About: Srx Physics is an academic journal. The journal publishes majorly in the area(s): Rayleigh number & Boundary layer. Over the lifetime, 9 publications have been published receiving 30 citations.
TL;DR: In this article, the steady mixed convection boundary layer flow from a solid sphere in a micropolar fluid, generated by Newtonian heating in which the heat transfer from the surface is proportional to the local surface temperature, is considered.
Abstract: The steady mixed convection boundary layer flow from a solid sphere in a micropolar fluid, generated by Newtonian heating in which the heat transfer from the surface is proportional to the local surface temperature, is considered. The governing boundary layer equations are first transformed into a system of nondimensional equations via the non-dimensional variables, and then into nonsimilar equations before they are solved numerically using an implicit finite-difference scheme known as the Keller-box method. Numerical solutions are obtained for the skin friction coefficient, wall temperature and heat transfer coefficient, as well as the velocity and temperature profiles with several parameters considered, namely the mixed convection parameter, the material or micropolar parameter, and the Prandtl number.
TL;DR: In this paper, the effects of mass loss on the orbital motion of a test particle around it were analyzed for a variation G ˙ / G of the Newtonian constant of gravitation.
Abstract: I work out the Newtonian and general relativistic effects due to an
isotropic mass loss M ˙ / M of a body on the orbital motion of a test particle around it; the present analysis is also valid for a variation G ˙ / G of the Newtonian constant of gravitation. Concerning the Newtonian
case, I use the Gauss equations for the variation of the elements and
obtain negative secular rates for the osculating semimajor axis a , the
eccentricity e , and the mean anomaly ℳ , while the argument of pericenter ω does not experience secular precession; the longitude of the
ascending node Ω and the inclination i remain unchanged as well. The true orbit, instead, expands, as shown by a
numerical integration of the equations of motion with MATHEMATICA; in fact, this is in agreement with the seemingly counter-intuitive decreasing of a and e because they refer to the osculating Keplerian
ellipses which approximate the trajectory at each instant. A comparison with the results obtained with different approaches by other researchers is made. General relativity induces positive secular rates
of the semimajor axis and the eccentricity completely negligible in the
present and future evolution of the solar system.
TL;DR: The infrared spectra of 60 B 2 O 3 -10 TeO 2 -(30-x)ZnO-xPbO glasses reveal that the glass network consists of [ TeO 3 ], [ BO 3 ], and [ BO 4 ] groups as discussed by the authors.
Abstract: The infrared (IR) spectra of (100-x) TeO 2 –x WO 3 glasses reveal that the glass network consists of [ TeO 3 ]/[ TeO 3 + 1 ], [ TeO 4 ], [ WO 4 ], and [ WO 6 ] groups as basic structural units. Addition of WO 3 oxide to the binary TeO 2 –W O 3 glasses increases the amount of lower coordination of [ TeO 3 ]/[ TeO 3 + 1 ] units and decreases the higher coordination of [ TeO 4 ] units and also the formation of Te–O–W linkages at the expense of Te–O–Te linkages. The IR spectra of 60 TeO 2 –(40-x) WO 3 –xPbO glasses reveal that the glass network consists of [ TeO 3 ], [ TeO 4 ], [ WO 4 ], [ WO 6 ], and [ PbO 4 ] units. Changes in the coordination state of tellurium and tungsten ions occur when the PbO and WO 3 concentrations are varied. The dual role of the lead ions is confirmed in 60 TeO 2 –(40-x) WO 3 –xPbO glass system. The W ion coordination state changes from 4 to 6 when WO 3 concentration increases beyond 30 mol% in both (100-x) TeO 2 –x WO 3 and 60 TeO 2 –(40-x) WO 3 –xPbO glass systems. The IR spectra of 60 B 2 O 3 –10 TeO 2 –(30-x)ZnO–xPbO glasses reveal that the glass network consists of [ TeO 3 ], [ BO 3 ], and [ BO 4 ] groups.
TL;DR: It is found that the system can achieve the transition of neural firing patterns from the lower period state to the higher one, when the number of shortcuts in the neural network is greater than a threshold, indicating that the nervous system may make the optimal response to the change of stimulation by a corresponding adjustment of the shortcuts.
Abstract: We study the effects of random long-range connections (shortcuts) on the firing patterns in a network composed of Hindmarsh-Rose neurons. It is found that the system can achieve the transition of neural firing patterns from the lower period state to the higher one, when the number of shortcuts in the neural network is greater than a threshold, indicating that the nervous system may make the optimal response to the change of stimulation by a corresponding adjustment of the shortcuts. Then we discuss the transition degree of firing patterns of neural network and its critical characteristics for different external stimulation current. Furthermore, the influences of coupling strength on such transition behavior of neural firing patterns are also considered. Our results may be useful in comprehending the real mechanism in neural coding and information transmission in neurobiological systems.
TL;DR: Quasilinear theory is developed by using canonical variables for a relativistic plasma as mentioned in this paper, including momentum, pitch angle, and spatial diffusions, which is special for tokamas and, therefore, simple and suitable for simulations of cyclotron heating, current drive, and radiofrequency wave-induced radial transport in ITER.
Abstract: Quasilinear theory is developed by using canonical variables for a relativistic plasma. It is self-consistent, including momentum, pitch angle, and spatial diffusions. By assuming the wave field as a superposition of known toroidal and poloidal Fourier modes, the quasilinear diffusion coefficients are written in a form which can be directly evaluated using the output of a spectral full-wave solver of Maxwell equations in toroidal plasmas. The formalism is special for tokamas and, therefore, simple and suitable for simulations of cyclotron heating, current drive, and radio-frequency wave-induced radial transport in ITER.