La vida y la obra de Herbert Marcuse

El brusco descubrimiento y exaltación de MARCUSE como una de las claves de la crisis contemporánea es uno de los fenómenos más notables de nuestro tiempo. [...]

A cooperative appproach to queue allocation of indivisible objects

We consider the allocation of a finite number of indivisible objects to the same number of agents according to an exogenously given queue. We assume that the agents collaborate in order to achieve an efficient outcome for society. We allow for side-payments and provide a method for obtaining stable outcomes.

On games corresponding to sequencing situations with precedence relations

In this paper we study a class of cooperative sequencing games that arise from one-machine sequencing situations in which chain precedence relations are imposed on the jobs. It is shown that these sequencing games are convex.

OpenURL i l'enllaçat SFX

No fa gaires anys de les primeres recerques acadèmiques liderades per Herbert Van de Sompel a la Universitat de Gant a Bèlgica, les quals van donar com a resultat la formulació de l'estàndard OpenURL i el desenvolupament del servidor d'enllaços per a les biblioteques SFX, posant el control dels enllaços en mans del bibliotecari. Aquest article considera breument les primeres iniciatives sobre els enllaços, explica el propòsit i l'estructura d'OpenURL i el paper dels components: les fonts, els objectius i el servidor d'enllaços, centrant-se en el servidor d'enllaços SFX.

Modelling of Mercury’s surface composition and remote detection from the orbit with the BepiColombo Mercury Planetary Orbiter

It can be assumed that the composition of Mercury’s thin gas envelope (exosphere) is related to thecomposition of the planets crustal materials. If this relationship is true, then inferences regarding the bulkchemistry of the planet might be made from a thorough exospheric study. The most vexing of allunsolved problems is the uncertainty in the source of each component. Historically, it has been believedthat H and He come primarily from the solar wind, while Na and K originate from volatilized materialspartitioned between Mercury’s crust and meteoritic impactors. The processes that eject atoms andmolecules into the exosphere of Mercury are generally considered to be thermal vaporization, photonstimulateddesorption (PSD), impact vaporization, and ion sputtering. Each of these processes has its owntemporal and spatial dependence. The exosphere is strongly influenced by Mercury’s highly ellipticalorbit and rapid orbital speed. As a consequence the surface undergoes large fluctuations in temperatureand experiences differences of insolation with longitude. We will discuss these processes but focus moreon the expected surface composition and solar wind particle sputtering which releases material like Caand other elements from the surface minerals and discuss the relevance of composition modelling