Theory of the kinetics of nucleation in adsorbing layer: the approach based on the relaxation of order parameter field

1996 ◽  
Vol 345 (1-2) ◽  
pp. 138-154 ◽  
Author(s):  
Yu.N. Devyatko ◽  
S.V. Rogozhkin ◽  
B.A. Fedotov
Keyword(s):  
Order Parameter ◽  
Parameter Field ◽  
Kinetics Of

The kinetics of phase transition in systems with nonconservative order parameter

1982 ◽  
Vol 32 (7) ◽  
pp. 772-776 ◽  
Author(s):  
O. I. Gerasimov ◽  
I. Z. Fischer ◽  
V. Lisý
Keyword(s):  
Phase Transition ◽  
Order Parameter ◽  
Kinetics Of

Magnetic Properties and Spin Kinetics of Two-Dimensional Heisenberg Antiferromagnets

2003 ◽  
Vol 17 (10n12) ◽  
pp. 487-490
Author(s):  
S. I. Belov ◽  
B. I. Kochelaev
Keyword(s):  
Order Parameter ◽  
Spin Fluctuations ◽  
Local Order ◽  
Nuclear Relaxation ◽  
Two Dimensional ◽  
Nuclear Spins ◽  
Static Magnetic Susceptibility ◽  
Spin Excitations ◽  
Local Order Parameter ◽  
Kinetics Of

In this report we present our study of two-dimensional Heisenberg magnets based on the picture of thermally excited skyrmions. The local order parameter, energy spectrum of elementary spin excitations above the skyrmion background, the skyrmion averaged radius and static magnetic susceptibility were obtained by the Green functions method. There was calculated the rate of nuclear relaxation caused by the interaction of nuclear spins with above mentioned spin excitations. The contribution of Moriya–Dsyloshinskii and anisotropic symmetric interactions into EPR line was considered. A comparison with NMR and neutron scattering experiments in cuprates and with the results obtained by other methods is given. We discuss the consequences of an interaction between skyrmions as the result of the spin fluctuations.

THE ORDER PARAMETER FIELD FOR COSMIC STRING, INFLATION AND DARK ENERGY

2003 ◽  
Vol 18 (36) ◽  
pp. 2587-2597 ◽  
Author(s):  
PENG-MING ZHANG ◽  
YI-SHI DUAN ◽  
LI-MING CAO
Keyword(s):  
Dark Energy ◽  
Scalar Field ◽  
Early Universe ◽  
Cosmic String ◽  
Order Parameter ◽  
Cosmic Strings ◽  
Complex Scalar ◽  
Parameter Field ◽  
Complex Scalar Field

We present a whole frame for the cosmic strings, inflation and dark energy with the complex scalar field which can be regarded as the order parameter of our universe. One can find that the comic strings emerge in the zeros of the complex scalar field in the early universe. And with the evolution of complex scalar field, inflation and dark energy can be understood in this frame.

Kinetics of Ordering in Fe3Al: Experiment

1990 ◽  
Vol 186 ◽  
Author(s):  
Brent Fultz ◽  
Zheng-Qiang Gao ◽  
Lawrence Anthony
Keyword(s):  
Long Range ◽  
Order Parameter ◽  
Range Order ◽  
Disordered Materials ◽  
Long Range Order ◽  
X Ray ◽  
Different Temperatures ◽  
Two Stages ◽  
Rates Of Growth ◽  
Kinetics Of

AbstractAlloys near the Fe3Al stoichiometry were prepared far from thermodynamic equilibrium by rapid solidification methods. These highly disordered materials were then annealed at low temperatures to develop B2 and D03 order. Both shortrange and long-range order (SRO and LRO) were measured by Mössbauer spectrometry and by x-ray diffractometry, respectively. The SRO was found to evolve in two stages: an initial quick growth of the SRO alone, followed by a slower growth of SRO along with LRO. As expected, at lower temperatures the absolute rates of growth of order were suppressed, but more interestingly, the relative rates of growth of B2 and D03 long-range order parameters were different at different temperatures of annealing. When the B2 order parameter is graphed against the D03 order parameter, at lower temperatures the “kinetic path” through this graph shows that B2 order evolves relatively more rapidly than D03 order.

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