Wednesday, November 27, 2019

Mary Whiton Calkins Essays - American Psychologists,

Mary Whiton Calkins INTRODUCTION Mary Whiton Calkins, is best known for two things: becoming the first woman president of The American Psychological Association and being denied her doctorate from Harvard. However, these two aspects only make up a small portion of what she accomplished in her life. Her entire life was dedicated to her work, especially the development of her Psychology of selves. She founded an early psychology laboratory and invented the paired-associate technique. She passionately dove into the new field of Psychology but also was highly active in the field of Philosophy. She was not deterred by being a woman and used her struggles to gain a voice to speak out against women's oppression. (5) EARLY LIFE Mary Whiton Calkins was born on March 30, 1863 in Buffalo, New York. Her father was Wolcott Calkins and a Presbyterian minister. She was from a close knit family, especially to her mother, and the eldest of five children. In 1880, when she was seventeen, she moved to Newton, Massachusetts where her family built a home that she lived in the rest of her life. Her father, knowing the education that women received, decided to design and supervise Mary's education. This enabled her to enter Smith College in 1882 with advanced standing as a sophomore. However, in 1893, an experience that permanently influenced her thinking and character, was the death of her sister, Maude. The following academic year she stayed home and took private lessons. She reentered Smith College in the fall of 1884 as a senior and graduated with a concentration in classics and philosophy (7). In 1886 her family went to Europe for sixteen months. This is where she broadened her knowledge of the classics. Upon returning to Massachusetts her father arranged an interview for Mary with the President of Wellesley College, a liberal arts college for women that was a few miles from their home. She was offered a position there as a tutor in Greek and began teaching in the fall of 1887. Mary remained in the Greek Department for three years. However, a professor in the Department of Philosophy noticed her talent of teaching. He discussed with Mary the position needed to teach the new field of Psychology, which was still a sub-discipline of Philosophy. Due to the scarcity of women in that area, it made it realistic to see her potential and offer her the position. EDUCATIONAL SETBACKS The only requirement that the professor had, was that Calkins study for one year in a Psychology program. However, she faced two problems meeting this condition. The first, being that there were few psychology departments in 1890. Secondly, getting admitted to these places that did offer the program was highly unlikely since she was a woman. Her first consideration was to study abroad. An instructor at Smith told her that her best chance was to try obtaining private instruction in psychology and philosophy at any of the German universities outside of Zurich (6). However, another instructor told her that would be a good idea if ladies had been allowed the same privileges as men (6). Calkins formally dismissed going to Germany when she received a letter from a woman student attending the University of Gottingen which stated, I wish I might encourage you; but past experience has proved to me the utter uselessness of trying to enlighten the authorities, at least, in our generation. Once Calkins started looking at the United States, she discovered that the University of Michigan, where she would be studying under John Dewey, and Yale, where she would be studying under G.T. Ladd, were promising. However, she received a letter from another woman student that dissuaded her. The letter stated, Personally, I should be immensely glad if you would come. We might be able to get some delightful work together...By the way Prof. Ladd thinks you ought to have some lady with you at the lectures. If there were only one or two other girls who would come to join us, we could get a tremendous amount...(4). She decided against both universities, most likely because they were further away from home that she would like and they did not have a psychological laboratory. However, one of the few universities that did have a

Sunday, November 24, 2019

Big Bills Battle essays

Big Bills Battle essays Big Bills Battle Gwynne McCauley November 14, 2001 English 3-W Big Bill Haywood (1869-1928) was one of the most radical, determined, and influential labor leaders of his time. He was sent by his mother to work in the mines at the mere age of nine, and thus started his life-long battle for the rights of miners. Haywood supported and donated his time and effort to many labor groups. Big Bill founded a chapter of the W.F.M (Western Federation of Miners) and later founded the largest union, the I.W.W (Industrial Workers of the World). He endured many hardships that came with his demanding covenant, jail time, death threats, and the continuous battles between the Pinkerton Detective Agency and the workers on strike. Nevertheless, he had a blind ambition to change the world of labor unions, and that he did. Mining was a profession that was very popular in the late 1800s through the middle 1900s. It was a tough job with many serious injuries; little notice was taken of these injuries. Every year hundreds of men lost their lives to the dangerous work of mining. These deaths and injuries were not fussed over in any way; the risk came with the job. There were many who objected to this cold, un-feeling attitude, not to mention the lack of health care or safety precautions. Others took it as a fact and went on, some claimed to have no opinion, hoping that someday an organization would rise up and change the harsh conditions of mining work. The process of ga...

Thursday, November 21, 2019

Dream of red chambers (chinese culyures and history ) Coursework

Dream of red chambers (chinese culyures and history ) - Coursework Example Chia Lan’s success was evident but Pao-Yu’s changed attitude towards studies was very curious in nature. This was displayed in his result when he stood seventh and Chia Lan ranked one hundred and thirteenth. After the exam, Pao-Yu disappeared from the gate of the examination hall and his feeling of non-attachment from the worldly duties and affairs and from all materialist attractions diminished. This became more obvious before his departure, he said to Precious Virtue: â€Å"Chieh-chieh, I am going now. You can wait with Tai-tai for the good tidings†.  And to his mother, Madame Wang he said, â€Å"I shall never be able to repay Tai-tais kindness to me but I shall try my best at the Examinations and earn the degree. Perhaps this will make Tai-tai happy and in a way atone for my past unworthiness."   Chia Cheng adhered to the teachings of Confucian canon and governed his life following those teachings. For him the sincerity lies in the mourning and true emotion and not in pompous and expensive ceremonies. Despite all the objections and criticisms, Chia Cheng abandoned the place of mourning and left the arrangement for the rituals on the hand of other people. And the impact the rituals had on the lives and minds of the subject and people around Chia Cheng can be well demonstrated from the sayings of Phoenix, â€Å"Lao Tai-tai was never extravagant in her life†. And also commented, â€Å"I do not understand what Lao-yeh meant about the sincerity of mourning and the teachings of the sages but I know that Lao Tai-tai used to love Nai-nai and myself and was kinder to us than the rest, and that I for one will be ashamed to face her in after ¬ life if her funeral is skimped. So I implore Nai-nai to spare no expense. Lao Tai-tai provided for this herself†. The success of Pao-yu and Chia Lan were also for their relation with Imperial Concubine. Emperor granted pardon to Chia Sheh and Chia Gen by restoring their title and property. The emperor also

Wednesday, November 20, 2019

Managerial economics and strategic analysis Essay

Managerial economics and strategic analysis - Essay Example Hays (2004) estimates that about 70 % of the sales volume for the Company comes from outside the United States and about 80% of the profits comes from non American countries. Coca cola Company is therefore one of the Companies with most presence in the world, which is attributed to the fact that the soft drink; Coca Cola is widely available globally and has become the world’s favorite soft drink (Hays, 2004). According to Dess (2012), the successful implementation of a Company’s strategy requires effective strategic control. Control is in the form of behavior and how information is used. In order to cater for the interests of the two key players in a Company, that is the shareholders and the managers, a Company must ensure that these interests are aligned (Dess, 2012). This can be achieved through establishing corporate governance. Globally, the soft drink market is dominated by three Companies; the Coca Cola, Cadbury’s Schweppes and Pepsi Cola Companies. Coca Cola laid claim to about 47% of the global market with Pepsi Cola following at 21 % and Schweppes at 8%. In aligning the interests of the Company shareholders and managers, Coca Cola separated the Company separated it’s ownership from its control. This was made possible through the employment of managers to run the Company on behalf of the owners. The company employs the use of incentives intended for its managers to facilitate the achievement of the Company’s goals. The control of governance mechanisms has been successfully achieved through the use of external auditors who check the Company books regularly to ensure that the financial information disclosed by the Managers is accurate and in doing so; protect the owners from financial risks (Dess, 2012). The Company is also subject to external regulatory bodies that check for the quality of their product and control the standards of these products. These bodies ensure that the consumer gets a product that fits their needs

Sunday, November 17, 2019

Marketing 4580 International Transportation Essay

Marketing 4580 International Transportation - Essay Example The current office automation systems improve on the limited capabilities of the early year’s soft ware packages. As technology improves further, managers and other members of staff analyze issues that have traditionally been solved by specially designed computer programs. Hence, the classic issue of transportation cost minimization at a minimum transportation cost is addressed (Murphy & Wood, 2010). Communication systems are another example of information systems that could be utilised. It is obvious that communication is an important component of any organisation (Murphy & Wood, 2010). Hence, communication systems help various organisational stakeholders work together by interacting and sharing information in many different forms. With regard to logistics, the importance of well-defined and well-executed communication systems was most appreciated by companies that use or provide airfreight services after the events of 9/11 terrorist attack (Murphy & Wood, 2010). As such, communication systems played a crucial role for airfreight providers. With current advancement in telecommunication technology, new technology is replacing old methods of communication. Case in point, wireless communication is the new yardstick that is replacing the honoured Electronic data interchange (EDI) (Murphy & Wood, 2010). On the other hand, the most commonly used type of wireless system, the global po sitioning systems (GPS), has become quite valuable to the transportation component of logistics due to high fuel costs and the relentless pressure to improve efficiency and productivity. These issues have since been resolved by the GPS system (Murphy & Wood, 2010). Other important systems are the Management Information System (MIS) and Executive Information System (EIS). These systems convert data into information. This information monitors the performance and the management structure in an organization. In this

Friday, November 15, 2019

Evidence and Theories of Supermassive Black Holes

Evidence and Theories of Supermassive Black Holes Supermassive Black Holes are at the centres of galaxies: The evidence for their existence and the theories for their formation and effect on the evolution of galaxies. Supermassive Black Holes are an area of astronomy that have been significantly studied and with thanks to the advance in technology, scientists have managed to better understand how they are formed and the impact they have on the evolution of galaxies. It is first wise to look at the definition of what a black hole is compared to a Supermassive Black Holes. NASAs World Book (2004) defines a black hole as a region of space whose gravitational force is so strong that nothing can escape from it. Scientists believe that a Supermassive Black Hole have the same characteristics as a black hole, with the main difference being, as the name Supermassive suggests, the size of the black hole. Many astronomers and scientists believe that a Supermassive Black Hole is the largest variety of black hole within a galaxy. What most have also believed is that as well as being the largest type of black hole, these Supermassive Black Holes can be found at the centre of galaxies. This essay will therefore look at the evidence for the existence of these Supermassive Black Holes, as well as theories for their formation and the effect they have on the evolution of galaxies. Firstly we should look at the evidence that suggests these Supermassive Black Holes exist at the centre of galaxies. Astronomers and scientists at first found it difficult to prove that black holes do exist in our galaxies. In 1916, Albert Einstein, one of the most well known physicists created his General Relativity theory. Although his theory was first published in 1916, it could be seen to indicate there could be objects in space in which his theory applies to. The theory of Einstein would suggest that there could be an object that alters both space and time, so much so that not even light can escape from it. This is what many modern scientists believe that a black hole is. Many scientists believe that the gravitational force that comes from these black holes is far too strong for anything to escape its pull, including light, which would then explain how these black holes appear invisible. To help prove the existence of this invisible force therefore, Theodore P. Snow (1991, p.514 ) suggests that the best chance of detecting a black holeis to look for an invisible object whose mass is too great to be anything else. Scientists have therefore looked at the movement of stars around this invisible object in several different galaxies, and thanks to these measurements in 1914 the Hubble Space Telescope (2003,p.198) managed to determine the mass of the object to be several million times the size of the sun was present in the stars orbit. Scientists and astronomers believe that the only object that could have this effect on the stars orbit and have as high a mass would have to be a Supermassive Black Hole. The Telegraph in December 2008, reported that a group of scientists had spent the last 16 years studying whether there was a Supermassive Black Hole at the centre of our galaxy, in the Milky Way. As before they studied the stars orbit circling the invisible object and found that the mass seems to be about four millions times the size of the sun. This would therefo re suggest that Supermassive Black Holes are at the centre of galaxies, including our own. Astronomers and Scientists therefore believe that if you measure the mass of a dark object and that it has a high mass in a small area of space it is most probably a Supermassive Black Hole. Once scientists and astronomers had seemed to provide substantial evidence to the existence of these Supermassive Black Holes, they did not stop their research in this area. Many sceptics believed that if these objects existed in our galaxy how did they appear? Thus scientists and astronomers continued to research Supermassive Black Holes and how they have been formed. Kuhn and Koupelis (2001, p.496) state that astronomers predicted the existence of black holes in the 1930s when they realized that a stars mass may cause it to collapse beyond neutron degeneracy. This is an explanation for how black holes are formed, however the majority of astronomers and scientists believe there could be more than one explanation for how Supermassive Black Holes are formed. One model that scientists believe could explain the formation of these objects in our galaxy is looking at the early years of the stars. This model looks at how the first stars were formed without a suitable make-up which could ha ve resulted in them leaving behind what is known as black hole seeds. The idea that black holes have been formed by these seeds has been studied in recent years with Volonteri, Haardt Madau (2003) believed that these black holes may have stemmed from seeds of the early stars, meaning Supermassive Black Holes could be millions of years old, which could explain how they are at the centre of our galaxies. Another model that looks to describe the formation of these Supermassive Black Holes is the idea that they are in fact formed due to the collapse of a large gas clouds. These large gas clouds would collapse into a rotating neutron star of an extremely high mass, this star would be unstable due it not containing the correct electron make-up and instead of a supernova explosion it would result in a Supermassive Black Hole as being its only remaining by-product. Haehnelt Rees (1993) studied this idea that the Supermassive Black Holes were formed due to the collapse of large gas clouds and have suggested that this model helps give a more modern understanding of how black holes are formed. Another model which has been suggested by a minority of researchers is the idea that Supermassive Black Holes are a by-product of the beginning of the galaxy, the Big Bang. These scientists believe that after the Big Bang, the pressure of the newly formed galaxy would be extremely high, so much so, that it could have resulted in areas of high density that would have formed black holes. They suggest that many of these black holes would not have lasted a long period of time as the galaxy was expanding, however some may still exist to this present day. According to J.PLuminet (1992, p.177) if this is the case, the galaxy would expand around the black hole leaving it and the centre of the galaxy. With researchers now able to provide evidence that Supermassive Black Holes do exist at the centre of our galaxies and being able to give various substantial evidence on the formation of these black holes, astronomers and scientists have also looked to explain how they have an effect on the evolution of galaxies. As we have seen, many researchers believe that there are Supermassive Black Holes at the centre of the galaxies. Researchers believe that roughly ten percent of the black holes contain high levels of ionised gas, which is released in opposite directions of the black hole. This is most likely to be released as kinetic energy. Astronomers believe that this would have an effect on how stars behave and play a vital role in the evolution of galaxies within the universe. For many years astronomers and scientists have been able to find a correlation between the mass of the Supermassive Black Holes and the galaxy it inhabits. In other words, many researchers believe that the size of the black hole does have an effect on the mass of that galaxy. More recently however researchers have managed to acquire some knowledge on how else a Supermassive Black Hole has an impact on its galaxy. Scientists have studied the spin of the black holes, as they believe this could result in the ionised gas being released from the black hole, which would then in turn control the growth of the galaxy it is at the centre of. Another way that these Supermassive Black Holes could have an impact on the evolution of galaxies could be as a result of two black holes colliding. Researchers have recently discovered what will happen when two Supermassive Black Holes collide with one another. The gravitational attraction between the two is believed to upset the stars positions surrounding the galaxies centre, but many researchers did not know whether the two would attract together to form one large supermassive black hole or whether they would repel from one another? Scientists have recently b een able to answer this thanks to a collision that occurred between a large and small black hole. The results of the collision were as expected with the stars surrounding the centre being upset and altered. The question to whether they would form a larger black hole or repel was also answered, as the two became closer they repel and eject the black hole from its galaxy, sending it at high speeds across space surviving on its accretion disk alone. According to Govert Schilling (2002, p.233) many researchers believe that thanks to this phenomenon that took place, they may be able to further explain formation of galaxies and their black holes, with further research and more advances in technology scientists and astronomers will continue to study Supermassive Black Holes. As we have seen from the proposed research put forward by various astronomers and scientists, it seems more than likely that Supermassive Black Holes do exist at the centre of our galaxies. Thanks to the research, they have helped in the understanding on how they exist, as being large invisible objects with an extremely large mass and large gravitational pull that is at the centre of every galaxy. As well as this, astronomers and scientists have also been able to explain how these objects could have formed in our galaxy, by looking at different models which include dying stars being turned into black holes millions of years ago, to models which suggest they are formed due to collapsing dense gas clouds. We have also seen researchers look at the impact such objects have had in our galaxies, and seen suggestions that these Supermassive Black Holes helped to create the way a galaxy looks, such as its stars positions and the galaxies mass. With further research and more advances in techn ology, the future could see more results into this area of astronomy, with researchers looking at a clearer definition to how these Supermassive Black Holes are formed and what effect they have on the evolution of the galaxies they inhabit. References Alleyne ,R. Proof that Albert Einsteins black holes do exist, claim scientists 2008, Telegraph, http://www.telegraph.co.uk/science/science-news/3690822/Proof-that-Albert-Einsteins-black-holes-do-exist-claim-scientists.html Haehnelt M. G., Rees M. J., 1993, MNRAS, 263, 168 Kuhn, K.F, Koupelis, T. (2001) In Quest of the Universe., 3rd Ed. Jones and Bartlett Publishers Inc, London. Livio. M, Noll. K, Stiavelli, M. (2003) A Decade of Hubble Space Telescope Science, Cambridge University Press, Cambridge U.K Luminet, J.P. (1992) Black Holes Cambridge University Press, New York McClintock, Jeffrey E. Black hole. World Book Online Reference Center. 2004. World Book, Inc. http://www.worldbookonline.com/wb/Article?id=ar062594. Schilling, G. (2002) Flash! The Hunt for the Biggest Explosions in the Universe. Cambridge University Press, United Kingdom Snow, T.P (1991) The Dynamic Universe: An Introduction to Astronomy, 4th Ed. West Publishing Company, St. Paul Volonteri M., Haardt F., Madau P., 2003, ApJ, 582, 559 Zeilik, M. (2002) Astronomy, The Evolving Universe 9th Edition, PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE, Cambridge, United Kingdom. Craig Jonathan Muir Matriculation: 200804070 1

Tuesday, November 12, 2019

Busl250 – Mid Semester Notes

BUSL250 – Mid-semester Notes Liabilities * Harm may be caused deliberately or carelessly * One person’s single harmful act to another person (deliberately or carelessly) can give rise to one or more legal liabilities * Legal Liabilities Tortious Liability: harmful act can be a tort (civil wrong), other than breach of contract, remedy is compensation (commenced through litigation) * Vicarious Liability: Liability for harmful act caused by another * Statutory liability: harmful act by breach of statute, prosecution is punishment * Contractual liability: harmful act by breach of contract, remedy is compensation * Criminal liability: harmful act and harmful act is a crime, incurs criminal liability, prosecution for punishment * A harmful act may incur one or more legal liabilities Tortious vs. contractual liability: tortious liability can incur in the absence of contract but contract liability can only incur if a contract exists. * Difference between tortious liability and criminal liability * Consequences of causing harm Tort of trespass * Trespass is actionable per se, which means that there is no need for the plaintiff to prove actual loss or damage in order to commence a civil action against the trespasser. It is, however, necessary to prove that the interference was either intentional or negligent. * Types of trespass You commit the tort of trespass to land if you directly and intentional interference with land in the rightful possession of X without X’s consent of other excuse. Lord Bernstein of Leigh (Baron) v Skyviews & General Ltd [1978] 1 QB 479 * * Doesn’t need to be physical trespass of airspace * A tenant in rightful possession of land has the right to sue for trespass, including the right to sue the landlord if the landlord enters the land without permission or lawful excuse. * No trespass to land if there is no attempt to make it clear that you are not welcomed to their land. i. e. mplied permission * You commit the tort o f trespass to goods if you directly and intentionally interfere with goods in the possession of X, without X’s consent or other excuse * Trespass against goods: direct and intentional interference with or use of personal property of another * Conversion: intentionally using/dealing the goods that is inconsistent with the owner or their rightful possession of the good * Dentine: committed when someone either intentionally or careless detains the goods of another. (i. e. carelessly through loosing the good not able to give back when demanded) * Trespass to persons: You commit the tort of battery if you directly, intentionally or negligently cause contact with the body of x without X’s consent. Courts established plaintiff’s not entitled to insist that no one ever touch them, and that a certain minimal level of physical contact is an unavoidable element of daily life. Rixon v Star City Pty Ltd [2001] NSWCA 265 * You commit a tort of assault if you unlawfully threat en another with imminent physical harm * You commit the tort of false imprisonment if you cause total deprivation of X’s freedom of movement without lawful justification or excuse * Defences * Accident * Consent * Necessity Self defence (usually for trespass to person) * Defence of property (usually for trespass to person) Tort of nuisance * You commit the tort of nuisance if you indirectly interfere (i. e. interfere with no actual physical contact e. g. through noise) with X’s use and enjoyment of private or public land * 2 types * Private nuisance * Public nuisance * Defences: * Consent from plaintiff (expressed or implied) * Statutory legislation * Contributory negligence Tort of defamation * You commit the tort of defamation if you publish to a third party, spoken or written form, a statement about x that would damage the reputation of X.Economic torts * Tort of deceit: a tort committed when one person makes a fraudulent misrepresentation to another * If you tell s omeone the truth then something happens that changes those facts, you must notify persons of that change or you will be charged with misrepresentation * You must know that the information you gave was false to misrepresent * No defence to expect plaintiff to check the information * Tort of passing off: a tort committed when one person misrepresents themselves or their product as having some kind of connection with another person or business.Pacific Dunlop v Hogan. * Tort of intimidation: a tort and/or crime committed when one person threatens to commit an unlawful act to force another to do something against their interest Rookes v Barnard. * Tort of interference with contractual relations: a tort committed when one person knowingly induces another to break a contract with a third party. Lumley v Wagner. *