themselves, or “inversion fillers” such as Co-Mg pyrophosphate which introduce dimensional change through a phase transformation during heating or cooling. Accordingly, to meet the OLED sealing temperature requirements, a low temperature filled fit 106 in combination with some form of localized edge heating such as an infrared lamp or CO2 laser 110a may be required to minimize the adjacent temperature rise during sealing.
Several potential low melting frits 106 suitable for sealing OLED displays 100 made from Code 1737 glass plates 102 and 107 are listed in TABLE #2. These potential frits 106 were selected on the basis of a low Tg (i.e., <350° C.), and a low furnace sealing temperature (<550° C.). Although these frits 106 were all prepared by normal glass-melting techniques, it should be noted that many of these frits 106 may also be prepared by sol-gel techniques. The compositions listed in TABLE 2 include the following fits 106:
As noted in TABLE #2, vanadium-phosphate based glass frits 106 offer a unique combination of low Tg, and low CTE. Vanadium is a strong infrared absorber in silicate glasses thus it is a strong candidate in localized sealing methods such as IR lamp, and both near-, and far infrared lasers (i.e., semiconductor lasers at 800-900 nm, and CO2 laser at 10.6 μm). The starting point for the vanadium phosphate work was several low Tg glasses in the Fe2O3—P2O5—V2O5 and TiO2—P2O5—V2O5 systems.
Although the 895 AFD vanadium phosphate glass frits 106 has a low CTE, its CTE may not be low enough to match the CTE of the Code 1737 glass plates 102 and 107 without the addition of fillers. Since, the frit 106 has a relatively-low CTE this permits the use of “additive” fillers to lower the CTE, rather than “inversion” fillers which can produce microcracking, resulting in non-hermetic seals. Unfortunately, the 895 AFD frit 106 even with filler levels close to the maximum amount (≈25-30 wt. %) still did not exhibit a satisfactory expansion match to Code 1737 glass plates 102 and 107.
However, continued composition research resulted in the discovery that zinc vanadium phosphate glass frits 106 can be made which have expansions low enough to permit a close CTE match to Code 1737 glass plates 102 and 107 when fillers are added. Measured values of Tg and CTE for one of these frits which has a composition 20ZnO-30P2O5-50V2O5 (molar basis) were, respectively, 300° C., and 70×10−7/° C. In fact, 5895 blend frit 106 described below but not listed in TABLE #2 has a combination of zinc vanadium phosphate and additive fillers which has shown excellent expansion compatibility and good bonding with Code 1737 glass plates 102 and 107. The 5895 blend frit 106 is composed of Zn vanadium phosphate frit (molar basis: 20ZnO-30P2O5-50V2O5) and β-eucryptite glass-ceramic (molar basis: 25Li2O-25Al2O3-50SiO2) as follows (wt. Basis)
It should be noted that the maximum expansion mismatch shown in
These zinc vanadium phosphate frits 106 also offer promise for meeting the hermeticity requirements for OLED sealing. Several 1″×1″ assemblies of Code 1737 glass plates heated either by an infrared lamp (not shown) or 810 nm laser 110a and sealed with the 5895 blend frit 106 passed the He-leak test by holding vacuum down to the lowest leak rate measured by the equipment, 1×10−8 cm3/s. In addition, separate temperature measurements by an infrared camera, thermocouple, and thermal indicator paint made during 810 nm laser frit sealing all indicated a maximum temperature ≦100° C. at 1 mm from the seal edge.
These zinc vanadium phosphate frits 106 also offer promise for meeting the hermeticity requirements for OLED sealing. Several 1″×1″ assemblies of Code 1737 glass plates heated either by infrared lamp 110b or 810 nm laser 110a and sealed with the 5895 blend frit 106 passed the He-leak test by holding vacuum down to the lowest leak rate measured by the equipment, 1×10−8 cm3/s. In addition, separate temperature measurements by an infrared camera, thermocouple, and thermal indicator paint made during 810 nm laser frit sealing all indicated a maximum temperature ≦100° C. at 1 mm from the seal edge.
Yet another potential low melting vanadium frit 106 suitable for sealing OLED displays 100 made from Code 1737 glass plates 102 and 107 is listed in TABLES 3 and 4. TABLE 3 reports this inventive vanadium frit 106, where all of the elements are specified in mole %:
TABLE 4 list a preferred composition of the vanadium frit 106 containing some of the elements listed in TABLE 3 and a β-eucryptite glass-ceramic additive filler. In particular, the preferred vanadium frit 106 had a 75:25 blend of the frit with the filler. Both these components making up the preferred vanadium frit 106 had a mean particle size of 5 microns.
In addition to the aforementioned frit compositions listed in TABLES 1-4, it should be understood that there may be other frit compositions which have yet to be developed but could be used to seal two glass plates.
Following are some of the different advantages and features of the present invention:
Although several embodiments of the present invention has been illustrated in the accompanying Drawings and described in the foregoing Detailed Description, it should be understood that the invention is not limited to the embodiments disclosed, but is capable of numerous rearrangements, modifications and substitutions without departing from the spirit of the invention as set forth and defined by the following claims.
This divisional application claims the priority of U.S. application Ser. No. 10/414,794, filed Apr. 16, 2003, now U.S. Pat. No. 6,998,776 entitled “GLASS PACKAGE THAT IS HERMETICALLY SEALED WITH A FRIT AND METHOD OF FABRICATION”.
Number | Name | Date | Kind |
---|---|---|---|
3414465 | Baak | Dec 1968 | A |
3520831 | Trap | Jul 1970 | A |
3614825 | Rottmiller | Oct 1971 | A |
3778126 | Wilson | Dec 1973 | A |
3885974 | Asahara et al. | May 1975 | A |
3973975 | Francel et al. | Aug 1976 | A |
3995941 | Nagahara et al. | Dec 1976 | A |
4206382 | DuBois | Jun 1980 | A |
4238704 | Bonk et al. | Dec 1980 | A |
4269617 | Shibuya et al. | May 1981 | A |
4330596 | Van Assche | May 1982 | A |
4400870 | Islam | Aug 1983 | A |
5192240 | Komatsu | Mar 1993 | A |
5281560 | Francis et al. | Jan 1994 | A |
5489321 | Tracy et al. | Feb 1996 | A |
5641611 | Shieh et al. | Jun 1997 | A |
5682453 | Daniel et al. | Oct 1997 | A |
5693111 | Kadowaki et al. | Dec 1997 | A |
5693956 | Shi et al. | Dec 1997 | A |
5734225 | Biebuyck et al. | Mar 1998 | A |
5771562 | Harvey, III et al. | Jun 1998 | A |
5821692 | Rogers et al. | Oct 1998 | A |
5855994 | Biebuyck et al. | Jan 1999 | A |
5872355 | Hueschen | Feb 1999 | A |
5874804 | Rogers | Feb 1999 | A |
5895228 | Biebuyck et al. | Apr 1999 | A |
5920080 | Jones | Jul 1999 | A |
5929474 | Huang | Jul 1999 | A |
5952778 | Haskal et al. | Sep 1999 | A |
5998805 | Shi et al. | Dec 1999 | A |
6069443 | Jones et al. | May 2000 | A |
6096496 | Frankel | Aug 2000 | A |
6137221 | Roitman et al. | Oct 2000 | A |
6146225 | Sheats et al. | Nov 2000 | A |
6226890 | Boroson et al. | May 2001 | B1 |
6268695 | Affinito | Jul 2001 | B1 |
6337381 | Biebuyck et al. | Jan 2002 | B1 |
6356376 | Tonar et al. | Mar 2002 | B1 |
6370019 | Matthies et al. | Apr 2002 | B1 |
6436222 | Andre et al. | Aug 2002 | B1 |
6436739 | Wickboldt et al. | Aug 2002 | B1 |
6465953 | Duggal | Oct 2002 | B1 |
6470594 | Boroson et al. | Oct 2002 | B1 |
6501044 | Klockhaus et al. | Dec 2002 | B1 |
6552488 | Roitman et al. | Apr 2003 | B1 |
6566805 | Tsai et al. | May 2003 | B1 |
6586496 | Takamatsu et al. | Jul 2003 | B1 |
6608283 | Liu et al. | Aug 2003 | B2 |
6661029 | Duggal | Dec 2003 | B1 |
6733850 | Domi et al. | May 2004 | B1 |
6734615 | Sugawara et al. | May 2004 | B2 |
6911667 | Pichler et al. | Jun 2005 | B2 |
6936963 | Langer et al. | Aug 2005 | B2 |
20010015620 | Affinito | Aug 2001 | A1 |
20010033135 | Duggal et al. | Oct 2001 | A1 |
20010045565 | Yamazaki | Nov 2001 | A1 |
20010048234 | Liu et al. | Dec 2001 | A1 |
20010049197 | Yamazaki et al. | Dec 2001 | A1 |
20010053082 | Chipalkatti et al. | Dec 2001 | A1 |
20010055841 | Yamazaki et al. | Dec 2001 | A1 |
20020003571 | Schofield et al. | Jan 2002 | A1 |
20020004577 | Biebuyck et al. | Jan 2002 | A1 |
20020008463 | Roch | Jan 2002 | A1 |
20020015032 | Koyama et al. | Feb 2002 | A1 |
20020031874 | Yamazaki et al. | Mar 2002 | A1 |
20020050958 | Matthies et al. | May 2002 | A1 |
20020080463 | Tonar et al. | Jun 2002 | A1 |
20020097368 | Kijima et al. | Jul 2002 | A1 |
20020109136 | Seo et al. | Aug 2002 | A1 |
20020113241 | Kubota et al. | Aug 2002 | A1 |
20020113763 | Koyama | Aug 2002 | A1 |
20020125484 | Silvernail et al. | Sep 2002 | A1 |
20020125822 | Graff et al. | Sep 2002 | A1 |
20020132047 | Yamazaki et al. | Sep 2002 | A1 |
20020133086 | Connelly et al. | Sep 2002 | A1 |
20020143258 | Weiner et al. | Oct 2002 | A1 |
20020149312 | Roberts et al. | Oct 2002 | A1 |
20020152800 | Bouten et al. | Oct 2002 | A1 |
20020154379 | Tonar et al. | Oct 2002 | A1 |
20020182828 | Asami et al. | Dec 2002 | A1 |
20020187254 | Ghosh et al. | Dec 2002 | A1 |
20020187594 | Yamazaki et al. | Dec 2002 | A1 |
20020190661 | Duggal et al. | Dec 2002 | A1 |
20030017297 | Song et al. | Jan 2003 | A1 |
20030066311 | Li et al. | Apr 2003 | A1 |
20030184219 | Duggal et al. | Oct 2003 | A1 |
20030222061 | Langer et al. | Dec 2003 | A1 |
20030227024 | Yoshii et al. | Dec 2003 | A1 |
20040069017 | Li et al. | Apr 2004 | A1 |
Number | Date | Country |
---|---|---|
1298397 | Apr 1970 | GB |
58-211743 | Dec 1983 | JP |
62-078128 | Apr 1987 | JP |
01-225140 | Sep 1989 | JP |
02-267137 | Oct 1990 | JP |
10-074583 | Mar 1998 | JP |
2001-319775 | Nov 2001 | JP |
2003-187962 | Jul 2003 | JP |
WO 9312049 | Jun 1993 | WO |
WO 0057499 | Sep 2000 | WO |
WO 0069002 | Nov 2000 | WO |
WO 0105205 | Jan 2001 | WO |
WO 0144865 | Jun 2001 | WO |
WO 0205361 | Jan 2002 | WO |
WO 0221557 | Mar 2002 | WO |
WO 03005774 | Jan 2003 | WO |
WO03005774 | Jan 2003 | WO |
WO 03100832 | Dec 2003 | WO |
Number | Date | Country | |
---|---|---|---|
20060009109 A1 | Jan 2006 | US |
Number | Date | Country | |
---|---|---|---|
Parent | 10414794 | Apr 2003 | US |
Child | 11228803 | US |