통합 검색 | Korea Science

Kim, Changsoo;Moon, Kyoung-Woong;Chun, Byong Sun;Kim, Dongseok;Hwang, Chanyong
- 한국자기공명학회논문지
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- 제23권2호
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- pp.46-50
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- 2019
Spin orbit torque would be applied as the next generation of MRAM, so many researchers are interested in related field. To make a more efficient device, electric current should convert into spin current with high efficiency. Moreover, it becomes important to measure efficiency of spin orbit torque accurately. We measured spin torque FMR of W/CoFeB hetero structure system with direct current. The efficiencies of the damping like torque and field like torque were measured by using the linewidth and on-resonance field proportional to direct current. In addition, we analyzed that a quadratic shift of the on-response field was caused by the Joule heating.
https://doi.org/10.6564/JKMRS.2019.23.2.046 인용 PDF KSCI HTML

윤상준;문준;황현석;최석봉
- 한국자기학회지
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- 제25권1호
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- pp.1-3
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- 2015
본 연구에서는 스핀-궤도 돌림힘의 광학적 측정 방법을 개발하였다. 사인파 전류에 의해 발생하는 스핀-궤도 돌림힘은 해당 주파수와 두 배 주파수로 진동하는 자화의 운동을 유발하는데, 이로 인해 변화하는 자화의 수직 성분을 극광자기 효과를 이용해 측정하였다. 스핀-궤도 돌림힘이 추가된 란다우-리프쉬츠-길버트 방정식의 평형 조건으로부터, 스핀-궤도 돌림힘에 의한 유효 자기장을 정량적으로 분석하였다. 이러한 측정법을 Pd/Co/Pt 박막 시료에 적용하여, 스핀-궤도 돌림힘 효율의 종 방향과 횡 방향의 성분 값을 각각 나누어 측정하는데 성공하였다. 본 연구에서 제시한 측정 및 분석 방법은 기존의 전기적 측정에 비해 오류가 적기 때문에, 스핀-궤도 돌림힘을 측정하는 더 개선된 방법으로 사용할 수 있다.
https://doi.org/10.4283/JKMS.2015.25.1.001 인용 PDF KSCI

Moon, Jun-Sung;An, Sung-Ho;Yoon, Suk-Jin
- 천문학회보
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- 제46권1호
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- pp.28.3-29
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- 2021
Galaxies are not just randomly distributed in space; instead, a variety of galaxy alignments have been found over a wide range of scales. Such alignments are the outcome of the combined effect of interacting neighbors and the surrounding large-scale structure. Here, we focus on the spin-orbit alignment (SOA) of galaxy pairs, the dynamical coherence between the spin of a target galaxy and the orbital angular momentum of its neighbor. Based on a recent cosmological hydrodynamic simulation, the IllustrisTNG project, we identify paired galaxies with mass ratios from 1/10 to 10 at z = 0 and statistically analyze their spin-orbit angle distribution. We find a clear preference for prograde orientations (i.e., SOA), which is more prominent for closer pairs. The SOA is stronger for less massive targets in lower-density regions. The SOA witnessed at z = 0 has been developed progressively since z = 2. There is a clear positive correlation between the alignment strength and the interaction duration with its current neighbor. Our results suggest the scenario in which the SOA is developed mainly by interactions with a neighbor for an extended period of time, rather than by the primordial torque exerted by the large-scale structure.
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