This application is related to the following: U.S. Pat. No. 10,490,216; Ser. No. 16/370,613, filed on Mar. 29, 2019; Ser. No. 16/370,634, filed on Mar. 29, 2019; and, Ser. No. 16/563,147, filed on Sep. 6, 2019; assigned to a common assignee, and herein incorporated by reference in their entirety.
The present disclosure relates to a Spin Hall Effect assisted magnetic recording (SHAMR) structure wherein a Spin Hall Effect (SHE) layer comprised of a giant positive or negative Spin Hall Angle (SHA) material is formed in the write gap between a main pole (MP) and trailing shield (TS), and wherein a direct current (ISHE) is applied from one or both of the MP and TS to the SHE layer, and then flows through the SHE layer to a lead and back to the source so that transverse spin transfer torque is applied to one or both of a local MP magnetization at the MP/SHE interface and to a local TS magnetization at the SHE/TS interface depending on SHE layer placement thereby enhancing the MP write field and TS return field, respectively, improving overwrite (OW), bit error rate (BER), and device reliability, and providing a more easily implemented process compared with SHAMR designs where ISHE is applied across the SHE layer and synchronized with a write current (Iw).
As the data areal density in hard disk drive (HDD) writing increases, write heads and media bits are both required to be made in smaller sizes. However, as the write head size shrinks, its writability degrades. To improve writability, new technology is being developed that assists writing to a media bit. Two main approaches currently being investigated are thermally assisted magnetic recording (TAMR) and microwave assisted magnetic recording (MAMR) where a spin torque device is employed to generate a high frequency field that helps writing. The latter is described by J-G. Zhu et al. in “Microwave Assisted Magnetic Recording”, IEEE Trans. Magn., vol. 44, pp. 125-131 (2008). A third approach called STRAMR (spin torque reversal assisted magnetic recording) relies on spin torque to reverse a magnetization in a layer in the write gap (WG), for example, to increase reluctance and force more magnetic flux from the MP at the ABS. STRAMR is described in U.S. Pat. No. 6,785,092. Related U.S. Pat. No. 10,490,216 describes a writer where the MAMR and STRAMR (spin flipping element) effects may exist simultaneously.
Spin transfer torque devices (also known as STO devices) are based on a spin-transfer effect that arises from the spin dependent electron transport properties of ferromagnetic-spacer-ferromagnetic multilayers. When current passes through a magnetic multilayer in a CPP (current perpendicular to plane) configuration, the first ferromagnetic layer (FM1) will generate spin polarized currents as the electrons traverse FM1. When the spin polarized current is transmitted through a polarization preservation spacer, the spin angular moment of electrons incident on a second FM layer (FM2) interacts with magnetic moments of FM2 near the interface between the non-magnetic spacer and FM2. Through this interaction, the electrons transfer a portion of their angular momentum to FM2. As a result, spin-polarized current can switch the magnetization direction of FM2 if the current density is sufficiently high.
Spin Hall Effect (SHE) is a physics phenomenon discovered in the mid 20th century, and is described by M. Dyaknov et al. in Physics Lett. A, Vol. 35, 459 (1971). Similar to a regular Hall Effect where conduction carriers with opposite charges are scattered to opposite directions perpendicular to the current density due to a certain scattering mechanism, SHE causes electrons with opposite spins to be scattered to opposite directions perpendicular to the charge current density as a result of strong spin-orbit coupling in the conducting layer. As shown in
During the past 10 years, materials with substantially larger (giant) SHA have been found. B. Gu et al. in Phys. Rev. Lett. 105, 216401 (2010), and L. Liu et al. in Phys. Rev. Lett. 106, 036601 (2011) provided examples of SHA˜0.07 in a Pt layer, and as large as 0.12 in a Au layer with Pt doping, and an application where giant transverse spin current is injected into an adjacent magnetic layer to induce reversal and ferromagnetic resonance by spin torque. A large but negative SHA of around −0.12 was found in β-Ta, meaning that electrons in the β-Ta layer are spin scattered in the opposite directions compared to what is shown in
All existing designs that provide an assist to magnetic recording have advantages, but also have disadvantages including a greater number of pads per head for all assisted designs, reliability concern for TAMR, and a limited WG thickness to fit a multilayer device in both MAMR and TAMR. Furthermore, we have found that SHAMR schemes where ISHE is confined within the SHE layer can cause heating that leads to SHE layer protrusion up to 1-2 nm out of the ABS. Also, synchronization of ISHE with Iw is difficult because of the required frequency in the GHz regime. Therefore, a new SHAMR scheme is desired where there is no current density threshold to initiate the assist mechanism, where ISHE is not confined within the SHE layer, and where the stack of layer(s) used to provide the assist is formed with fewer process steps than in existing designs where a spin torque oscillator (STO) in MAMR or STRAMR usually has three or more layers.
One objective of the present disclosure is to provide a SHE assisted magnetic recording scheme that provides better overwrite (OW), bit error rate (BER), and transition sharpness compared with existing magnetic recording assist designs.
A second objective of the present disclosure is to provide the SHAMR scheme of the first objective that also enables better device reliability and requires fewer fabrication steps than for STO devices comprised of three or more layers.
A third objective of the present disclosure is to provide a SHAMR scheme that satisfies the first two objectives and also does not have a current threshold to begin the assist, and is compatible with advanced designs where write gap thickness is reduced to 10 nm or less.
A fourth objective of the present disclosure is to provide a SHAMR scheme that satisfies the first three objectives, and does not require synchronization of a write current with a current through the SHE layer, and where SHE layer protrusion is avoided during a write process.
According to a first embodiment of the present disclosure, these objectives are achieved by forming a SHE layer in a write gap, and with a bottom surface that interfaces with a portion of the MP trailing side from the ABS to a first height (h), and having a top surface that contacts a portion of the trailing shield (TS) from the ABS to a second height (h1) where h and h1 are between 10 nm and 70 nm. The SHE layer may be made of a positive giant SHA material such as Pt or a negative giant SHA material such as β-Ta, and has a front side at the ABS in preferred embodiments, or recessed from the ABS in other embodiments. Preferably, the SHE layer is comprised of a so-called giant SHA material having an absolute value for SHA that is >0.05. In all embodiments, the SHE layer has a width greater than or equal to the track width of the MP trailing side at the ABS.
When a SHE layer made of a positive giant SHA material is in the write gap, and contacts a front portion of each of the MP trailing side and TS bottom surface, a first current (I1) is applied from the MP trailing side to the SHE layer, and a second current (I2) is applied from the TS bottom surface to the SHE layer. I1 and I2 flow through the SHE layer to a backend thereof and then through a lead back to the source of the direct current. The direction of I1 and I2 is independent of the direction of the MP write field. However, the direction of I1 and I2 is reversed when the SHE layer is comprised of a negative giant SHA material. The MP trailing side at a height>h and the TS bottom surface at a height>h1 are separated from the SHE layer by a portion of the write gap to prevent shorting.
Without a current in the SHE layer, the MP has a local magnetization at the MP/SHE interface that is aligned substantially in the direction of the write gap field (HWG) that is either toward or away from the TS depending on the transition being written. Similarly, the TS has a local magnetization at the SHE/TS interface that is substantially parallel to HWG. When I1 and I2 are applied as described previously, the SHE layer spin polarizes I1 proximate to the MP trailing side and thereby exerts a transverse spin transfer torque toward the MP/SHE layer interface that causes the MP local magnetization to tilt down and more towards the ABS, or up and more away from the ABS depending on the transition. Similarly, the SHE layer spin polarizes I2 proximate to the TS bottom surface and generates a transverse spin transfer torque proximate to the TS/SHE layer interface that tilts the local TS magnetization up and away from the ABS, or down and toward the ABS depending on the transition. The result is a higher effective write field for better overwrite, and a higher TS return field that typically correlates to better BER. Although an Oersted field is also generated in the SHE layer at the interfaces with the MP and TS, the Oersted field is oriented orthogonal to the transverse spin transfer torque and has no effect on the magnetic recording assist provided by the SHE layer spin polarization.
In other embodiments, the write gap is formed between the SHE layer top surface and the entire TS bottom surface so that the SHE layer contacts the MP, and provides a transverse spin transfer torque only to the local MP magnetization when I1 is applied from the MP to a SHE layer made of a positive giant SHA material. Alternatively, the write gap is formed between the SHE layer bottom surface and the entire MP trailing side so that the SHE layer contacts the TS, and provides a transverse spin transfer torque only to the local TS magnetization when I2 is applied from the TS to a SHE layer made of a positive giant SHA material.
In yet another embodiment, the SHE layer may be comprised of at least two sub-layers made of different SHA materials in order to tune the current density in each sub-layer, and the magnitude of the resulting transverse spin transfer torque. Accordingly, there is flexibility in using two different materials to tune the spin transfer torque to the MP trailing side and TS bottom surface individually. Thus, with one or both of a larger I1 and I2, and a larger absolute value for SHA, the amount of transverse spin torque applied to the local MP magnetization and to the local TS magnetization, respectively, is increased.
A process sequence is provided for forming a SHE layer having a top surface contacting the trailing shield and a bottom surface that forms an interface with a MP trailing side.
The present disclosure is a PMR writer based on SHAMR technology hereinafter referred to as a SHAMR device wherein a SHE layer is formed between a MP trailing side and a trailing shield and is configured to apply transverse spin transfer torque to one or both of local MP magnetization and a local TS magnetization during a write process to enhance write field, and TS return field, respectively. A (+) SHE layer is comprised of a giant positive SHA material, and a (−) SHE layer is comprised of a giant negative SHA material. In the drawings, the y-axis is in a cross-track direction, the z-axis is in a down-track direction, and the x-axis is in a direction orthogonal to the ABS and towards a back end of the writer structure. Thickness refers to a down-track distance, width is a cross-track distance, and height is a distance orthogonal to the ABS in the x-axis direction. In some of the drawings, a magnetic bit is considerably enlarged over actual size in order to more easily depict a bit magnetization therein. The terms “magnetic moment” and “magnetization” may be used interchangeably. The term “down” with respect to MP field direction indicates a direction out of the ABS toward the magnetic medium, and the term “up” refers to a direction opposite to “down”, which is into the MP from the magnetic medium. A front side of a layer is at the ABS or faces the ABS while a backside of a layer faces away from the ABS.
Referring to
HGA 100 is mounted on an arm 230 formed in the head arm assembly 103. The arm moves the magnetic recording head 1 in the cross-track direction y of the magnetic recording medium 140. One end of the arm is mounted on base plate 224. A coil 231 that is a portion of a voice coil motor is mounted on the other end of the arm. A bearing part 233 is provided in the intermediate portion of arm 230. The arm is rotatably supported using a shaft 234 mounted to the bearing part 233. The arm 230 and the voice coil motor that drives the arm configure an actuator.
Next, a side view of a head stack assembly (
With reference to
Referring to
A magnetoresistive (MR) element also known as MR sensor 86 is formed on bottom shield 84 at the ABS 30-30 and typically includes a plurality of layers (not shown) including a tunnel barrier formed between a pinned layer and a free layer where the free layer has a magnetization (not shown) that rotates in the presence of an applied magnetic field to a position that is parallel or antiparallel to the pinned layer magnetization. Insulation layer 85 adjoins the backside of the MR sensor, and insulation layer 83 contacts the backsides of the bottom shield and top shield 87. The top shield is formed on the MR sensor. An insulation layer 88 and a top shield (S2B) layer 89 are sequentially formed on the top magnetic shield. Note that the S2B layer 89 may serve as a flux return path (RTP) in the write head portion of the combined read/write head. Thus, the portion of the combined read/write head structure formed below layer 89 in
The present disclosure anticipates that various configurations of a write head (SHAMR writer) may be employed with the read head portion. In the exemplary embodiment, magnetic flux 70 in main pole (MP) layer 14 is generated with flowing a current called Iw (not shown) through bucking coil 80b and driving coil 80d that are below and above the MP layer, respectively, and are connected by interconnect 51. Magnetic flux 70 exits the MP layer at pole tip 14p at the ABS 30-30 and is used to write a plurality of bits on magnetic media 140. Magnetic flux 70b returns to the main pole through a trailing loop comprised of trailing shield 17, write shield 18, PP3 shield 26, and top yoke 18x. There is also a leading return loop for magnetic flux 70a that includes leading shield 11, leading shield connector (LSC) 33, S2 connector (S2C) 32, return path 89, and back gap connection (BGC) 62. Alternatively, in a non-dual write shield (nDWS) design (not shown), the LSC, S2C, return path and BGC are omitted such that the leading return loop terminates at the leading shield. The magnetic core may also comprise a bottom yoke 35 below the MP layer. Dielectric layers 10, 13, 36-39, and 47-49 are employed as insulation layers around magnetic and electrical components. A protection layer 27 covers the PP3 trailing shield and is made of an insulating material such as alumina. Above the protection layer and recessed a certain distance u from the ABS 30-30 is an optional cover layer 29 that is preferably comprised of a low coefficient of thermal expansion (CTE) material such as SiC. Overcoat layer 28 is formed as the uppermost layer in the write head.
Referring to
As shown in
The MP leading side 14b1 is generally tapered and connects with the MP bottom surface 14b2. In other embodiments (not shown), one or both of the MP leading side and trailing side 14t1 are orthogonal to the ABS. Write gap field HWG is shown across the SHE layer in a direction from the MP 14 to TS 17. A local MP field 14m proximate to MP trailing side 14t1, and a local TS field 17m proximate to the TS bottom surface are pointing substantially in the same direction as HWG.
The benefits of the SHE layer according to the present disclosure are realized when a first current I1 of sufficient current density flows from direct current (dc) source 50 through lead 57a and MP 14 and into SHE layer 19 before returning through lead 58 to the dc source. Moreover, a second current I2 of sufficient current density flows from the dc source through lead 57b and TS 17, and into the SHE layer before returning through lead 58 to the dc source. In the exemplary embodiment, a backside 19e of the SHE layer is at a greater height from the ABS 30-30 than a throat height h2 of TS backside 17e. In other embodiments (not shown), the SHE layer backside may be less than h2 from the ABS.
In
Meanwhile, as a result of I2, the direction of spin polarized electrons 19p2 proximate to TS bottom surface 17b is into the plane of the paper, and is responsible for generating transverse spin transfer torque 19t2 that is substantially orthogonal to TS bottom surface 17b and pointing toward TS 17. The transverse spin transfer torque 19t2 causes local TS magnetization 17m to tilt and become TS magnetization 17m1 that is oriented more away from the ABS (and more parallel to return field 70b shown in
The mechanism for each SHE assist is similar to that described in
Preferably, SHE thickness d depicted in
Referring to
The local moment of the MP 14 (and TS 17) that receives the spin torque interactions follows the Landau-Lifshitz-Gilbert (LLG) equation (shown below) plus the spin torque with spin polarized by the SHE layer 19.
In the equation above, {circumflex over (m)} is the unit vector of the local magnetic moment, {circumflex over (σ)} is the unit vector of the injected spin polarization, y is the gyromagnetic ratio, α is the damping parameter, and t is the effective depth by which the spin transfer torque occurs in the MP and TS, typically several atomic layers. After the first equality sign “=”, the first term is the precession along the total magnetic field vector Beff, and the second is the damping term. The last term is the spin torque term which can be merged to the first term so that
functions like me additional effective field to tilt local MP magnetization 14m to 14m1 and to tilt local TS magnetization 17m to 17m1, which work together with the magnetic fields 70, 70b, respectively. Js is the spin current density, and Ms is the magnetization density of the MP and TS where the spin current is injected. A MP layer (not shown) adjoining MP trailing side 14t1 and a TS layer (not shown) adjoining the TS bottom surface 17b each have a magnetization that is rotated by the additional effective field. The rotation is then propagated to the effective depth mentioned above through magnetic exchange interactions.
Unlike a current threshold requirement for assist effects to occur with SOT-MRAM or STT-MRAM, there is no current threshold for I1 and I2 to begin an assist in the SHAMR embodiments of the present disclosure. This advantage is related to the fact that injected spin current from MP 14 and TS 17 to the SHE layer (or in the reverse direction in other embodiments) always carries spin direction parallel to the MP/SHE and SHE/TS interfaces and is substantially orthogonal to the local MP magnetization 14m and local TS magnetization 17m, respectively. The magnitude of the transverse spin transfer torque increases as I1 and I2 are increased. A maximum SHE assist occurs when local MP magnetization 14m1 is parallel to MP trailing side 14t1, and when local TS magnetization 17m1 is parallel to TS bottom surface 17b. There is no risk of an over-push situation where local MP and local TS magnetizations are tilted beyond a position that is parallel to the MP trailing side and to the TS bottom surface, respectively.
Referring to
As shown in
Referring to
Referring to
In all embodiments, WG layers 16a, 16b may be a single layer or multilayer including but not limited to AlOx, SiOx, MgO, AINx, TiOx, and other insulating oxides, oxynitrides, or nitrides used in the art.
Referring to
Referring to
The present disclosure also encompasses an embodiment illustrated in
According to another embodiment illustrated in
In all embodiments, the constant direct current in the SHE layer 19 or 19n is around 1-6 mA zero-to-peak amplitude (AMP). Ideally, the write current (Iw) waveform used to generate write field 70 is a step transition at each of transition T0-T4 between write periods P1-P4 (
However, when there is a SHAMR assist with a positive giant SHA material depicted in
In actual practice, there is an overshoot in Iw immediately after a transition to ensure a fast rise time in a conventional PMR writer. Using a SHAMR assist according to an embodiment of the present disclosure, an overshoot in current through the SHE layers would increase transverse spin transfer torque as well. Faster rise time with a SHAMR assist will improve the writer's transition speed and provide better transition sharpness as an additional advantage to enhancing the MP write field, and boosting the TS return field in certain embodiments.
A simulation was performed to demonstrate the benefits of the present disclosure according to the embodiment shown in
Referring to
The present disclosure also encompasses a process sequence for fabricating a SHE layer in a write gap according to an embodiment described herein and is provided in the ABS views of
Referring to
In
In all SHAMR device embodiments described herein, kilo flux change per inch (kFCI) and area density capability (ADC) are expected to improve with one or both of MP write field enhancement (better overwrite property), and enhanced TS return field (better BER).
While the present disclosure has been particularly shown and described with reference to, the preferred embodiments thereof, it will be understood by those skilled in the art that various changes in form and details may be made without departing from the spirit and scope of this disclosure.
Number | Name | Date | Kind |
---|---|---|---|
6785092 | Covington et al. | Aug 2004 | B2 |
6809899 | Chen et al. | Oct 2004 | B1 |
6954340 | Shukh et al. | Oct 2005 | B2 |
7009812 | Hsu et al. | Mar 2006 | B2 |
7589600 | Dimitrov et al. | Sep 2009 | B2 |
7724469 | Gao et al. | May 2010 | B2 |
7835111 | Flint et al. | Nov 2010 | B2 |
7957098 | Yamada et al. | Jun 2011 | B2 |
7963024 | Neuhaus | Jun 2011 | B2 |
7978442 | Zhang et al. | Jul 2011 | B2 |
7982996 | Smith et al. | Jul 2011 | B2 |
8027110 | Yamanaka et al. | Sep 2011 | B1 |
8064244 | Zhang et al. | Nov 2011 | B2 |
8068312 | Jiang et al. | Nov 2011 | B2 |
8154825 | Takashita et al. | Apr 2012 | B2 |
8203389 | Zhou et al. | Jun 2012 | B1 |
8264792 | Bai et al. | Sep 2012 | B2 |
8270112 | Funayama et al. | Sep 2012 | B2 |
8295008 | Sasaki et al. | Oct 2012 | B1 |
8310787 | Sasaki et al. | Nov 2012 | B1 |
8320079 | Iwasaki et al. | Nov 2012 | B2 |
8427781 | Sasaki et al. | Apr 2013 | B1 |
8446690 | Alex et al. | May 2013 | B2 |
8462461 | Braganca et al. | Jun 2013 | B2 |
8477452 | Sasaki et al. | Jul 2013 | B2 |
8493687 | Sasaki et al. | Jul 2013 | B2 |
8582240 | Chen et al. | Nov 2013 | B1 |
8582241 | Yu et al. | Nov 2013 | B1 |
8604886 | Nikonov et al. | Dec 2013 | B2 |
8634163 | Tanabe et al. | Jan 2014 | B2 |
8749919 | Sasaki et al. | Jun 2014 | B2 |
8767347 | Sasaki et al. | Jul 2014 | B1 |
8792210 | de la Fuente et al. | Jul 2014 | B2 |
9142228 | Fujita et al. | Sep 2015 | B2 |
9230571 | Chen et al. | Jan 2016 | B1 |
9299367 | Tang et al. | Mar 2016 | B1 |
9361912 | Liu et al. | Jun 2016 | B1 |
9406317 | Tang et al. | Aug 2016 | B1 |
9466319 | Tang et al. | Oct 2016 | B1 |
9824701 | Tang et al. | Nov 2017 | B2 |
9934797 | Takahashi et al. | Apr 2018 | B2 |
9966091 | Chen et al. | May 2018 | B2 |
10032469 | Lim et al. | Jul 2018 | B2 |
10037772 | Okamura et al. | Jul 2018 | B2 |
10079057 | Ozbay et al. | Sep 2018 | B2 |
10141037 | Ohsawa et al. | Nov 2018 | B2 |
10181334 | Song et al. | Jan 2019 | B1 |
10210888 | Li et al. | Feb 2019 | B1 |
10559318 | Chen | Feb 2020 | B1 |
10580441 | Chen | Mar 2020 | B1 |
20020034043 | Okada et al. | Mar 2002 | A1 |
20040150910 | Okada et al. | Aug 2004 | A1 |
20050128637 | Johnston et al. | Jun 2005 | A1 |
20050141137 | Okada | Jun 2005 | A1 |
20060044682 | Le et al. | Mar 2006 | A1 |
20060087765 | Iwakura et al. | Apr 2006 | A1 |
20060103978 | Takano et al. | May 2006 | A1 |
20070177301 | Han et al. | Aug 2007 | A1 |
20080013209 | Sasaki et al. | Jan 2008 | A1 |
20080088972 | Sasaki et al. | Apr 2008 | A1 |
20090059426 | Sasaki et al. | Mar 2009 | A1 |
20090080106 | Shimizu et al. | Mar 2009 | A1 |
20090128953 | Jiang et al. | May 2009 | A1 |
20090296275 | Sasaki et al. | Dec 2009 | A1 |
20100165517 | Araki et al. | Jul 2010 | A1 |
20110211271 | Ng et al. | Sep 2011 | A1 |
20120292723 | Luo et al. | Nov 2012 | A1 |
20140071562 | Chen et al. | Mar 2014 | A1 |
20140177092 | Katada et al. | Jun 2014 | A1 |
20150043106 | Yamada et al. | Feb 2015 | A1 |
20150287426 | Mihajlovic | Oct 2015 | A1 |
20160218728 | Zhu | Jul 2016 | A1 |
20170133044 | Lim et al. | May 2017 | A1 |
20180075868 | Koui et al. | Mar 2018 | A1 |
Number | Date | Country |
---|---|---|
2002-133610 | May 2002 | JP |
2002-298309 | Oct 2002 | JP |
2008-021398 | Jan 2008 | JP |
2010-157303 | Jul 2010 | JP |
Entry |
---|
PTO Office Action, U.S. Appl. No. 12/964,202, Applicant: Sasaki et al., Notification date: Nov. 28, 2012, 11 pages. |
“The Feasibility of Magnetic Recording at 10 Terabits Per Square Inch on Conventional Media,” by Roger Wood et al., IEEE Transactions on Magnetics, vol. 45, No. 2, Feb. 2009, pp. 917-923. |
Microwave Assisted Magnetic Recording, by Jian-Gang Zhu et al., IEEE Transactions on Magnetics, vol. 44, No. 1, Jan. 1, 2008, pp. 125-131. |
Nov. 13, 2012, Office Action issued in Japanese Patent Application No. 2011-149242, with English language translation. ,. |
Nov. 13, 2012, Office Action issued in Japanese Patent Application No. 2011-149243, with English language translation. |
Nov. 13, 2012, Office Action issued in Japanese Patent Application No. 2011-149244, with English language translation. |
“Spin-Torque Oscillator Based on Magnetic Tunnel Junction with a Perpendicularly Magnetized Free Layer and In-Plane Magnetized Polarizer,” by Hitoshi Kubota, et al., 2013 The Japan Society of Applied Physics, Applied Physics Express 6 (2013) 103003, Sep. 27, 2013, pp. 1-3. |
“High-Power Coherent Microwave Emission from Magnetic Tunnel Junction Nano-oscillators with Perpendicular Anisotropy,” by Zhongming Zeng, et al, 2012 American Chemical Society, Jun. 4, 2012, vol. 6, No. 7, pp. 6115-6121. |
“Spin-Torque Switching with the Giant Spin Hall Effect of Tantalum,” by Luqiao Liu et al., Science May 4, 2012: vol. 336, Issue 6081, pp. 555-558, DOI: 10.1126/science.1218197. |
D'Yakonov, M. I., Spin Hall Effect. Int. J. Mod. Phys. B 23, 2556-2565 (2009). |
“Spin-Torque Ferromagnetic Resonance Induced by the Spin Hall Effect,” by Luqiao Liu et al, Physical Review Letters, PRL 106, 036601 (2011), Jan. 21, 2011, pp. 1-4. |
“Surface-Assisted Spin Hall Effect in Au Films with Pt Impurities,” by B. Gu et al., Physical Review Letters, PRL 105, 216401 (2010), Nov. 19, 2010, pp. 1-4. |