The 76th JSAP Autumn Meeting, 2015

Presentation information

Oral presentation

10 Spintronics and Magnetics » 10.3 Giant magnetoresistance (GMR), tunnel magnetoresistance (TMR) and magnetic recording technologies

[14a-2J-1~12] 10.3 Giant magnetoresistance (GMR), tunnel magnetoresistance (TMR) and magnetic recording technologies

Mon. Sep 14, 2015 9:00 AM - 12:15 PM 2J (223)

座長:谷口 知大(産総研)

12:00 PM - 12:15 PM

[14a-2J-12] Investigation of the emission power and Q factor of the MgO-based spin-torque oscillators with different diameters

〇(P)BOCHONG WANG1, Hitoshi Kubota1, Kay Yakushiji1, Shingo Tamaru1, Akio Fukushima1, Shinji Yuasa1 (1.AIST)

Keywords:spin-torque oscillators,MgO-MTJs,emission power Q factor

Spin-torque oscillators (STOs) with a narrow linewidth and large emission power have been proposed as a new type of microwave generators and highly sensitive magnetic field sensors, based on the theoretical predictions and experimental observations of spin transfer torque. MgO-based magnetic tunnel junctions (MgO-MTJs) which exhibit large tunnel magneto-resistance ratio are beneficial for enhancing the emission power [1-3]. In this research, nanopillar STOs with different diameters were fabricated and the emission power and Q factor were studied.
Figure 1 shows the structure of STO film. The CoFeB reference layer is coupled to the CoFe pinned layer to form a synthetic antiferromagnet. The FeB free layer is perpendicularly magnetized due to the large perpendicular interfacial magnetic anisotropy induced by two FeB/MgO interfaces. The film was patterned into cylindrical pillars with a diameter from 200 nm to 400 nm by e-beam lithography. The magnetoresistance (MR) ratio is around 25% and the resistance-area (RA) product is 1.7 Ωμm2. The magnetic field dependence of Q factor and total emission power of the STOs with different diameters are shown in Figure 2, where the bias voltage was -260 mV for all plots. The Q factor and emission power fluctuate with the magnetic field. It is clear that the 300-nm-diameter STO has the largest Q factor and the emission power among these samples. The maximum Q factor is as high as 602 at 310 mT, and the largest emission power is 1.42 μW at 335 mT. The size dependence of Q factor and emission power may come from the change of the perpendicular magnetic anisotropy and the impedance mismatch.