physics in current

2010年12月30日星期四

Resistor

A resistor is an electronic component that restricts the flow of current in an electrical or electronic circuit. It is used to control voltage. It can also be used to protect sensitive components from exploding/blowing. The higher the resistance, the less current there can be. Some look like microchips, and others look like a wire with a small colored cylinder of material around them.
Resistors can be linked in various combinations to help make a circuit:
1) Series - Where the resistors are linked one after another.
2) Parallel - Where the resistors are linked over one another.
There are many different types of resistors. Not only do some have a higher resistance to electricity than others, but resistors also have different ratings to tell electricians how much power they can handle before they break, and how accurately they can slow the flow of electricity. A lot of resistors have colored rings on them to help people knowledgeable about electronics quickly tell what their resistance and accuracy they are rated at.
Resistors can be made out of many materials. Older resistors are made out of solid carbon. These are still being used, but not very often, because they do not hold up well to air moisture, and because they are usually too expensive to make these days. Resistors using carbon as a film, however, are newer and are still being made. Other newer resistors can be made out of wire or metal. Newer resistors can handle air moisture and the heat from all the electricity that has to go through them a lot better than the old ones could.

Uncertainty principle

The Heisenberg uncertainty principle says that the more we know about where a particle is right now, the less we know about how fast it's going and the direction that it's going. This also works the other way around (so the more we know about how fast it's going and the direction it's going, the less we know about where it is right now.)
Werner Heisenberg was the first person to find out about it in 1927. This uncertainty principle helped to make the study of quantum mechanics.
In quantum physics, the outcome of even the most perfect measurement of a system is not already a fact, but instead is shown by a probability distribution. The larger the related standard deviation is, the more "uncertain" we might say what we're showing is for the system.
The uncertainty principle is often confused with the observer effec.
An important part of quantum mechanics, which shows itself in the Heisenberg Uncertainty Principle, is that no physical event can be (really specifically) described as a "classic point particle" or as a wave, but rather the tiny event is best described in terms of wave-particle duality. Basically, small bits of matter and small waves of energy are sometimes very hard to tell apart, because they can act like both at the same time.
The Heisenberg uncertainty principle is caused by this.
A quantum mechanical particle wave is sort of like a sound wave. When people try to measure the frequency of a sound wave, they are trying to figure out how often something happens in a given amount of time. That means there's basically no such thing as "frequency" in one single moment of time. In order to be really have a sure frequency, a signal has to be around for a long time (which means it doesn't really exist in only a really specific "moment in time"). It works the other way, too: if a signal exists for only a second, it wasn't around long enough to have a really specific frequency band. This is basically Math's "version" of the Uncertainty Principle.

Physicists who studied light in the 1700's and 1800's were having a big argument about whether light was made of particles shooting around like tiny bullets, or waves washing around like water waves. At times, light seems to do both. At times, light seems to go only in a straight line, as if it were made of particles. But other experiments show that light has a frequency and wavelength, just like a sound wave or water wave. Until the 20th century, most physicists thought that light was either one or the other, and that the scientists on the other side of the argument were simply wrong.
In 1909, a scientist named Geoffrey Taylor decided that he was going to settle this argument once and for all. He borrowed an experiment invented earlier by Thomas Young, where light was shone through two small holes right next to each other. When bright light was shone through these two small holes, it created an interference pattern that seemed to show that light was actually a wave.
Taylor's idea was to photograph the film coming out of the holes with a special film that was unusually sensitive to light. When bright light was shined through the holes, the film showed an interference pattern, just like Young showed earlier. Taylor then turned down the light to a very dim level. When the light was dim enough, Taylor's photographs showed tiny pinpoints of light scattering out of the holes. This seemed to show that light was actually a particle. If Taylor allowed the dim light to shine through the holes for long enough, the dots eventually filled up the film to make an interference pattern again. This demonstrated that light was somehow both a wave and a particle.
To make matters even more confusing, Victor de Broglie suggested that matter might act the same way. Scientists then performed these same experiments with electrons, and found that electrons too are somehow both particles and waves.
Today, these experiments have been done in so many different ways by so many different people that scientists simply accept that both matter and light are somehow both waves and particles. Scientists generally admit that even they do not fully understand how this can be, but they are quite certain that it must be true. Although it seems impossible to understand how anything can be both a wave and a particle, scientists do have a number of equations for describing these things that have variables for both wavelength (a wave property) and momentum (a particle property). This seeming impossiblity is referred to as the wave-particle duality.

Particles as waves

An electron has a wavelength called the "de Broglie wavelength". It can be calculated using the equation
\lambda_D = \frac{h}{\rho}
λD is the de Broglie wavelength.
h is Planck's constant
ρ is the momentum of the particle.
This made the idea that electrons in atoms show a standing wave pattern

Waves as particles

The photoelectric effect shows that a light photon which has enough energy (a high enough frequency), can cause an electron to be released off a metal's surface. Electrons in this case can be called photoelectrons.

Quantum mechanics ("QM") is a part of physics, which is the study of matter and energy. Quantum mechanics explains how things smaller than the size of atoms act. The main things studied are called subatomic particles and electromagnetic waves.
Quantum is a Latin word which means 'how much'. So a quantum of energy is a definite amount of energy. Any lamp such as a candle or laser shoots out light unit by unit. The more of these units (photons) are given off per second, the brighter, or more intense, the light. The wavelength (or frequency) decides the color of the light.
Black at left is ultraviolet; black at right is infrared.
If the color of the light is infrared (lower in frequency than red light), each photon can heat up what it hits. So, if a strong infrared lamp (a heat lamp) is pointed at a person, that person will feel warm, or even hot. However, the person cannot get a sunburn, because the photons do not have enough energy to kill living cells. Infrared photons are sometimes called "black light" because humans cannot see infrared light. Humans can feel the radiation in the form of heat. For example, a person walking by a brick building that has been heated by the sun will feel heat from the building without having to touch it.
If the color of the light is ultraviolet (higher in frequency than violet light), then each photon has a lot of energy, enough to hurt skin cells and cause a sunburn. Even higher frequencies of light (or electromagnetic radiation) cause even more damage. X-rays can go deep into the human body and do things like kill cells. Humans cannot see or feel ultraviolet light. They may only know they have been under ultraviolet light when they get a sunburn. Areas where it is important to kill germs often use ultraviolet lamps to destroy bacteria, fungi, etc.
Quantum mechanics started when it was discovered that a certain frequency means a certain amount of energy. The higher the frequency, the more power a photon has, the more damage it can do. Quantum mechanics later grew to explain the internal structure of atoms. Quantum mechanics also explains the way that a photon can interfere with itself, and many other things never imagined in classical physics.
Planck discovered the relationship between frequency and energy. Nobody earlier than he had guessed that frequency would be proportional to energy (this means that as one increases, the other does too). If we choose to use what are called natural units, then the number representing the frequency of a photon would also represent its energy. The equation would have been:
e = f
But the way physics grew, there was no natural connection between the units then used to measure energy and the units commonly used to measure time (and therefore frequency). So the formula that Planck worked out to make the numbers all come out right was:
e = h × f
 
 
r, energy equals h times frequency. This h is a special proportionality constant, called Planck's constant, after its discoverer. Quantum mechanics is based on the realization that a photon of a certain frequency means a photon of a certain amount of energy. Besides that, a certain kind of atom can only give off certain frequencies of radiation, so it can also only give off photons that have certain amounts of energy.

Schrödinger equation

the Schrödinger equation is a mathematical formula that physicists use to study quantum mechanics. It is a mathematical equation that was thought of by Erwin Schrödinger in 1925. It shows how particles act in lots of time based situations. It can predict the position and velocity of a particle (where it is and how fast it is moving) at a certain time. It cannot be very accurate, however, because of the uncertainty principle. It uses something called a wavefunction to make questions about how the particle acts. The wavefunction is a picture of how this particle acts with time and describes the particle as fully as possible.
For one particle that only moves in one direction other than time, the Schrödinger equation looks like:
i\hbar\frac{\partial}{\partial t} \Psi(\mathbf{x},\,t) = \hat H \Psi(\mathbf{x},\,t)
where:
i is the square root of minus one
\hbar is the reduced Planck's constant
t is time
x is a place in space
\psi(\mathbf{x},\,t) is the wavefunction
\hat H is the Hamiltonian energy operator

The spring equation

the length of a spring always changes by the same amount when it is pushed or pulled. The equation for that is:
F = − kx
where
F is how much push or pull is on the spring (e.g. 10 kilograms)
k is the spring constant, or how strong the spring is. Different springs have different strengths or k.
x is how far the spring was pushed or pulled
The negative sign is because the direction of the force is always opposite of the direction that the spring was pushed or pulled. When x = 0, the spring how far it was when there was no push or pull on it. The spring is at the equilibrium position. There is a minus sign because the force of the spring does not go to the same direction as the spring moves. This equation only works on a linear spring. A linear spring is a spring that is only being pushed or pulled in one direction, like left or right or up or down.

Elastic Potential Energy

Elastic potential energy is the energy saved in an object that is stretched, compressed (compression is pressing objects together), twisted or bent. For example, an arrow gets the elastic potential energy from the bow. When it leaves the bow, the potential energy turns into kinetic energy. The equation of the elastic potential energy is:
U=\frac{1}{2}kx^2
where
U is the elastic potential energy.
k is the spring constant.
x is the distance pushed or pulled.

Phonon

Condensed matter physics

 Ferromagnetism 

Ferromagnetism is the basic mechanism by which certain materials (such as iron) form permanent magnets, or are attracted to magnets. In physics, several different types of magnetism are distinguished. Ferromagnetism is the strongest type; it is the only type that can produce forces strong enough to be felt.

 

German physicist Georg Ohm :Ohm's law

treatise published in 1827.
described measurements of applied voltage and current through simple electrical circuits containing various lengths of wire.

In physics, the term Ohm's law is also used to refer to various generalizations of the law originally formulated by Ohm. The simplest example of this is:
\boldsymbol{J} = \sigma \boldsymbol{E},
where J is the current density at a given location in a resistive material, E is the electric field at that location, and σ is a material dependent parameter called the conductivity. This reformulation of Ohm's law is due to Gustav Kirchhoff

Microscopic origins of Ohm's law

The dependence of the current density on the applied electric field is essentially quantum mechanical in nature; 

Classical and quantum mechanical views of conductivity have both described the movements of electrons in a metallic solid. The free electron gas that is present in metallic solids is the reason for an important property of all metals: conductivity.

Solid states

Solids can be split into two groups: amorphous and crystalline 

Amorphous solid structures occur when a liquid is cooled too rapidly for the crystalline structure to form. Glass is a typical amorphous solid.
however, ample time is allowed during the cooling of a liquid, then a crystalline structure will form.
crystalline structures, several different types of bonding are possible. These include ionic bonding, covalent bonding, and metallic bonding.
structure of a specific crystal is dependent on the bonding type, along with the sizes of the atoms involved.

Paul Drude 

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