scholarly journals Spinor Dynamics in Pristine and Mn2+-Doped CsPbBr3 NC: Role of Spin–Orbit Coupling in Ground- and Excited-State Dynamics

2018 ◽  
Vol 122 (45) ◽  
pp. 26196-26213 ◽  
Author(s):  
Aaron Forde ◽  
Talgat Inerbaev ◽  
Dmitri Kilin
2018 ◽  
Vol 20 (48) ◽  
pp. 30219-30230 ◽  
Author(s):  
Romain Letrun ◽  
Bernhard Lang ◽  
Oleksandr Yushchenko ◽  
Roland Wilcken ◽  
Denis Svechkarev ◽  
...  

Intramolecular charge separation and enhanced spin orbit coupling explain the weak fluorescence of a T-shaped dyad comprising two strong fluorophores.


2021 ◽  
Vol 7 (1) ◽  
Author(s):  
Woo Seung Ham ◽  
Abdul-Muizz Pradipto ◽  
Kay Yakushiji ◽  
Kwangsu Kim ◽  
Sonny H. Rhim ◽  
...  

AbstractDzyaloshinskii–Moriya interaction (DMI) is considered as one of the most important energies for specific chiral textures such as magnetic skyrmions. The keys of generating DMI are the absence of structural inversion symmetry and exchange energy with spin–orbit coupling. Therefore, a vast majority of research activities about DMI are mainly limited to heavy metal/ferromagnet bilayer systems, only focusing on their interfaces. Here, we report an asymmetric band formation in a superlattices (SL) which arises from inversion symmetry breaking in stacking order of atomic layers, implying the role of bulk-like contribution. Such bulk DMI is more than 300% larger than simple sum of interfacial contribution. Moreover, the asymmetric band is largely affected by strong spin–orbit coupling, showing crucial role of a heavy metal even in the non-interfacial origin of DMI. Our work provides more degrees of freedom to design chiral magnets for spintronics applications.


1972 ◽  
Vol 50 (10) ◽  
pp. 1468-1471 ◽  
Author(s):  
Alan D. Westland

An expression for the magnetic susceptibility of octahedral d1 complexes is derived exactly in terms of an orbital reduction factor k taking into account the presence of the formal 2E excited state. Sample calculations show that the improved expression gives results for susceptibility which are lower at times by several percent from those given by previous expressions. The results given by Figgis using Kotani's method are adequately precise when the spin–orbit coupling constant is no larger than ~0.1 Dq.


2001 ◽  
Vol 37 (4) ◽  
pp. 2411-2413 ◽  
Author(s):  
You Xu ◽  
Jiehui Yang ◽  
Xijuan Zhang ◽  
Fang Zhang ◽  
M. Guillot

2019 ◽  
Vol 18 ◽  
pp. e00360
Author(s):  
H.A. Alluhaybi ◽  
S.K. Ghoshal ◽  
B.O. Alsobhi ◽  
W.N. Wan Shamsuri

2010 ◽  
Vol 108 (3) ◽  
pp. 486-494 ◽  
Author(s):  
E. A. Gastilovich ◽  
V. G. Klimenko ◽  
N. V. Korol’kova ◽  
R. N. Nurmukhametov

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