The electron follows a semicircle under the transverse Lorentz force. Parallel, oppositely directed incoming and outgoing paths are separated by a diameter, so the orbit radius is . Acceleration from rest through the electric potential difference gives kinetic energy , where is the elementary electric charge. Equating the Lorentz force magnitude to the required centripetal force gives
The magnetic field must be perpendicular to the plane of the turn, with its sign chosen for the electron's negative electric charge. In the illustration the electron enters rightwards at the upper endpoint, so a magnetic field into the page bends it downwards.
The nonrelativistic estimate has . If the small special relativity correction is retained, use with and . This gives , about larger. The leading answer is adequate at the precision implicit in the classical treatment.
Put the two coil centres at . By superposition, their axial magnetic field is
Both magnetic field contributions point the same way. Evaluation gives
The corresponding coefficients are and . Each individual magnetic field falls as one moves away from its own coil; their sum is much flatter near the midpoint.
For a single coil, differentiating twice produces . At this vanishes. Thus the pair has by reflection symmetry and by its chosen separation; all odd derivatives vanish there. In fact,
This Helmholtz coil arrangement produces a nearly uniform central magnetic field, useful for controlled charged particle in a uniform magnetic field and magnetic field calibration. The small orbit used below lies within that central region.
Figure 1.
Helmholtz axial magnetic field and a semicircular electron trajectory
. Details.
For a circular coil, use the Biot-Savart law
At an axial position , every wire element is at distance . The transverse magnetic field contributions cancel by rotational symmetry. The axial part of is , and . Multiplying by the turns gives
The electric current's sense fixes the axial direction by the right-hand rule.
Set the red image at coordinate zero, the blue image at , and the screen at . Let the correcting thin lens be at , with . Both original images are then real objects for the correcting thin lens, with positive object distances , , and common positive image distance . The thin lens equation gives
The refractive indices and Lensmaker's equation require
Substitute the two focal lengths and cancel :
Thus the correcting thin lens is beyond the red image and before the screen. The required focal lengths and surface radius are
The blue focal length is shorter because the blue refractive index is larger; these two differing object distances are mapped to the same screen, removing the specified longitudinal chromatic aberration.
In the paraxial approximation, apply refraction at each surface of the thin lens in air. With signed radii and , the first surface obeys , and the second obeys . The separation of the surfaces is neglected, so the intermediate image coordinate cancels:
This is Lensmaker's equation, with Cartesian coordinate system object coordinate for a real object. For an equiconvex thin lens and light travelling left to right, and . Hence
Electrical contact equalizes electric potential and preserves total electric charge. The usual isolated-sphere approximation assigns the two conducting spheres the capacitances and . It then gives
These are accurate when the conducting spheres are far apart and joined by a thin wire. Literal touching changes the answer: each conducting sphere polarizes the other, so its electric potential is not its isolated value. The source does not specify an approximation which would remove this effect.
For completeness, the exact result for ideal externally tangent conducting spheres can be obtained by the method of images. Let their radii be , their centre separation , and their common electric potential . Begin with central image charges and . Reflect each external image charge at centre-distance into the other conducting sphere of radius : the new image charge is at centre-distance toward the original. Repeat, alternately, in the two conducting spheres. Pairing successive opposite-sign terms gives the convergent net electric charges
Each reflection cancels a nonconstant surface electric potential; the remaining central term fixes . The total internal image charge equals the exterior electric flux divided by , so these sums give the physical net electric charges.
For , multiply both dimensionless sums by the common factor . Their values follow by writing reciprocals as integrals and setting :
Dividing by enforces conservation of electric charge and yields
This concrete touching-sphere result disproves applying the isolated sharing rule to literal contact.
At electrostatic equilibrium the electric field in the metal is zero. The empty cavity also has zero electric field, by the uniqueness theorem for the electrostatic potential. The electric charge lies on the outer surface. For the isolated conducting sphere, spherical symmetry and Gauss's law give
Taking the electric potential to vanish at infinity and using gives
The electric potential is continuous at the surface, while the normal electric field jumps by , with surface charge density .
The two wavelengths have independent interference patterns. Their interference fringe spacings are
Different optical frequencies do not maintain a fixed mutual phase over the detector's integration time, so their intensities add. For narrow equal slits, suppressing the slowly varying diffraction envelopes, one may write
The relative line strengths are not supplied; the figure illustrates equal peak intensities rather than inferring a quantitative brightness ratio. At both colours are bright, producing a blue-green mixture. Away from the centre the green and blue interference fringes progressively separate, creating alternating colour and brightness variations; places where one line is dark can still be bright in the other. Neither two-line mixing nor its central maximum is generally white.
Across , the green maxima occur at for , and the blue maxima at for . Near , the fourth green and fifth blue maxima nearly coincide: and . The mismatch shows that these are near coincidences, not exact ones for the given wavelengths. The plotted central interval includes all these maxima.
Illuminate a narrow entrance slit with the mercury-vapor lamp, use a collimating lens to illuminate two parallel narrow slits coherently, and insert a bandpass filter selecting the green line. Place a screen or scanning detector a measured distance beyond the double slit. The source slit and the two apertures should be parallel. The aperture widths should be appreciably smaller than their separation to provide an extended diffraction envelope; the green filter should reject the other strong mercury lines. The layout is drawn below.
For slit separation and observation angle , the optical path difference in air is . At a bright interference fringe, . For a distant screen and small angles, , giving
Measuring several interference fringe spacings and dividing by their number reduces relative position error. The derivation assumes the slits have equal phase on illumination and that the screen region lies within their common diffraction envelope.
Figure 1.
Double-slit layout and two-colour fringes across the central thirty millimetres
. Details.
A mercury-vapor lamp is an extended, spontaneously emitting source, so practical interference requires spatial filtering and spectral selection. A narrow illuminated source slit gives sufficient spatial coherence; selecting one strong spectral line improves temporal coherence and avoids overlapping differently spaced interference fringes.
In the classical double-slit experiment, both apertures are illuminated by the same narrow source. The arrangement is symmetric, permits direct measurement and adjustment of slit separation, and has equal optical materials in the two paths. Its main drawbacks are low transmitted intensity through narrow apertures, the need for a well-made closely spaced slit pair and alignment, and the finite single-slit diffraction envelope. A broad source washes out interference fringes.
Lloyd's mirror uses the direct wave from a narrow source and the reflected wave, which appears to come from its virtual image behind a plane mirror. It requires only one physical source slit; the mirror can be adjusted to make a small effective source separation without manufacturing a double aperture. Only the direct-reflected overlap region shows interference fringes. Finite mirror size, alignment, surface quality, unequal intensities and the polarization-dependent reflection coefficient can reduce visibility. For the usual grazing reflection from glass, the reflected electric wave acquires approximately a phase shift, so the zero path-difference position is dark rather than the bright central fringe of the symmetric classical double-slit experiment. Both arrangements still require adequate spatial coherence and temporal coherence.
The passive RC low-pass filter is simple, inexpensive, requires no power supply, and has no operational amplifier saturation or finite bandwidth limitation. It offers no voltage gain; its output impedance is finite, and both source electrical resistance and loading can change the observed frequency response. Its resistor also produces thermal noise.
The active inverting low-pass amplifier provides a low-frequency voltage gain of magnitude five and, within the usable bandwidth, a small output impedance, so it can drive a load with much less change in frequency response. The input electrical resistance is approximately and may itself load the source. It needs a power supply and adds electrical noise and offset; finite operational amplifier gain, bandwidth, slew rate, available output swing, and output electric current limit the ideal formula. Its inversion must also suit the application. The best choice depends on required voltage gain, source and load electrical impedances, and the signal's frequency and amplitude.
For an ideal operational amplifier under negative feedback, the grounded non-inverting terminal makes the inverting terminal a virtual ground, and no electric current enters either input. The feedback resistor and capacitor have parallel electrical impedance
Kirchhoff's current law at the inverting node gives , and hence
With the stated components, and . Thus this inverting low-pass amplifier has exactly the same ideal cutoff frequency and normalized frequency response as the passive RC low-pass filter, with output multiplied by :
Its amplitude ratios at the three stated frequencies are , , and . One principal choice of phase shift is : respectively , , and . Adding or subtracting describes the same output; the extra inversion must be retained.
Use complex phasors with time dependence and assume an unloaded output. The capacitor has electrical impedance . The voltage divider formed with the resistor gives the transfer function
For input , the output amplitude and phase shift are
so .
Here , and the cutoff frequency is . This is an RC low-pass filter: at small frequency the capacitor has large electrical impedance and the output nearly equals the input; at large frequency it increasingly shunts the signal to ground. The amplitude then falls as , and the phase shift approaches .
Frequency | Output amplitude divided by | Output phase shift \ | | \ | | \ | |
No numerical input amplitude is supplied, so the output voltages are specified as fractions of . An application is suppression of high-frequency electrical noise on a slowly varying signal. A finite load changes the transfer function and must be included if its electrical impedance is comparable with the circuit's output electrical impedance.
Figure 1.
Passive and active low-pass amplitude and phase responses
. Details.
At the terminal velocity, the acceleration in iii vanishes. Thus
For and nonzero , the magnetic drag increases linearly with speed and this terminal state is stable. Horizontal rails have no gravitational drive. Vertical rails have no linked vertical magnetic flux change, so the model gives free fall rather than a finite terminal velocity.
Project Newton's second law down the slope. The normal reaction has no component along the rails, while the magnetic term opposes motion:
This first-order linear differential equation has the release-from-rest solution
The electrical self-inductance has been neglected; retaining it introduces a coupled electric current equation rather than this instantaneous resistive response.
The component of magnetic force along the slope has magnitude . The rate at which the sliding bar does work against this magnetic braking is
By Ohm's law, , so
This exactly equals the Joule heating in the resistor in the negligible-self-inductance approximation. The normal force does no work because it is perpendicular to the velocity.
The gravitational power is instead . By the work-energy theorem,
It equals the Joule heating only at constant speed. For a concrete counterexample, during the initial acceleration the kinetic energy increases, so some gravitational power remains mechanical.
Use the coordinates in 8. At downhill speed , the moving bar has . The electromotive force and induced electric current are therefore
Here is positive along across the sliding bar, then returns through the rails and resistor. This direction makes the magnetic force oppose downhill motion, as required by Lenz's law. The factor is essential: only the component of magnetic field normal to the rail plane threads the circuit. Rail and bar electrical resistances and circuit self-inductance are neglected relative to the stated large model.
For an inductor, . In the steady AC solution with no added constant electric current,
The electric current lags the voltage by . An ideal inductor can also sustain an arbitrary DC current, fixed by initial conditions; it is excluded from this steady sinusoidal comparison.
For a capacitor, , so
The electric current leads the voltage by .

Pinned article: Introduction to the OurBigBook Project

Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
We have two killer features:
  1. topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculus
    Articles of different users are sorted by upvote within each article page. This feature is a bit like:
    • a Wikipedia where each user can have their own version of each article
    • a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
    This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.
    Figure 1.
    Screenshot of the "Derivative" topic page
    . View it live at: ourbigbook.com/go/topic/derivative
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    This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
    Figure 5. . You can also edit articles on the Web editor without installing anything locally.
    Video 3.
    Edit locally and publish demo
    . Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension.
  3. https://raw.githubusercontent.com/ourbigbook/ourbigbook-media/master/feature/x/hilbert-space-arrow.png
  4. Infinitely deep tables of contents:
    Figure 6.
    Dynamic article tree with infinitely deep table of contents
    .
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Further documentation can be found at: docs.ourbigbook.com
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