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Thus, Equation (38) together with (30) and (33) to (37) constitutes a Bianchi type II string cosmological model with bulk viscosity in isotropic form in Nordtvedt's general scalar-tensor theory of gravitation.
Lohmann and Diehl (2006) employed a parametrization based on Levkov et al. (1992) to calculate the contact-freezing probability only through Brownian diffusion of aerosol particles in their global aerosol transport model with bulk cloud microphysics.
Thus, Equation (45) together with (30) and (40) to (44) constitutes a Bianchi type VIII string cosmological model with bulk viscosity in isotropic form in Nordtvedt's general scalar-tensor theory of gravitation.
Masterlark (2003) suggests that a model with bulk permeability of the oceanic crust less than 10−17 maymay explain the quasi-static coupling of an earthquake swarm that has a 63-day lag time following the 1980 M w 8.0 Jalisco-Colima earthquake.
The corrected sensograms were analysed using a steady state affinity one-to-one model with bulk refractive index contribution factor (Biacore, GE HealthCare).
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Here, we obtain the string cosmological models with bulk viscosity in Nordtvedt's general scalar-tensor theory with the help of a special case proposed by Schwinger in the form 3 + 2 ω φ = 1 λφ, λ = constant.
In this paper, we have presented Bianchi types II, VIII, and IX string cosmological models with bulk viscosity in Nordtvedt's [1] general scalar-tensor theory with the help of a special case proposed by Schwinger [2].
Recently, Rao and Sireesha [37, 38] have obtained Bianchi types II, VIII, and IX string cosmological models with bulk viscosity in Lyra [15] and Brans and Dicke [4] theory of gravitation, respectively.
We have obtained and presented spatially homogeneous Bianchi types II, VIII, and IX string cosmological models with bulk viscosity in Nordtvedt's (Astrophys. J. 161 1059, 1970) general scalar-tensor theory of gravitation with the help of a special case proposed by Schwinger.
In this paper, we will discuss Bianchi types II, VIII, and IX string cosmological models with bulk viscosity in Nordtvedt's [1] general scalar-tensor theory with the help of a special case proposed by Schwinger [2], i.e., 3 + 2 ω ϕ = 1 λϕ Open image in new window, where λ is a constant.
This paper explores the feasibility of designing a rotatable magnetic levitation (maglev) plate model with HTS bulks placed beneath a permanent magnet (PM) plate.
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