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The χ3 parameter refers to the node degree associated with particle p i.
The three parameters are composed of a three-dimensional particle P = [J, B, K].
We will assume each particle p to have the same interaction list.
χ4 is the probability of choosing a node in particle p i on the basis of its head count.
In our optimization function we provide comparatively more valuation to the residual energy associated with the particle p i.
The Euclidean distance between node n j and particle p i is represented by notation n j, x i.
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These spectra registered at 90o for particle arrays P(S/PGL1), P(S/PGL2), P(S/PGL1)–OVA, and P(S/PGL2)–OVA microspheres are shown in Fig. 5.
What is clear is that fine particles (P M1) mostly originate from combustion processes.
Soil and zeolite particles tend to adsorb these bivalent cations than Na, and a significant difference was recognized between their adsorptions by soil and zeolite particles (p = 0.05).
We obtain the angular and energy distributions of secondary particles (p, e−, e+, photons, muons) at different atmospheric levels as a function of primary proton spectra.
Calculate the probability of existence about the target according to the unnormalized weights of particles P ^ k = M ˜ b + M ˜ c M ˜ b + M ˜ c + P d P ^ k - 1 + 1 - P b 1 - P ^ k - 1 (22).
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