A Multi-Theory Approach to Managing Knowledge Assets: The Case of Complex Professional Human Service Organizations

A multi-theory framework is offered for guiding managerial decision making in complex professional human service organizations; a growing segment of the economy for which the ability to proactively and dynamically manage knowledge assets is naturally critical to performance. Following a call for greater theoretical integration, this framework synthesizes essential and complimentary elements of three theoretical domains. It combines Transaction Economics’ focus on the appropriate procurement of knowledge assets, with Knowledge Management’s focus on how to dynamically unleash the potential of those assets, and Contingency Thinking’s focus on how to structurally harness and direct that potential. Two key “bridging constructs” emerge offering useful insights both for theory and practice: 1) learning systems as a key element of functional design for managing knowledge assets, and 2) learning costs as a key factor in managing the economic structure of knowledge assets. We apply our integrated framework to two professional human services sectors – business education and health service delivery– and discuss broader implications for research and practice

Navigating the innovation landscape: past research, present practice, and future trends

The management of innovation is among the most critical capabilities contributing to the success of modern organizations. It is also complex and frequently misunderstood. In this paper we first provide a broad overview of the organizational innovation literature [the Past] to distill five fundamental themes: What is innovation, why is it important, where does it come from, who engages in it, and how can it be best executed? Second, we illustrate how these concepts are applied by three companies on the vanguard of innovation management [the Present] – Google, Walt Disney, and Johnson & Johnson. Third, we project the discussion forward by considering key issues and emerging trends [the Future] of innovation management such as nanotechnology, ethical dilemmas, information technology, globalization, and sustainability. Fourth, we derive from the above analyses concrete guidelines for managers to leverage these insights and enable more effective innovation practices

Near-Infrared Molecular Hydrogen Emission from the Central Regions of Galaxies: Regulated Physical Conditions in the Interstellar Medium

The central regions of many interacting and early-type spiral galaxies are actively forming stars. This process affects the physical and chemical properties of the local interstellar medium as well as the evolution of the galaxies. We observed near-infrared H2 emission lines: v=1-0 S(1), 3-2 S(3), 1-0 S(0), and 2-1 S(1) from the central ~1 kpc regions of the archetypical starburst galaxies, M82 and NGC 253, and the less dramatic but still vigorously star-forming galaxies, NGC 6946 and IC 342. Like the far-infrared continuum luminosity, the near-infrared H2 emission luminosity can directly trace the amount of star formation activity because the H2 emission lines arise from the interaction between hot and young stars and nearby neutral clouds. The observed H2 line ratios show that both thermal and non-thermal excitation are responsible for the emission lines, but that the great majority of the near-infrared H2 line emission in these galaxies arises from energy states excited by ultraviolet fluorescence. The derived physical conditions, e.g., far-ultraviolet radiation field and gas density, from [C II] and [O I] lines and far-infrared continuum observations when used as inputs to photodissociation models, also explain the luminosity of the observed H2 v=1-0 S(1) line. The ratio of the H2 v=1-0 S(1) line to far-IR continuum luminosity is remarkably constant over a broad range of galaxy luminosities; L_H2/L_FIR = about 10^{-5}, in normal late-type galaxies (including the Galactic center), in nearby starburst galaxies, and in luminous IR galaxies (LIRGs: L_FIR > 10^{11} L_sun). Examining this constant ratio in the context of photodissociation region models, we conclude that it implies that the strength of the incident UV field on typical molecular clouds follows the gas density at the cloud surface.Comment: Accepted for ApJ, 24 pages, 17 figures, for complete PDF file, see http://kao.re.kr/~soojong/mypaper/2004_pak_egh2.pd

Comparative acute efficacy and tolerability of OROS and immediate release formulations of methylphenidate in the treatment of adults with attention-deficit/hyperactivity disorder

<p>Abstract</p> <p>Background</p> <p>The main aim of this study was to compare the safety and efficacy of IR MPH administered three times daily to those of once daily OROS-MPH.</p> <p>Methods</p> <p>Subjects were outpatient adults satisfying full diagnostic criteria for DSM-IV ADHD between 19 and 60 years of age. Data from two independently conducted 6-week placebo controlled, randomized clinical trials of IR-MPH (tid) and of OROS-MPH were pooled to create three study groups: Placebo (N = 116), IR-MPH (tid) (N = 102) and OROS-MPH (N = 67).</p> <p>Results</p> <p>Eight-five percent (N = 99) of placebo treated subjects, 77% (N = 79) of the IR-MPH (tid) treated subjects, and 82% (N = 55) of the OROS-MPH treated subjects completed the 6-week trial. Total daily doses at endpoint were 80.9 ± 31.9 mg, 74.8 ± 26.2 mg, and 95.4 ± 26.3 mg in the OROS-MPH, IR-MPH (tid), and placebo groups, respectively. At endpoint, 66% (N = 44) of subjects receiving OROS-MPH and 70% (N = 71) of subjects receiving IR-MPH (tid) were considered responders compared with 31% (N = 36) on placebo.</p> <p>Conclusion</p> <p>Comparison of data from two similarly designed, large, randomized, placebo-controlled, trials, showed that equipotent daily doses of once daily OROS-MPH had similar efficacy to that of TID administered IR MPH.</p> <p>Trial Registration</p> <p>The trial of OROS-MPH was registered at clinicaltrials.gov, number NCT00181571.</p

The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey

We present measurements of the cosmic microwave background (CMB) power spectrum made by the Atacama Cosmology Telescope at 148 GHz and 218 GHz, as well as the cross-frequency spectrum between the two channels. Our results clearly show the second through the seventh acoustic peaks in the CMB power spectrum. The measurements of these higher-order peaks provide an additional test of the {\Lambda}CDM cosmological model. At l > 3000, we detect power in excess of the primary anisotropy spectrum of the CMB. At lower multipoles 500 < l < 3000, we find evidence for gravitational lensing of the CMB in the power spectrum at the 2.8{\sigma} level. We also detect a low level of Galactic dust in our maps, which demonstrates that we can recover known faint, diffuse signals.Comment: 19 pages, 13 figures. Submitted to ApJ. This paper is a companion to Hajian et al. (2010) and Dunkley et al. (2010