Wednesday, March 18, 2020

Charlemagne2 essays

Charlemagne2 essays Charlemagne, also known as Charles the Great, became the undisputed ruler of Western Europe. As Western Europe was deteriorating Charlemagne was crowned the privilege of being joint king of the Franks in 768 A.D. People of Western Europe, excluding the church followers, had all but forgotten the great gifts of education and arts that they had possessed at one time. Charlemagne solidly defeated barbarians and kings in identical fashion during his reign. Using the re-establishment of education and order, Charlemagne was able to save many political rights and restore culture in Western Europe. Charlemagne was born in 742 A.D., to a very famous and well-known family. Charlemagnes grandfather was Charles Martel, the man who was responsible for the defeat of the Saracens. Charlemagne was also the eldest son of Bertrade (also known as Bertha Greatfoot) and Pepin the Short, the first to become king of the Franks. With the almost full extinction of schools in the 8th century, many historians say that Charlemagne received very little education, but did learn the art of reading from Bertrade. The one thing that kept Charlemagne motivated throughout his entire life was his deep devotion to the church. Charlemagne was a tall young man with light blond hair, and was described by his secretary as stately and dignified. Charlemagne had great wit, but was stern at times. He had simple and moderate tastes; he enjoyed hunting, riding and swimming. Charlemagne had a large wardrobe with many Frankish dresses, linen shirts and breeches, silk-fringed tunics, hoses wrapped with bands, and for the winter he had coats made of otter or marten skins. Charlemagne asked his people to improve their lifestyles, but he divorced two of his four fives without any given cause. In 768 A.D., Charlemagne at the age of 26, along with his brother Carloman inherited the kingdom of Franks. However, in 771 A.D. Carloman died, making Charlemagne...

Sunday, March 1, 2020

Dark Energy (Definition)

Dark Energy (Definition) Dark energy is a hypothetical form of energy that permeates space and exerts a negative pressure, which would have gravitational effects to account for the differences between the theoretical and observational results of gravitational effects on visible matter. Dark energy is not directly observed, but rather inferred from observations of gravitational interactions between astronomical objects. The term dark energy was coined by the theoretical cosmologist Michael S. Turner. Dark Energys Predecessor Before physicists knew about dark energy, a cosmological constant  was a feature of Einsteins original general relativity equations that caused the universe to be static. When it was realized the universe was expanding, the assumption was that the cosmological constant had a value of zeroan assumption that remained dominant among physicists and cosmologists for many years. Discovery of Dark Energy In 1998, two different teamsthe Supernova Cosmology Project and the High-z Supernova Search Teamboth failed at their goal of measuring the deceleration of the universes expansion. In fact, they measured not only a deceleration, but a totally unexpected acceleration  (Well, almost totally unexpected: Stephen Weinberg had once made such a prediction). Further evidence since 1998 has continued to support this finding, that distant regions of the universe are actually speeding up with respect to each other. Instead of a steady expansion, or a slowing expansion, the expansion rate is getting faster, which means that Einsteins original cosmological constant prediction manifests in todays theories in the form of dark energy. The latest findings indicate that over 70% of the universe is composed of dark energy. In fact, only about 4% is believed to be made up of ordinary, visible matter. Figuring out more details about the physical nature of dark energy is one of the major theoretical and observational goals of modern cosmologists. Also Known As: vacuum energy, vacuum pressure, negative pressure, cosmological constant