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One of the more annoying aspects of the life of a popular music academic is that we study music that is primarily made and used by people who seem to have no interest at all in what we have to say. Popular musicians and fans are engaged with what we're talking about but not with how we talk about it. When the first volume of our history of live music came out, covering 1950–67 (Frith et al. 2013), I did some non-academic promotional work for it – presenting our book at a literary festival, library events and pensioners’ clubs (these were the people who had lived through what we were describing). Audiences were, like my non-academic friends, sufficiently interested in live music history to discuss our findings with enthusiasm but, at the same time, found the book unreadable. They couldn't be doing with academic research conventions, with the references constantly interrupting the narrative flow, with the painstaking collection and assessment of evidence, the stolid back and forth between the particular (the facts) and the general (the concepts).
We continue with the systematic study of the speed of extinction of continuous-state branching processes in Lévy environments under more general branching mechanisms. Here, we deal with the weakly subcritical regime under the assumption that the branching mechanism is regularly varying. We extend recent results of Li and Xu (2018) and Palau et al. (2016), where it is assumed that the branching mechanism is stable, and complement the recent articles of Bansaye et al. (2021) and Cardona-Tobón and Pardo (2021), where the critical and the strongly and intermediate subcritical cases were treated, respectively. Our methodology combines a path analysis of the branching process together with its Lévy environment, fluctuation theory for Lévy processes, and the asymptotic behaviour of exponential functionals of Lévy processes. Our approach is inspired by the last two previously cited papers, and by Afanasyev et al. (2012), where the analogue was obtained.
This article firstly advances a methodological critique of Hans-Joachim Voth's influential study of labour input during the English industrial revolution, arguing that Voth's ingenious and potentially widely applicable method of inferring time-use from court testimony has flaws such that at least the absolute figures yielded are likely unreliable. Secondly, with the method's deficiencies in mind, this article applies a version of it to the Old Bailey court records in order to examine change in women's working time in London between the 1750s and 1830. Results include that women in London did not observe Saint Monday even in the 1750s, and that the time that women in London spent in paid work increased only slightly between the 1750s and 1830.
Archaeological narratives have traditionally associated the rise of social and political ‘complexity’ with the emergence of agricultural societies. However, this framework neglects the innovations of the hunter-gatherer populations occupying the Siberian taiga 8000 years ago, including the construction of some of the oldest-known fortified sites in the world. Here, the authors present results from the fortified site of Amnya in western Siberia, reporting new radiocarbon dates as the basis for a re-evaluation of the chronology and settlement organisation. Assessed within the context of the changing social and environmental landscape of the taiga, Amnya and similar fortified sites can be understood as one facet of a broader adaptive strategy.
Pharmacy Benefit Managers (PBM) induce drug manufacturers to offer rebates to insurers and employers by denying coverage through formulary exclusions, impeding physician prescription through prior authorization, and reducing patient drug use through cost sharing. As they tighten these access obstacles, PBMs reduce the net prices received by the manufacturers.
This article confronts the challenges and opportunities presented by medical-legal partnerships (MLPs) representing families impacted by the family regulation system. Based on the authors’ experience developing a collaboration between a medical-legal partnership, interdisciplinary law school clinic and nurse home visiting program focused on clients impacted by the family regulation system, the article challenges traditional conceptions of the MLP model and proposes an expanded vision for MLPs to address systemic injustice and improve outcomes for families.
The Classic Maya polities of Baking Pot and Lower Dover developed along two dramatically different trajectories. At Baking Pot, the capital and associated apical elite regime grew concomitantly with surrounding populations over a thousand-year period. The smaller polity of Lower Dover, in contrast, formed when a Late Classic political center was established by an emergent apical elite regime amidst several long-established intermediate elite-headed districts. The different trajectories through which these polities formed should have clear implications for residential size variability. We employ the Gini coefficient to measure variability in household volume to compare patterns of residential size differentiation between the two polities. The Gini coefficients, while similar, suggest greater differentiation in residential size at Baking Pot than at Lower Dover, likely related to the centralized control of labor by the ruling elite at Baking Pot. While the Gini coefficient is synonymous with measuring wealth inequalities, we suggest that in the Classic period Belize River Valley, residential size was more reflective of labor control.
Compact obscured nuclei (CONs) are relatively common in the centers of local (U)LIRGs, yet their nature remains unknown. Both AGN activity and extreme nuclear starbursts have been suggested as plausible nuclear power sources. The prevalence of outflows in these systems suggest that CONs represent a key phase in the nuclear feedback cycle, in which material is ejected from the central regions of the galaxy. Here, we present results from MUSE for the confirmed local CON galaxy NGC4418. For the first time we spatially map the spectral features and kinematics of the galaxy in the optical, revealing several previously unknown structures. In particular, we discover a bilateral outflow along the minor axis, an outflowing bubble, several knot structures and a receding outflow partially obscured by the galactic disk. Based on the properties of these features, we conclude that the CON in NGC4418 is most likely powered by an AGN.