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... The set of nine constants αij constitute the polarizability tensor for the molecular. It is always possible to choose “principal” axies such that the off-diagonal terms vanish, learning just three nonzero polarizabilities. ...
... The set of nine constants αij constitute the polarizability tensor for the molecular. It is always possible to choose “principal” axies such that the off-diagonal terms vanish, learning just three nonzero polarizabilities. ...
Mathematical Fundamentals
... influence of electric field. Kirchhoff's Current Law (KCL) is an assertion of the conservative property of charges under the implicit assumption that there is no accumulation of charge at the junction. Electromagnetic theory deals directly with the electric and magnetic field vectors where as circui ...
... influence of electric field. Kirchhoff's Current Law (KCL) is an assertion of the conservative property of charges under the implicit assumption that there is no accumulation of charge at the junction. Electromagnetic theory deals directly with the electric and magnetic field vectors where as circui ...
CHAPTER 1. SPECIAL RELATIVITY AND QUANTUM MECHANICS 1.1 PARTICLES AND FIELDS §
... Suppose we consider space to be free of charges so that the photons are noninteracting (or alternatively, consider these photons to be in a charge free volume with periodic boundary conditions so that their wave-vectors are integer multiples of 2π over the volume’s linear dimension in each direction ...
... Suppose we consider space to be free of charges so that the photons are noninteracting (or alternatively, consider these photons to be in a charge free volume with periodic boundary conditions so that their wave-vectors are integer multiples of 2π over the volume’s linear dimension in each direction ...
NIFS-886 (pdf file)
... required for the whole system, this could significantly ease the problems related to the local enhancement of the magnetic field around the cables. Such cables will become more feasible if new superconducting materials with higher critical temperatures are found in the future. We may also use these ...
... required for the whole system, this could significantly ease the problems related to the local enhancement of the magnetic field around the cables. Such cables will become more feasible if new superconducting materials with higher critical temperatures are found in the future. We may also use these ...
Millikan`s Oil-Drop Experiment
... To obtain the value of e from the measured fall and rise times, one needs to know the mass of the drop (or its radius, since the density is known). The radius is obtained from Stokes’ law using Equation 3-12. Notice that the right sides of Equations 3-16 and 3-17 are equal to the same constant, albe ...
... To obtain the value of e from the measured fall and rise times, one needs to know the mass of the drop (or its radius, since the density is known). The radius is obtained from Stokes’ law using Equation 3-12. Notice that the right sides of Equations 3-16 and 3-17 are equal to the same constant, albe ...
ECT1026 Field Theory_Chapter 3 Magnetostatics
... Figure 3.3-1: Magnetic flux density dB generated by a current element Id . The direction of the field induced at point P is into the page there as indicates by . ...
... Figure 3.3-1: Magnetic flux density dB generated by a current element Id . The direction of the field induced at point P is into the page there as indicates by . ...
Chapter 21 The Electric Field I: Discrete Charge Distributions
... the speed of light c, relativistic kinematics must be used to calculate its motion, but at speeds of 0.01c or less, non-relativistic kinematics is sufficiently accurate for most purposes.) (d) How far does the electron travel in that time? Picture the Problem We can use Newton’s 2nd law of motion to ...
... the speed of light c, relativistic kinematics must be used to calculate its motion, but at speeds of 0.01c or less, non-relativistic kinematics is sufficiently accurate for most purposes.) (d) How far does the electron travel in that time? Picture the Problem We can use Newton’s 2nd law of motion to ...
Field (physics)
In physics, a field is a physical quantity that has a value for each point in space and time. For example, on a weather map, the surface wind velocity is described by assigning a vector to each point on a map. Each vector represents the speed and direction of the movement of air at that point. As another example, an electric field can be thought of as a ""condition in space"" emanating from an electric charge and extending throughout the whole of space. When a test electric charge is placed in this electric field, the particle accelerates due to a force. Physicists have found the notion of a field to be of such practical utility for the analysis of forces that they have come to think of a force as due to a field.In the modern framework of the quantum theory of fields, even without referring to a test particle, a field occupies space, contains energy, and its presence eliminates a true vacuum. This lead physicists to consider electromagnetic fields to be a physical entity, making the field concept a supporting paradigm of the edifice of modern physics. ""The fact that the electromagnetic field can possess momentum and energy makes it very real... a particle makes a field, and a field acts on another particle, and the field has such familiar properties as energy content and momentum, just as particles can have"". In practice, the strength of most fields has been found to diminish with distance to the point of being undetectable. For instance the strength of many relevant classical fields, such as the gravitational field in Newton's theory of gravity or the electrostatic field in classical electromagnetism, is inversely proportional to the square of the distance from the source (i.e. they follow the Gauss's law). One consequence is that the Earth's gravitational field quickly becomes undetectable on cosmic scales.A field can be classified as a scalar field, a vector field, a spinor field or a tensor field according to whether the represented physical quantity is a scalar, a vector, a spinor or a tensor, respectively. A field has a unique tensorial character in every point where it is defined: i.e. a field cannot be a scalar field somewhere and a vector field somewhere else. For example, the Newtonian gravitational field is a vector field: specifying its value at a point in spacetime requires three numbers, the components of the gravitational field vector at that point. Moreover, within each category (scalar, vector, tensor), a field can be either a classical field or a quantum field, depending on whether it is characterized by numbers or quantum operators respectively. In fact in this theory an equivalent representation of field is a field particle, namely a boson.