Abstract:In this research, drawing vacuum arc (VA) experiments were conducted using composite contacts under currents ranging from 5 kA to 20 kA root mean square (rms). The new type of contact comprised an axial magnetic field (AMF) configuration and a transverse magnetic field (TMF) configuration. The TMF plate was in the center, surrounded by the AMF plate. The contact generated both AMFs and TMFs simultaneously. VA appearances and arc voltages were recorded, and the VA was modeled as a conductor for electromagnetic … Show more
“…Conventionally, the arc motion is studied using high-speed optical photography. The arc motion and behaviour have been observed and analysed for different variants of the RMF contact such as contrate cup type contacts [7,8], spiral petal contacts [9,10], SWASTIK shaped contacts [11] and also hybrid RMF-axial magnetic flux contact designs [12]. Finite-element method (FEM) is extensively used in analysis and design of VIs [13,14] including the computation of the Lorentz force on the arc [5,6,11].…”
The SWASTIK type radial magnetic field (RMF) contact design is widely used in vacuum interrupters. The mutually perpendicular petal limbs are a unique feature of this contact design. The focus of this work is to relate the Lorentz force acting on the arc with petal dimensions through closed-form expressions. Considering the petal limbs as equivalent to finite current carrying conductors, analytical equations are derived to compute the magnetic flux density at any point in space. The results are verified by using finite-element method (FEM) simulations of rail electrodes. The expressions are then used to compute the Lorentz force on the arc in SWASTIK contacts. The analytical predictions are compared with three-dimensional FEM simulations of a CAD model of the contacts. Applicability of the analytical results is investigated in the context of parametric variation of the radius, length and position of the arc and temporal variation of the contact current. The present work can be used in the first iteration of contact petal design. It is also applicable for the design of rail gun geometries.
“…Conventionally, the arc motion is studied using high-speed optical photography. The arc motion and behaviour have been observed and analysed for different variants of the RMF contact such as contrate cup type contacts [7,8], spiral petal contacts [9,10], SWASTIK shaped contacts [11] and also hybrid RMF-axial magnetic flux contact designs [12]. Finite-element method (FEM) is extensively used in analysis and design of VIs [13,14] including the computation of the Lorentz force on the arc [5,6,11].…”
The SWASTIK type radial magnetic field (RMF) contact design is widely used in vacuum interrupters. The mutually perpendicular petal limbs are a unique feature of this contact design. The focus of this work is to relate the Lorentz force acting on the arc with petal dimensions through closed-form expressions. Considering the petal limbs as equivalent to finite current carrying conductors, analytical equations are derived to compute the magnetic flux density at any point in space. The results are verified by using finite-element method (FEM) simulations of rail electrodes. The expressions are then used to compute the Lorentz force on the arc in SWASTIK contacts. The analytical predictions are compared with three-dimensional FEM simulations of a CAD model of the contacts. Applicability of the analytical results is investigated in the context of parametric variation of the radius, length and position of the arc and temporal variation of the contact current. The present work can be used in the first iteration of contact petal design. It is also applicable for the design of rail gun geometries.
“…On the other hand we may ask why there is dominance of the cosmological constant over the matter component at the present epoch. These two basic problems prompt us to propose some alternatives, which include an evolving scalar field called quintessence [2][3][4][5][6][7][8], a noncanonical scalar field (such as K-essence [9][10][11], phantom [7,8,[12][13][14][15][16][17][18]), modified gravity [7,8,[19][20][21][22][23], coupled dark energy [8,24,25] or decaying dark energy [26] models, and so on. On the other hand, the equation of state (EoS) parameter of the cosmological constant is precisely ω de = −1.…”
Astrophysical observations have put unprecedentedly tight constraints on cosmological theories. The CDM model, mathematically simple and fits observational data sets well, is preferred for explaining the behavior of universe. But many basic features of the dark sectors are still unknown, which leaves room for various nonstandard cosmological hypotheses. As the pressure of the cosmological constant dark energy is unvarying, ignoring contributions from radiation and curvature terms at low redshift, the effective pressure keeps constant. In this paper, we propose two parametric models for a non-constant effective pressure in order to study the tiny deviation from CDM at low redshift. We recover our phenomenological models in the scenarios of quintessence and phantom fields, and we explore the behavior of the scalar field and potential. We constrain our model parameters with SNe Ia and BAO observations, and we detect subtle hints of ω de < −1 from the data-fitting results of both models, which indicates possibly a phantom dark energy scenario at present.
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