This application is a U.S. national phase application of PCT International Application PCT/KR2006/004716, filed Nov. 10, 2006, which claims priority to Korean Patent Application No. 2006-0110490, filed Nov. 9, 2006, and to Korean Patent Application No. 2005-0108274, filed Nov. 11, 2005, the contents of which are incorporated herein by reference in their entirety.
This invention relates generally to copper-alkaline-earth Silicate mixed crystal compounds activated by rare earth elements for using them as luminescent materials for ultraviolet as well as for visible light excitation for examples.
Copper is well-known as a monovalent activator in some orthophosphates (Wanmaker, W. L. and Bakker, C., J. Electrochem. Soc. 106, 1027, 1959) with an emission maximum at 490 nm.
The ground state of monovalent copper is a filled shell 3d10. That is the level 1S0. After exciting the lowest excited configuration is 3d94s. This configuration has two terms, 3D and 1D. The next higher configuration, 3d94p, gives 6 terms 3Po, 3Fo, 3Do, 1Fo, 1Do and 1Po. The transitions between the ground state 1S0 and the 1D and 3D are forbidden by parity or spin, respectively. In copper ions the excitation to the crystal field levels of 4p terms are allowed. Emission will be got either by a direct return from the crystal field odd state to the ground state or by a combination of transitions first from the odd state to a crystal field level and after that a second transition from these 3D or 1D state of the 3d94s configuration to the ground state.
The ground state of bivalent copper has 3d9-configuration. That is the level 2D5/2. In the bivalent copper one of the d-electrons can be excited to the 4s or 4p orbital. The lowest exciting configuration is the 3d84s with two quartet terms 4F, 4P and four doublet terms, 2F, 2D, 2P and 2G without emission caused by forbidden transitions. The higher exciting configuration is the 3d84p-configuration with four terms 4Do, 4Go, 4Fo, and 4Po, where emission can occur.
Copper (I) activated or co-activated sulphide-phosphors are well known and they are commercial used for cathode ray tubes. The green-emitting ZnS:Cu, Al (copper=activator, Al=co-activator) is very important in CRT applications.
In zinc-sulphide phosphors the luminescence can be classified into five kinds, depending on the relative ratio of the concentration of activators and co-activators (van Gool, W., Philips Res. Rept. Suppl., 3, 1, 1961). Here the luminescent centers are formed from deep donors or deep acceptors, or by their association at the nearest-neighbor sites (Phosphor Handbook, edited under the Auspice of Phosphor Research Society, CRC Press New York,
Orthophosphates activated by monovalent copper (Wanmaker, W. L., and Spier, H. L., JECS 109 (1962), 109), and pyrophosphates, alumosilicates, silicates, tripolyphosphates all activated by copper (I) are described in “Keith H. Butler, The Pennsylvania State University Press, 1980, S. 281”. Such phosphors can only be used for a short wave U.V. excitation, they are not excitable by longerwave radiation above about 350 nm. Because of their unstable chemical properties and their temperature behavior they cannot be used in fluorescent lamps.
The influence of copper ions as host lattice component in oxygen dominated compounds, activated by rare earth ions such as Eu2+, Ce3+ and others has not yet been described until now. From the theory of luminescent and solid state chemistry it should to be expected that the incorporation of copper as a host lattice component influences the luminescent-optical properties positively regarding improved luminescent intensity as well as desirable shifting of emission maxima, color points, shape of emission spectra and stabilizing of the lattice.
The influence of copper-ion as a component in a solid state mixed crystal should show improved luminescent properties for excitation wavelength higher than 360 nm. In this region of wavelength copper does not show own radiation transfers due to the energy levels of its electron configuration, so that any kind of exciting radiation can't be lost.
Copper containing luminescent mixed crystals or solid solutions should show improved emission intensities compared to luminescent materials having not that component in the host lattice. Furthermore, as a desirable effect copper containing luminescent mixed materials should show a shifting of the emission wavelengths to higher or to lower energies. For mixed crystals containing copper as a basic element this ion doesn't react as activator but the use of this ion leads to an influence of the crystal field splitting as well as the covalence, because copper (II) has a smaller radius (about 60 pm) and the electro-negativity (1.8) is higher than these of Barium, Strontium and Calcium (1). Furthermore, Cu (II) has a positive electrochemical reduction potential of +0.342 in contradiction to the negative potential of Alkaline Earth metals (−2.8 to −2.9).
Here an additional influence should to be expected. Due to the higher ionic potential of copper as a quotient of ionic charge and ionic radius compared to the bigger alkaline earth ions the copper ions can attract the neighboring oxygen ions stronger than the alkaline earth ions. So the substitution of the bigger alkaline earth ions Ca, Sr and Ba by copper leads to a changed crystal field in the surrounding of the activator ions, too. Thus the shape of emission bands can be influenced, the shifting of the emission peak to longer wavelength is connected with a broadening of the emission curves for band emission. Additionally it should be possible to increase the intensity of emission by substitution of copper ion for other basic metal ions. Generally the shifts of emission peaks to longer as well as to shorter wavelength are desirable in the field of LED lighting. Here it is necessary to realize a fine tuning to get a special wavelength for special color points as well as for better brightness of optical devices. By using the basic cation copper for substituting other cations like Ba, Sr, Ca, Mg, Zn and others such a fine tuning should be possible.
It is known, that some luminescent materials and phosphors and also Alkaline Earth Silicate phosphors are unstable in water, air humidity, water steam or polar solvents. For instance silicates with orthorhombic as well as Akermanite or Merwinite structures show more or less high sensitivity to water, air humidity, water steam or polar solvents caused by high basicity. Due to a higher covalence and a lower basicity as well as a positive reduction potential the incorporation of copper in a host lattice should improve this behavior of luminescent materials against water, air humidity and polar solvents if substituted for cations with a high basicity and a strongly negative reduction potential.
In view of the prior art described above, it is an object of the present invention to provide copper containing luminescent mixed crystal compounds which is a very good possibility to substitute earth alkaline ions by copper for shifting of the emission bands to longer or shorter wave lengths, respectively. In contrast to all papers prior art copper does not act as activator for emitting radiation. It is a component of the metal basic sublattice for modifying some properties determined by the metal ions like lattice parameters, electromagnetivity, surface properties and others, caused by the electromagnetic interactions within the lattice.
Another object of the present invention is to provide luminescent mixed crystal compounds between Copper Silicate and Alkaline Earth Silicates with improved luminescent properties and also with improved stability against water, humidity as well as other polar solvents.
Still another object of the present invention is to provide copper-alkaline-earth luminescent silicate mixed crystals, which have high color temperature range about 2,000K to 8,000K or 10,000K and CRI over 90, when mixed together with other phosphors.
To achieve these and other objects, as embodied and broadly described herein, luminescent materials for ultraviolet light or visible light excitation are containing copper-alkaline-earth mixed crystals from the basic family of Silicates or Germanates.
The luminescent material is composed of one or more than one compounds of silicate which is expressed in Formula 1, germanate/or germanate-silicate which is expressed in Formula 2:
a(M′O).b(M″O).c(M′″X).d(M′″2O).e(M″″2O3).f(M′″″oOp).g(SiO2).h(M″″″xOy) and (Formula 1)
a(M′O).b(M″2O).c(M″X).d(GeO2).e(M′″O).f(M″″2O3).g(M′″″oOp).h(M″″″xOy). (Formula 2)
Meanwhile, copper containing mixed crystals are used as a converter for the primary long-wave ultraviolet radiation in the range from 300-400 nm and/or blue radiation in the range from 380-500 nm from one or more single primary elements within a light emitting device to produce light in the visible region of the spectrum up to a high color rendering index Ra>90. And, copper containing mixed crystals characterized in that the phosphors are used in LED as single phosphors and/or in phosphor mixtures with different known phosphors for realizing white light with a color rendering up to a high color rendering >90.
Hereinafter, the present invention will be described in detail. Although the present invention has been described in connection with the preferred exemplary embodiments and the drawings, it is not limited thereto. The scope of the present invention is defined by the appended claims. Thus, it will be apparent to those skilled in the art that various changes and modifications can be made thereto without departing from the technical spirit and scope of the invention defined by the appended claims.
Luminescent materials for ultraviolet light or visible light excitation comprise a copper-alkaline-earth dominated mixed crystal silicate according to Formula 1 as follows:
a(M′O).b(M″O).c(M′″X).d(M′″2O).e(M″″2O3).f(M′″″oOp).g(SiO2).h(M″″″xOy) (Formula 1)
wherein M′ is Cu;
M″ is at least one or more divalent elements from the group consisting of Be, Mg, Ca, Sr, Ba, Zn, Cd, and Mn;
M′″ is at least one or more monovalent elements from the group consisting of Li, Na, K, Rb, Cs, Au, and Ag;
M″″ is at least one or more elements from the group consisting of B, Al, Ga, and In;
M′″″ is at least one or more elements from the group consisting of Ge, V, Nb, Ta, W, Mo, Ti, Zr, and Hf;
M″″″ is at least one or more elements from the group consisting of Bi, Sn, Sb, Sc, Y, La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu;
X is at least one or more elements from the group consisting of F, Cl, Br, and I;
0<a≦2;
0<b≦8;
0≦c≦4;
0≦d≦2;
0≦e≦2;
0≦f≦2;
0≦g≦10;
0≦h≦5;
1≦o≦2;
1≦p≦5;
1≦x≦2; and
1≦y≦5.
Examples of Preparation:
Preparation of the luminescent material having formula:
Cu0.05Sr1.7Ca0.25SiO4:Eu
Starting materials: CuO, SrCO3, CaCO3, SiO2, Eu2O3 and/or any combination thereof.
The starting materials in form of very pure oxides as well as carbonates have been mixed in stoichiometric proportions together with small amounts of flux (NH4Cl). In a first step the mixture will be fired in an alumina crucible at 1,200° C. in an inert gas atmosphere (N2 or noble gas) for 2-4 hours. After pre-firing the material will be milled again. In a second step the mixing will be fired in an alumina crucible at 1,200° C. in weakly reducing atmosphere for additional 2 hours. After that the material will be milled, washed, dried and sieved. The luminescent material has an emission maximum at 592 nm.
Preparation of the luminescent material having formula:
Cu0.2Ba2Zn0.2Mg0.6Si2O7:Eu
Starting materials: CuO, BaCO3, ZnO, MgO, SiO2, Eu2O3 and/or any combination thereof.
The starting materials in form of very pure oxides as well as carbonates have been mixed in stoichiometric proportions together with small amounts of flux (NH4Cl). In a first step the mixture will be fired in an alumina crucible at 1,100° C. in inert gas atmosphere for 1-2 hours. After pre-firing the material will be milled again. In a second step the mixing will be fired in an alumina crucible at 1,235° C. in reducing atmosphere for 2 hours. After that the material will be milled, washed, dried and sieved. The luminescent material has an emission maximum at 467 nm.
Results obtained concerning copper containing silicate mixed crystals activated by Rare Earths are shown in table 3.
Copper containing mixed crystals with Alkaline Earth germanates and/or germanate-silicates with the Formula 2 as follows:
a(M′O).b(M″2O).c(M″X).d(GeO2).e(M′″O).f(M″″2O3).g(M′″″oOp).h(M″″″xOy) (Formula 2)
wherein M′ is Cu;
M″ is at least one or more monovalent elements from the group consisting of Li, Na, K, Rb, Cs, Au, and Ag;
M′″ is at least one or more divalent elements from the group consisting of Be, Mg, Ca, Sr, Ba, Zn, Cd, and Mn;
M″″ is at least one or more trivalent elements from the group consisting of Sc, Y, B, Al, Ga, In, and La;
M′″″ is at least one or more elements from the group consisting of Si, Ti, Zr, Mn, V, Nd, Ta, W, Mo, and Nb;
M″″″ is at least one or more elements from the group consisting of Bi, Sn, Pr, Sm, Eu, Gd, Dy, and Tb;
X is at least one or more elements from the group consisting of F, Cl, Br, and I;
0<a≦2;
0≦b≦2;
0≦c≦10;
0<d≦10;
0≦e≦14;
0≦f≦14;
0≦g≦10;
0≦h≦2;
1≦o≦2;
1≦p≦5;
1≦x≦2; and
1≦y≦5
Preparation of the luminescent material with following formula:
Cu0.46Sr0.54Ge0.6Si0.4O3:Mn
Starting materials: CuO, SrCO3, GeO2, SiO2, MnCO3 and/or any combination thereof.
The starting materials in form of oxides as well as carbonates have been mixed in stoichiometric proportions together with small amounts of flux (NH4Cl). In a first step the mixture will be fired in an alumina crucible at 1,100° C. in oxygen containing atmosphere for 2 hours. After pre-firing the material will be milled again. In a second step the mixing will be fired in an alumina crucible at 1,180° C. in oxygen containing atmosphere for 4 hours again. After that the material will be milled, washed, dried and sieved. The luminescent material has an emission maximum at 658 nm.
Results obtained in respect to copper containing Alkaline Earth mixed crystals from the group consisting of germanates or germanate-silicates are shown in table 5.
In respect to changes in some properties of the compounds under consideration by introducing Cu the following physico—chemical changes could be achieved:
As shown in Table 6, caused by the slight changes of the lattice parameters of the phosphor contained copper, a slight change in the emission spectra can be observed. In general a shift of 0.5-1.0 nm to shorter wavelengths occurs.
Result of these changes are changes in sensitivity against water. The water stability of copper containing compounds are much higher than the water stability of compounds without copper. (table 8)
As shown in Table 7 and 8, this is caused by the decreasing mobility of the Alkaline Earths ions in the dissolving process. That means the rate and from this number of dissolved cations becomes lower resulting in lower hydrolysis and higher water stability.
Number | Date | Country | Kind |
---|---|---|---|
10-2005-0108274 | Nov 2005 | KR | national |
10-2006-0110490 | Nov 2006 | KR | national |
Filing Document | Filing Date | Country | Kind | 371c Date |
---|---|---|---|---|
PCT/KR2006/004716 | 11/10/2006 | WO | 00 | 8/18/2008 |
Publishing Document | Publishing Date | Country | Kind |
---|---|---|---|
WO2007/055538 | 5/18/2007 | WO | A |
Number | Name | Date | Kind |
---|---|---|---|
2110162 | Leverenz | Mar 1938 | A |
2402760 | Leverenz | Jun 1946 | A |
2570136 | Lyon | Oct 1951 | A |
2617773 | Nagy et al. | Nov 1952 | A |
2719128 | Kressin et al. | Sep 1955 | A |
2780600 | Wollentin | Feb 1957 | A |
3143510 | Wanmaker et al. | Aug 1964 | A |
3598752 | Sisneros et al. | Aug 1971 | A |
3644212 | McAllister et al. | Feb 1972 | A |
3893939 | De Kalb et al. | Jul 1975 | A |
3905911 | Kelsey, Jr. et al. | Sep 1975 | A |
4215289 | De Hair et al. | Jul 1980 | A |
4770950 | Ohnishi | Sep 1988 | A |
4972086 | Bryan et al. | Nov 1990 | A |
5032316 | Takahashi et al. | Jul 1991 | A |
5433295 | Murphy | Jul 1995 | A |
5472636 | Forster et al. | Dec 1995 | A |
5518808 | Bruno et al. | May 1996 | A |
5770110 | Schrell et al. | Jun 1998 | A |
5770111 | Moriyama et al. | Jun 1998 | A |
5853614 | Hao et al. | Dec 1998 | A |
5952681 | Chen | Sep 1999 | A |
5965192 | Potter | Oct 1999 | A |
5998925 | Shimizu | Dec 1999 | A |
6045722 | Leblans et al. | Apr 2000 | A |
6066861 | Hohn et al. | May 2000 | A |
6084250 | Justel et al. | Jul 2000 | A |
6373184 | Suh et al. | Apr 2002 | B1 |
6472765 | Sano | Oct 2002 | B1 |
6482664 | Lee | Nov 2002 | B1 |
6565771 | Ono et al. | May 2003 | B1 |
6670751 | Song et al. | Dec 2003 | B2 |
6686691 | Mueller | Feb 2004 | B1 |
6842664 | Harada | Jan 2005 | B2 |
6982045 | Menkara et al. | Jan 2006 | B2 |
6982048 | Atwater et al. | Jan 2006 | B1 |
6987353 | Menkara et al. | Jan 2006 | B2 |
7019335 | Suenage | Mar 2006 | B2 |
7029602 | Oshio | Apr 2006 | B2 |
7045078 | Choi | May 2006 | B2 |
7138770 | Uang et al. | Nov 2006 | B2 |
7189340 | Shimomura et al. | Mar 2007 | B2 |
7206507 | Lee et al. | Apr 2007 | B2 |
7229571 | Ezuhara | Jun 2007 | B2 |
7244965 | Andrews et al. | Jul 2007 | B2 |
7332746 | Takahashi et al. | Feb 2008 | B1 |
7554129 | Roth et al. | Jun 2009 | B2 |
7608200 | Seto et al. | Oct 2009 | B2 |
7679101 | Ota et al. | Mar 2010 | B2 |
7679281 | Kim et al. | Mar 2010 | B2 |
8070983 | Roth et al. | Dec 2011 | B2 |
8089084 | Roth et al. | Jan 2012 | B2 |
20020015013 | Ragle | Feb 2002 | A1 |
20030038295 | Koda | Feb 2003 | A1 |
20030168636 | Dobson | Sep 2003 | A1 |
20040051111 | Ota et al. | Mar 2004 | A1 |
20040135504 | Tamaki et al. | Jul 2004 | A1 |
20040136891 | Kijima et al. | Jul 2004 | A1 |
20040206970 | Martin | Oct 2004 | A1 |
20040251809 | Shimomura et al. | Dec 2004 | A1 |
20050001225 | Yoshimura et al. | Jan 2005 | A1 |
20050001537 | West et al. | Jan 2005 | A1 |
20050029927 | Setlur et al. | Feb 2005 | A1 |
20050117334 | Lee | Jun 2005 | A1 |
20050139846 | Park et al. | Jun 2005 | A1 |
20050141048 | Mizutani | Jun 2005 | A1 |
20050239227 | Aanegola et al. | Oct 2005 | A1 |
20050264161 | Oaku et al. | Dec 2005 | A1 |
20050274930 | Roth et al. | Dec 2005 | A1 |
20050274972 | Roth et al. | Dec 2005 | A1 |
20060158090 | Wang et al. | Jul 2006 | A1 |
20060261309 | Li et al. | Nov 2006 | A1 |
20060261350 | Kawazoe et al. | Nov 2006 | A1 |
20060267042 | Izuno et al. | Nov 2006 | A1 |
20070029526 | Cheng et al. | Feb 2007 | A1 |
20070247051 | Kuze et al. | Oct 2007 | A1 |
20070284563 | Lee | Dec 2007 | A1 |
20080036364 | Li et al. | Feb 2008 | A1 |
20080067472 | Roth et al. | Mar 2008 | A1 |
20080067920 | Roth et al. | Mar 2008 | A1 |
20080224163 | Roth et al. | Sep 2008 | A1 |
20090050847 | Xu et al. | Feb 2009 | A1 |
20090050849 | Lee | Feb 2009 | A1 |
20090134413 | Roth et al. | May 2009 | A1 |
20090262515 | Lee et al. | Oct 2009 | A1 |
20090303694 | Roth et al. | Dec 2009 | A1 |
20100002454 | Lee et al. | Jan 2010 | A1 |
20100207132 | Lee et al. | Aug 2010 | A1 |
Number | Date | Country |
---|---|---|
410266 | Mar 2003 | AT |
1218084 | Jun 1999 | CN |
1289454 | Mar 2001 | CN |
1317537 | Oct 2001 | CN |
1344777 | Apr 2002 | CN |
1434521 | Aug 2003 | CN |
1707819 | Dec 2005 | CN |
WO9812757 | Mar 1998 | DE |
10233050 | Feb 2004 | DE |
10259946 | Jul 2004 | DE |
0094132 | Nov 1983 | EP |
0382295 | Aug 1990 | EP |
0862794 | Sep 1998 | EP |
0 896 994 | Feb 1999 | EP |
1249837 | Oct 2002 | EP |
1249873 | Oct 2002 | EP |
1605030 | Dec 2005 | EP |
2031038 | Mar 2009 | EP |
1336053 | Nov 1973 | GB |
2016034 | Sep 1979 | GB |
31-1118 | Feb 1956 | JP |
33-8177 | Sep 1958 | JP |
38-6082 | May 1963 | JP |
39-8803 | May 1964 | JP |
47-6258 | Apr 1972 | JP |
49-38994 | Oct 1974 | JP |
55135190 | Oct 1980 | JP |
57109886 | Jul 1982 | JP |
61258892 | Nov 1986 | JP |
62-197487 | Sep 1987 | JP |
5-78659 | Mar 1993 | JP |
9-40946 | Feb 1997 | JP |
9040946 | Feb 1997 | JP |
9-153644 | Jun 1997 | JP |
WO9805078 | Feb 1998 | JP |
11-177143 | Jul 1999 | JP |
2000-260580 | Sep 2000 | JP |
2000-294387 | Oct 2000 | JP |
2001-115157 | Apr 2001 | JP |
2001-308393 | Nov 2001 | JP |
2001-524163 | Nov 2001 | JP |
2002-057376 | Feb 2002 | JP |
2002094122 | Mar 2002 | JP |
2002-97466 | Apr 2002 | JP |
200297466 | Apr 2002 | JP |
2002173677 | Jun 2002 | JP |
2002-531956 | Sep 2002 | JP |
2002335019 | Nov 2002 | JP |
2002-359403 | Dec 2002 | JP |
2002368277 | Dec 2002 | JP |
200364358 | Mar 2003 | JP |
2003-133595 | May 2003 | JP |
2003152229 | May 2003 | JP |
2003183649 | Jul 2003 | JP |
2003-224306 | Aug 2003 | JP |
2003321675 | Nov 2003 | JP |
2004-006582 | Jan 2004 | JP |
2004010786 | Jan 2004 | JP |
2004-88011 | Mar 2004 | JP |
2004071726 | Mar 2004 | JP |
2004-134699 | Apr 2004 | JP |
2004127988 | Apr 2004 | JP |
2004-192833 | Jul 2004 | JP |
2005-100799 | Apr 2005 | JP |
2005-100800 | Apr 2005 | JP |
2005-101296 | Apr 2005 | JP |
2005-153606 | Jun 2005 | JP |
2005-167177 | Jun 2005 | JP |
2006-503431 | Jan 2006 | JP |
2006-073656 | Mar 2006 | JP |
2006-252944 | Sep 2006 | JP |
2009-007545 | Jan 2009 | JP |
100232395 | Dec 1999 | KR |
10-2001-0032450 | Apr 2001 | KR |
1020010050839 | Jun 2001 | KR |
2001-101910 | Nov 2001 | KR |
1020020000835 | Jan 2002 | KR |
2002-0053975 | Jul 2002 | KR |
10-2002-0079513 | Oct 2002 | KR |
10-2003-0063211 | Jul 2003 | KR |
10-0392363 | Jul 2003 | KR |
200382395 | Oct 2003 | KR |
100426034 | Jul 2004 | KR |
10-2004-0088418 | Oct 2004 | KR |
10-2005-0008426 | Jan 2005 | KR |
10-2005-0070349 | Jul 2005 | KR |
1020050098462 | Oct 2005 | KR |
10-2005-0106945 | Nov 2005 | KR |
10-2005-0108816 | Nov 2005 | KR |
10-2005-0117164 | Dec 2005 | KR |
1020050117165 | Dec 2005 | KR |
100626272 | Sep 2006 | KR |
10-2006-0134728 | Dec 2006 | KR |
10-2007-0016900 | Feb 2007 | KR |
1020070050833 | May 2007 | KR |
10-2007-0064275 | Jun 2007 | KR |
10-2007-0084659 | Aug 2007 | KR |
10-2007-0086483 | Aug 2007 | KR |
10-2007-0098194 | Oct 2007 | KR |
10-2008-0074241 | Jul 2008 | KR |
10-2008-0075181 | Jul 2008 | KR |
I328885 | Mar 1999 | TW |
WO 9632457 | Oct 1996 | WO |
98-39805 | Sep 1998 | WO |
98-42798 | Oct 1998 | WO |
00-19546 | Apr 2000 | WO |
0033390 | Jun 2000 | WO |
01-41215 | Jun 2001 | WO |
02-054502 | Jul 2002 | WO |
02-054503 | Jul 2002 | WO |
02089219 | Nov 2002 | WO |
03-021691 | Mar 2003 | WO |
03030274 | Apr 2003 | WO |
2004036962 | Apr 2004 | WO |
2004-085570 | Oct 2004 | WO |
2004-111156 | Dec 2004 | WO |
2005068584 | Jul 2005 | WO |
WO 2005068584 | Jul 2005 | WO |
2005-109532 | Nov 2005 | WO |
2005-112137 | Nov 2005 | WO |
2006-043682 | Apr 2006 | WO |
2006-068359 | Jun 2006 | WO |
2006081803 | Aug 2006 | WO |
2006109659 | Oct 2006 | WO |
2007-035026 | Mar 2007 | WO |
2007-055538 | May 2007 | WO |
2007-069869 | Jun 2007 | WO |
2007-114614 | Nov 2007 | WO |
2009-028818 | Mar 2009 | WO |
Number | Date | Country | |
---|---|---|---|
20090152496 A1 | Jun 2009 | US |