Cluster evolution in molecular three-dimensional spin-crossover systems

2017 ◽  
Vol 96 (6) ◽  
Author(s):  
Laurentiu Stoleriu ◽  
Masamichi Nishino ◽  
Seiji Miyashita ◽  
Alexandru Stancu ◽  
Andreas Hauser ◽  
...  
2007 ◽  
Vol 46 (10) ◽  
pp. 4220-4229 ◽  
Author(s):  
Matthias Bartel ◽  
Alina Absmeier ◽  
Guy N. L. Jameson ◽  
Franz Werner ◽  
Kenichi Kato ◽  
...  

2012 ◽  
Vol 12 (3) ◽  
pp. 1482-1488 ◽  
Author(s):  
Wen-Ting Liu ◽  
Jin-Yan Li ◽  
Zhao-Ping Ni ◽  
Xin Bao ◽  
Yong-Cong Ou ◽  
...  

2010 ◽  
Vol 91 (2) ◽  
pp. 27003 ◽  
Author(s):  
C. Enachescu ◽  
M. Nishino ◽  
S. Miyashita ◽  
A. Hauser ◽  
A. Stancu ◽  
...  

2017 ◽  
Vol 46 (18) ◽  
pp. 5786-5789 ◽  
Author(s):  
Suguru Murata ◽  
Kazuyuki Takahashi ◽  
Tomoyuki Mochida ◽  
Takahiro Sakurai ◽  
Hitoshi Ohta ◽  
...  

The first neutral spin-crossover FeIII complex with a N3O3 coordination sphere formed a purely π-stacking interaction network and exhibited the cooperative transition.


2018 ◽  
Vol 779 ◽  
pp. 110-114
Author(s):  
Feng Shao ◽  
Jia Jia Zhuang ◽  
Gang Luo ◽  
Ke Zhang ◽  
Chang Jiang Li ◽  
...  

A new three-dimensional metal-organic complex, [{Fe (NCSe)2}3(TPB)4]x(guest), was prepared with the ligand of TPB (1,3,5-tris (4-pyridyl) benzene). The X-ray single crystal diffraction studied in 100 K and 173 K shown the change of bonds and angles of the framework. The guest exchange and magnetic properties indicated that the 3D framework can be responsible to the solvent guest molecules and shows guest-dependent spin-crossover behaviour.


2020 ◽  
Vol 7 (8) ◽  
pp. 1685-1690 ◽  
Author(s):  
Yuan-Yuan Peng ◽  
Si-Guo Wu ◽  
Yan-Cong Chen ◽  
Wei Liu ◽  
Guo-Zhang Huang ◽  
...  

An unprecedented hysteretic seven-/eight-step spin-crossover behavior is revealed. Most importantly, a molecular alloy based on a Hofmann-type framework is used as a strategy to explore multi-step spin-crossover materials for the first time.


2020 ◽  
Vol 494 (3) ◽  
pp. 4539-4547 ◽  
Author(s):  
Congyao Zhang ◽  
Eugene Churazov ◽  
Klaus Dolag ◽  
William R Forman ◽  
Irina Zhuravleva

ABSTRACT Several types/classes of shocks naturally arise during formation and evolution of galaxy clusters. One such class is represented by accretion shocks, associated with deceleration of infalling baryons. Such shocks, characterized by a very high Mach number, are present even in 1D models of cluster evolution. Another class is composed of ‘runaway merger shocks’, which appear when a merger shock, driven by a sufficiently massive infalling subcluster, propagates away from the main-cluster centre. We argue that, when the merger shock overtakes the accretion shock, a new long-living shock is formed that propagates to large distances from the main cluster (well beyond its virial radius), affecting the cold gas around the cluster. We refer to these structures as Merger-accelerated Accretion shocks (MA-shocks) in this paper. We show examples of such MA-shocks in one-dimensioanal (1D) and three-dimensional (3D) simulations and discuss their characteristic properties. In particular, (1) MA-shocks shape the boundary separating the hot intracluster medium (ICM) from the unshocked gas, giving this boundary a ‘flower-like’ morphology. In 3D, MA-shocks occupy space between the dense accreting filaments. (2) Evolution of MA-shocks highly depends on the Mach number of the runaway merger shock and the mass accretion rate parameter of the cluster. (3) MA-shocks may lead to the misalignment of the ICM boundary and the splashback radius.


2005 ◽  
Vol 17 (24) ◽  
pp. 2949-2953 ◽  
Author(s):  
A. Galet ◽  
A. B. Gaspar ◽  
M. C. Muñoz ◽  
G. V. Bukin ◽  
G. Levchenko ◽  
...  

2012 ◽  
Vol 86 (5) ◽  
Author(s):  
Cristian Enachescu ◽  
Masamichi Nishino ◽  
Seiji Miyashita ◽  
Laurentiu Stoleriu ◽  
Alexandru Stancu

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