Ferrin s Process Of Inductive Bible Study - 964 Words

Ferrin’s process of inductive Bible study takes on a relational approach that consists of three essential parts or phases titled Foundation, Framing, and Finish Work. The structured methods encompass studying a book of the Bible and internalizing it rather than just memorizing the words (p. 3). The author diligently explains how that through the devoted application of all phases individuals and group Bible study participants are sure to â€Å"fall in love with God’s Word† (p. 3). Ferrin presents and or describes Scripture internalization as taking in the truth and then applying it to everyday life or living. Ferrin pointed out that the benefits of understanding biblical messages book by book include the Living Word of God becoming a reality within persons that grow more enjoyable and rewarding as time comes and goes. On a personal note, I practice reading the Bible through the process of observation. For instance, I practice learning what to look for in the text; interpreting the meaning; I prayerfully seek God and through the power of the Holy Spirit I can apply what I read. Nevertheless, I feel Ferrin’s process of inductive Bible study might prove more productive and edifying both personally and in a group. Moving forward and upon careful consideration, I find that Ferrin’s four- step â€Å"building a house† analogy approach might help me to get to know a book of the Bible and all of its elements. For example, during the foundation phase the background study of the author,Show MoreRelatedStephen P. Robbins Timothy A. Judge (2011) Organizational Behaviour 15th Edition New Jersey: Prentice Hall393164 Words   |  1573 Pagesand permission should be obtained from the publisher prior to any prohibited reproduction, storage in a retrieval system, or transmission in any form or by any means, electronic, mechanical, photocopying, recording, or likewise. To obtain permission(s) to use material from this work, please submit a written request to Pearson Education, Inc., Permissions Department, One Lake Street, Upper Saddle River, New Jersey 07458, or you may fax your request to 201-236-3290. Many of the designations by manufacturers

The Medieval Islamic Attitude Towards Christianity

The medieval Islamic attitude towards Christianity varied quite considerably; often Christians would be considered as either ‘People of the Book’, or as heretics. There was a common belief among Muslims that, while Muslims tolerated Christians and accepted them, Christians had a tendency to pre-condemn Muslims. On the other hand, although Christians did undeniably attempt to convert Muhammad, and many other Muslims, to Christianity, as well as refer to them repeatedly as pagans within their literature, it is almost understandable; within a century of the death of Muhammad in 632, Islam had spread across much of the known world, a dilemma that was unfathomable, theologically incomprehensible and simply terrifying for most Christians. The†¦show more content†¦It is clear that the East was a place that filled many European Christians with both fear and fascination, but the very nature of the Christian holy places being largely ruled by Muslims meant that the Christian West could not help but come into repeated contact with the East. The Islamic world was generally associated with relentless stereotypes, such as the character of the oppressive Oriental ruler, as well as the persistent idea of sexual immorality within Eastern customs. Some Christian doctrines, for example the thirteenth century Franciscan friars, strongly identifies Islam with the coming of the anti-Christ, and many medieval Christian writers displayed resentment towards Islam through attacking the basis of the religion in an attempt to undermine its validity. Muslims in Christian literature were ultimately not Muslims at all, but the fictional, projected Western archetype; as Matsushita states, the ‘medieval Christian literary repres entation of the Muslim was no

My favourite game free essay sample

A star is a massive, luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun, which is the source of most of the planets energy. Some other stars are visible from Earth during the night, appearing as a multitude of fixed luminous points due to their immense distance. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the stars interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the stars lifetime and, for some stars, by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, luminosity, and spectrum respectively. The total mass of a star is the principal determinant of its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the stars environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung–Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined. A stars life begins with the gravitational collapse of a gaseous nebula of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. Once the stellar core is sufficiently dense, hydrogen becomes steadily converted into helium through nuclear fusion, releasing energy in the process. [1] The remainder of the stars interior carries energy away from the core through a combination of radiative and convective processes. The stars internal pressure prevents it from collapsing further under its own gravity. Once the hydrogen fuel at the core is exhausted, a star with at least 0.4 times the mass of the Sun[2] expands to become a red giant, in some cases fusing heavier elements at the core or in shells around the core. The star then evolves into a degenerate form, recycling a portion of its matter into the interstellar environment, where it will contribute to the formation of a new generation of stars with a higher proportion of heavy elements. [3] Meanw hile, the core becomes a stellar remnant: a white dwarf, a neutron star, or (if it is sufficiently massive) a black hole. Binary and multi-star systems consist of two or more stars that are gravitationally bound, and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution. [4] Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy. Distribution A white dwarf star in orbit around Sirius (artists impression). NASA image In addition to isolated stars, a multi-star system can consist of two or more gravitationally bound stars that orbit each other. The simplest and most common multi-star system is a binary star, but systems of three or more stars are also found. For reasons of orbital stability, such multi-star systems are often organized into hierarchical sets of binary stars. [77] Larger groups called star clusters also exist. These range from loose stellar associations with only a few stars, up to enormous globular clusters with hundreds of thousands of stars. It has been a long-held assumption that the majority of stars occur in gravitationally bound, multiple-star systems. This is particularly true for very massive O and B class stars, where 80% of the stars are believed to be part of multiple-star systems. However the proportion of single star systems increases for smaller stars, so that only 25% of red dwarfs are known to have stellar companions. As 85% of all stars are red dwarfs, most stars in the Milky Way are likely single from birth. [78] Stars are not spread uniformly across the universe, but are normally grouped into galaxies along with interstellar gas and dust. A typical galaxy contains hundreds of billions of stars, and there are more than 100 billion (1011) galaxies in the observable universe. [79] A 2010 star count estimate was 300 sextillion (3 ?1023) in the observable universe. [80] While it is often believed that stars only exist within galaxies, intergalactic stars have been discovered. [81] The nearest star to the Earth, apart from the Sun, is Proxima Centauri, which is 39. 9 trillion kilometres, or 4. 2 light-years away. Travelling at the orbital speed of the Space Shuttle (8 kilometres per second—almost 30,000 kilometres per hour), it would take about 150,000 years to get there. [82] Distances like this are typical inside galactic discs, including in the vicinity of the solar system. Stars can be much closer to each other in the centres of galaxies and in globular clusters, or much farther apart in galactic halos. Due to the relatively vast distances between stars outside the galactic nucleus, collisions between stars are thought to be rare. In denser regions such as the core of globular clusters or the galactic center, collisions can be more common. [84] Such collisions can produce what are known as blue stragglers. These abnormal stars have a higher surface temperature than the other main sequence stars with the same luminosity in the cluster. [85] Characteristics OBESERVATION HISTORY Historically, stars have been important to civilizations throughout the world. They have been part of religious practices and used for celestial navigation and orientation. Many ancient astronomers believed that stars were permanently affixed to a heavenly sphere, and that they were immutable. By convention, astronomers grouped stars into constellations and used them to track the motions of the planets and the inferred position of the Sun. [5] The motion of the Sun against the background stars (and the horizon) was used to create calendars, which could be used to regulate agricultural practices. The Gregorian calendar, currently used nearly everywhere in the world, is a solar calendar based on the angle of the Earths rotational axis relative to its local star, the Sun. The oldest accurately dated star chart appeared in ancient Egyptian astronomy in 1534 BC. [8] The earliest known star catalogues were compiled by the ancient Babylonian astronomers of Mesopotamia in the late 2nd millennium BC, during the Kassite Period (ca. 1531–1155 BC). [9] The first star catalogue in Greek astronomy was created by Aristillus in approximately 300 BC, with the help of Timocharis. The star catalog of Hipparchus (2nd century BC) included 1020 stars and was used to assemble Ptolemys star catalogue. [11] Hipparchus is known for the discovery of the first recorded nova (new star). [12] Many of the constellations and star names in use today derive from Greek astronomy. In spite of the apparent immutability of the heavens, Chinese astronomers were aware that new stars could appear. [13] In 185 AD, they were the first to observe and write about a supernova, now known as the SN 185. The brightest stellar event in recorded history was the SN 1006 supernova, which was observed in 1006 and written about by the Egyptian astronomer Ali ibn Ridwan and several Chinese astronomers. [15] The SN 1054 supernova, which gave birth to the Crab Nebula, was also observed by Chinese and Islamic astronomers. [16][17][18] Medieval Islamic astronomers gave Arabic names to many stars that are still used today, and they invented numerous astronomical instruments that could compute the positions of the stars. They built the first large observatory research institutes, mainly for the purpose of producing Zij star catalogues. Among these, the Book of Fixed Stars (964) was written by the Persian astronomer Abd al-Rahman al-Sufi, who observed a number of stars, star clusters (including the Omicron Velorum and Brocchis Clusters) and galaxies (including the Andromeda Galaxy). [20] According to A. Zahoor, in the 11th century, the Persian polymath scholar Abu Rayhan Biruni described the Milky Way galaxy as a multitude of fragments having the properties of nebulous stars, and also gave the latitudes of various stars during a lunar eclipse in 1019. According to Josep Puig, the Andalusian astronomer Ibn Bajjah proposed that the Milky Way was made up of many stars which almost touched one another and appeared to be a continuous image due to the effect of refraction from sublunary material, citing his observation of the conjunction of Jupiter and Mars on 500 AH (1106/1107 AD) as evidence. [22] Early European astronomers such as Tycho Brahe identified new stars in the night sky (later termed novae), suggesting that the heavens were not immutable. In 1584 Giordano Bruno suggested that the stars were like the Sun, and may have other planets, possibly even Earth-like, in orbit around them,[23] an idea that had been suggested earlier by the ancient Greek philosophers, Democritus and Epicurus,[24] and by medieval Islamic cosmologists[25] such as Fakhr al-Din al-Razi. [26] By the following century, the idea of the stars being the same as the Sun was reaching a consensus among astronomers. To explain why these stars exerted no net gravitational pull on the Solar System, Isaac Newton suggested that the stars were equally distributed in every direction, an idea prompted by the theologian Richard Bentley. [27] The Italian astronomer Geminiano Montanari recorded observing variations in luminosity of the star Algol in 1667. Edmond Halley published the first measurements of the proper motion of a pair of nearby fixed stars, demonstrating that they had changed positions from the time of the ancient Greek astronomers Ptolemy and Hipparchus. [23] William Herschel was the first astronomer to attempt to determine the distribution of stars in the sky. During the 1780s, he performed a series of gauges in 600 directions, and counted the stars observed along each line of sight. From this he deduced that the number of stars steadily increased toward one side of the sky, in the direction of the Milky Way core. His son John Herschel repeated this study in the southern hemisphere and found a corresponding increase in the same direction. [28] In addition to his other accomplishments, William Herschel is also noted for his discovery that some stars do not merely lie along the same line of sight, but are also physical companions that form binary star systems. The science of stellar spectroscopy was pioneered by Joseph von Fraunhofer and Angelo Secchi. By comparing the spectra of stars such as Sirius to the Sun, they found differences in the strength and number of their absorption lines—the dark lines in a stellar spectra due to the absorption of specific frequencies by the atmosphere. In 1865 Secchi began classifying stars into spectral types. [29] However, the modern version of the stellar classification scheme was developed by Annie J. Cannon during the 1900s. Alpha Centauri A and B over limb of Saturn The first direct measurement of the distance to a star (61 Cygni at 11. 4 light-years) was made in 1838 by Friedrich Bessel using the parallax technique. Parallax measurements demonstrated the vast separation of the stars in the heavens. [23] Observation of double stars gained increasing importance during the 19th century. In 1834, Friedrich Bessel observed changes in the proper motion of the star Sirius, and inferred a hidden companion. Edward Pickering discovered the first spectroscopic binary in 1899 when he observed the periodic splitting of the spectral lines of the star Mizar in a 104-day period. Detailed observations of many binary star systems were collected by astronomers such as William Struve and S. W. Burnham, allowing the masses of stars to be determined from computation of  the orbital elements. The first solution to the problem of deriving an orbit of binary stars from telescope observations was made by Felix Savary in 1827. [30] The twentieth century saw increasingly rapid advances in the scientific study of stars. The photograph became a valuable astronomical tool. Karl Schwarzschild discovered that the color of a s tar, and hence its temperature, could be determined by comparing the visual magnitude against the photographic magnitude. The development of the photoelectric photometer allowed very precise measurements of magnitude at multiple wavelength intervals. In 1921 Albert A. Michelson made the first measurements of a stellar diameter using an interferometer on the Hooker telescope. [31] Important theoretical work on the physical structure of stars occurred during the first decades of the twentieth century. In 1913, the Hertzsprung-Russell diagram was developed, propelling the astrophysical study of stars. Successful models were developed to explain the interiors of stars and stellar evolution. Cecilia Payne-Gaposchkin first proposed that stars were made primarily of hydrogen and helium in her 1925 PhD thesis. The spectra of stars were further understood through advances in quantum physics. This allowed the chemical composition of the stellar atmosphere to be determined. [33] With the exception of supernovae, individual stars have primarily been observed in our Local Group of galaxies,[34] and especially in the visible part of the Milky Way (as demonstrated by the detailed star catalogues available for our galaxy). [35] But some stars have been observed in the M100 galaxy of the Virgo Cluster, about 100 million light years from the Earth.

Youth Then Now Essay Example For Students

Youth : Then Now Essay The spirit of youth has changed dramatically since the days ofJoseph Conrad and his story, Youth. Conrad strongly emphasises thedesire and strong will of the young crewmen. Whereas, todays youth donot posses he drive and motivation of their ancestors. All in all, itis clear through the passing time, attitudes have changed. 1 O Youth! The strength of it, the faith of it, the imaginationof it! Conrads example of youth powerfully describes the greatness ofit all. Marlow and the other young crewmen possessed this quality ofyouth and powerfully exemplified it on the treacherous voyage of the Judea. The youth of today, as many feel, do not have the strong characteristics ofpast generations. One hundred years ago, a young man may have gone on adangerous voyage like Marlow, but a young man today leads a more secure,cushioned life. We will write a custom essay on Youth : Then Now specifically for you for only $16.38 $13.9/page Order now The changes in attitudes over time may be due to the fact thattodays generations do not have nearly as many hardships as in the past. With all the technology and scientific breakthroughs, have it easy. To conquer a problem in a modern lifestyle today, is to have a steadysource of income. In retrospect, todays youth benefit much greater thanthe youth of the past. Although the youth of the past benefit in the factthat they accomplished thier goals, and have many special memories toreflect on, as Marlow did. 1. Joseph Conrad, Youth, Story and StructureLaurence Perrine (ed) (Toronto, Harcourt Brace, 1966)p. 14BibliographyConrad, JosephYouth Story and Structure. Perrine, Laurence. Toronto. Harcourt, Brace World, Inc. 1966

Political Aspects of the Classical Age of Greece

Political Aspects of the Classical Age of Greece This is a brief introduction to the Classical Age in Greece, a period that followed the Archaic Age and lasted through the creation of a Greek empire, by Alexander the Great. The Classical Age was characterized by most of the cultural wonders that we associate with ancient Greece. It corresponds with the period of the height of democracy, the flowering of Greek tragedy, and the architectural marvels at Athens. The Classical Age of Greece begins either with with the fall of the Athenian tyrant Hippias, son of Peisistratos/Pisistratus, in 510 B.C., or the Persian Wars, which the Greeks fought against the Persians in Greece and Asia Minor from 490-479 B.C. When you think of the movie 300, youre thinking of one of the battles fought during the Persian Wars. Solon, Peisistratus, Cleisthenes, and the Rise of Democracy When the Greeks adopted democracy it wasnt an overnight affair or a question of throwing out monarchs. The process developed and changed over time. The Classical Age of Greece ends with the death of Alexander the Great in 323 B.C. Besides war and conquest, in the Classical period, the Greeks produced great literature, poetry, philosophy, drama, and art. This was the time when the genre of history was first established. It also produced the institution we know of as Athenian democracy. Alexander the Great Profile The Macedonians Philip and Alexander put an end to the power of the individual city-states at the same time they spread the culture of the Greeks all the way to the Indian Sea. Rise of Democracy One unique contribution of the Greeks, democracy lasted beyond the Classical period and had its roots in the earlier time, but it still characterized the Classical age. During the era before the Classical Age, in what is sometimes called the Archaic Age, Athens and Sparta had followed different paths. Sparta had two kings and an oligarchic government while Athens had instituted democracy. Etymology of Oligarchy oligos few arche rule Etymology of Democracy demos the people of a country krateo rule A Spartan woman had the right to own property, whereas, in Athens, she had few freedoms. In Sparta, men and women served the state; in Athens, they served the Oikos household/family. Etymology of Economy Economy oikos home nomos custom, usage, ordinance Men were trained in Sparta to be laconic warriors and in Athens to be public speakers. Persian Wars Despite an almost endless series of differences, the Hellenes from Sparta, Athens, and elsewhere fought together against the monarchical Persian Empire. In 479 they repelled the numerically mightier Persian force from the Greek mainland. Peloponnesian and Delian Alliances For the next few decades after the end of the Persian Wars, relations between the 2 major poleis city-states deteriorated. The Spartans, who had earlier been the unquestioned leaders of the Greeks, suspected Athens (a new naval power) of trying to take control of all of Greece. Most of the poleis on the Peloponnese allied with Sparta. Athens was at the head of the poleis in the Delian League. Its members were along the coast of the Aegean Sea and on islands in it. The Delian League initially had been formed against the Persian Empire, but finding it lucrative, Athens transformed it into its own empire. Pericles, the foremost statesman of Athens from 461-429, introduced payment for public offices so more of the population than just the rich could hold them. Pericles initiated the building of the Parthenon, which was supervised by the famed Athenian sculptor Pheidias. Drama and philosophy flourished. Peloponnesian War and Its Aftermath Tensions between the Peloponnesian and Delian alliances mounted. The Peloponnesian War broke out in 431 and lasted for 27 years. Pericles, along with many others, died of plague early in the war. Even after the end of the Peloponnesian War, which Athens lost, Thebes, Sparta, and Athens continued to take turns as the dominant Greek power. Instead of one of them becoming the clear leader, they dissipated their strength and fell prey to the empire-building Macedonian king Phillip II and his son Alexander the Great. Historians of the Archaic and Classical Period HerodotusPlutarchStraboPausaniasThucydidesDiodorus SiculusXenophonDemosthenesAeschinesNeposJustin Historians of the Period When Greece Was Dominated by the Macedonians DiodorusJustinThucydidesArrian fragments of Arrian found in PhotiusDemosthenesAeschinesPlutarch

The List of All U.S. Colleges With a Music Major

Studying music allows one to engage with the subtle intersections of mathematics, theory, artistic expression, and material technique. If you’re thinking about pursuing your interest in music through your major, we’ve put together this post to offer some information on potential career paths as well as a comprehensive list of which schools may offer programs that fit your aspirations. For students interested in studying music in college, there are generally two paths: the music conservatory or the music major at a traditional higher-education institution. If you’re set on the pursuit of a path in performance or composition, then the more rigorous and specialized path of a conservatory is for you. However, for many students, the opportunity to couple music with other disciplines is enticing. In these cases, a more traditional institution has its merits. Music majors can double-major or pursue a minor to build up skills and experiences in two fields that complement each other. Popular subjects studied in conjunction with music include communications, psychology, business, and technology. Music programs themselves are usually well-balanced between scholarship and performance, emphasizing both practice and theory, as well as a good understanding of music history. In addition to the technical skills you gain in performance, composition, and music theory, you will come out of college with many transferable and in-demand skills, such as innovative thinking, communication and collaboration, and the ability to articulate meaning. Music majors often drawn upon their experiences and skills from their other courses when stepping into the job market. It’s useful to note that except for a few specialized, professional majors, it’s normal for a student’s eventual career to be unrelated to their undergraduate degree. That being said, music majors will find a plethora of related opportunities in the job market. Careers in music therapy, music education, and game design are directly related to undergraduate studies in music. One degree removed, careers in arts administration, app development, recording engineering, and music law also have high demand for music majors and are lucrative paths to take. Whether you’re planning on studying music or physics at college, a strong and dedicated application—with emphasis on a promising academic record—is just as important as your musical accomplishments. Colleges want to know that you will be able to excel not only in your program, but as a general student at their institution. Show your passion for music through you extracurriculars. Take music classes in high school; join a band or orchestra; participate in recitals or competitions. Start researching which schools have music programs, and begin narrowing down from there. Then you can put together your school list. Many students need help when putting together their college lists and then their applications. It’s a lot of work, and even more so if you need to tailor your profile to schools as a potential music student. can help you apply to your dream school no matter what point in high school you are at. If you’re still in your first two years of high school, our    Early Advising Program will help you build a strong extracurricular and academic base to prepare you for the college application process. We’ll guide you in choosing the right classes and extracurricular activities and how to draw on your strengths to optimize your profile in advance. If you’re a junior, our College Strategy Program will help you improve your admissions chances by strengthening your extracurricular profile, setting goals with you, developing a college list, and making school-specific adjustments to increase your chances at your dream schools. Estimating your chance of getting into a college is not easy in today’s competitive environment. Thankfully, with our state-of-the-art software and data, we can analyze your academic and extracurricular profile and estimate your chances. Our profile analysis tool can also help you identify the improvement you need to make to enter your dream school. Anderson University (South Carolina) Arkansas State University | A–State Austin Peay State University | APSU California State University, East Bay | CSU East Bay Bowling Green State University | BGSU C.W. Post Campus of Long Island University | LIU Post California Baptist University | CBU California Institute of the Arts | Cal Arts California Lutheran University | CLU California Polytechnic State University | Cal Poly California State Polytechnic University, Pomona | Cal Poly Pomona California State University Channel Islands | CSU Channel Islands California State University San Marcos | CSUSM California State University, Bakersfield | CSU Bakersfield California State University, Chico | CSU Chico California State University, Dominguez Hills | CSUDH California State University, Fresno | CSU Fresno California State University, Fullerton | CSU Fullerton California State University, Long Beach | Long Beach State California State University, Los Angeles | Cal State LA California State University, Monterey Bay | CSUMB California State University, Northridge | CSUN California State University, Sacramento | Sacramento State California State University, San Bernardino | CSUSB California State University, Stanislaus | Stanislaus State Catholic University of America | CUA Central Christian College of Kansas Central Connecticut State University | CCSU Central Washington University | CWU Delaware State University | Del State Charleston Southern University | CSU Christopher Newport University | CNU Eastern Washington University | EWU Coastal Carolina University | Coastal College of Staten Island | CUNY CSI College of the Holy Cross | Holy Cross College of William & Mary | William & Mary Colorado Christian University | CCU Colorado State University–Pueblo | CSU Pueblo Columbia International University | CIU Concordia University Wisconsin | CUW Massachusetts Institute of Technology | MIT East Texas Baptist University | ETBU Eastern Connecticut State University | ECSU Eastern New Mexico University | ENMU North Carolina Central University | NCCU Elizabeth City State University | ECSU North Dakota State University | NDSU Fayetteville State University | FSU Florida Gulf Coast University | FGCU Florida International University | FIU Fort Valley State University | FVSU Franciscan University of Steubenville Franklin and Marshall College | F&M Georgia Institute of Technology | Georgia Tech Georgia Southwestern State University | GSW Northwest Missouri State University Grand Valley State University | GVSU Hannibal–LaGrange University | HLGU Hobart and William Smith Colleges | HWS Pennsylvania State University | PSU Indiana University – Purdue University Indianapolis | IUPUI Indiana University Bloomington | Indiana Indiana University of Pennsylvania | IUP Indiana University South Bend | IU South Bend Indiana University Southeast | IU Southeast Jacksonville State University | JSU Kutztown University of Pennsylvania | KU Lock Haven University of Pennsylvania | LHU Los Angeles College of Music | LACM Louisiana Tech University | La. Tech Mansfield University of Pennsylvania State University of New York at Potsdam | SUNY Potsdam Stephen F. Austin State University | SFA Metropolitan State University of Denver | MSU Denver MidAmerica Nazarene University | MNU Middle Tennessee State University | MTSU Millersville University of Pennsylvania | MU Tennessee Technological University | Tennessee Tech Minnesota State University Moorhead | MSUM Minnesota State University, Mankato | MNSU Mississippi University for Women | MUW Mississippi Valley State University | MVSU Montana State University Billings | MSU Billings University of California, Berkeley | UC Berkeley University of California, Davis | UC Davis Mount Vernon Nazarene University | MVNU University of California, Irvine | UC Irvine New Mexico Highlands University | NMHU New Mexico Institute of Mining and Technology | New Mexico Tech New York City College of Technology | CUNY City Tech North Carolina A&T State University | N.C. A&T University of California, San Diego | UCSD North Carolina State University | NC State Northeastern Illinois University | NEIU Northeastern State University | NSU Northwest Christian University | NCU Northwest Florida State College | NWFSC University of Massachusetts Dartmouth | UMass Dartmouth Northwest Nazarene University | NNU Northwestern Oklahoma State University | NWOSU Oklahoma Panhandle State University | OPSU Oklahoma Wesleyan University | OKWU Oregon Institute of Technology | Oregon Tech Our Lady of the Lake University | OLLU Palm Beach Atlantic University | PBA Point Loma Nazarene University | PLNU Prairie View A&M University | PVAMU Queens College, City University of New York | CUNY QC Ramapo College of New Jersey | RCNJ Rensselaer Polytechnic Institute | RPI University of Wisconsin–River Falls | UW–River Falls Rutgers University–New Brunswick | Rutgers Saginaw Valley State University | SVSU Saint Martin’s University | St. Martin’s Saint Mary-of-the-Woods College | SMWC Saint Mary’s College of California | St. Mary’s Saint Mary’s University of Minnesota | SMU Sam Houston State University | SHSU San Francisco State University | SF State School of the Art Institute of Chicago | SAIC Sewanee: The University of the South | Sewanee Shippensburg University of Pennsylvania Slippery Rock University of Pennsylvania | SRU South Carolina State University | SCSU Southeast Missouri State University | SEMO Southeastern Oklahoma State University | SOSU Southern Connecticut State University | SCSU Southern Illinois University Carbondale | SIU Southern Illinois University Edwardsville | SIUE Southern Methodist University | SMU Southern New Hampshire University | SNHU Southern University and A&M College | SUBR Southwest Minnesota State University | SMSU Southwestern Assemblies of God University | SAGU Southwestern Christian College | SwCC Southwestern Oklahoma State University | SWOSU St. John’s College | SJC (New Mexico) State University of New York at Fredonia | SUNY 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UAM University of Arkansas at Pine Bluff | UAPB University of Arkansas–Fort Smith | UAFS University of California, Los Angeles | UCLA University of California, Riverside | UC Riverside University of California, Santa Barbara | UCSB University of California, Santa Cruz | UCSC University of Central Arkansas | UCA University of Central Florida | UCF University of Central Missouri | UCM University of Central Oklahoma | UCO University of Colorado Boulder | CU Boulder University of Colorado Denver | CU Denver University of Hawaii at Manoa | UH Manoa University of Illinois at Chicago | UIC University of Illinois at Urbana–Champaign | UIUC University of Louisiana at Lafayette | UL Lafayette University of Louisiana at Monroe | ULM University of Maine at Augusta | UMA University of Maine at Farmington | UMF University of Mary Hardin–Baylor | UMHB University of Mary Washington | UMW University of Maryland Eastern Shore | UMES University of Maryland, Baltimore County | UMBC University of Maryland, 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How has the UK retail sector adapted to recent changes in the economic Literature review

How has the UK retail sector adapted to recent changes in the economic climate effectively - Literature review Example The Global Financial Crisis had a profound impact on almost all parts of the world. Millions of people around the world had to change their lifestyles, many financial institutions went bankrupt, thousands of employees lost their jobs, many people ended up living on the streets, governments in most part of world had to interfere, with bail out plans regardless of the fact that how capitalistic and free market their economy was, to save their institutions. Many countries, which were climbing up the ladder of economic growth, witnessed decline in growth rates and worse, many western countries ended up posing shrinking of the economy. Stock markets in all around the world crashed very badly. The Gross Domestic Product of the world economy was 61.38 Trillion US dollars in the year 2008, which fell down to the level of 58.26 trillion in the year 2009. The trend also continued in the year 2010, however, there are no authentic figures released for the same yet (Buckley, pp. 201-203, 2011; Un ited States Financial Crisis Inquiry Commission, pp. 28-30, 2011). Most the countries, specifically the United States government turned towards the Keynesian school of thought of overcoming an economic recession. John Maynard Keynes, who became prominent in the United States and Europe during the great depression, strongly believed that there is no invisible hand in the economy, which causes business troughs and peaks. If an economy wants to move upwards in the business cycle then the economy will have to increase its aggregate demand, which is the sum of consumption, investment, government spending and net exports (exports minus imports). Higher aggregate demand would force the economy to move towards an upward spiral of growth and thus pushing the economy towards a boom. In hope of stimulating the economy with fiscal packages, the US government announced bailout packages of worth more than one trillion US dollars to help the economy to recover (Carpenter, Sanders & Harling, pp. 3148-352, 2011). The UK government also injected money into the econo my in various fashions to help solve the liquidity crisis. The United States injected money into various corporations such Fannie Mae and Freddie Mac,