Body and Grotesque as Self-Disruption in Kerstin Hensel’s Gothic East(ern) German Novel Lärchenau (2008)

[EN] By analysing the novel Lärchenau and its -to a certain point- gothic features, this article interprets the elaboration of body in this novel as a site of the expression of power, but also as an alternative language. The grotesque dimension and the representation of the bodily numbness and pain as projections of historical awareness are key elements for the interpretation of Lärchenau in the context of Post-Unification Germany.

Wende und Körperdarstellung in Hensels Lärchenau

[EN] Kerstin Hensel’s literary universe is haunted by fallen heroes, outsiders and gregarious figures with no success. They experience the German Wende in a very peculiar constellation, they perceive Post-Unification Germany at times from a fantastic perspective, always from a painful experience. In this context the analysis of the representations of the body in Hensel’s narrative before and after 1989 offers a rich insight on Hensel’s critical view of Post-Unification Germany. By analysing her texts such as Hallimasch and Lärchenau this article shows that the suffering grotesque bodies in both works stand for a political metaphor of a social body with hardly a cure.

Hartle's model within the general theory of perturbatiye matchings: the change in mass

Hartle's model provides the most widely used analytic framework to describe isolated compact bodies rotating slowly in equilibrium up to second order in perturbations in the context of General Relativity. Apart from some explicit assumptions, there are some implicit, like the "continuity" of the functions in the perturbed metric across the surface of the body. In this work we sketch the basics for the analysis of the second order problem using the modern theory of perturbed matchings. In particular, the result we present is that when the energy density of the fluid in the static configuration does not vanish at the boundary, one of the functions of the second order perturbation in the setting of the original work by Hartle is not continuous. This discrepancy affects the calculation of the change in mass of the rotating star with respect to the static configuration needed to keep the central energy density unchanged.