Proceedings of the Conference on Globalization and Its Discontents

This paper aims to put forward an original conceptual framework and a renewed perspective on monetary analysis applied to trans-national corporations based on some of the views of Bernard Schmitt developed over the last forty years. After reviewing the terminological principles of the theory of money emissions, we show that Bernard Schmitt’s theoretical insights have enabled the successful integration of money and output at the conceptual level along the lines of a Keynesian monetary theory of production. We then examine the issue of the definition of the trans-national corporation and its exponential rise in the world economy with regard to the globalisation process. Finally, the inclusion of trans-national corporations in the theory of money emissions allows us to redefine transnational production as an additional conceptual level in monetary macroeconomics, with far-reaching implications as far as the monetisation of trans-national production and the subsequent reform of international payments are concerned.trans-national corporations, Bernard Schmitt, Monetary Theory of Production

Can Global Elites Pave the Way for a New Transnational Unit of Account? A Reflection on the Numerical Nature of Money

In this article, we investigate the issue of the dollar-based international monetary system. We start by listing the reasons why money has essentially become a numerical form in the contemporary world economy. After reviewing the salient characteristics of the flawed international monetary and financial architecture of the world economy, we assess whether a transnational unit of account could constitute a viable political alternative to the current international payments system. The latter scenario is envisaged both with regard to the field of international relations and with the help of a revisited definition of the transnational capitalist class

Star polymers reduce IAPP toxicity via accelerated amyloid aggregation

Protein aggregation into amyloid fibrils is a ubiquitous phenomenon across the spectrum of neurodegenerative disorders and type 2 diabetes. A common strategy against amyloidogenesis is to minimize the populations of toxic oligomers and protofibrils by inhibiting protein aggregation with small molecules or nanoparticles. However, melanin synthesis in nature is realized by accelerated protein fibrillation to circumvent accumulation of toxic intermediates. Accordingly, we designed and demonstrated the use of star-shaped poly(2-hydroxyethyl acrylate) (PHEA) nanostructures for promoting the aggregation while ameliorating the toxicity of human islet amyloid polypeptide (IAPP), the peptide involved in glycemic control and the pathology of type 2 diabetes. The binding of PHEA elevated the beta-sheet content in IAPP aggregates while rendered a new morphology of ‘stelliform’ amyloids originating from the polymers. Atomistic molecular dynamics simulations revealed that the PHEA arms served as rod-like scaffolds for IAPP binding and subsequently accelerated IAPP aggregation by increased local peptide concentration. The tertiary structure of the star nanoparticles was found to be essential to drive the specific interactions required to impel the accelerated IAPP aggregation. This study shed new light on the structure-toxicity relationship of IAPP and points to the potential of exploiting star polymers as a new class of therapeutic agents against amyloidogenesis

New standards for reducing gravity data: The North American gravity database

The North American gravity database as well as databases from Canada, Mexico, and the United States are being revised to improve their coverage, versatility, and accuracy. An important part of this effort is revising procedures for calculating gravity anomalies, taking into account our enhanced computational power, improved terrain databases and datums, and increased interest in more accurately defining long-wavelength anomaly components. Users of the databases may note minor differences between previous and revised database values as a result of these procedures. Generally, the differences do not impact the interpretation of local anomalies but do improve regional anomaly studies. The most striking revision is the use of the internationally accepted terrestrial ellipsoid for the height datum of gravity stations rather than the conventionally used geoid or sea level. Principal facts of gravity observations and anomalies based on both revised and previous procedures together with germane metadata will be available on an interactive Web-based data system as well as from national agencies and data centers. The use of the revised procedures is encouraged for gravity data reduction because of the widespread use of the global positioning system in gravity fieldwork and the need for increased accuracy and precision of anomalies and consistency with North American and national databases. Anomalies based on the revised standards should be preceded by the adjective “ellipsoidal” to differentiate anomalies calculated using heights with respect to the ellipsoid from those based on conventional elevations referenced to the geoid

Search for dark matter produced in association with bottom or top quarks in √s = 13 TeV pp collisions with the ATLAS detector

A search for weakly interacting massive particle dark matter produced in association with bottom or top quarks is presented. Final states containing third-generation quarks and miss- ing transverse momentum are considered. The analysis uses 36.1 fb−1 of proton–proton collision data recorded by the ATLAS experiment at √s = 13 TeV in 2015 and 2016. No significant excess of events above the estimated backgrounds is observed. The results are in- terpreted in the framework of simplified models of spin-0 dark-matter mediators. For colour- neutral spin-0 mediators produced in association with top quarks and decaying into a pair of dark-matter particles, mediator masses below 50 GeV are excluded assuming a dark-matter candidate mass of 1 GeV and unitary couplings. For scalar and pseudoscalar mediators produced in association with bottom quarks, the search sets limits on the production cross- section of 300 times the predicted rate for mediators with masses between 10 and 50 GeV and assuming a dark-matter mass of 1 GeV and unitary coupling. Constraints on colour- charged scalar simplified models are also presented. Assuming a dark-matter particle mass of 35 GeV, mediator particles with mass below 1.1 TeV are excluded for couplings yielding a dark-matter relic density consistent with measurements