The Influence of Inter-Stakeholders’ Communication on University – Industry Collaboration

Aliu, Dorian; Akatay, Ayten; Aliu, Armando

doi:10.19085/journal.sijbpg040801

Cited by 2 publications

(4 citation statements)

References 10 publications

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“…Freeman (1984) stakeholder theory is popular among studies that explore HEI–industry collaborations (Aliu and Aliu, 2017; Langrafe et al, 2020). Freeman defined a stakeholder as ‘any group or individual who can affect or is affected by the achievement of the organization’s objectives’ (p.46).…”

Section: Stakeholder Theorymentioning

confidence: 99%

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Enhancing graduates’ employability through polytechnic–industry collaboration

Otache

2021

Industry and Higher Education

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The unemployability of many Nigerian graduates is somewhat attributable to the existing wide collaboration gap between Nigerian higher education institutions and industry. Against this backdrop, this study explores how Nigerian polytechnics and industry can collaborate to enhance graduates’ employability. Adopting a focus group discussion approach, three focus groups involving 20 people (eight polytechnic lecturers, six National Board for Technical Education officials and six industry executives) participated in the study. Content analysis of the focus group discussions revealed the need to involve industry experts in curriculum development and review to meet today’s job requirements in industry. The need to involve industry experts in teaching certain aspects of the curriculum was also highlighted. The findings further revealed the desirability of exposing students and lecturers to industrial work situations to equip them with workplace skills and experience. Additionally, the study found that a comprehensive collaboration policy framework, funding, commitment, mutual benefits and trust are required to achieve successful polytechnic–industry collaboration. This research demonstrates that effective collaboration between polytechnics and industry will help to improve the employability of graduates. The findings provide policy and practical implications for polytechnics, regulatory bodies, industry and government.

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Section: Stakeholder Theorymentioning

confidence: 99%

“…Previous studies have applied stakeholder theory (Aliu and Aliu, 2017; Langrafe et al, 2020; Nwajiuba et al, 2020). For example, Nwajiuba et al (2020) used stakeholder theory to explain the role of government, HEIs and industry in improving higher education quality and graduate employability in Nigeria.…”

Section: Stakeholder Theorymentioning

confidence: 99%

Enhancing graduates’ employability through polytechnic–industry collaboration

Otache

2021

Industry and Higher Education

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“…The regions with extended emission have been fitted with Gaussian sources with free locations and widths (by their respective collaborations). The best fitting coordinates and areas are shown for ARGO J2031+4157 [26], 2HWC J2031+415 [48], TeV J2032+4130 (HEGRA) [7], Cygnus Cocoon [6], and MGRO J2031+41 [49].…”

Section: B the Cygnus Cocoonmentioning

confidence: 99%

“…Hard γ-ray emission from the region was confirmed with HEGRA by [7]. Properties of the γ-rays from the Cygnus X region have since been extensively explored at both GeV and TeV energies with Milagro [22], MAGIC [23], Fermi [6,24], ARGO-YBJ [25], and VERITAS [26,27].…”

Section: Introductionmentioning

confidence: 99%

Gamma-ray puzzle in Cygnus X: Implications for high-energy neutrinos

et al. 2017

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The Cygnus X region contains giant molecular cloud complexes and populous associates of massive young stars. The discovery of spatially extended, hard γ-ray emission in Cygnus X by both Milagro and Fermi indicates that Cygnus X is also a potential source of high-energy Galactic neutrinos. Here, we adapt our single-zone model for cosmic ray interactions in the central molecular zones of starburst galaxies for use in Cygnus X. We calculate the potential neutrino flux corresponding to the hard γ-ray emission from the "Cygnus Cocoon" and to the soft, diffuse interstellar γ-ray emission. We check our results by comparing the corresponding γ-ray emission against the Fermi interstellar emission model and Milagro, ARGO-YBJ, and HAWC observations. In comparing our results against a recent IceCube analysis and the current sensitivity limits, we find that neutrino emission from the Cocoon has a large enough flux that it could plausibly be detected, provided hadronic interactions are occurring at sufficiently high energies. High energy neutrinos from Cygnus X would provide direct evidence for the presence of as yet unidentified PeV energy accelerators in the Galactic disk.

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The Influence of Inter-Stakeholders’ Communication on University – Industry Collaboration

Abstract: Purpose: The aim of this study is to examine the influence of inter-stakeholders' communication on universities which mutually collaborate with both internal and external stakeholders in frame of university -industry collaboration (UIC

Cited by 2 publications

References 10 publications

Enhancing graduates’ employability through polytechnic–industry collaboration

Enhancing graduates’ employability through polytechnic–industry collaboration

Gamma-ray puzzle in Cygnus X: Implications for high-energy neutrinos

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