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Sunday, March 7, 2010

Princeton University

Princeton University, established in 1746, has a rich history that includes being an original member of the Ivy League and one of nine Colonial Colleges founded prior to the American revolution that created the United States of America.

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The nine schools that make up the Colonial Colleges are in order of establishment:
o New College (est. 1636, now Harvard University)
o The College of William and Mary (est. 1693)
o Collegiate School (est. 1701, now Yale University)
o College of New Jersey (est. 1746, now Princeton University)
o King's College (est. 1754, now Columbia University)
o College in the English Colony of Rhode Island and Providence Plantations (est. 1764, now Brown University)
o Queen's College (est. 1766, now Rutgers University)
o Dartmouth College (est. 1769)
Of the nine Colonial Colleges seven are now members of the esteemed Ivy League with the eighth member, Cornell University, being founded later on in 1865. William and Mary and Rutgers, the two Colonial Colleges that are not part of the Ivy League, transitioned to eventually become public institutions.
Although some of the Ivy League schools are over three hundred years old the term "Ivy League" was never used until 1933 and did not become official until 1954. While initially attached specifically to athletics the term Ivy League has more generally come to be associated with the eight high ranking academically focused institutions which are located in Connecticut, Massachusetts, New Hampshire, New Jersey, New York, Pennsylvania, and Rhode Island.
A sportswriter by the name of Stanley Woodward while writing for the New York Tribune made the first known reference to the phrase "ivy colleges" in an October, 1933 piece about the football season. While there is some debate as to whether Woodward borrowed the phrase from fellow Tribune sports writer Caswell Adams the details are hazy. Regardless of who coined the term it is noteworthy to recognize that the phrase Ivy League is a relatively recent moniker when compared to the age of the schools.
Princeton University, like all of the Ivy League schools (with the notable exception of the more recently established Cornell University), was founded with religious influences as was custom for the time for all schools. Originally founded under the name the College of New Jersey, present day Princeton University (modern name given in 1896) began with Presbyterian influence. Despite a public position officially stating that the school was nonsectarian the purpose of the college in its earliest years was to train ministers in the beliefs held by the Presbyterian founders.
With a rich history that includes the attendance of three United States Presidents (James Madison, Woodrow Wilson, and John F. Kennedy) Princeton University has clearly established itself as one of the most academically successful schools in America, as is evident by the college's recurring position atop the US News and World Reports best colleges rankings.
In today's increasingly smaller and flatter world technological and travel advancements make the communities we live in increasingly global. Regardless of Princeton University's history in the Colonial Colleges and Ivy League the school must look towards the future in terms of global influence to continue its tradition of excellence.

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Why You Need a High School Education

Hopefully, you go via high school, graduate, and then go on to have a great life. If you are one of the teenagers out there that is struggling in school, you might ask yourself why a high school education is so essential if you do not plan on likely to university and possibly you have a employment waiting for you. No matter what is about to happen immediately after you happen to be done with your high school years, acquiring you diploma is extra significant than you imagine. Obtaining your diploma and finishing high school seriously isn't just about about to college, it can be about being prepared for life. You discover things in school that you require for each day living whether you are planning to university or any other sort of higher understanding following you are accomplished or not. With no these skills and classes, you will be about to struggle with points everyone else finds to become rather simple.
Classes aren't the only thing that shape your high school education. It doesn't matter what type of job or career you're going to pursue, you are going to deal with persons that are not like you. You also learn about lifetime in methods that you might not learn otherwise. When you miss out on these parts of your high school education, you could have to understand this stuff somewhere else, which just isn't always simple.
High school education isn't just about understanding the above mentioned elements. It truly is also about having a good time and enjoying your youth. Yes, you could have tests and homework to worry about, but you also have friends much more plentiful than possibly in any other time in life. You also have organized sports teams and clubs that you simply can join. These are all excellent parts of growing up that essentially contribute to your school education and also to who you're going to be once you go out into the world on your own. Don't feel about the work involved without having thinking about the fun you are able to have as well.
You need to actually feel about your high school education as your job whilst you are a teenager. Those people that have a high school diploma are gonna be paid extra for the same employment than people that do not have one. This seriously isn't continually true, but it normally is. Finishing school also shows that you're committed to finishing what you started, which continually looks beneficial to a potential employee. And who knows, you might change your mind about college or high studying inside the future, and already having your diploma is likely to make your life so much easier.

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History Curriculum For High School Homeschoolers


Finding a good history curriculum for high school was one of the greatest challenges I faced when I was being homeschooled. It seemed like most of the good history books stop at the Civil War or World War II. What about modern history? It's hard to find a history book from a Christian perspective about modern history. This difficulty has been overcome with a high school history curriculum from Notgrass Company. Exploring America by Ray Notgrass is an amazing curriculum that is exciting as well as educational. Each day is broken up into short concise lessons.
Sometimes history books seem to make the exciting events sound like nothing more than boring facts, Mr. Notgrass has an engaging writing style that makes the events come to life. There are also daily assignments that encourage the students to dig deeper. Sometimes they will read a document, speech, or hymn from American Voices, which is a 400+ page companion book that comes with the curriculum. Other times they will look up relevant Bible verses and also memorize verses. Writing assignments (including writing a research paper) are also part of the assignments. How's that for hitting 3 birds with one stone?
This book is essential for every high school student and will give them the tools to take an in-depth look at American history from a Biblical perspective. If you are looking for a really good American history high school curriculum look no further. Exploring America has filled a big gap in the history curriculum for homeschoolers. Exploring America is the best high school curriculum for American history I have ever seen!




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A Brief History of Bank Checks


There is no surviving documented proof of exactly when financial checks came to be part of financial transactions. Banks were a part of commercial life in ancient civilizations, but there are no records of any of the types of transactions that they carried out. However the ancient Mesopotamians, Greeks, and the Romans used banks. Some historians have dated the process of using checks at about 350 BC.

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Certainly in Medieval Italy the banks played a vital part in commercial transactions. Venice and Genoa were an important trading centers. Historical research indicated that Marco Polo brought the idea of a check back to Italy from the court of Kublai Khan in 1275. Once written instructions were acceptable it made a wider number of transactions possible.
Medieval Tuscan banks began the process of letters of credit and letters of exchange and the by fifteenth hundreds these types of transactions were common. They allowed the Italian mercantile trade to flourish because it was safer to write a check rather than carry large amounts of cash around.
By the early Sixteenth Century the practice had expanded to the Netherlands and once the banks had accepted a policy of paying money upon written instructions, this was the start of the modern account based payments by check. The English called their checks "cheque", and they still use the "que" at the end of the word.
The process of adapting checks occurred very quickly in America, in the 1600's the tobacco farmers in Virginia mortgaged their land and began to utilize their funds by writing checks. The oldest surviving check dates back to an English banker Lawrence Childs and it is dated 1762. The etymology of the word is unclear some view the root source to come from a double check to clarify the signatory. The Norman Kings developed a fiscal system and all the accounting was done on a piece of cloth which was divided into squares, with counters like draughts pieces.
When checks were first adapted the transactions were more secure for the customer and the recipient who could transfer funds without actually carrying cash. As the system grew in popularity so did the number of messengers travelling between banks. Eventually clearing houses were developed where the checks were exchanged. Historically this was supposed to have started in London when two chatting messengers realized that they were each carrying a check for the other bank and they exchanged them on the spot.
In the U.S.A. the bankers have a choice they can present checks to other banks, the Federal Reserve or private clearing houses for clearance. There is no reason to transport checks from bank to bank the clearing houses scan them and read the characters at the bottom of the check, which identifies the banks they are to be drawn against this is what is known as the routing or sort code. Then there is the individual account number at the base of the check and the number of the check. Once they have been scanned and identified they are presented to the bank electronically to draw the funds.
Until a few years ago checks were very basic as they still are in Europe, they have the banks name, the account name and number and the cheque number as well as a number identifying the bank that they are drawn against. In America theme checks are now all the rage. From a small change the individualization of checks snowballed.
Nowadays the checks are not issued necessarily by the bank; it is possible to purchase checks from outside approved sources. They are printed with family photographs in some cases. They are available in a huge arrangement of themes, colors, prints and borders.
In the twenty first Century there are other methods of paying bills, by credit, debit or charge card, and this has reduced the number of checks issued, the heyday for check numbers was the sixties, but none the less it is difficult to imagine that the need for checks will cease anytime soon. Who knows the credit crunch may well increase the amount of checks written as credit becomes harder to come by.

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A History of Quantum Mechanics


Robert Hooke and Christiaan Huygens begun working on a wave theory of light in the 1670s, this was reliant on the idea that light waves must propagate through a medium and so the void between the Sun and the Earth must be filled with an aether. In 1704 Newton suggested a corpuscular (particle) theory of light and presented experimental results proving his theory. Newton's corpuscular theory suggested that light would travel faster in a denser medium, something which was denied by the wave theory of light and so it was possible to experimentally verify Newton's result. It was not possible to do these experiments until 1850 and Foucault's results proved Newton wrong. Thomas Young and Augustin-Jean Fresnel had already provided experimental evidence in favour of the wave theory of light at the turn of the 19th century. Their famous double-slit experiments showed that light produced interference patterns which are expected from waves and Young went on to explain Newton's results in terms of his wave theory.
Towards the end of the 1800s Maxwell proposed that light could be understood as the propagation of electromagnetic waves; at any point on a beam of light there is an electric and a magnetic force moving perpendicularly to each other in the direction of the beams propagation. These force fields oscillate periodically and are therefore detected as waves. Maxwell showed this by verifying a set of four equations which describe the interrelationship between electric field, magnetic field, electric charge, and electric current.
Max Planck first introduced the concept of quanta in 1900, this reintroduced a corpuscular theory of light. Planck was looking at the relationship between the amount of radiation a blackbody emits and its temperature and he found that the experimental data only made sense if it was assumed that energy radiates in discrete 'quanta', or photons, each containing a packet of energy proportional to the frequency with which they radiate. This proportionality constant is known as Planck's constant.
Einstein applied the idea of Planck's constant to the problem of the photoelectric effect in 1905. The photoelectric effect shows that electrons can be released from certain metals by interacting with light, and that the amount of electrons that released depended not upon the intensity of the light, as Maxwell's theory suggested, but on the lights frequency. Einstein showed that this could be explained with a quantum theory of light whereby electrons are released only when particular frequencies are reached, corresponding to multiples of Planck's constant.
The double slit experiment can be performed on one photon at a time by letting sufficiently weak light travel through the slits. It was expected that no interference pattern would form as the photon must travel through either one slit or the other and would have nothing to interfere with. Yet this experiment has been performed numerous times and after letting a stream of photons through one at a time, what looked like random distribution soon turned into an interference pattern. This implies that the photon split when going through the two slits and reformed to be detected as a single photon on the other side. In order to see if this is what happened a photon detector was placed at each slit and the experiment was repeated. Yet no matter how many times this was done an interference pattern was never formed. The same results were found even when the detectors were placed on the other side of the slits, implying that the photon somehow knew that the detector would be there. It was found that photons behave as a particle when equipment is used to test for a particle and as a wave when a wave is being tested for.
In 1913 Bohr used the idea of quantised energy to explain how electrons orbit a nucleus by relating the angular momentum of electrons to Planck's constant. He deduced that electrons orbit with energy and momenta that are quantised to multiples of Planck's constant. All other values are not accessible to the electron, including certain spatial regions, and so when traveling between orbits the electrons seem to disappear and simultaneously appear somewhere else. This is why electrons do not loose energy as they orbit the nucleus but do so when 'jumping' between states. Just over a decade after Bohr extended the quantum theory to electrons, de Broglie proposed that all matter behaves this way.
In 1926 Schrodinger showed that quantum states can be represented not as waves or particles but by a complex function which evolves according to a second-order differential wave equation. Schrodinger's wave equation shows that a quantum state has a unitary evolution, with quanta existing in all physically possible states at once, this is known as a superposition. Schrodinger saw that if two quantum objects influence each other and are then parted they will be in a state of entanglement, such that interacting with one will change the state of another. If a pair of electrons are emitted from a common origin in an entangled state, and travel in different directions, then we can measure the spin of the electron in one plane and know the result of the other because they are always anti-correlated. Schrodinger showed that there is no equation for the state of a single entangled electron, they cannot really be said to possess individual spin states.
Around the same time as Schrodinger produced the wave equation Niels Bohr and his assistant at Copenhagen, Werner Heisenberg, used a matrix theory to interpret quantum mechanics, leading to the formulation of Heisenberg's uncertainty principle. Bohr and Heisenberg showed that properties corresponding to more than one physical possibility cannot be measured simultaneously for an object in a superpositional state, these properties are said to be non-commuting. The wave and particle properties of light are non-commuting and so by detecting a photon with a particle detector we remove our ability to measure any of its wavelike properties.
Energy and time are also non-commuting properties. The lowest energy state for waves is always right at the peak, if you imagine a pendulum swung on a string, it is stationary for just a second as it passes through the point between swinging from one side to the other. Here gravitational potential energy converts to kinetic energy, the position and momentum would be zero and so if we apply this logic to quantum mechanics we would assume that a quantum state would have zero energy at this point. The analogy is flawed however because quantum systems cannot have their position and momentum measured simultaneously, they can not both be zero and so they must have a non-zero minimum energy. In fact, quanta can have extremely high energies for very short periods of time. When a stream of quanta are fired at an impenetrable wall some will gain enough energy to tunnel through and appear on the other side.
These fluctuations are occurring everywhere and so if we look closely Einstein's smooth spacetime is in fact 'foaming' with quantum energy, this energy can create objects like electrons or photons which are continuously coming into existence for extremely short periods of time. The energy from these quantum fluctuations adds up to an enormous amount and since Einstein discovered that energy is interchangeable with mass this huge amount of energy would be so heavy that it should bend space, curving it up into a small ball. Later that year Max Born proposed a statistical interpretation of Schrodinger's wave function, with the square of the wavefunction interpreted as a probability amplitude. The mathematical interpretation of quantum mechanics was completed when the matrix mechanics used in Heisenberg's theories and the wave mechanics used in the Schrodinger equation were made compatible. This problem was tackled most notably by John von Neumann and Paul Dirac. In the standard von Neumann theory a quantum system is thought of as a point in Hilbert space. Hilbert space is analogous to the dimensional phase space of classical mechanics but includes an infinite amount of dimensions, representing the infinite amount of linear combinations of vectors corresponding to all of the possible states. Measurable properties, are represented as linear Hermitian operators on Hilbert spaces and the uncertainty principle can be explained by the fact that the two operators are non-commutating. A different approach came in 1926 when Pascual Jordan provided an independent unification of matrix and wave mechanics known as transformation theory.
Einstein was amongst many who believed that the theory of quantum mechanics must be incomplete because of the appearance of action at a distance. Einstein proposed a hidden variable theory with the motion of the quantum objects guided by the electromagnetic field. This was similar to the de Broglie-Bohm pilot-wave model of the wavefunction. In 1964 John Stewart Bell devised a way to theoretically test whether a hidden variable theory could be correct. In 1972 the experiments were conducted and they showed that Einstein was wrong and the Aspect experiments, performed in 1982, showed that this is true even if the distance between the entangled objects was such that any 'message' would have to travel faster than the speed of light. The Bell experiments strongly imply that entangled quantum systems can instantaneously influence each other even when separated across vast regions. The idea of action at a distance could be seen as analogous to Newtonian action at a distance but it differs in two respects. Firstly, quantum action at a distance does not have the symmetry that gravitational force has because in quantum mechanics the first measurement always determines the outcome of the other, they are not of mutual influence. Secondly in quantum mechanics the effects are irrespective of distance, whereas in the Newtonian model the force decreases proportionally to the square of the distance between objects. A better interpretation may be quantum holism. Holism refers to the idea that aspects of a state are not determined by its constituent parts but of the state as a whole.

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