The dark side of AI-powered service interactions: exploring the process of co-destruction from the customer perspective

2020 ◽  
pp. 1-26
Author(s):  
Daniela Castillo ◽  
Ana Isabel Canhoto ◽  
Emanuel Said
2021 ◽  
pp. 002224292110230
Author(s):  
Gautham G. Vadakkepatt ◽  
Sandeep Arora ◽  
Kelly D. Martin ◽  
Neeru Paharia

Firms spend a substantial amount on lobbying—devoting financial resources on teams of lobbyists to further their interests among regulatory stakeholders. Previous research acknowledges that lobbying positively influences firm value, but it has not examined the parallel effects for customers. Building on the attention-based view (ABV) of the firm, we examine these customer effects. Findings reveal that lobbying negatively affects customer satisfaction so that the positive relationship between lobbying and firm value is mediated by losses to customer satisfaction. These findings suggest a dark side of lobbying and challenge current thinking. However, several customer-focused moderators attenuate the negative effect of lobbying on customer satisfaction, predicted by ABV theory, including the CEO’s background (marketing vs. other functional area) and the firm’s strategic use of resources (advertising spending, R&D spending, or lobbying for product market issues). These moderators ensure consistency between lobbying and customer priorities or direct firm attention toward customers even while firms continue to lobby. Finally, we verify that lobbying reduces the firm’s customer focus by measuring this focus directly using text analysis of firm communications with shareholders. Collectively, the research provides managerial implications for navigating both lobbying activities and customer priorities, and public policy implications for lobbying disclosure requirements.


Author(s):  
P.M. Rice ◽  
MJ. Kim ◽  
R.W. Carpenter

Extrinsic gettering of Cu on near-surface dislocations in Si has been the topic of recent investigation. It was shown that the Cu precipitated hetergeneously on dislocations as Cu silicide along with voids, and also with a secondary planar precipitate of unknown composition. Here we report the results of investigations of the sense of the strain fields about the large (~100 nm) silicide precipitates, and further analysis of the small (~10-20 nm) planar precipitates.Numerous dark field images were analyzed in accordance with Ashby and Brown's criteria for determining the sense of the strain fields about precipitates. While the situation is complicated by the presence of dislocations and secondary precipitates, micrographs like those shown in Fig. 1(a) and 1(b) tend to show anomalously wide strain fields with the dark side on the side of negative g, indicating the strain fields about the silicide precipitates are vacancy in nature. This is in conflict with information reported on the η'' phase (the Cu silicide phase presumed to precipitate within the bulk) whose interstitial strain field is considered responsible for the interstitial Si atoms which cause the bounding dislocation to expand during star colony growth.


2006 ◽  
Vol 40 (12) ◽  
pp. 30
Author(s):  
BARBARA J. HOWARD
Keyword(s):  

2008 ◽  
Author(s):  
Ivelina N. Naydenova ◽  
Warren H. Jones
Keyword(s):  

2008 ◽  
Author(s):  
Amanda Poole ◽  
Julie Carswell ◽  
Rhys Lewis ◽  
Deborah Powell ◽  
Bernd Marcus

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