Cyberbullying Across the Lifespan of Education: Issues and Interventions from School to University

Research on cyberbullying amongst students has tended to be conducted separately within specific education institutional contexts, schools, further education (FE) and higher education (HE), neglecting a view that takes account of the entire educational lifespan. The present article addresses this gap in the literature, providing a novel take on examining its nature, social environments, legal consequences and potentially helpful interventions. To facilitate this, the article conceptualises cyberbullying in broad terms, recognising that it can take multiple forms of online and digital practice including: spreading rumours, ridiculing and/or demeaning another person, casting aspirations on the grounds of race, disability, gender, religion or sexual orientation; seeking revenge or deliberately embarrassing a person by posting intimate photos or videos about them without their consent; accessing another’s social networking profiles with malicious intent and socially excluding a person from a social network or gaming site. This article demonstrates that harm from cyberbullying is a cause for concern for students at each developmental stage and that there are continuities in its appearance that need to be challenged at each point in the educational lifespan. And inaccurately, by university, the idea that ‘nothing can be done’ still is one of the main concerns for the victims. The article concludes with five key recommendations for future research and practice across the educational lifespan

How can we prevent and reduce bullying amongst university students?

While it has long been recognized that bullying occurs at school and in the workplace, recent research confirms that bullying also takes place among university students, including undergraduates, post-graduates and doctoral research students. In the UK, the National Union of Students (NUS) alerted staff and students to the issue in a series of reports but it is not confined to the UK. Authors in the book edited by Cowie and Myers (2016a, 2016b) present cross-national findings on the theme of bullying among university students (Pörhöla et al., 2016). In this article we discuss the urgent need for interventions to prevent and reduce bullying in this context. We also indicate the areas where little or no intervention is taking place, notably in the field of university policy

Bullying amongst University Students in the UK

This study with 20 university students examined perspectives in three different participant roles: the perpetrator, the target and the bystander. The purpose of the exercise was to resolve the outcome of an alleged incident of cyberbullying using a social network site via the means of a restorative conference. The findings suggest that the power of the peer group needs to be fully understood if cyberbullying, is to be tackled efficiently. The bystanders tended to blame the victim and were reluctant to intervene, the victim felt let down and marginalised by peers’ indifference and hostility, and the bully failed to realise or understand the consequences of their actions. The study offers ideas for strategies and policies to address the issue of cyberbullying with university students

The Use of Participatory Methods in Researching the Experiences of Children and Young People

Participatory research methods offer a very promising approach for gaining in-depth understanding of young people’s lives. However, when adopting such approaches, researchers need to be aware of methodological and theoretical issues. The aim of this article is to present a discussion of ways in which participatory methods may be used as a research strategy when investigating young people’s experiences and emotions. We explore the potential of these methods as well as some of their limitations

Short-term fate of phytodetritus in sediments across the arabian sea oxygen minimum zone

The short-term fate of phytodetritus was investigated across the Pakistan margin of the Arabian Sea at water depths ranging from 140 to 1850 m, encompassing the oxygen minimum zone (~100–1100 m). Phytodetritus sedimentation events were simulated by adding ~44 mmol 13C-labelled algal material per m2 to surface sediments in retrieved cores. Cores were incubated in the dark, at in situ temperature and oxygen concentrations. Overlying waters were sampled periodically, and cores were recovered and sampled (for organisms and sediments) after durations of two and five days. The labelled carbon was subsequently traced into bacterial lipids, foraminiferan and macrofaunal biomass, and dissolved organic and inorganic pools. The majority of the label (20 to 100%) was in most cases left unprocessed in the sediment at the surface. The largest pool of processed carbon was found to be respiration (0 to 25% of added carbon), recovered as dissolved inorganic carbon. Both temperature and oxygen were found to influence the rate of respiration. Macrofaunal influence was most pronounced at the lower part of the oxygen minimum zone where it contributed 11% to the processing of phytodetritus

Local Large-Scale Structure and the Assumption of Homogeneity

Our recent estimates of galaxy counts and the luminosity density in the near-infrared (Keenan et al. 2010, 2012) indicated that the local universe may be under-dense on radial scales of several hundred megaparsecs (Mpc). Such a large-scale local under-density could introduce significant biases in the measurement and interpretation of cosmological observables, such as the inferred effects of dark energy on the rate of expansion. In Keenan et al. (2013), we measured the K-band luminosity density as a function of distance from us to test for such a local under-density. We made this measurement over the redshift range 0.01 < z < 0.2 (radial distances D ~ 50-800 Mpc). We found that the shape of the K-band luminosity function is relatively constant as a function of distance and environment. We derive a local (z < 0.07, D < 300 Mpc) K-band luminosity density that agrees well with previously published studies. At z > 0.07, we measure an increasing luminosity density that by z~ 0.1 rises to a value of ~1.5 times higher than that measured locally. This implies that the stellar mass density follows a similar trend. Assuming that the underlying dark matter distribution is traced by this luminous matter, this suggests that the local mass density may be lower than the global mass density of the universe at an amplitude and on a scale that is sufficient to introduce significant biases into the measurement of basic cosmological observables. At least one study has shown that an under-density of roughly this amplitude and scale could resolve the apparent tension between direct local measurements of the Hubble constant and those inferred by Planck team. Other theoretical studies have concluded that such an under-density could account for what looks like an accelerating expansion, even when no dark energy is present.Comment: Proceedings of IAU Symposium 308 "The Zeldovich Universe: Genesis and Growth of the Cosmic Web", 23-28 June 2014, Tallinn, Estoni

Does diversity in society inevitably lead to a rise in xenophobia among children and young people?

Across Europe, and in the context of a post - BREXIT situation, society is having to accommodate to large numbers of people from diverse cultures. There is a reported increase in xenophobic incidents, bullying and social exclusion, indicating that diversity runs the risk of intolerance and prejudice. This is played out in all manner of social situations in schools and universities, in the community and in the workplace. This discussion paper, written by three U.K. Social Scientists representing the disciplines of psychology, criminology, education and sociology, focuses on the legal and moral aspects of the issue as well as on interventions that promote tolerance and xenophilia in a range of social contexts. It concludes with recommendations to social scientists in all European countries to enter the debate and carry out research in this challenging and highly topical field

TORCH: A Cherenkov Based Time-of-Flight Detector

TORCH is a novel high-precision time-of-flight detector suitable for large area applications and covering the momentum range up to 10 GeV/c. The concept uses Cherenkov photons produced in a fused silica radiator which are propagated to focussing optics coupled to fast photodetectors. For this purpose, custom MCP-PMTs are being produced in collaboration with industrial partners. The development is divided into three phases. Phase 1 addresses the lifetime requirements for TORCH, Phase 2 will customize the MCP-PMT granularity and Phase 3 will deliver prototypes that meet the TORCH requirements. Phase 1 devices have been successfully delivered and initial tests show stable gain performance for integrated anode current &gt;5 C/cm2 and a single photon time resolution of ≤ 30 ps. Initial simulations indicate the single photon timing resolution of the TORCH detector will be ∼70 ps