Thermal barrier layers and seed layers for control of thermal and structural properties of HAMR media

Information

  • Patent Grant
  • 10236026
  • Patent Number
    10,236,026
  • Date Filed
    Friday, November 6, 2015
    8 years ago
  • Date Issued
    Tuesday, March 19, 2019
    5 years ago
Abstract
Thermal barrier layers and seed layers for control of thermal and structural properties of heat assisted magnetic recording (HAMR) media are provided. One such HAMR medium includes a substrate, a heat sink layer on the substrate, a thermal barrier layer of SrTiO3 on the heat sink layer, an underlayer of MgO on the thermal barrier layer, and a magnetic recording layer on the underlayer. Another such HAMR medium includes a substrate, a heat sink layer on the substrate, a thermal barrier layer of an ABO3-type oxide on the heat sink layer, and a magnetic recording layer on the thermal barrier layer.
Description
BACKGROUND

Energy/Heat Assisted Magnetic Recording (EAMR/HAMR) systems can potentially increase the areal density of information recorded magnetically on various media. For example, to achieve magnetic information storage levels beyond 1 terabit per inch squared, smaller grain size media may be required. Such designs can demand higher Ku materials for a magnetic recording layer to sustain thermal stability, such as L10 ordered FePt alloys. The underlayer beneath the FePt magnetic recording layer is critical to the media design as it promotes ordering of the FePt magnetic recording layer, thereby affecting the texture and thermal properties of the media stack. Obtaining a high quality underlayer with good texture and a narrow rocking curve is important to achieve an FePt magnetic recording layer with acceptable recording performance.


HAMR media generally includes a heat sink positioned beneath the magnetic recording layer to dissipate heat and/or light energy from the magnetic recording layer. In addition, the introduction of a thermal barrier layer between the magnetic recording layer and the heat sink in HAMR media design has been demonstrated to improve the life-time of the recording head through laser power reduction. The inclusion of a thermal barrier layer may also have a positive impact on the signal-to-noise-ratio (SNR) of the system. However, most of the material candidates for thermal barriers are either amorphous or do not have the proper crystal structure to grow a high quality underlayer.


To address this problem, a seed layer for underlayer growth may be included in the HAMR media design. However, the addition of the seed layer not only complicates the structure of the HAMR media, but also reduces the effectiveness of the thermal barrier layer. Accordingly, an improved HAMR media structure that addresses these shortcomings is needed.





BRIEF DESCRIPTION OF THE DRAWINGS


FIG. 1 is a top schematic view of a disk drive configured for heat assisted magnetic recording (HAMR) and including a magnetic medium with a thermal barrier layer in accordance with one embodiment of the invention.



FIG. 2 is a side cross sectional schematic view of selected components of the HAMR system of FIG. 1 including the magnetic medium with the thermal barrier layer in accordance with one embodiment of the invention.



FIG. 3 is side cross sectional view of a HAMR medium having a thermal barrier layer and an underlayer in accordance with one embodiment of the invention.



FIG. 4 illustrates exemplary rocking curve full width half maximum (RC-FWHM) for MgO at various deposition temperatures of SrTiO3 (STO) compared against an amorphous underlayer (AUL) in accordance with one embodiment of the invention.



FIG. 5 illustrates an exemplary X-ray diffraction (XRD) pattern of MgO deposited over SrTiO3 (STO) at a temperature of 650° C. in accordance with one embodiment of the invention.



FIG. 6 is a flowchart of a process for manufacturing a HAMR medium including an underlayer and a thermal barrier layer in accordance with one embodiment of the invention.



FIG. 7 is a plan view of a static magnet that can be used to manufacture a HAMR medium in accordance with one embodiment of the invention.



FIG. 8 is a schematic side view of an exemplary deposition chamber including the static magnet of FIG. 7 in accordance with one embodiment of the invention.



FIG. 9 is a side cross sectional view of a HAMR medium having an underlayer serving as a thermal barrier layer in accordance with one embodiment of the invention.



FIG. 10 is side cross sectional transmission electron microscope (TEM) view of a HAMR medium including an underlayer serving as a thermal barrier layer between the magnetic recording layer and the heat sink layer in accordance with one embodiment of the invention.



FIG. 11 is a flowchart of a process for manufacturing a HAMR medium including an underlayer serving as a thermal barrier layer in accordance with one embodiment of the invention.





DETAILED DESCRIPTION

Referring now to the drawings, embodiments of heat assisted magnetic recording (HAMR) media that include a magnetic recording layer, a thermal barrier layer and a heat sink are illustrated. One such HAMR media design utilizes an underlayer of MgO in between a thermal barrier layer of SrTiO3 and the magnetic recording layer. The SrTiO3 is used both as a seed to promote growth of high quality MgO and as a thermal barrier beneath the MgO. In an exemplary embodiment, the SrTiO3 thermal barrier layer enables the MgO underlayer to be produced with good texture and a narrow rocking curve, thereby promoting L10 ordering of an FePt magnetic recording layer. In an aspect, the thermal barrier layer, heat sink layer and underlayer each have a cubic structure with (200) texture. In one embodiment, the thermal barrier layer and underlayer are deposited at a temperature greater than 450 degrees Celsius using respective radio frequency (RF) magnetron sputtering processes. In some embodiments, the thermal barrier layer is further deposited using a static magnet.


Another HAMR media design utilizes an ABO3-type oxide in between the magnetic recording layer and the heat sink. The ABO3-type oxide serves as both a thermal barrier layer and as an underlayer to promote L10 ordering of an FePt magnetic recording layer. In an aspect, the thermal barrier layer and heat sink layer each have a cubic structure with (200) texture. In one embodiment, the ABO3-type oxide may be BaTiO3, SrHfO3, SrZrO3, PbTiO3, BaZrO3, or combinations thereof.


The terms “above,” “over,” “on,” “below,” “under,” and “between” as used herein refer to a relative position of one layer with respect to other layers. As such, one layer deposited or disposed above, over, on, below, or under another layer may be directly in contact with the other layer or may have one or more intervening layers. Moreover, one layer deposited or disposed between layers may be directly in contact with the layers or may have one or more intervening layers.


It shall be appreciated by those skilled in the art in view of the present disclosure that although various exemplary fabrication methods are discussed herein with reference to magnetic recording disks, the methods, with or without some modifications, may be used for fabricating other types of recording disks, for example, optical recording disks such as a compact disc (CD) and a digital-versatile-disk (DVD), or magneto-optical recording disks, or ferroelectric data storage devices.



FIG. 1 is a top schematic view of a disk drive 100 configured for heat assisted magnetic recording (HAMR) and including a magnetic medium 102 with a thermal barrier layer (not shown in FIG. 1, but see FIG. 3) in accordance with one embodiment of the invention. The laser (not visible in FIG. 1, but see FIG. 2) is positioned with a head/slider 108. Disk drive 100 may include one or more disks/media 102 to store data. Disk/media 102 resides on a spindle assembly 104 that is mounted to drive housing 106. Data may be stored along tracks in the magnetic recording layer of disk 102. The reading and writing of data is accomplished with the head 108 that may have both read and write elements. The write element is used to alter the properties of the magnetic recording layer of disk 102 and thereby write information thereto. In one embodiment, head 104 may have magneto-resistive (MR), or giant magneto-resistive (GMR) elements. In another embodiment, head 104 may be another type of head, for example, an inductive read/write head or a Hall effect head.


In operation, a spindle motor (not shown) rotates the spindle assembly 104, and thereby rotates disk 102 to position head 108 at a particular location along a desired disk track. The position of head 104 relative to disk 102 may be controlled by position control circuitry 110.



FIG. 2 is a side cross sectional schematic view of selected components of the HAMR system of FIG. 1 including the magnetic medium 102 with the thermal barrier layer (not shown in FIG. 2, but see FIG. 3) in accordance with one embodiment of the invention. The HAMR system components also include a sub-mount 112 attached to a top surface of the slider 108. A laser 114 is attached to the sub-mount 112, and possibly to the slider 108. The slider 108 includes the write element and the read element positioned along an air bearing surface (ABS) of the slider for writing information to, and reading information from, respectively, the media 102.


In operation, the laser 114 is configured to direct light energy to a waveguide in the slider 108 which directs the light to a near field transducer (NFT) near the air bearing surface (e.g., bottom surface) of the slider. Upon receiving the light from the laser via the waveguide, the NFT generates localized heat energy that heats a portion of the media 102 near the write element and the read element. FIGS. 1 and 2 illustrate a specific embodiment of a HAMR system. In other embodiments, the improved media with the thermal barrier layer can be used in other suitable HAMR systems.



FIG. 3 is side cross sectional view of a HAMR medium 200 having an underlayer 212 of MgO and a thermal barrier layer 210 of SrTiO3 (STO) or similar crystalline oxide material in accordance with one embodiment of the invention. The medium 200 has a stacked structure with a glass substrate 202 at a bottom/base layer, an adhesion layer 204 on the glass substrate 202, a seed layer 206 on the adhesion layer 204, a heat sink layer 208 on the seed layer 206, the thermal barrier layer 210 on the heat sink layer 208, the underlayer 212 on the thermal barrier layer 210, a magnetic recording layer 214 on the underlayer 212, and a carbon overcoat layer 216 on the magnetic recording layer 214. In some embodiments, the adhesion layer 204, seed layer 206, and carbon overcoat layer 216 can be omitted from the medium structure.


In one embodiment, the substrate 202 can be made of one or more materials such as an Al alloy, NiP plated Al, glass, glass ceramic, and/or combinations thereof. In one embodiment, the adhesion layer 204 can includes one or more materials such as CrTi, CrTa, NiTa, CoCrTaZr, CoFeZrBCr, CoTaZr, CoFeTaZr, CoCrWTaZr, CoCrMoTaZr, CoZrWMo, combinations thereof, and/or other suitable materials known in the art.


In one embodiment, the seed layer 206 can be made of one or more materials such as RuAl, CrTa, NiTa, combinations thereof, and/or other suitable materials known in the art. In one embodiment, the heat sink layer 208 can be made of one or more materials such as Ag, Al, Au, Cu, Cr, Mo, Ru, W, CuZr, MoCu, AgPd, CrRu, CrV, CrW, CrMo, CrNd, combinations thereof, and/or other suitable materials known in the art.


In one embodiment, the magnetic recording layer 214 can be made of one or more materials such as FePt and/or other suitable materials known in the art. In addition, the magnetic recording layer 214 may further include one or more segregants, such as carbon. In an exemplary embodiment, the magnetic recording layer 214 includes L1o phase FePt.


In several embodiments, the thermal conductivity (κ) of the thermal barrier layer 210 is less than the thermal conductivity of the underlayer 212. In one embodiment, the bulk thermal conductivity of SrTiO3 is about 11.2 Watts per meter Kelvin (W/mK), whereas the bulk thermal conductivity of MgO is between 45 W/mK and 60 W/mK. In thin film form, the thermal conductivity of SrTiO3 may be about 1.5 W/mK, whereas the thermal conductivity of MgO may be about 10 W/mK.


In several embodiments, the thermal barrier layer 210 is configured to (e.g., the materials for the first thermal barrier layer are selected to) facilitate a heat transfer from the magnetic recording layer 214 to the heat sink layer 208, and impede a heat transfer from the heat sink layer 208 to the magnetic recording layer 214. In a number of embodiments, the thermal barrier layer 210 is deposited at high temperature using a radio frequency (RF) magnetron sputtering process. In one embodiment, the thermal barrier layer 210 is deposited at a temperature greater than 450 degrees Celsius (° C.). In some embodiments, the thermal barrier layer 210 is deposited using a static magnet.


In further embodiments, the underlayer 212 is also deposited at high temperature using an RF magnetron sputtering process. In one embodiment, the underlayer 212 is deposited at a temperature greater than 450° C. For example, the thermal barrier layer 210 may be deposited at a temperature greater than 450° C., and the underlayer 212 may then be deposited on the thermal barrier layer 210 without cooling of the thermal barrier layer 210.


In several embodiments, the thermal barrier layer 210 of SrTiO3 is used as a seed to promote growth of a high quality MgO underlayer 212. In an exemplary embodiment, the SrTiO3 thermal barrier layer 210 enables the MgO underlayer 212 to be produced with good texture and a narrow rocking curve, thereby promoting good L10 ordering and low RC-FWHM of an FePt magnetic recording layer 214. In one embodiment, the MgO underlayer 212 grown on the SrTiO3 thermal barrier layer 210 has a cubic structure (cubic crystal structure) with (200) texture. In an exemplary embodiment, an SrTiO3 thermal barrier layer 210 having a cubic structure with (200) texture is deposited on the heat sink layer 208 as a seed to grow the MgO underlayer 212 with (200) texture.


In further embodiments, the heat sink layer 208 also has a cubic structure with (200) texture and the lattice mismatching between the heat sink layer 208 and the thermal barrier layer 210 is less than eight (8) percent. In an exemplary embodiment, the heat sink layer 208 includes W, Mo, Cr or a Cr-based alloy to achieve the desired lattice mismatching. For example, the heat sink layer 208 may include CrW or CrMo. In addition, in embodiments in which the heat sink layer 208 includes W, Cr and their alloys, a (200) textured heat sink layer 208 may be grown using a seed layer 206 including a textured layer of RuAl over an amorphous layer of CrTa. In embodiments in which the heat sink layer 208 includes Cr and its alloys, a (200) textured heat sink layer 208 may be grown using a seed layer 206 including an amorphous layer of NiTa.


In several embodiments, the thickness of the thermal barrier layer 210 is between about 3 nm and about 10 nm and the thickness of the underlayer 219 is between about 2 nm and about 11 nm. In an exemplary embodiment, the thickness of the thermal barrier layer 210 is about 7 nm and the thickness of the underlayer 212 is about 3 nm.



FIG. 4 illustrates exemplary rocking curve full width half maximum (RC-FWHM) for MgO at various deposition temperatures of SrTiO3 (STO) compared against an amorphous underlayer (AUL) in accordance with one embodiment of the invention. As can be seen in FIG. 4, as the deposition temperature of SrTiO3 increases from 450° C. to 650° C., the RC-FWHM of MgO desirably decreases from 6.2268 to 4.6271, indicating a higher quality of film. This can be compared with an MgO RC-FWHM of 5.68 when deposited over an AUL. The RC-FWHM of MgO when deposited over SrTiO3 at a deposition temperature of 450° C. is comparable to the RC-FWIHM of MgO when deposited over an AUL. In addition, the RC-FWHM of MgO when deposited over SrTiO3 at a deposition temperature greater than 450° C. (e.g., at 550° C. and 650° C.) is improved with respect to MgO deposited over AUL, indicating that MgO deposited over SrTiO3 at deposition temperatures greater than 450° C. has a higher quality than MgO deposited over AUL.



FIG. 5 illustrates an exemplary X-ray diffraction (XRD) pattern of MgO deposited over SrTiO3 (STO) at a temperature of 650° C. in accordance with one embodiment of the invention. An XRD scan involves measuring the intensity over a range of angles of the detector (20). As can be seen in FIG. 5, a pronounced peak of MgO (200) appears in the XRD pattern, indicating a high quality MgO layer when deposited over SrTiO3 at high temperature. In addition, the SrTiO3 (200) peak can also be observed from FIG. 5.



FIG. 6 is a flowchart of a process 300 for manufacturing a HAMR medium including a thermal barrier layer and underlayer in accordance with one embodiment of the invention. In particular embodiments, the process 300 can be used to manufacture the HAMR magnetic media of FIG. 3, FIG. 2, or FIG. 1. The process first provides a substrate in block 302. The process then provides a heat sink layer on the substrate in block 304. The process then provides a thermal barrier layer of SrTiO3 on the heat sink layer in block 306. The process then provides an underlayer of MgO on the thermal barrier layer in block 308. The process then provides a magnetic recording layer on the underlayer in block 310.


In a number of embodiments, the process can manufacture the layers of the HAMR medium with any of the numerous variations described above for the embodiments of FIGS. 1, 2, and 3. For example, in one such case, the process can also provide an adhesion layer between the substrate and the heat sink layer, a seed layer between the adhesion layer and the heat sink layer, and a carbon overcoat layer on the magnetic recording layer. In several embodiments, the layers can include the materials as are described above.


In some embodiments, the process provides the thermal barrier layer on the heat sink layer by depositing the thermal barrier layer at high temperature using an RF magnetron sputtering process. In one such case, the temperature can be greater than 450° C.


In some embodiments, the process provides the underlayer on the thermal barrier layer by depositing the underlayer at high temperature using an RF magnetron sputtering process. In one such case, the temperature can be greater than 450° C. For example, the thermal barrier layer may be deposited at a temperature greater than 450° C. and the underlayer may be deposited on the thermal barrier layer without cooling the thermal barrier layer.


In some embodiments, the process provides the thermal barrier layer using a static magnet during an RF magnetron sputtering process. In one such case, the in plane magnetic field on the top surface of the target is greater than 300 Gauss.


In one embodiment, the process can perform the sequence of actions in a different order. In another embodiment, the process can skip one or more of the actions. In other embodiments, one or more of the actions are performed simultaneously. In some embodiments, additional actions can be performed.



FIG. 7 is a plan view of a static magnet 400 that can be used to manufacture a HAMR medium in accordance with one embodiment of the invention. The static magnet 400 has an unbalanced design including a plurality of cylindrical magnets 402 concentrically arranged around a center circular magnet 404. The height of the cylindrical magnets 402 gradually increases around one half of the center magnet 404 and gradually decrease around the other half of the center magnet 404. For example, the cylindrical magnets 402 along one half 406 of the center magnet 404 have greater heights than those of the cylindrical magnets 402 along the other half 408 of the center magnet 404.



FIG. 8 is a schematic side view of an exemplary deposition chamber 500 including the static magnet 400 of FIG. 7 in accordance with one embodiment of the invention. The deposition chamber 500 further includes a cooling plate 502, a bonding plate 504 and a target 506. The target 506 (e.g., sputter target) contains the thermal barrier layer material to be deposited onto a HAMR medium 508 (e.g., substrate) and forms a cathode in the deposition chamber 500, while the HAMR medium 508 forms the anode. In an exemplary embodiment, the in-plane magnetic field on the top surface of the target 506 is greater than 300 Gauss during deposition of the thermal barrier layer.


For a conventional magnetron sputter deposition, rotating a magnet below the target 506 (cathode) during the sputtering process may improve the utilization of the sputter target and uniformity of material deposited from the sputter target (e.g., target 506). However, for ceramic materials, such as SrTiO3, using the static magnet 400 positioned in the manner shown in FIG. 8 may improve the stability of the plasma in the deposition chamber 500 and improve both the film quality and repeatability of the process.



FIG. 9 is a side cross sectional view of a HAMR medium having an underlayer of an ABO3-type oxide serving as a thermal barrier layer in accordance with one embodiment of the invention. The medium 600 has a stacked structure with a glass substrate 602 at a bottom/base layer, an adhesion layer 604 on the glass substrate 602, a seed layer 606 on the adhesion layer 604, a heat sink layer 608 on the seed layer 606, the thermal barrier layer 610 on the heat sink layer 608, a magnetic recording layer 612 on the thermal barrier layer 610, and a carbon overcoat layer 614 on the magnetic recording layer 612. In some embodiments, the adhesion layer 604, seed layer 606, and carbon overcoat layer 614 can be omitted from the medium structure.


In several embodiments, the thermal conductivity (κ) of the thermal barrier layer 610 is less than the thermal conductivity of, for example, the MgO underlayer shown in FIG. 3. In one embodiment, in thin film form, the thermal conductivity of the thermal barrier layer 610 is less than 10 W/mK. In another embodiment, the thermal conductivity of the thermal barrier layer 610 is less than 3 W/mK. In an exemplary embodiment, the thermal barrier layer 610 is configured to (e.g., the materials for the first thermal barrier layer are selected to) facilitate a heat transfer from the magnetic recording layer 612 to the heat sink layer 608, and impede a heat transfer from the heat sink layer 608 to the magnetic recording layer 612.


In addition, the thermal barrier layer 610 further functions as a seed layer for the magnetic recording layer 612 to promote growth of a high quality magnetic recording layer 612. In an exemplary embodiment, the thermal barrier layer 610 promoting good L10 ordering and low RC-FWHM of an FePt magnetic recording layer 612. In one embodiment, the ABO3-type oxide of the thermal barrier layer 610 has a lattice parameter (a) between about 3.8 angstroms and 4.4 angstroms. Such ABO3-type oxides exhibit low thermal conductivity as compared to MgO. In an exemplary embodiment, the ABO3-type oxide can be made of one or more materials such as BaTiO3, SrTiO3, SrHfO3, SrZrO3, PbTiO3 and BaZrO3, combinations thereof, and/or other suitable materials known in the art. The lattice mismatching between such ABO3-type oxides and L10 phase FePt is similar to MgO, which promotes good L10 ordering and low RC-FWHM of the FePt magnetic recording layer.


In one embodiment, the substrate 602 can be made of one or more materials such as an Al alloy, NiP plated Al, glass, glass ceramic, and/or combinations thereof. In one embodiment, the adhesion layer 604 can includes one or more materials such as CrTi, CrTa, NiTa, CoCrTaZr, CoFeZrBCr, CoTaZr, CoFeTaZr, CoCrWTaZr, CoCrMoTaZr, CoZrWMo, combinations thereof, and/or other suitable materials known in the art.


In one embodiment, the seed layer 606 can be made of one or more materials such as RuAl, CrTa, NiTa, combinations thereof, and/or other suitable materials known in the art. In one embodiment, the heat sink layer 608 can be made of one or more materials such as Ag, Al, Au, Cu, Cr, Mo, Ru, W, CuZr, MoCu, AgPd, CrRu, CrV, CrW, CrMo, CrNd, combinations thereof, and/or other suitable materials known in the art.


In one embodiment, the magnetic recording layer 612 can be made of one or more materials such as FePt and/or other suitable materials known in the art. In addition, the magnetic recording layer 612 may further include one or more segregants, such as carbon. In an exemplary embodiment, the magnetic recording layer 612 includes L10 phase FePt.


In several embodiments, the thermal barrier layer 610 has a cubic structure (cubic crystal structure) with (200) texture. In further embodiments, the heat sink layer 608 also has a cubic structure with (200) texture and the lattice mismatching between the heat sink layer 608 and the thermal barrier layer 610 is between about three (3) percent and about eight (8) percent. In an exemplary embodiment, the heat sink layer 608 includes W, Mo, Cr or a Cr-based alloy to achieve the desired lattice mismatching. For example, the heat sink layer 608 may include CrW or CrMo. In addition, in embodiments in which the heat sink layer 608 includes W, Cr and their alloys, a (200) textured heat sink layer 608 may be grown using a seed layer 606 including a textured layer of RuAl over an amorphous layer of CrTa. In embodiments in which the heat sink layer 608 includes Cr and its alloys, a (200) textured heat sink layer 608 may be grown using a seed layer 606 including an amorphous layer of NiTa.


In several embodiments, the thickness of the thermal barrier layer 610 is between about 2 nm and about 11 nm. In an exemplary embodiment, the thickness of the thermal barrier layer 610 is about 3 nm.



FIG. 10 is side cross sectional transmission electron microscope (TEM) view of a HAMR medium including an underlayer serving as a thermal barrier layer (SrTiO3) between the magnetic recording layer (FePt—C) and the heat sink layer (Cr) in accordance with one embodiment of the invention. As illustrated, the grains of the magnetic recording layer (FePt—C) are segregated and are similar to FePt—C grown on an MgO underlayer. The carbon overcoat layer is designated as COC.



FIG. 11 is a flowchart of a process 700 for manufacturing a HAMR medium including an underlayer serving as a thermal barrier layer in accordance with one embodiment of the invention. In particular embodiments, the process 700 can be used to manufacture the HAMR magnetic media of FIG. 9, FIG. 2, or FIG. 1. The process first provides a substrate in block 702. The process then provides a heat sink layer on the substrate in block 704. The process then provides an underlayer serving as a thermal barrier layer of an ABO3-type oxide on the heat sink layer in block 706. The process then provides a magnetic recording layer on the underlayer in block 708.


In a number of embodiments, the process can manufacture the layers of the HAMR medium with any of the numerous variations described above for the embodiments of FIGS. 1, 2, and 9. For example, in one such case, the process can also provide an adhesion layer between the substrate and the heat sink layer, a seed layer between the adhesion layer and the heat sink layer, and a carbon overcoat layer on the magnetic recording layer. In several embodiments, the layers can include the materials as are described above.


In some embodiments, the process provides the thermal barrier layer on the heat sink layer by depositing the thermal barrier layer at high temperature using an RF magnetron sputtering process. In one such case, the temperature can be greater than 450° C.


In some embodiments, the process provides the thermal barrier layer using a static magnet during an RF magnetron sputtering process. In one such case, the in plane magnetic field on the top surface of the target is greater than 300 Gauss.


In one embodiment, the process can perform the sequence of actions in a different order. In another embodiment, the process can skip one or more of the actions. In other embodiments, one or more of the actions are performed simultaneously. In some embodiments, additional actions can be performed.


While the above description contains many specific embodiments of the invention, these should not be construed as limitations on the scope of the invention, but rather as examples of specific embodiments thereof. Accordingly, the scope of the invention should be determined not by the embodiments illustrated, but by the appended claims and their equivalents.

Claims
  • 1. A medium for heat assisted magnetic recording, the medium comprising: a substrate;a heat sink layer on the substrate;a thermal barrier layer directly on the heat sink layer, the thermal barrier layer comprising SrTiO3;an underlayer on the thermal barrier layer, the underlayer comprising MgO; anda magnetic recording layer on the underlayer,wherein the heat sink layer is configured to dissipate heat from the magnetic recording layer.
  • 2. The medium of claim 1, wherein the thermal barrier layer has a cubic structure with (200) texture.
  • 3. The medium of claim 2, wherein the heat sink layer has a cubic structure with (200) texture.
  • 4. The medium of claim 3, wherein a lattice mismatch between the heat sink layer and the thermal barrier layer is less than 8 percent.
  • 5. The medium of claim 4, wherein the heat sink layer comprises a Cr-based alloy.
  • 6. The medium of claim 5, wherein the heat sink layer comprises CrW and the magnetic recording layer comprises FePt with a segregant.
  • 7. The medium of claim 2, wherein the underlayer has a cubic structure with (200) texture.
  • 8. The medium of claim 1, wherein a first thickness of the thermal barrier layer is between about 3 nm and about 10 nm and a second thickness of the underlayer is between about 2 nm and about 11 nm.
  • 9. The medium of claim 1, wherein a first thickness of the thermal barrier layer is about 7 nm and a second thickness of the underlayer is about 3 nm.
  • 10. The medium of claim 1, wherein the thermal barrier layer is configured to: facilitate a heat transfer from the magnetic recording layer to the heat sink layer; andimpede a heat transfer from the heat sink layer to the magnetic recording layer.
  • 11. The medium of claim 1, wherein the thermal barrier layer is deposited at a temperature greater than 450 degrees Celsius using a first radio frequency (RF) magnetron sputtering process and the underlayer is deposited at a temperature greater than 450 degrees Celsius using a second RF magnetron sputtering process.
  • 12. The medium of claim 11, wherein the thermal barrier layer is deposited using a static magnet.
  • 13. A heat assisted magnetic recording system comprising: the medium of claim 1;a near-field transducer light source configured to direct light energy on to the medium; anda magnetic transducer configured to write information to the medium.
  • 14. A method for fabricating a medium for heat assisted magnetic recording, the method comprising: providing a substrate;providing a heat sink layer on the substrate;providing a thermal barrier layer directly on the heat sink layer, the thermal barrier layer comprising SrTiO3;providing an underlayer on the thermal barrier layer, the underlayer comprising MgO; andproviding a magnetic recording layer on the underlayer,wherein the heat sink layer is configured to dissipate heat from the magnetic recording layer.
  • 15. The method of claim 14, wherein providing the thermal barrier layer on the heat sink layer comprises: depositing the thermal barrier layer on the heat sink layer at a temperature greater than 450 degrees Celsius using a first RF magnetron sputtering process.
  • 16. The method of claim 15, wherein providing the underlayer on the thermal barrier layer comprises: depositing the underlayer at a temperature greater than 450 degrees Celsius using a second RF magnetron sputtering process.
  • 17. The method of claim 16, wherein providing the underlayer on the thermal barrier layer further comprises: depositing the thermal barrier layer using a static magnet.
  • 18. The method of claim 14, wherein the thermal barrier layer, the underlayer and the heat sink layer each has a cubic structure with (200) texture.
  • 19. The method of claim 14, wherein a lattice mismatch between the heat sink layer and the thermal barrier layer is less than 8 percent.
  • 20. The method of claim 19, wherein the heat sink layer comprises a Cr-based alloy.
  • 21. The method of claim 14, wherein a first thickness of the thermal barrier layer is between 3 nm and 10 nm and a second thickness of the underlayer is between 2 nm and 11 nm.
  • 22. A medium for heat assisted magnetic recording, the medium comprising: a substrate;a heat sink layer on the substrate;a thermal barrier layer directly on the heat sink layer, the thermal barrier layer comprising an ABO3-type oxide; anda magnetic recording layer on the thermal barrier layer,wherein the heat sink layer is configured to dissipate heat from the magnetic recording layer.
  • 23. The medium of claim 22, wherein the thermal barrier layer has a cubic structure with (200) texture.
  • 24. The medium of claim 23, wherein the heat sink layer has a cubic structure with (200) texture.
  • 25. The medium of claim 22, wherein the magnetic recording layer comprises FePt with a segregant.
  • 26. The medium of claim 22, wherein a lattice mismatch between the thermal barrier layer and the magnetic recording layer is between about 3 percent and about 8 percent.
  • 27. The medium of claim 22, wherein the ABO3-type oxide is selected from the group consisting of BaTiO3, SrHfO3, SrZrO3, PbTiO3 and BaZrO3.
  • 28. The medium of claim 22, wherein a thermal conductivity of the thermal barrier layer is less than 10 Watts per meter Kelvin.
  • 29. The medium of claim 22, wherein the thermal barrier layer is configured to: facilitate a heat transfer from the magnetic recording layer to the heat sink layer; andimpede a heat transfer from the heat sink layer to the magnetic recording layer.
  • 30. A heat assisted magnetic recording system comprising: the medium of claim 22;a near-field transducer light source configured to direct light energy on to the medium; anda magnetic transducer configured to write information to the medium.
  • 31. A method for fabricating a medium for heat assisted magnetic recording, the method comprising: providing a substrate;providing a heat sink layer on the substrate;providing a thermal barrier layer directly on the heat sink layer, the thermal barrier layer comprising an ABO3-type oxide; andproviding a magnetic recording layer on the thermal barrier layer,wherein the heat sink layer is configured to dissipate heat from the magnetic recording layer.
  • 32. The method of claim 31, wherein the thermal barrier layer and the heat sink layer each has a cubic structure with (200) texture.
  • 33. The method of claim 31, wherein the ABO3-type oxide is selected from the group consisting of BaTiO3, SrHfO3, SrZrO3, PbTiO3 and BaZrO3.
  • 34. The method of claim 31, wherein a thermal conductivity of the thermal barrier layer is less than 10 Watts per meter Kelvin.
US Referenced Citations (336)
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 Gomicki 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
7226668 Nagaraj et al. Jun 2007 B2
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
7357994 Hazel et al. Apr 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
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
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
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
8603653 Matsumoto 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
8696404 Sun 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
8792211 Yuan et al. 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
20040022387 Weikle Feb 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
20070231589 Smeggil et al. Oct 2007 A1
20070245909 Homola Oct 2007 A1
20080075845 Sonobe et al. Mar 2008 A1
20080093760 Harper et al. Apr 2008 A1
20090117408 Umezawa 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
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
20120147718 Hellwig 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
20120214021 Sayama 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 et al. 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
20140043947 Hohlfeld Feb 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
20140376350 Cheng et al. Dec 2014 A1
20150004437 Moriya Jan 2015 A1
20160358622 Arora Dec 2016 A1