James M. Buchanan 2018
DOI: 10.1007/978-3-030-03080-3_47
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Paretian Fiscal Sociology

Abstract: This work is a draft chapter for the forthcoming book "James Buchanan: A Theorist of Political Economy and Social Philosophy", which is being edited by Ricard E Wagner for Palgrave Macmillan. It considers Pareto's treatment of fiscal issues, first as a middle age economist and subsequently as a mature age sociologist. It establishes that Pareto never regarded fiscal studies as a purely theoretical exercise. Even as an economist, he relegated 'fiscal effects' to the aspect of applied economics that he called th… Show more

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“…Note how cosmic downsizing implies that fewer FRII quasars will form at low redshift since FRII quasars require retrograde accretion in the paradigm which occurs only if the following conditions apply: 1) They occur statistically only in a -26subset of major mergers but the merger function drops with decrease in redshift (Bertone & Conselice 2009;Treister et al 2012); 2) retrograde accretion is unstable unless the black hole is massive (Perego et al 2009;Garofalo 2013b), so less massive black holes are less likely to live long in retrograde configurations. And the observations in fact support this idea (Dunlop et al 2003;McLure & Jarvis 2004;Floyd et al 2013). This drop in the density of FRII objects as the redshift decreases is captured in Figure 1, with the smaller size of the FRII boxes.…”
Section: Agn-star Formation Link and Peak In Jet Vs Disk Powermentioning
confidence: 88%
“…Note how cosmic downsizing implies that fewer FRII quasars will form at low redshift since FRII quasars require retrograde accretion in the paradigm which occurs only if the following conditions apply: 1) They occur statistically only in a -26subset of major mergers but the merger function drops with decrease in redshift (Bertone & Conselice 2009;Treister et al 2012); 2) retrograde accretion is unstable unless the black hole is massive (Perego et al 2009;Garofalo 2013b), so less massive black holes are less likely to live long in retrograde configurations. And the observations in fact support this idea (Dunlop et al 2003;McLure & Jarvis 2004;Floyd et al 2013). This drop in the density of FRII objects as the redshift decreases is captured in Figure 1, with the smaller size of the FRII boxes.…”
Section: Agn-star Formation Link and Peak In Jet Vs Disk Powermentioning
confidence: 88%