Analysis of neutral active particle loss in afterglow in krypton at 2.6mbar pressure

2008 ◽  
Vol 15 (1) ◽  
pp. 013502 ◽  
Author(s):  
Momcilo M. Pejovic ◽  
Jugoslav P. Karamarkovic ◽  
Goran S. Ristic ◽  
Milic M. Pejovic
1966 ◽  
Vol 241 (17) ◽  
pp. 4101-4109
Author(s):  
Leo P. Vernon ◽  
Elwood R. Shaw ◽  
Bacon Ke
Keyword(s):  

2019 ◽  
Vol 100 (5) ◽  
Author(s):  
Prachi Bisht ◽  
Mustansir Barma

2020 ◽  
Vol 125 (26) ◽  
Author(s):  
Alvaro Domínguez ◽  
M. N. Popescu ◽  
C. M. Rohwer ◽  
S. Dietrich
Keyword(s):  

Soft Matter ◽  
2017 ◽  
Vol 13 (41) ◽  
pp. 7609-7616 ◽  
Author(s):  
Saroj Kumar Nandi ◽  
Nir S. Gov

The physics of active systems of self-propelled particles, in the regime of a dense liquid state, is an open puzzle of great current interest, both for statistical physics and because such systems appear in many biological contexts. We obtain a nonequilibrium mode-coupling theory for such systems and present analytical scaling relations through mapping with a simpler model of a single trapped active particle.


Author(s):  
Pulak Kumar Ghosh ◽  
Fabio Marchesoni ◽  
Yunyun Li ◽  
Franco Nori

Undesired advection effects are unavoidable in most nano-technological applications involving active matter. However, it is conceivable to govern the transport of active particles at the small scales by suitably tuning...


2018 ◽  
Vol 30 (26) ◽  
pp. 264002 ◽  
Author(s):  
F Cecconi ◽  
A Puglisi ◽  
A Sarracino ◽  
A Vulpiani

Soft Matter ◽  
2022 ◽  
Author(s):  
Shannon E. Moran ◽  
Isaac R. Bruss ◽  
Philip Shoenhofer ◽  
Sharon C Glotzer

Studies of active particle systems have demonstrated that particle anisotropy can impact the collective behavior of a system. However, systems studied to date have served as one-off demonstrations of concept,...


2020 ◽  
Vol 86 (2) ◽  
Author(s):  
Christopher G. Albert ◽  
Sergei V. Kasilov ◽  
Winfried Kernbichler

Accelerated statistical computation of collisionless fusion alpha particle losses in stellarator configurations is presented based on direct guiding-centre orbit tracing. The approach relies on the combination of recently developed symplectic integrators in canonicalized magnetic flux coordinates and early classification into regular and chaotic orbit types. Only chaotic orbits have to be traced up to the end, as their behaviour is unpredictable. An implementation of this technique is provided in the code SIMPLE (symplectic integration methods for particle loss estimation, Albert et al., 2020b, doi:10.5281/zenodo.3666820). Reliable results were obtained for an ensemble of 1000 orbits in a quasi-isodynamic, a quasi-helical and a quasi-axisymmetric configuration. Overall, a computational speed up of approximately one order of magnitude is achieved compared to direct integration via adaptive Runge–Kutta methods. This reduces run times to the range of typical magnetic equilibrium computations and makes direct alpha particle loss computation adequate for use within a stellarator optimization loop.


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