Gravity's pull: The identity-related motives and outcomes of hiring stars
File(s)Gravity’s Pull 9_9_22.docx (188.3 KB)
Accepted version
Author(s)
Lyle, Matthew CB
Eckardt, Rory
Corley, Kevin G
Lepak, David P
Type
Journal Article
Abstract
Strategic human capital scholarship, alongside a wealth of evidence from the popular press, suggests that star employees can influence an organization's socially constructed identity. However, an overarching conceptual framework that explains these shifts has yet to emerge. In this paper, we draw upon Hatch and Schultz's (2002) theory of identity change to discuss how organizational identity-change related motives – defined as decision makers' interest in spurring changes to socially constructed, internal perceptions of their organization's central and distinctive features – act in concert with considerations of value creation and capture to influence the hiring of different identity-aspirant stars (i.e., stars that embody a desired future organizational identity). Given that stars represent catalysts for identity change that have agency and become part of the social fabric of an organization, we then explain how the mechanisms by which stars' attempts to gain or retain status – coupled with organization members' willingness to emulate their behaviors – can affect internal-oriented organizational identity change. This paper advances consideration of social-psychological factors alongside economic views of stars and offers implications for the literatures on strategic human capital and organizational identity.
Date Issued
2023-06
Date Acceptance
2022-09-16
Citation
Human Resource Management Review, 2023, 33 (2), pp.1-17
ISSN
1053-4822
Publisher
Elsevier BV
Start Page
1
End Page
17
Journal / Book Title
Human Resource Management Review
Volume
33
Issue
2
Copyright Statement
© 2022 Elsevier Ltd. All rights reserved. This manuscript is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International Licence http://creativecommons.org/licenses/by-nc-nd/4.0/
Identifier
https://www.sciencedirect.com/science/article/pii/S1053482222000511?via%3Dihub
Publication Status
Published
Article Number
100932
Date Publish Online
2022-09-23