Responding to the gig economy: A comparative case-study of platform work in Norway and United Kingdom

The rise of the gig economy is a challenge facing many established economies in Europe. The ongoing digital transformation of society has resulted in rapid changes to the labour market. Work through digital labour platforms is one of the rising trends in the gig economy. Workers are categorised as self-employed, but work under strict control from the platform companies. The division between being self-employed and being employed is becoming less distinct, and more people fall into a grey area between the two categories. The theoretical framework for this analysis is the Varieties of Capitalism theory by Hall and Soskice, which distinguishes between two types of political economies; liberal market economies and coordinated market economies. The theory argues for a more significant divide between countries’ responses to the gig economy based on existing institutional arrangements. By utilising qualitative document analysis to do a comparative case study of Norway and the UK, this thesis aims at identifying enabling and restricting factors to the growth of platform work. The Norwegian and UK governments have published public reports on the gig economy and the challenges of platform work. The analysis of these documents identifies several restricting and enabling factors that support a greater divide between the two countries in their response to the gig economy. The highly regulated labour market in Norway, with strong unions, tripartite cooperation and high coverage of collective agreements, are factors that should restrict the growth of platform work. The emphasis on flexibility in the UK labour market, firm-level wage negotiations and weaker unions are factors that should enable the growth of platform work. The problem of misclassification of workers is found to be a restricting factor in both countries. In the UK, workers must be classified as employees or workers to be entitled to the National Minimum Wage. Whereas in Norway, the classification of workers is important because of the collective agreements’ role in regulating the labour market.MasteroppgaveSAMPOL350MASV-SAP

Pathways to change: the effect of a Web application on treatment interest.

Most individuals with drinking problems do not receive treatment, generally because they do not perceive the need for it. It is difficult to access this population of problem drinkers in order to encourage treatment-seeking. A Web-based program was written, designed to increase motivation for change. The program guided non-treatment-seekers through a multi-stage assessment and provided them with feedback. The level of interest in treatment was measured pre-and post-intervention. Compared to baseline, after the intervention, significantly more individuals rated themselves very interested in participating in some form of traditional treatment (19% vs. 28%), and their focus on a specific modality increased

Employee Relations: A Major Antecedent in Employee Satisfaction

Operations of all the organizations mainly comprise of service deliverance which in turn lie how the things are conducted or performed. The righteous act or effective performance in any operation can be achieved largely by the satisfied employees. Employees play the major role in all the sectors therefore it is of paramount importance to keep them satisfied with the working environment. There are several factors affecting the employees’ state of satisfaction; the chief one is Employee Relations. The paper analyses the role and effects of Employee Relations on Employee Satisfaction. The paper includes the recommendations for the betterment of Employees and their relations with the Management

A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds

From a survey of the 3400 Å region in the earliest O-type spectra, we have found that two of the four O2 giants observed in the Large Magellanic Cloud have O IV lines there that are stronger than the N IV lines, while the other two have the opposite. A Small Magellanic Cloud counterpart also has N IV stronger than O IV. Inspection of the blue spectra of these stars shows that the former pair have weaker N lines in all ionization states (III, IV, and V) present as well as lines of C IV λ4658, while the latter three have stronger N lines and greater He/H. Space ultraviolet observations of two of the N-strong stars show N V wind profiles substantially stronger than those of C IV, while in the N-weak stars the C IV features are equal to or stronger than the N V. The N-strong stars are now reclassified as ON2 III(f*), newly defining that category. These characteristics strongly suggest a larger fraction of processed material in the atmospheres of the ON2 stars, which we confirm by modeling the optical spectra. In the context of current models, it is in turn implied that the ON2 stars are in a more advanced evolutionary state than the others, and/or that they had higher initial rotational velocities. The recent formulation of the effects of rotation on massive stellar evolution introduces an additional fundamental parameter, which the CNO abundances are in principle able to constrain. We present some illustrative comparisons with current Geneva evolutionary models for rotating massive stars. It is possible that these very hot, nitrogen-rich objects are products of homogeneous evolution. Our results will provide motivation for further physical modeling of the atmospheres and evolutionary histories of the most massive hot stars.Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados UnidosFil: Morrell, Nidia Irene. Las campanas observatory; ChileFil: Howarth, Ian D.. University College London; Estados UnidosFil: Crowther, Paul A.. University of Sheffield; Reino UnidoFil: Lennon, Daniel J.. Isaac Newton Group of Telescopes; EspañaFil: Massey, Philip. Lowell Observatory; Estados UnidosFil: Arias, Julia Ines. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentin

Mohave rattlesnake (Crotalus scutulatus) identification revisited

Crotalus scutulatus (Mohave rattlesnake) is a clinically significant pit viper broadly distributed across much of the arid southwestern United States and mainland Mexico. Identification of C scutulatus is a concern among emergency medical service and emergency department personnel owing to its reputation for severe envenomations and difficulty in visually differentiating between C scutulatus and other species, primarily Crotalus atrox (western diamond-backed rattlesnake). We contrast distinctive characteristics of C scutulatus, C atrox, and 3 other sympatric species: Crotalus molossus, Crotalus ornatus, and Crotalus viridis (western and eastern black-tailed rattlesnakes and prairie rattlesnake, respectively). Greenish coloration eliminates C atrox but does not confirm C scutulatus. Obvious coarse and fine speckling of the dorsal pattern and a pale postocular stripe intersecting the mouth characterize C atrox. Dorsal speckling is insignificant or absent in the other species, whereas the pale postocular stripe passes above the mouth in C scutulatus and C viridis and is absent in C molossus and C ornatus. Tails boldly ringed with alternating black and white or contrasting shades of gray are shared by C atrox and C scutulatus, respectively, but a lack of boldly ringed tails characterizes the other species. The proximal rattle segment is yellow and black, or entirely yellow, in C scutulatus but black in the others. The most reliable visual identifications are based on evaluations of multiple traits, all of which are variable to some extent. Traits such as tail ring width and the size and number of crown scales have frequently been overemphasized in the past.Open access articleThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]

Stern v. Marshall Panel

The Stern v. Marshall Panel discussed the issues of the case and its potential impact on practitioners

The Effects of Stellar Rotation. I. Impact on the Ionizing Spectra and Integrated Properties of Stellar Populations

We present a sample of synthetic massive stellar populations created using the Starburst99 evolutionary synthesis code and new sets of stellar evolutionary tracks, including one set that adopts a detailed treatment of rotation. Using the outputs of the Starburst99 code, we compare the populations' integrated properties, including ionizing radiation fields, bolometric luminosities, and colors. With these comparisons we are able to probe the specific effects of rotation on the properties of a stellar population. We find that a population of rotating stars produces a much harder ionizing radiation field and a higher bolometric luminosity, changes that are primarily attributable to the effects of rotational mixing on the lifetimes, luminosities, effective temperatures, and mass loss rates of massive stars. We consider the implications of the profound effects that rotation can have on a stellar population, and discuss the importance of refining stellar evolutionary models for future work in the study of extragalactic, and particularly high-redshift, stellar populations.Comment: 13 pages, 8 figures; accepted for publication in the Astrophysical Journa

Recent Developments: The Uniform Arbitration Act

Since 1983, this annual Article 2 has been prepared to provide a survey of recent developments in the case law interpreting and applying the various state versions of the Uniform Arbitration Act3. The purpose is to promote uniformity in the interpretation of the U.A.A. by developing and explaining the underlying principles and rationales courts have applied in recent cases.

Student motivations, perceptions and opinions of participating in student evaluation of teaching surveys: A scoping review

Several times each year the teaching performance of academics at higher education institutions are evaluated through anonymous, online student evaluation of teaching (SET) surveys. Universities use SETs to inform decisions about staff promotion and tenure, but low student participation levels make the surveys impractical for this use. This scoping review aims to explore student motivations, perceptions and opinions of SET survey completion. Five EBSCO® databases were searched using key words. Thematic analysis of a meta-synthesis of qualitative findings derived from 21 papers identified five themes: (i) the value students’ place on SET, (ii) the knowledge that SET responses are acted upon to improve teaching, (iii) assurance of survey confidentiality and anonymity, (iv) incentives for completing SET, and (v) survey design and timing of survey release. Perceptions, knowledge and attitudes about the value of SET are essential factors in motivating students to engage and complete SETs, particularly if surveys are easy to interpret, time for completion is incentivised and responses are valued