Hrm Annotated Bibliography free essay sample

The misconceptions are replaced with evidence based strategies that show the underlying factors beyond pay compensation that drive turnover in addition the employee morale. One of the meta-analytical relationships that affect the rate of employee’s turnover includes leadership and relationships in the workplace. Another area that impacts an employee’s loyalty and turnover is the job satisfaction; however, human resource management can influence turnover through socialization of new entering employees and providing training and development opportunities that increase the desire for employees to stay with the organization. Overall, this article provides evidence based strategies that unquestionably impact employee morale and hence employee turnover. Cascio, W. F. (2012). Be a Ringmaster of Risk. HR Magazine, 57(4), 38-43. Retrieved from http://www. astd. org/Publications/Magazines/TD Cascio’s compares human resource management to the human capital risks involved in conducting business. Three types of human capital risk that will be highlighted in this research are: Strategic, Behavioral, and Skills Gaps. We will write a custom essay sample on Hrm Annotated Bibliography or any similar topic specifically for you Do Not WasteYour Time HIRE WRITER Only 13.90 / page Strategic human capital risks that are believed to have a negative impact on the leadership development because these risks often seen as poor configuration of Human Resource strategies combined with corporate strategies. Behavioral human risk impact many facets of employee morale such as human actions and tendencies that undermine change and loyalty. Skills gaps are deficits between ability of employees capabilities and business goals which can reduce the development of growth and leadership frequency and the negatively influence on organizational goals and stability. Cascio gives human resource managers techniques to minimize the human capital risks associated with dealing with each of these areas. Jusko, J. (2012). How to Develop High-Potential Employees. Industry Week/IW, 261(9), 26-29. Retrieved from http://www. industryweek. com/ Jusko informs those interested in developing high-potential employees of the basic steps to create efficient leaders. To have a successful employee development program, it is very beneficial for the upper-level management of organizations to have an extensive involvement in leadership development. The organization should also have dependable, clear-cut, high moral level culture which should look toward what skills will be needed in future occupational endeavors when reviewing current talent’s work performance. High-potential employees should be given opportunities to learn and develop skills that will be rewarding for themselves as well as the organization in the future. Motivation increases the retention of high-potential employees. Furthermore, managers of these employees should be held responsible for the development of their skills. Ketter, P. (2012). New Career Development Thinking. T+D, 66(9), 10. Retrieved from http://www. astd. org/Publications/Magazines/TD As the editor of a training and development magazine, Ketter give insight on the importance of career development and the responsibilities of training and development managers to encourage employees. Ketter gives a brief summary of how this influence impacts the future of the career ad personal growth of new and current employees within an organization. Lykins, L. (2012). Getting Results: Aligning Learnings Goals with Business Performance. T+D, 66(4), 28. Retrieved from http://www. astd. rg/Publications/Magazines/TD Lykins’ presents statistical information that shows the significance of effective learning goals being associated with the business strategy. The research that is presented shows the correlation of leaning objectives and the organizations economic success. In addition, it shows a correlation to the goals of the organization’s employees. The employees with higher optimism of the or ganizational goals tended to learn more and were deem as high-performers. Newstrom, J. W. (2007). Supervision: Managing for Results (9th ed. ). Boston: McGraw-Hill/Irwin. Newstrom gives insight on the duties of supervision in the specific area of training and developing employees. The training and developing of employees is rewarding to the employer if the training is done in a sufficient manner. There are various factors of learning and multiple training aids that are available for employees; however, it is very important that the trainee/employee has an aid that accommodates their learning style. Noe, R. A. , Hollenbeck, J. R. , Gerhart, B. , amp; Wright, P. M. (2010) Fundamentals of Human Resource Management (4th ed. ), New York, NY: McGraw-Hill/Irwin The premise of this textbook is in-depth knowledge about the structure and polices of Human Resource Management. Two areas emphasized in this research paper are training employees and job satisfaction. First, training and development is addressed because the authors of the book give insight on the stages of instructional design and the best techniques of training employees. Then, job satisfaction issues are addressed to give insight to the reasons employees are unsatisfied. In addition, the job satisfaction may lead to symptoms of job withdrawal which may lead to employee morale issues. Pace, A. (2012). The Best Keep Learning. T+D, 66(4), 22. Retrieved from http://www. astd. org/Publications/Magazines/TD In this article, research is presented that was conducted by the Institute for Corporate Productivity. This research gives insight the top five critical areas for high performing organizations. Furthermore, one of the top areas critical areas of concern is the importance of leadership development. In a human capital report comparing 2010 to 2012, high performing organizations are seven times more efficient at supervision of learning and development. In addition the organizations that are considered high performers are five times more resourceful with leadership development, coaching, and recognition as their low performing colleagues. High performers tend to emphasize on the introducing new ideas and meeting the needs of the present without compromising the ability of future generations to meet their own needs. Petts, D. (2012). Next-generation education. Modern Metals, 68(3), 8. . Retrieved from http://www. modernmetals. com/ Petts details the advances of technology and the impact on training and development of employees. Petts made one significant point is that online education is one of the current technological advances that help managers train and employees learn. Self-administered training segments and timed quizzes give employees a tool for empowerment and help them increase skills needed to do better with less time than before. As a result, this training increases self-reliance, determination, and critical thinking skills of the employees. Subsequently, managers and businesses are getting more qualified and productive employees.

Consulting Analysis essays

Consulting Analysis essays The current system that we have been working with is Undergraduate Business Advising. After doing some research we have found that there are a number of different problems with the current system. The main problem we have discovered is inconsistent information. One of the proposed solutions is an Undergraduate Business Advising website. The website will provide a way for advisors to communicate information to students more clearly and efficiently. It will also, in the same way, provide a way for students to access the information much quicker and easier. In addition, it will allow students to schedule appointments online. By offering this feature, we hope to increase the number of appointments and in turn decrease the number of walk-ins. Our goal is to decrease the amount of inconsistent information that students are receiving. Absolute Consulting was hired by the Undergraduate Business Advising Office to develop a web page to help enhance the advising process. We were approached by Monica Farrell to update the current process by integrating user-friendly tools on the web. Our role in the project was to gather information from students and faculty to determine what requirements are necessary for the web page. We have accomplished this through extensive interviewing, research, and questionnaires. Our team is comprised of six students from Dr. Sauters analysis class. Each member has strengths in different areas of the project, thus increasing our proficiency. The team has an excellent set of checks and balances to ensure that no one part is overshadowed by another. One of our main concerns was keeping within the scope of the project. We had to pay careful attention as to not get outside of our parameters. Through much discussion with Monica Farrell, we determined what would and would not be appropriate for the project. Monica, our contact, took our ideas to the other advisors to get feedback and we were ...

An Examination of the Benefits, Issues and Impact of Implementing the Dissertation

An Examination of the Benefits, Issues and Impact of Implementing the Integrated Electronic Patient Record System in the UK - Dissertation Example This system provides accessibility and flexibility advantages for both medical personnel and patients; it improves information management and communications, and ultimately improves patient care. On the other hand, there are issues concerning privacy and security of patient information, and its development is very costly and an administrative burden. Moreover, there are still concerns over patient safety. The development of an IEPRS in the UK began in 2002, but the project was beset by continual delays due to the enormity and complexity of the task and escalating costs. In the end, it was abandoned in September 2010. The focus of the investigation thus turned to the experiences of its implementation at local NHS Trusts. Recommendations are also discussed to ensure the effectiveness of an IEPRS by addressing the concerns. An analytical research method was then adopted to further examine the implementation of an IEPRS in the UK. Its findings are discussed and conclusions are drawn foll owed by the researcher's own recommendations. Keywords: medical records, medical information, Integrated Electronic Patient Record System, medical information security, medical information management Table of Contents Section1: Introduction 5 Purpose of the study 5 The UK’s Integrated Electronic Patient Record System 5 Issues related to the implementation of an IEPRS 7 Research Objectives 8 Section 2: Research Methodology and Approach 10 Adopted method of research 10 Justification for the adopted method 11 Limitations 13 Section 3: Literature Review 14 Benefits of an IEPRS 14 General benefits 14 Range, access and flexibility 14 Improved information management 15 Improved communications and patient care 16 Barriers and Issues 16 General risks 16 Privacy and security 17 Information suitability, flexibility and accessibility 17 Financial barriers 18 Administrative burden 19 Patient safety 20 Other concerns 21 Summary of challenges 21 Impact of an IEPRS implementation 22 NHS†™ abandonment of the system 22 Continuation of the implementation at local levels 22 EPR systems in practice 24 EPR system guidelines 25 Elements of the security of patient records 29 Recommendations for an effective IEPRS 30 Raising awareness 30 Promoting involvement 30 Accessibility 30 Information management 30 Information security 31 Ensuring patient safety 35 Remaining concerns 37 Section 4: Findings, Conclusions and Recommendations 39 References 44 CARAT Completeness, Accuracy, Relevance, Accessibility, Timeliness DCR Detailed Care Record DoH Department of Health DPA Data Protection Act EDMS Electronic Document Management Software EMR Electronic Medical Record EPRS Electronic Patient Record System ERDIP Electronic Record Development and Implementation Project FOI Freedom of Information HCHC House of Commons Health Committee HCP Health Care Practitioner (or Provider) HIS Health Information System IEPRS Integrated Electronic Patient Record System IMS Information Management Syst em IT Information Technology LOD Limit of Detection LOQ Limit of Quantitation NAST National Association for Science and Technology NCRS NHS Care Records Service NHS National Health Service (UK) NIGB National Information Governance Board NPfIT National Programme for Information Technology NPSA National Patient Safety Agency PAS Patient Administration System PDS Personal Demographics Service RCGP Royal College of General Practitioners SCR Summary Care Record SUS Secondary Uses Service Project proposal An Examination of the Benefits, Issues and Impact of Implementing the Integrated Electronic Patient Record System in the UK Section1: Introdu

The Environment and Technology in Feed (responses) Assignment

The Environment and Technology in Feed (responses) - Assignment Example However, on the other, it is causes serious environmental problems such as the destruction of Jefferson Park. When more artificial elements are incorporated into life, the natural elements are apparently forced out. Therefore, Feed just like every other dystopian piece of literature shows how the future might end in apocalypse if necessary actions are not taken immediately. It shows how government uses technology to literally control the minds of people, thus, the story serves as a gentle reminder to make young readers see beyond the truth shown to them. The Teen Ink article as well as the Colson Article provide in depth information regarding the genre of YA dystopia and further exemplify how the genre has shifted throughout time. The latter furthermore identifies that it is the â€Å"courage and vision to begin anew† portrayed through stories of this genre that make it so popular among modern day teens (Colson 2012). Hope is identified as the â€Å"most powerful emotion† in YA dystopia, however, in Feed, Anderson does not seem to portray it too much, as in the end, the rebellious Violet dies and throughout the story her thoughts are always dismissed and no one listens to her (Teen Ink 2014). I completely agree with the plot and themes presented in the novel, however, I believe that Anderson could have inclined a bit more towards hope rather than truth so that his readers could end with a better note of â€Å"uplifting sense of triumph†

Macroeconomics In Healthcare Essay Example | Topics and Well Written Essays - 2250 words

Macroeconomics In Healthcare - Essay Example It is estimated that the global community currently provides roughly $2 billion per year to health in the poorest countries. For the poorest economies, spending does appear to make a difference. Gro Harlem Bruntland, Director General of the World Health Organization, believes that â€Å"health has a central role in the world economy. Yet, few finance officials and development economists have so far explored the potential importance of health investment as an instrument for reducing poverty† (Ivinson551). Improved health is potentially advantageous to poor economies. Increased life expectancy can lead to increased productivity and economic stability for many poor families, assuming that opportunities for work and education are readily available. However, in some of the poorest economies, opportunity for increased income from work is very limited. In some areas, basic infrastructure such as roads, utilities and means for production does not exist. Often political corruption prev ents those who are healthy and physically able to work for many years from realizing their true income potential. Even relocation to areas with more work opportunities are difficult with limited income and few safe roads. In those areas, it is a combination of increased spending on health care, increased development of infrastructure and acitivities which remove or reduce corruption that must take place simultaneously for the poorest economies to benefit overall. Improved health care alone will not bring about much change in economic conditions.

Field Trip To Observatoire De Haute-Provence Report

Field Trip To Observatoire De Haute-Provence Report Shaoshan Zeng Abstract A group of 9 students from University College London (UCL) will be visiting the Observatoire de Haute-Provence (OHP) in France between 14th February and 22nd February 2015. Students are expected to use the CCD camera on the 1.20m telescope to image two RR Lyrae variable stars: XY CVn and RR Gem. Also, students will use the Aurelie spectrograph on the 1.52m telescope to obtain high resolution spectra of bright spectroscopic binary systems within the spectral region 4070-4130Ã…. The main content of this report will focus on the observing facilities available at the OHP and background information of the objects to be targeted. And the last section of this report is the observing diary containing all the data obtained at the telescope. Contents Overview of l’Observatorie de Haute-Provence (OHP) Brief History Location Previous scientific work Observing conditions Observing Instruments The 1.20m Telescope The 1.52m Telescope The Aurelie Spectrogrph Scientific Programme for 1.2m Telescope Scientific Programme for 1.52m Telescope Targets RR Lyrae variable stars Spectroscopic binaries Observing Diary References Appendix 1. Light curves of RR Lyrae variables. Appendix 2. Finder Charts 1. Overview of l’Observatorie de Haute-Provence (OHP) History The observatory is owned by the Centre National de la Recherche Scientifique (CNRS) and is funded by the Institut National des Sciences de l’Univers (INSU). Originally, OHP was built as a national facility for Frence astronomers in 1937 and later on in 1949, the facilities at the OHP were available to be used by foreign visiting astronomers. In 1943, the first astronomical observations were made with the 1.20m telescope and the first research paper were published a year later. 1.2 Location OHP is located in St Michel, near Forcalquier in the Alpes de Haute-Provence, south-east France. The coordinates of OHP are: Longitude = 0h 22m 52s E Latitude = +43 ° 55’ 46† Altitude = 650m Previous scientific work OHP has done some remarkable work on the detection of extra-solar planets. This studies started with the discovery of 51 Peg-b in 1995 using the ELODIE spectrograph on the 1.93m telescope and followed by many more discoveries such as Glises 876, the third closest known star to the Sun were found in 1998 and HD190228b was announced in 2000 as a giant planet orbiting the host star. In 2006, ELODIE was replaced by a stabilised high resolution spectrograph called SOPHIE at the 1.93m telescope of OHP. It is operated by using a large survey for search for northern extrasolar planets through the radial velocity method. Nowadays, SOPHIE plays a significant contribution to the follow-up of transiting exoplanet candidates from photometric surveys include SWASP, CoRoT and Kepler. 1.4 Observing Conditions The reason for OHP grounded on this site is mainly because the benefit of having higher probabilities on clear sky and favourable weather conditions throughout the year and the average atmospheric extinction at OHP is approximately twice that for ESO at La Silla. On average, about 60% of nights are considered to be suitable for astronomical observations. This can be showed by the yearly breakdown which based on a statistics made from 1965 to 2004: 170 nights are excellent conditions, 50 nights with very slight cloud and 70 nights are being partly cloudy. Despite of the weather conditions, the image quality is also the key factor to provide good observation. At OHP, the seeing disk is around 2 arcsec and can be lower down to 1 arcsec occasionally which compares to the image quality at ULO is about 4-5 arcsec. However, about 45 days per year on average (commonly in winter) cold wind flows from the northwest which is known as Mistral would cause the degradation of seeing, sometimes the quality of the seeing can severely decline to over 10 arcsec. But the advantage of having the Mistral winds is good weather usually follow as the winds usually clear up the sky. 2. Observing Instruments There are four main telescopes operate at OHP: 1.93m, 1.52m, 1.20m and 0.80m. Typically, 1.52m and 1.20m telescopes will be used to undertake studies during the field trip. 2.1 The 1.20m Telescope This is the first telescope installed at OHP and operates since 1943. It only has a Newton focus which is corresponded to a focus ratio of f/6. As an improvement, the telescope is now equipped with a CCD camera for direct imaging and photometry. It is usually operated for studies of variability of X-ray sources, imaging of galaxies and H II regions as well as the faint solar system objects. 2.2 The 1.52m Telescope This is the telescope that have been in use since 1967 at OHP and is used accompanied with the high resolution Aurelie spectrograph which is positioned at the Coude focus. Thus, most of the spectroscopic studies are carried out by using this telescope. The Coude focus is the only focus of this telescope and the focal ratio is f/27.6 which is almost identical to the 1.52m telescope at the ESO at La Silla. Even though it needed to be pointed manually, all other functions are automated. The telescope is equipped with a CCD camera, used from acquiring the target and automatic guiding. The camera has a field of view of 3’ x 4’. 2.3 The Aurelie Spectrograph The Aurelie spectrograph is a high resolution spectrograph that has been developed and installed on the 1.52m telescope in 1989 at the OHP. The goal of using such high quality instrument is to obtain spectra at very high resolutions over the spectral range of 3900 to 10000Ã… and because of the average seeing conditions at the OHP, the Aurelie spectrograph is also designed to obtain the largest optical efficiency and small amount of scattered light with an entrance aperture at about 3 arcsec wide. The detector attached to the spectrograph is called Thomson TH7832 which is a linear array CCD-like detector. The array is made of 2048 pixels of which 2036 are usable. The advantage of using this detector is: it is very clean meaning it exhibits no interference fringes or persistence effects and this would give the benefit to detect very weak absorption lines. 3. Scientific Programme for 1.2m Telescope The main purpose of this programme is to obtain images of two RR Lyrae variable stars RR Gem and XY CVn by using Cousins B- and V-band filters followed by calibrating these images with respect to stars of known magnitude near to the target star. This will be down over the course of 6 nights with 1.2m telescope. As a result, light curves of these stars will be obtained over several cycles of variation in order to calculate the pulsation period of each of the two stars. The light curve of XY CVn will be compared to that of RR GEM as the light curve of XY CVn is more symmetrical. From experience gained last few years (between 2003 and 2014) of UCL field trips who also completed the task with the same telescope, CCD and filters conclude that the exposure times should be around 1-3 minutes in each of the filter for RR Gem and because XY CVn is fainter than RR Gem, it requires longer exposure time of around 4 minutes in each of the B and V-bands. If the star has magnitude at around 11, a s ignal to noise ratio of at least 100 should be obtained with a 60 second or even shorter exposure in the V-band. The same signal to noise ratio is also kept for the B-band. Other than evaluating the result obtaining in the programme, observations of these two targets will also be compared to those obtained during the UCL field trip of 2000 to 2014. This should give more accurate calculated period and overtone modulation of the light curves to the stars. RR Lyrae stars are pulsating variables with about half the mass of the Sun but probably much older and hotter than the Sun. They belong to low mass Population II and they are abundant in globular clusters. RR Lyrae variables are special because they growing larger and smaller in size with their brightness changing significantly. In general, they have periods of 0.2 to 1 day and spectral types of A2 to F6 which have an average effective temperature of 7000K and a luminosity typical around 80 Lsun. Some of them have similar light curves to those of Cepheid variables and obey a period luminosity relation which is approximately: Log10 P = -0.85M + constant These properties make RR Lyrae variables become excellent standard candles as if the period of time it takes for an RR Lyrae to go through its cycle of brightening and dimming is known, then the absolute luminosity of that star can be estimated. The absolute luminosity shows how bright a star would be if it was a certain distance away from us. From this, the distance to the star can be determined if the measure brightness of the star appear to us compared to its absolute luminosity. 4. Scientific Programme for 1.52m Telescope For this programme, the Aurelie spectrograph on the 1.52m telescope will be used to obtain high resolution spectra of a selection of targets which are known to be spectroscopic binary systems that in the spectral region of 4070-4130Ã…. By analysing these spectra, weak absorption lines should be resolved to measure the changes in the radial velocity of a star by applying the cross correlation technique. Since the field trip group in 2006 and 2010-2014 also completed the similar task with Aurelie, the analysed results from this field trip will be compared to those obtained in previous years and hopefully this will result in an improvement of phase coverage for all of the systems, especially for targets with long period. By combining all the data sets, a number of physical parameters such as the mass ratio, the mass function, the period and the orbital eccentricity can be estimated for each binary system. As HÃŽ ´ (ÃŽ »4101Ã…) is included in the targeted spectral region, the appea rance of this line in obtained spectra also need to be investigated as it changes as a function of spectral type. In order to resolve the weak lines and measure their wavelengths accurately, a spectrographic resolving power of at least R = 40000 is required. Such high resolution that in use should also provide accurate information of radial and rotational velocities for each target. A wavelength coverage of at least 60Ã… is needed to include enough weak lines simultaneously and to make sure the continuum level outside the HÃŽ ´ line could be estimated. Despite of these, useful weak lines can only be obtain with a signal to noise ratio of at least 250 due to the fact that the equivalent widths of the weak lines are expected to be with several mÃ…. And more importantly, the total integration time of all of the start should be controlled to be 120 minutes or less because the resolution of orbital phase of 1.52m telescope would become poor if longer exposure time is used. Spectroscopic binaries involve two stars orbiting around their common centre of mass. These two stars are so close together that can only be seen as one object, and over period of time, there is Doppler shift change in the observing spectrum. In other words, if the star does exist in a binary system, they are of similar luminosity, each spectral line will twice over the course of one orbit, split into two, reach a maximum separation and then move back together again due to the Doppler shift caused by their radial velocity. Among all the targets, the star ÃŽ ± Uma is of particular interest as it has a long period of 44 years while other target stars have relatively short periods and has an orbit that is not clearly determined. It thought to have passed periastron in 2000, so it would be interesting to compare its measured radial velocity with that from spectral obtained during 2006 to 2014. 5. Target stars 5.1 RR Lyrae Variable Stars The stars that will be observing for the investigation of the light curves of RR Lyrae variable stars on the 1.2m telescope are shown below in Table 1 along with their coordinate, magnitudes and period. Table 1. Investigate RR Lyrae variable stars RR Gem is a type â€Å"a† RR Lyrae variable, it is well located for observation between UT 18:00 to 24:00 in late January to February at OHP. This light curve of this type of star will show a steep increase in brightness at first, the brightness will then gently fade away until a minimum is reached. The finding charts for RR Gem can be found in Appendix 1. (A1) and the calibration stars are shown in Table 2 below. Table 2. Calibration stars for RR Gem XY CVn is a type â€Å"c† RR Lyrae variable, it is well located for observation in the morning in January and February at OHP. Different to RR Gem, the light curve of this type of star is more symmetrical. The finding charts for both target stars can be found in Appendix 1. 5.2 Spectroscopic binaries targets The stars for which I am responsible for background research for the programme occurring on the 1.52m telescope are shown in Table 3 below. Table 3. Spectroscopic binaries targets Both of the targets are circumpolar which will never set throughout the night, this makes them easily observable in night time. For HR 4072, it would be best observed at around 0:00-1:00 UT and ÃŽ ¹ CrB should be best observed at 6:00-7:00 UT as these time will be the target just across the meridian i.e at their highest point in the sky. However, 6:00-7:00UT would correspond to 7:00-8:00 local time at OHP, would pass the sun rise time and the sky is bright already. Thus, target ÃŽ ¹ CrB can be observed in the early morning before sunrise when it still high up in the sky before crossing the meridian. The finding charts for both target stars can be found in Appendix 2. 6. Observing Journal References http://www.obs-hp.fr -the OHP website http://www.simbad.com -online star catalogue http://www.aavso.org/ -online database for variable stars, obtain light curves and finding charts 2015 UCL Field Trip Observation Plans (Stephen Boyle, September 2014) Appendix 1 A1. Finding Chart of RR Gem (AAVSO) A2. Finding chart of XY CVn (AAVSO)

Greed in Julius Caesar :: Julius Caesar Essays

Greed in Julius Caesar Greed can disrupt a family, town, or even a country. The play "Julius Caesar" was a great example of the power of greed. In the play "Julius Caesar" the driving forces were Cassius, Brutus, Marc Antony, and Octavius Caesar. Cassius was the brother in-law of Brutus and was also the creator of the group of conspirators. Cassius was also a senator of Rome. Cassius's greed for power, good reputation, and his jealousy lead to Caesars death. Cassius had the most honorable man in Rome to help in his plot to kill Caesar. Brutus was the honorable roman which Cassius took control of. Brutus loved Rome and all of the Roman people. Brutus was actually the true leader of the conspirators because he made the important decisions. Brutus had a different motivation for killing Caesar. The conspirators killed Julius Caesar because they were worried that if Caesar had succeeded in becoming king all the conspirators would lose their power. Brutus's motive for killing Julius Caes ar was his fear of Caesar destroying the city of Rome. Mark Antony was a regular Roman citizen, who was good friends with Julius Caesar. After Julius Caesar's death, Marc Antony recited a speech at Julius Caesar's funeral to all the people of Rome. The speech caused the plebeians to destroy everything in sight. It was by his speech that Marc Antony got his revenge towards Brutus and Cassius. Octavius Caesar was the nephew of Julius Caesar. When he got to Rome he and Marc Antony teamed up to fight against the forces of Brutus and Cassius. It was at Brutus and Cassius's last battle where Octavius and Marc Antony succeeded in their plan. Cassius had many motives for the killing of Julius Caesar. One of Cassius's motives was his greed for power. Cassius believed that he should have as much power as Julius Caesar. Cassius was also worried that if Julius Caesar had been king he would lose all of his power and become another regular citizen of Rome. Cassius showed his greed for power when he would always talk about how Caesar would get so much power and he was treated like he was nothing.