Seeking legitimacy through CSR: Institutional Pressures and Corporate Responses of Multinationals in Sri Lanka

Arguably, the corporate social responsibility (CSR) practices of multinational enterprises (MNEs) are influenced by a wide range of both internal and external factors. Perhaps most critical among the exogenous forces operating on MNEs are those exerted by state and other key institutional actors in host countries. Crucially, academic research conducted to date offers little data about how MNEs use their CSR activities to strategically manage their relationship with those actors in order to gain legitimisation advantages in host countries. This paper addresses that gap by exploring interactions between external institutional pressures and firm-level CSR activities, which take the form of community initiatives, to examine how MNEs develop their legitimacy-seeking policies and practices. In focusing on a developing country, Sri Lanka, this paper provides valuable insights into how MNEs instrumentally utilise community initiatives in a country where relationship-building with governmental and other powerful non-governmental actors can be vitally important for the long-term viability of the business. Drawing on neo-institutional theory and CSR literature, this paper examines and contributes to the embryonic but emerging debate about the instrumental and political implications of CSR. The evidence presented and discussed here reveals the extent to which, and the reasons why, MNEs engage in complex legitimacy-seeking relationships with Sri Lankan institutions

Modes of Participation

This paper focuses on the notion of ‘participation’ as it has been used in the social sciences throughout the twentieth century. It proposes that there are two main traditions of use—a ‘poorer’ and a ‘richer’ one—and it argues in favour of the second. It does this by examining how Simmel and Goffman, on the one hand, and Lévy-Bruhl and Durkheim, on the other, defined participation. Developed by Lucien Lévy-Bruhl in the first part of last century, ‘participation’ in the richer sense is today being given new live by sociocultural anthropologists such as Marshall Sahlins and phenomenologically inclined cognitive scientists such as Shaun Gallagher. The paper addresses the roots of the concept in Scholastic theology and proposes to show how central it can come to be to a sociocultural anthropology that is willing to take on frontally the challenges presently being posed by embodied cognition

A produção de conhecimentos na interface entre as ciências sociais e humanas e a saúde coletiva

Este artigo trata da intercessão, no âmbito do conhecimento, entre as ciências sociais e humanas e a saúde coletiva. Parte-se do legado das ciências sociais clássicas, discute-se esse aporte, debate-se como e em que medida as ciências sociais e humanas em saúde constituem um subcampo que, por sua vez, articula diversas racionalidades. O texto se baseia numa pesquisa sobre a produção científica das sete principais revistas da área: Revista de Saúde Pública; Cadernos de Saúde Pública; Ciência & Saúde Coletiva; Saúde e Sociedade, Physis, Interface e História, Ciência e Saúde no período de janeiro de 2011 a agosto de 2012 (20 meses). Foram ao todo 1757 artigos publicados nessas revistas, sendo 545 (31,0%) sobre ciências sociais e saúde ou fazendo interface desse campo com a saúde coletiva. O artigo se debruça na análise dessa produção e conclui: que é pujante a participação das ciências sociais e humanas no campo da saúde; que existe um polo irradiador de conhecimentos que parte de autores seminais, mas já conta com a contribuição de estudiosos importantes de segunda e terceira geração; e que os problemas referidos pelos cientistas sociais e de humanidades da área de saúde são os mesmos que hoje ocupam os teóricos sociais, filósofos e historiadores do mundo inteiro

Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)

This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands

Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams. </p

Localization and broadband follow-up of the gravitational-wave transient GW150914

A gravitational-wave transient was identified in data recorded by the Advanced LIGO detectors on 2015 September 14. The event candidate, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the gravitational wave data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network Circulars, giving an overview of the participating facilities, the gravitational wave sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the electromagnetic data and results of the electromagnetic follow-up campaign will be disseminated in the papers of the individual teams