Conventional magnetic recording disk drives include a slider attached to a suspension and a media such as a disk. The slider typically includes a magnetic read transducer (reader) and a magnetic write transducer (writer). The writer magnetically records data as bits along a tracks in the media. The reader reads data back from the media.
The trend in magnetic recording is to higher areal densities. For example, densities of up to 1 Tbit/in2 and higher are desired. To read, write and store data at such areal densities, the reader, writer, and media have evolved. For example, tunneling magnetoresistance (TMR) sensors may be used to read higher density media with sufficiently high signals. Perpendicular magnetic recording (PMR) writers and heat assisted magnetic recording (HAMR) writers, which utilize laser light to heat regions of the media to temperatures near and/or above the Curie temperature of the media, may be used to write to such high density media. Similarly, magnetic media have been developed to store data at higher areal densities.
Although such conventional magnetic recording disk drives function, there are drawbacks. For example, for high areal densities reduced noise, improved signal to noise ratio, and mechanisms to address other issues may be desired. Media that may be capable of providing these features are desired. Accordingly, what is needed is a system and method for improving the performance of a magnetic recording disk drive at higher areal densities.
The disk drive 100 includes a slider 110, a transducer 120 and media 150. Additional and/or different components may be included in the disk drive 100. For example, if the write transducer 120 is a HAMR writer, a laser might be included on or affixed to the slider 110. Although not shown, the slider 110, and thus the laser assembly 130 and transducer 120 are generally attached to a suspension (not shown).
The transducer 120 is fabricated on the slider 110 and includes an air-bearing surface (ABS) proximate to the media 150 during use. In general, the transducer 120 includes a write transducer and a read transducer. However, for clarity, only the write portion of the writer 120 is shown. The write transducer 120 includes a write pole 124 and coil(s) 126. The media 150 is configured to be usable at higher recording densities and, in some embodiments, to be used in the disk drive 100. In some embodiments, the media 150 is configured to store data with an areal density of at least 0.8 Tbit/in2. In some such embodiment, the media 150 may store data having an areal density of 1 Tbit/in2 or more.
The magnetic recording stack 154 stores magnetic data. The magnetic recording stack 154 is on the intermediate layer(s) 160 such that the intermediate layer(s) are between the substrate 152 and the magnetic recording stack 156. In some embodiments, the magnetic recording stack 154 includes multiple layers. For example, the magnetic recording stack 154 may include including exchange-control layers or exchange-break layers as well as magnetic layer(s) in which data are stored.
The intermediate layer(s) 160 include one or more layers. At least one of these layers is a multi-phase layer. The multi-phase layer is an alloy layer having multiple phases. The multiple phases include a majority phase and a secondary phase. Additional phases might be present. The majority phase has a first diffusion constant. The secondary phase has a second diffusion constant greater than the first diffusion constant. Thus, it is believed that the secondary phase segregates to the grain boundaries of the multi-phase layer. The majority phase has a first crystal structure, a first orientation, and a first composition. The secondary phase is a precipitate that segregates out of the majority. The secondary phase may have a second composition different from the first composition of the majority phase. The crystal structure and orientation of the secondary phase may be different from or the same as that of the majority phase. The first orientation and the first crystal structure of the majority phase are substantially unchanged by the secondary phase. For example, in the Ru layers described below, the majority phase of the layer may remain with a hexagonal close packed (HCP) crystal structure and the desired orientation despite the presence of the secondary phase. In some embodiments, this secondary phase is a eutectic phase.
The multi-phase layers may be considered to be formed by a primary material, or constituent, and at least one additional material that alloy to form the majority and secondary phases described above. The primary material may be an element or an alloy. Additional material(s) may be added in order to form the multiphase layer. The additional material(s) have limited solubility in the primary material(s) and form the secondary (e.g. eutectic) phase with the primary material(s) over a particular concentration range.
Composition of the alloy(s) used in the multi-phase layers may understood with reference to
For example, the multi-phase layer(s) in the intermediate layer(s) 160 may include an alloy that contains Ru. A multi-phase Ru-containing layer may include Ru and Co. In such a multi-phase RuCo layer, the Ru and Co may be alloyed with one or more other materials. There may be equal amount of Ru and Co. In other embodiments, there may be different concentrations of Ru and Co. However, both types of alloys are referred to herein as RuCo. In some embodiments, the additional material(s) added to RuCo to form the multi-phase layer may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is an alloy that forms the majority and secondary phases described above for certain concentration ranges. The secondary phase formed in such RuCo layers is a eutectic phase. For example, if the multi-phase layer is a (RuCo)100-wXw layer, where X is a material and w is a concentration, then X:w may be as follows: Al:0-30, Be:0-25, C:0-20, Dy:0-20, Gd:0-20, Ge:0-25, Ho:0-20, Lu:0-20, Mo:0-35, Nb:0-20, Nd:0-20, Pd:0-30, Sm:0-20, Tb:0-20, W:0-50, Y:0-20, Zr:0-20. Note that although zero concentrations are indicated above for the second constituents, there must be some of the material present. For example, if Al used, the concentration of Al is greater than zero and not more than thirty atomic percent. Such alloys include a first phase and a secondary eutectic phase having the properties described above.
Similarly, the multi-phase Ru-containing layer may include one or more layers in which Ru is alloyed with another material. In some embodiments, the additional material(s) may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is a Ru alloy that forms the majority and secondary phases described above for certain concentration ranges. In some embodiments, the secondary phase formed is a eutectic phase. For example, the multi-phase Ru containing layer may be a Ru—Mo alloy that includes not more than thirty-five atomic percent Mo. In other embodiments, the Ru-containing layer may be a Ru—Nb alloy that includes not more than twenty atomic percent Nb. In still other embodiments, the multi-phase Ru-containing layer may be a Ru—W alloy that includes not more than fifty percent of W if the Ru-containing layer includes W. If Al, Be, C, Dy, Gd, Ho, Lu, Sm, Tb, Y, Zr are used, then the multi-phase alloy includes Ru and both greater than zero and not more than twenty atomic percent of Al, Be, C, Dy, Gd, Ho, Lu, Sm, Tb, Y, Zr. If Ge is used, then the multi-phase alloy includes Ru and both greater than zero and not more than twenty-five atomic percent of Ge. If Pd is used, then the multi-phase alloy includes Ru and both greater than zero and not more than thirty atomic percent of Pd.
Further, multiple Ru layers may be included. One or more of these Ru layers may be multi-phase alloys. In some embodiments, two Ru layers that are sputtered at different pressures may be included. For example, a first Ru alloy layer may be sputtered at a first pressure and a second Ru layer may be sputtered at a second pressure. The second pressure is greater than the first pressure. For example, the first layer may be a Ru alloy layer that is sputtered at less than twenty mTorr. In some such embodiments, the pressure is on the order of seven mTorr. The second layer may be a Ru alloy layer that is sputtered at greater than 60 mTorr and not more than 120 mTorr. For example, the pressure may be ninety mTorr. The intermediate layer(s) 160 may include multiple Ru alloy layers and a Ru—Co containing layer. Some combination of these Ru-containing layers may be a multi-phase layer.
The magnetic media 150 may have improved performance. The magnetic media 150 includes intermediate layer(s) 160 that has at least one multi-phase layer. In this multi-phase layer, the grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries. In other words, the grain size (measure of the diameter/length of the grain) may be smaller and the variation in grain size may be smaller. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, the coercive squareness, nucleation field, coercivity and thermal stability of the magnetic recording stack 154 may be improved. Noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150 at higher densities may be improved.
In addition to the substrate 152, intermediate layer(s) 160 and magnetic recording stack 154, optional adhesion layer(s) 155, antiferromagnetically coupled soft underlayer 156, orientation control layer 158 and overcoat layer 159 are shown. The overcoat layer 159 is on the magnetic recording stack 154 and between the magnetic recording stack 154 and the slider 110. The optional adhesion layer(s) 155 may include Cr, CrTa, and/or CrTi layers. Although not shown, Ta based seed layer(s), Ni—W, Ni—W—Al, and/or Ni—W—Al—Fe based seed layer(s) (not explicitly shown in
The magnetic media 150′ may have improved performance for similar reasons as the magnetic media 150. The intermediate layer(s) 160 have at least one multi-phase layer for which the grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150′ at higher densities may be improved.
The high pressure Ru alloy layer 164 is a multi-phase layer. Thus, the high pressure Ru alloy layer 164 includes a majority phase and a secondary phase. The characteristics of the majority and secondary phases are as discussed above. The secondary phase has a diffusion constant greater than the majority phase's diffusion constant. Thus, it is believed that the secondary phase precipitates out of the majority and segregates to the grain boundaries of the layer 164. The majority phase has a first crystal structure, a first orientation, and a first composition. The secondary phase may have a second composition different from the first composition of the majority phase. The crystal structure and orientation of the secondary phase may be different from or the same as that of the majority phase. The first orientation and the first crystal structure of the majority phase are substantially unchanged by the secondary phase. For example, the majority phase of the layer 164 may remain with a hexagonal close packed (HCP) crystal structure and the desired orientation despite the presence of the secondary phase. In some embodiments, this secondary phase is a eutectic phase.
In some embodiments, the layer 164 is formed by alloying Ru with additional materials. The additional material(s) added to Ru to form the multi-phase layer may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is an alloy that forms the majority and secondary phases described above for certain concentration ranges. For example, if the multi-phase layer is a (Ru)100-wXw layer, where X is a material and w is a concentration, then X:w may be as follows: Al:0-30, Be:0-25, C:0-20, Dy:0-20, Gd:0-20, Ge:0-25, Ho:0-20, Lu:0-20, Mo:0-35, Nb:0-20, Nd:0-20, Pd:0-30, Sm:0-20, Tb:0-20, W:0-50, Y:0-20, Zr:0-20. Note that in the concentrations above, a concentration of zero for the additional material indicates the presence of greater than zero atomic percent of the material. Such alloys include a first phase and a secondary eutectic phase having the properties described above.
The intermediate layer 160′ may aid in improving the performance of the magnetic media 150 and/or 150′. The grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries in the layer 164. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150/150′ at higher densities may be improved by the layer 160′.
In the intermediate layer(s) 160″, the high pressure layer 164′ is a Ru layer while the low pressure layer 162′ is a multi-phase layer. Thus, the low pressure Ru alloy layer 162′ includes a majority phase and a secondary phase. The characteristics of the majority and secondary phases are as discussed above. The secondary phase has a diffusion constant greater than the majority phase's diffusion constant. Thus, it is believed that the secondary phase precipitates out of the majority and segregates to the grain boundaries of the low pressure layer 162′. The majority phase has a first crystal structure, a first orientation, and a first composition. The secondary phase may have a second composition different from the first composition of the majority phase. The crystal structure and orientation of the secondary phase may be different from or the same as that of the majority phase. The first orientation and the first crystal structure of the majority phase are substantially unchanged by the secondary phase. For example, the majority phase of the layer 162′ may remain with a hexagonal close packed (HCP) crystal structure and the desired orientation despite the presence of the secondary phase. In some embodiments, this secondary phase is a eutectic phase.
In some embodiments, the layer 162′ is formed by alloying Ru with additional materials. The additional material(s) added to Ru to form the multi-phase layer may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is an alloy that forms the majority and secondary phases described above for certain concentration ranges. For example, if the multi-phase layer is a (Ru)100-wXw layer, where X is a material and w is a concentration, then X:w may be as follows: Al:0-30, Be:0-25, C:0-20, Dy:0-20, Gd:0-20, Ge:0-25, Ho:0-20, Lu:0-20, Mo:0-35, Nb:0-20, Nd:0-20, Pd:0-30, Sm:0-20, Tb:0-20, W:0-50, Y:0-20, Zr:0-20. A concentration of 0 atomic percent for the additional material corresponds to a concentration of greater than zero atomic percent. Such alloys include a first phase and a secondary eutectic phase having the properties described above.
The intermediate layer 160″ may aid in improving the performance of the magnetic media 150 and/or 150′. The grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries in the layer 162′. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150/150′ at higher densities may be improved by the layer 160″.
The layers 162′ and 164 are both multi-phase alloy layers. Thus, each of the layers 162′ and 164 includes a majority phase and a secondary phase. The characteristics of the majority and secondary phases are as discussed above. The secondary phase has a diffusion constant greater than the majority phase's diffusion constant. Thus, it is believed that the secondary phase precipitates out of the majority and segregates to the grain boundaries of the layers 162′ and 164. The majority phase has a first crystal structure, a first orientation, and a first composition. The secondary phase may have a second composition different from the first composition of the majority phase. The crystal structure and orientation of the secondary phase may be different from or the same as that of the majority phase. The first orientation and the first crystal structure of the majority phase are substantially unchanged by the secondary phase. For example, the majority phase of the layers 162′ and 164 may remain with a hexagonal close packed (HCP) crystal structure and the desired orientation despite the presence of the secondary phase. In some embodiments, this secondary phase is a eutectic phase.
In some embodiments, the layers 162′ and 164 are each formed by alloying Ru with additional materials. The additional material(s) added to Ru to form the multi-phase layer may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is an alloy that forms the majority and secondary phases described above for certain concentration ranges. For example, if the multi-phase layer is a (Ru)100-wXw layer, where X is a material and w is a concentration, then X:w may be as follows: Al:0-30, Be:0-25, C:0-20, Dy:0-20, Gd:0-20, Ge:0-25, Ho:0-20, Lu:0-20, Mo:0-35, Nb:0-20, Nd:0-20, Pd:0-30, Sm:0-20, Tb:0-20, W:0-50, Y:0-20, Zr:0-20. Note that a 0 atomic percent in the previous sentence indicates a concentration of greater than zero atomic percent for the additional material(s). Such alloys include a first phase and a secondary eutectic phase having the properties described above. Note that the compositions of the layers 162′ and 164 may be the same or different. For example, layers 162′ and 164 may be both Ru—Mo layers. In another embodiment, the layer 162′ may be a Ru—W layer while the layer 164 is a Ru—Mo layer.
The intermediate layer 160′″ may aid in improving the performance of the magnetic media 150 and/or 150′. The grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries in the layers 162′ and 164. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150/150′ at higher densities may be improved by the layer 160′″.
The intermediate layer 170 may aid in improving the performance of the magnetic media 150 and/or 150′. The grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries in the layers 174 and/or 176. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150/150′ at higher densities may be improved by the layer 170.
The RuCo layer 172′ includes RuCo alloyed with at least a second material. In some embodiments, the RuCo layer 172′ is at least two nanometers thick and not more than twelve nanometers thick. In some embodiments, the RuCo layer 172′ is at least five nanometers thick and not more than eight nanometers thick. Thus, the RuCo layer 172′ includes a majority phase and a secondary phase. The characteristics of the majority and secondary phases are as discussed above. In some embodiments, the additional material(s) added to RuCo to form the multi-phase layer may be selected from Mo, Nb, W, Al, Be, C, Dy, Gd, Ge, Ho, Lu, Nd, Pd, Sm, Tb, Y and Zr. The combination is an alloy that forms the majority and secondary phases described above for certain concentration ranges. The secondary phase formed in such RuCo layers is a eutectic phase. For example, if the multi-phase layer is a (RuCo)100-wXw layer, where X is a material and w is a concentration, then X:w may be as follows: Al:0-30, Be:0-25, C:0-20, Dy:0-20, Gd:0-20, Ge:0-25, Ho:0-20, Lu:0-20, Mo:0-35, Nb:0-20, Nd:0-20, Pd:0-30, Sm:0-20, Tb:0-20, W:0-50, Y:0-20, Zr:0-20. Note that although zero concentrations are indicated above for the second constituents, there must be some of the material present. Such an alloys include a first, majority phase and a secondary eutectic phase having the properties described above.
In one embodiment, the intermediate layer(s) 170′ include a multi-phase RuCo alloy layer 172′, a low pressure Ru layer 174 analogous to the layer 162, and a high pressure multi-phase layer 176 analogous to the layer 164. In another embodiment, the intermediate layer(s) 170′ include a multi-phase RuCo alloy layer 172′, a low pressure multi-phase Ru layer 174 analogous to the layer 162′, and a high pressure layer 176 analogous to the layer 164′. In another embodiment, the intermediate layer(s) 170′ include a multi-phase RuCo alloy layer 172′, a low pressure multi-phase Ru layer 174 analogous to the layer 162′, and a high pressure multi-phase layer 176 analogous to the layer 164. Thus, the RuCo layer 172′ and one or both of the layers 174 and 176 includes a majority phase and a secondary phase. The characteristics of the majority and secondary phases are as discussed above.
The intermediate layer 170′ may aid in improving the performance of the magnetic media 150 and/or 150′. The grain size and distribution may be controlled by the segregation of secondary (e.g. eutectic) phase to the grain boundaries in the layers 172′ and one or both of the layers 174 and 176. Thus, the grain size may be smaller and the variation in grain size may be reduced. This reduction in grain size and distribution may be passed on to the magnetic recording stack 154. As a result, noise may thus be reduced and signal-to-noise ratio enhanced. Thus, performance of the magnetic recording media 150/150′ at higher densities may be improved by the layer 170′.
Referring to
The magnetic recording stack 154 is provided on the intermediate layer(s) 160, via step 204. Step 204 may include depositing multiple layers such as exchange coupling or exchange breaking layer(s). Fabrication of the media 150/150′ may then be completed.
Using the method 200, the magnetic disk drive 100 and magnetic recording media 150/150′ may be provided. Thus, the benefits of the magnetic recording media 150/150′ and magnetic recording transducer 120 may be achieved.
Referring to
The magnetic recording layer 154 may be deposited, via step 224. Step 222 may include depositing multiple magnetic layers. Fabrication of the magnetic recording media 150/150′ may then be completed. For example, the overcoat layer 159 may also be provided after step 222.
Using the method 210, the magnetic disk drive 100 and magnetic recording media 150/150′ may be provided. Thus, the benefits of the magnetic recording media 150′ and disk drive 100 may be achieved.
Number | Name | Date | Kind |
---|---|---|---|
6013161 | Chen et al. | Jan 2000 | A |
6063248 | Bourez et al. | May 2000 | A |
6068891 | O'Dell et al. | May 2000 | A |
6086730 | Liu et al. | Jul 2000 | A |
6099981 | Nishimori | Aug 2000 | A |
6103404 | Ross et al. | Aug 2000 | A |
6117499 | Wong et al. | Sep 2000 | A |
6136403 | Prabhakara et al. | Oct 2000 | A |
6143375 | Ross et al. | Nov 2000 | A |
6145849 | Bae et al. | Nov 2000 | A |
6146737 | Malhotra et al. | Nov 2000 | A |
6149696 | Jia | Nov 2000 | A |
6150015 | Bertero et al. | Nov 2000 | A |
6156404 | Ross et al. | Dec 2000 | A |
6159076 | Sun et al. | Dec 2000 | A |
6164118 | Suzuki et al. | Dec 2000 | A |
6200441 | Gornicki et al. | Mar 2001 | B1 |
6204995 | Hokkyo et al. | Mar 2001 | B1 |
6206765 | Sanders et al. | Mar 2001 | B1 |
6210819 | Lal et al. | Apr 2001 | B1 |
6216709 | Fung et al. | Apr 2001 | B1 |
6221119 | Homola | Apr 2001 | B1 |
6248395 | Homola et al. | Jun 2001 | B1 |
6261681 | Suekane et al. | Jul 2001 | B1 |
6270885 | Hokkyo et al. | Aug 2001 | B1 |
6274063 | Li et al. | Aug 2001 | B1 |
6283838 | Blake et al. | Sep 2001 | B1 |
6287429 | Moroishi et al. | Sep 2001 | B1 |
6290573 | Suzuki | Sep 2001 | B1 |
6299947 | Suzuki et al. | Oct 2001 | B1 |
6303217 | Malhotra et al. | Oct 2001 | B1 |
6309765 | Suekane et al. | Oct 2001 | B1 |
6358636 | Yang et al. | Mar 2002 | B1 |
6362452 | Suzuki et al. | Mar 2002 | B1 |
6363599 | Bajorek | Apr 2002 | B1 |
6365012 | Sato et al. | Apr 2002 | B1 |
6381090 | Suzuki et al. | Apr 2002 | B1 |
6381092 | Suzuki | Apr 2002 | B1 |
6387483 | Hokkyo et al. | May 2002 | B1 |
6391213 | Homola | May 2002 | B1 |
6395349 | Salamon | May 2002 | B1 |
6403919 | Salamon | Jun 2002 | B1 |
6408677 | Suzuki | Jun 2002 | B1 |
6426157 | Hokkyo et al. | Jul 2002 | B1 |
6429984 | Alex | Aug 2002 | B1 |
6482330 | Bajorek | Nov 2002 | B1 |
6482505 | Bertero et al. | Nov 2002 | B1 |
6500567 | Bertero et al. | Dec 2002 | B1 |
6528124 | Nguyen | Mar 2003 | B1 |
6548821 | Treves et al. | Apr 2003 | B1 |
6552871 | Suzuki et al. | Apr 2003 | B2 |
6565719 | Lairson et al. | May 2003 | B1 |
6566674 | Treves et al. | May 2003 | B1 |
6571806 | Rosano et al. | Jun 2003 | B2 |
6628466 | Alex | Sep 2003 | B2 |
6664503 | Hsieh et al. | Dec 2003 | B1 |
6670055 | Tomiyasu et al. | Dec 2003 | B2 |
6682807 | Lairson et al. | Jan 2004 | B2 |
6683754 | Suzuki et al. | Jan 2004 | B2 |
6730420 | Bertero et al. | May 2004 | B1 |
6743528 | Suekane et al. | Jun 2004 | B2 |
6759138 | Tomiyasu et al. | Jul 2004 | B2 |
6778353 | Harper | Aug 2004 | B1 |
6795274 | Hsieh et al. | Sep 2004 | B1 |
6855232 | Jairson et al. | Feb 2005 | B2 |
6857937 | Bajorek | Feb 2005 | B2 |
6893748 | Bertero et al. | May 2005 | B2 |
6899959 | Bertero et al. | May 2005 | B2 |
6916558 | Umezawa et al. | Jul 2005 | B2 |
6939120 | Harper | Sep 2005 | B1 |
6946191 | Morikawa et al. | Sep 2005 | B2 |
6967798 | Homola et al. | Nov 2005 | B2 |
6972135 | Homola | Dec 2005 | B2 |
7004827 | Suzuki et al. | Feb 2006 | B1 |
7006323 | Suzuki | Feb 2006 | B1 |
7016154 | Nishihira | Mar 2006 | B2 |
7019924 | McNeil et al. | Mar 2006 | B2 |
7045215 | Shimokawa | May 2006 | B2 |
7070870 | Bertero et al. | Jul 2006 | B2 |
7090934 | Hokkyo et al. | Aug 2006 | B2 |
7099112 | Harper | Aug 2006 | B1 |
7105241 | Shimokawa et al. | Sep 2006 | B2 |
7119990 | Bajorek et al. | Oct 2006 | B2 |
7147790 | Wachenschwanz et al. | Dec 2006 | B2 |
7161753 | Wachenschwanz et al. | Jan 2007 | B2 |
7166319 | Ishiyama | Jan 2007 | B2 |
7166374 | Suekane et al. | Jan 2007 | B2 |
7169487 | Kawai et al. | Jan 2007 | B2 |
7174775 | Ishiyama | Feb 2007 | B2 |
7179549 | Malhotra et al. | Feb 2007 | B2 |
7184139 | Treves et al. | Feb 2007 | B2 |
7196860 | Alex | Mar 2007 | B2 |
7199977 | Suzuki et al. | Apr 2007 | B2 |
7208236 | Morikawa et al. | Apr 2007 | B2 |
7220500 | Tomiyasu et al. | May 2007 | B1 |
7229266 | Harper | Jun 2007 | B2 |
7239970 | Treves et al. | Jul 2007 | B2 |
7252897 | Shimokawa et al. | Aug 2007 | B2 |
7277254 | Shimokawa et al. | Oct 2007 | B2 |
7281920 | Homola et al. | Oct 2007 | B2 |
7292329 | Treves et al. | Nov 2007 | B2 |
7301726 | Suzuki | Nov 2007 | B1 |
7302148 | Treves et al. | Nov 2007 | B2 |
7305119 | Treves et al. | Dec 2007 | B2 |
7314404 | Singh et al. | Jan 2008 | B2 |
7320584 | Harper et al. | Jan 2008 | B1 |
7329114 | Harper et al. | Feb 2008 | B2 |
7375362 | Treves et al. | May 2008 | B2 |
7420886 | Tomiyasu et al. | Sep 2008 | B2 |
7425719 | Treves et al. | Sep 2008 | B2 |
7471484 | Wachenschwanz et al. | Dec 2008 | B2 |
7498062 | Calcaterra et al. | Mar 2009 | B2 |
7531485 | Hara et al. | May 2009 | B2 |
7537846 | Ishiyama et al. | May 2009 | B2 |
7549209 | Wachenschwanz et al. | Jun 2009 | B2 |
7569490 | Staud | Aug 2009 | B2 |
7597792 | Homola et al. | Oct 2009 | B2 |
7597973 | Ishiyama | Oct 2009 | B2 |
7608193 | Wachenschwanz et al. | Oct 2009 | B2 |
7632087 | Homola | Dec 2009 | B2 |
7656615 | Wachenschwanz et al. | Feb 2010 | B2 |
7682546 | Harper | Mar 2010 | B2 |
7684152 | Suzuki et al. | Mar 2010 | B2 |
7686606 | Harper et al. | Mar 2010 | B2 |
7686991 | Harper | Mar 2010 | B2 |
7695833 | Ishiyama | Apr 2010 | B2 |
7722968 | Ishiyama | May 2010 | B2 |
7733605 | Suzuki et al. | Jun 2010 | B2 |
7736768 | Ishiyama | Jun 2010 | B2 |
7755861 | Li et al. | Jul 2010 | B1 |
7758732 | Calcaterra et al. | Jul 2010 | B1 |
7833639 | Sonobe et al. | Nov 2010 | B2 |
7833641 | Tomiyasu et al. | Nov 2010 | B2 |
7910159 | Jung | Mar 2011 | B2 |
7911736 | Bajorek | Mar 2011 | B2 |
7924519 | Lambert | Apr 2011 | B2 |
7944165 | O'Dell | May 2011 | B1 |
7944643 | Jiang et al. | May 2011 | B1 |
7955723 | Umezawa et al. | Jun 2011 | B2 |
7983003 | Sonobe et al. | Jul 2011 | B2 |
7993497 | Moroishi et al. | Aug 2011 | B2 |
7993765 | Kim et al. | Aug 2011 | B2 |
7998912 | Chen et al. | Aug 2011 | B2 |
8002901 | Chen et al. | Aug 2011 | B1 |
8003237 | Sonobe et al. | Aug 2011 | B2 |
8012920 | Shimokawa | Sep 2011 | B2 |
8038863 | Homola | Oct 2011 | B2 |
8057926 | Ayama et al. | Nov 2011 | B2 |
8062778 | Suzuki et al. | Nov 2011 | B2 |
8064156 | Suzuki et al. | Nov 2011 | B1 |
8076013 | Sonobe et al. | Dec 2011 | B2 |
8089829 | Akagi et al. | Jan 2012 | B2 |
8092931 | Ishiyama et al. | Jan 2012 | B2 |
8100685 | Harper et al. | Jan 2012 | B1 |
8101054 | Chen et al. | Jan 2012 | B2 |
8125723 | Nichols et al. | Feb 2012 | B1 |
8125724 | Nichols et al. | Feb 2012 | B1 |
8137517 | Bourez | Mar 2012 | B1 |
8142916 | Umezawa et al. | Mar 2012 | B2 |
8163093 | Chen et al. | Apr 2012 | B1 |
8171949 | Lund et al. | May 2012 | B1 |
8173282 | Sun et al. | May 2012 | B1 |
8178480 | Hamakubo et al. | May 2012 | B2 |
8206789 | Suzuki | Jun 2012 | B2 |
8218260 | Iamratanakul et al. | Jul 2012 | B2 |
8247095 | Champion et al. | Aug 2012 | B2 |
8257783 | Suzuki et al. | Sep 2012 | B2 |
8298609 | Liew et al. | Oct 2012 | B1 |
8298689 | Sonobe et al. | Oct 2012 | B2 |
8309239 | Umezawa et al. | Nov 2012 | B2 |
8316668 | Chan et al. | Nov 2012 | B1 |
8331056 | O'Dell | Dec 2012 | B2 |
8354618 | Chen et al. | Jan 2013 | B1 |
8367228 | Sonobe et al. | Feb 2013 | B2 |
8383209 | Ayama | Feb 2013 | B2 |
8390956 | Tonooka et al. | Mar 2013 | B2 |
8394243 | Jung et al. | Mar 2013 | B1 |
8397751 | Chan et al. | Mar 2013 | B1 |
8399809 | Bourez | Mar 2013 | B1 |
8402638 | Treves et al. | Mar 2013 | B1 |
8404056 | Chen et al. | Mar 2013 | B1 |
8404369 | Ruffini et al. | Mar 2013 | B2 |
8404370 | Sato et al. | Mar 2013 | B2 |
8406918 | Tan et al. | Mar 2013 | B2 |
8414966 | Yasumori et al. | Apr 2013 | B2 |
8425975 | Ishiyama | Apr 2013 | B2 |
8431257 | Kim et al. | Apr 2013 | B2 |
8431258 | Onoue et al. | Apr 2013 | B2 |
8453315 | Kajiwara et al. | Jun 2013 | B2 |
8488276 | Jung et al. | Jul 2013 | B1 |
8491800 | Dorsey | Jul 2013 | B1 |
8492009 | Homola et al. | Jul 2013 | B1 |
8492011 | Itoh et al. | Jul 2013 | B2 |
8496466 | Treves et al. | Jul 2013 | B1 |
8517364 | Crumley et al. | Aug 2013 | B1 |
8517657 | Chen et al. | Aug 2013 | B2 |
8524052 | Tan et al. | Sep 2013 | B1 |
8530065 | Chernyshov et al. | Sep 2013 | B1 |
8546000 | Umezawa | Oct 2013 | B2 |
8551253 | Na'im et al. | Oct 2013 | B2 |
8551627 | Shimada et al. | Oct 2013 | B2 |
8556566 | Suzuki et al. | Oct 2013 | B1 |
8559131 | Masuda et al. | Oct 2013 | B2 |
8562748 | Chen et al. | Oct 2013 | B1 |
8565050 | Bertero et al. | Oct 2013 | B1 |
8570844 | Yuan et al. | Oct 2013 | B1 |
8580410 | Onoue | Nov 2013 | B2 |
8584687 | Chen et al. | Nov 2013 | B1 |
8591709 | Lim et al. | Nov 2013 | B1 |
8592060 | Tamai et al. | Nov 2013 | B2 |
8592061 | Onoue et al. | Nov 2013 | B2 |
8596287 | Chen et al. | Dec 2013 | B1 |
8597723 | Jung et al. | Dec 2013 | B1 |
8603649 | Onoue | Dec 2013 | B2 |
8603650 | Sonobe et al. | Dec 2013 | B2 |
8605388 | Yasumori et al. | Dec 2013 | B2 |
8605555 | Chernyshov et al. | Dec 2013 | B1 |
8608147 | Yap et al. | Dec 2013 | B1 |
8609263 | Chernyshov et al. | Dec 2013 | B1 |
8619381 | Moser et al. | Dec 2013 | B2 |
8623528 | Umezawa et al. | Jan 2014 | B2 |
8623529 | Suzuki | Jan 2014 | B2 |
8634155 | Yasumori et al. | Jan 2014 | B2 |
8658003 | Bourez | Feb 2014 | B1 |
8658292 | Mallary et al. | Feb 2014 | B1 |
8665541 | Saito | Mar 2014 | B2 |
8668953 | Buechel-Rimmel | Mar 2014 | B1 |
8674327 | Poon et al. | Mar 2014 | B1 |
8685214 | Moh et al. | Apr 2014 | B1 |
8685547 | Bian et al. | Apr 2014 | B2 |
8696404 | Sun et al. | Apr 2014 | B2 |
8696874 | Wang et al. | Apr 2014 | B2 |
8711499 | Desai et al. | Apr 2014 | B1 |
8743666 | Bertero et al. | Jun 2014 | B1 |
8758912 | Srinivasan et al. | Jun 2014 | B2 |
8787124 | Chernyshov et al. | Jul 2014 | B1 |
8787130 | Yuan et al. | Jul 2014 | B1 |
8791391 | Bourez | Jul 2014 | B2 |
8795765 | Koike et al. | Aug 2014 | B2 |
8795790 | Sonobe et al. | Aug 2014 | B2 |
8795857 | Ayama et al. | Aug 2014 | B2 |
8800322 | Chan et al. | Aug 2014 | B1 |
8811129 | Yuan et al. | Aug 2014 | B1 |
8817410 | Moser et al. | Aug 2014 | B1 |
20020060883 | Suzuki | May 2002 | A1 |
20030022024 | Wachenschwanz | Jan 2003 | A1 |
20030219630 | Moriwaki | Nov 2003 | A1 |
20040022387 | Weikle | Feb 2004 | A1 |
20040047758 | Olson et al. | Mar 2004 | A1 |
20040132301 | Harper et al. | Jul 2004 | A1 |
20040202793 | Harper et al. | Oct 2004 | A1 |
20040202865 | Homola et al. | Oct 2004 | A1 |
20040209123 | Bajorek et al. | Oct 2004 | A1 |
20040209470 | Bajorek | Oct 2004 | A1 |
20050036223 | Wachenschwanz et al. | Feb 2005 | A1 |
20050142990 | Homola | Jun 2005 | A1 |
20050150862 | Harper et al. | Jul 2005 | A1 |
20050151282 | Harper et al. | Jul 2005 | A1 |
20050151283 | Bajorek et al. | Jul 2005 | A1 |
20050151300 | Harper et al. | Jul 2005 | A1 |
20050155554 | Saito | Jul 2005 | A1 |
20050167867 | Bajorek et al. | Aug 2005 | A1 |
20050263401 | Olsen et al. | Dec 2005 | A1 |
20060147758 | Jung et al. | Jul 2006 | A1 |
20060181697 | Treves et al. | Aug 2006 | A1 |
20060207890 | Staud | Sep 2006 | A1 |
20070070549 | Suzuki et al. | Mar 2007 | A1 |
20070245909 | Homola | Oct 2007 | A1 |
20080075845 | Sonobe et al. | Mar 2008 | A1 |
20080093760 | Harper et al. | Apr 2008 | A1 |
20080131735 | Das et al. | Jun 2008 | A1 |
20090117408 | Umezawa et al. | May 2009 | A1 |
20090130346 | Osawa et al. | May 2009 | A1 |
20090136784 | Suzuki et al. | May 2009 | A1 |
20090169922 | Ishiyama | Jul 2009 | A1 |
20090191331 | Umezawa et al. | Jul 2009 | A1 |
20090202866 | Kim et al. | Aug 2009 | A1 |
20090311557 | Onoue et al. | Dec 2009 | A1 |
20100143752 | Ishibashi et al. | Jun 2010 | A1 |
20100190035 | Sonobe et al. | Jul 2010 | A1 |
20100196619 | Ishiyama | Aug 2010 | A1 |
20100196740 | Ayama et al. | Aug 2010 | A1 |
20100209601 | Shimokawa et al. | Aug 2010 | A1 |
20100215992 | Horikawa et al. | Aug 2010 | A1 |
20100232065 | Suzuki et al. | Sep 2010 | A1 |
20100247965 | Onoue | Sep 2010 | A1 |
20100261039 | Itoh et al. | Oct 2010 | A1 |
20100279151 | Sakamoto et al. | Nov 2010 | A1 |
20100300884 | Homola et al. | Dec 2010 | A1 |
20100304186 | Shimokawa | Dec 2010 | A1 |
20110097603 | Onoue | Apr 2011 | A1 |
20110097604 | Onoue | Apr 2011 | A1 |
20110151280 | Takahashi | Jun 2011 | A1 |
20110171495 | Tachibana et al. | Jul 2011 | A1 |
20110206947 | Tachibana et al. | Aug 2011 | A1 |
20110212346 | Onoue et al. | Sep 2011 | A1 |
20110223446 | Onoue et al. | Sep 2011 | A1 |
20110244119 | Umezawa et al. | Oct 2011 | A1 |
20110299194 | Aniya et al. | Dec 2011 | A1 |
20110311841 | Saito et al. | Dec 2011 | A1 |
20120069466 | Okamoto et al. | Mar 2012 | A1 |
20120070692 | Sato et al. | Mar 2012 | A1 |
20120077060 | Ozawa | Mar 2012 | A1 |
20120127599 | Shimokawa et al. | May 2012 | A1 |
20120127601 | Suzuki et al. | May 2012 | A1 |
20120129009 | Sato et al. | May 2012 | A1 |
20120140359 | Tachibana | Jun 2012 | A1 |
20120141833 | Umezawa et al. | Jun 2012 | A1 |
20120141835 | Sakamoto | Jun 2012 | A1 |
20120148875 | Hamakubo et al. | Jun 2012 | A1 |
20120156523 | Seki et al. | Jun 2012 | A1 |
20120164488 | Shin et al. | Jun 2012 | A1 |
20120170152 | Sonobe et al. | Jul 2012 | A1 |
20120171369 | Koike et al. | Jul 2012 | A1 |
20120175243 | Fukuura et al. | Jul 2012 | A1 |
20120189872 | Umezawa et al. | Jul 2012 | A1 |
20120196049 | Azuma et al. | Aug 2012 | A1 |
20120207919 | Sakamoto et al. | Aug 2012 | A1 |
20120225217 | Itoh et al. | Sep 2012 | A1 |
20120251842 | Yuan et al. | Oct 2012 | A1 |
20120251846 | Desai et al. | Oct 2012 | A1 |
20120276417 | Shimokawa et al. | Nov 2012 | A1 |
20120308722 | Suzuki et al. | Dec 2012 | A1 |
20130040167 | Alagarsamy et al. | Feb 2013 | A1 |
20130071694 | Srinivasan | Mar 2013 | A1 |
20130165029 | Sun et al. | Jun 2013 | A1 |
20130175252 | Bourez | Jul 2013 | A1 |
20130216865 | Yasumori et al. | Aug 2013 | A1 |
20130230647 | Onoue et al. | Sep 2013 | A1 |
20130314815 | Yuan et al. | Nov 2013 | A1 |
20140011054 | Suzuki | Jan 2014 | A1 |
20140044992 | Onoue | Feb 2014 | A1 |
20140050843 | Yi et al. | Feb 2014 | A1 |
20140151360 | Gregory et al. | Jun 2014 | A1 |
20140234666 | Knigge et al. | Aug 2014 | A1 |
Entry |
---|
Kumar Srinivasan, et al., U.S. Appl. No. 14/497,299, filed Sep. 25, 2014, 37 pages. |
Brown, A.M., “Correlations for Diffusion Constants,” Acta Metallurgica, vol. 28, Jan. 1980, pp. 1085-1101. |
MSE 201, Introduction to Materials Science, Diffusion, Callister, Ch. 5, University of Tennessee, Dept. of Materials Science and Engineering, pp. 1-26. |
Number | Date | Country | |
---|---|---|---|
20160155460 A1 | Jun 2016 | US |