scholarly journals Fluctuating nonlinear hydrodynamics of flocking

2018 ◽  
Vol 97 (3) ◽  
Author(s):  
Sunil Kumar Yadav ◽  
Shankar P. Das
2021 ◽  
Vol 117 ◽  
pp. 102924
Author(s):  
N. Tran ◽  
N.Y. Sergiienko ◽  
B.S. Cazzolato ◽  
B. Ding ◽  
P.-Y. Wuillaume ◽  
...  

2020 ◽  
Vol 147 ◽  
pp. 1895-1908 ◽  
Author(s):  
Fantai Meng ◽  
Ashkan Rafiee ◽  
Boyin Ding ◽  
Benjamin Cazzolato ◽  
Maziar Arjomandi

2015 ◽  
Vol 767 ◽  
pp. 52-64 ◽  
Author(s):  
Oleg A. Godin

AbstractWe consider strongly nonlinear waves in fluids in a uniform gravity field, and demonstrate that an incompressible wave motion, in which pressure remains constant in each fluid parcel, is supported by compressible fluids with free and rigid boundaries. We present exact analytic solutions of nonlinear hydrodynamics equations which describe the incompressible wave motion. The solutions provide an extension of the Gerstner wave in an incompressible fluid with a free boundary to waves in compressible three-dimensionally inhomogeneous moving fluids such as oceans and planetary atmospheres.


1993 ◽  
Vol 02 (04) ◽  
pp. 855-872 ◽  
Author(s):  
A. LUDU ◽  
W. GREINER ◽  
A. SANDULESCU

Alpha decay is described as a new large amplitude collective motion in nuclei. The total energy is evaluated in the frame of the nonlinear hydrodynamics approach which leads to the formation of solitons on the nuclear surface. A new minimum appears in the total energy due to the shell effects for 208 Pb and 4 He introduced phenomenologically. The minimum was chosen to be degenerate with the ground state minimum. Consequently a new coexistence model consisting of the usual shell model and an alpha particle cluster-like model describing a soliton moving on the nuclear surface is obtained. The corresponding amplitudes describe excellently the experimental preformation factors for alpha decay of Po isotopes.


1986 ◽  
Vol 34 (3) ◽  
pp. 2265-2282 ◽  
Author(s):  
Shankar P. Das ◽  
Gene F. Mazenko

2007 ◽  
Vol 46 (5) ◽  
pp. 1632-1641 ◽  
Author(s):  
H. Y. Lin ◽  
W. Chen ◽  
A. Tsutsumi

1976 ◽  
Vol 70 ◽  
pp. 313-313
Author(s):  
Richard I. Klein

In order to understand the Be star phenomenon, and move in directions away from ad hoc models, detailed calculations have been made that treat nonlinear hydrodynamics self-consistently with non-L.T.E. radiative transfer.


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