Asymmetrical Reciprocity. From Recognition to Responsibility and Back

In this article, I argue that Hegel’s concept of recognition and Levinas’ concept of responsibility complement each other and lead to the idea of an asymmetrical reciprocity in which the origin of our social relations is not mutual equality, but rather mutual inequality. I will unfold this argument in three steps. I will first work out a fundamental asymmetry of recognition in Hegel by means of the figure of the bondsman before elucidating in a second step the asymmetry of responsibility in Levinas by means of the figure of the hostage. In the last and third step, I will correlate both asymmetries and show how far the asymmetry of recognition and the asymmetry of responsibility constantly develop from and transition into one another in our social relationships

Recognition and Disrespect. Lordship and Bondage in Hegel's Phenomenology of Spirit

With regard to the contemporary discussion of recognition and disrespect in social philosophy, this chapter argues that Hegel is not only a seminal 'theorist of recognition,' but also a sophisticated 'theorist of disrespect.' By means of the relationship of lord and bondsman as developed in the Phenomenology of Spirit it is shown that for Hegel the emergence of recognition not only involves freedom and autonomy but can also result in dependency and asymmetry. Building on this assumption, the paper pursues a threefold aim: first, to show, through a reconstruction of Hegel's thoughts on the development of self-consciousness, that a successful form of subjectivation is only possible when a subject can actualize itself in so called 'egalitarian' and 'differential' acts of recognition. The second part aims at a re-reading of Hegel's thinking of the lord/bondsman-relationship. In opposition to the classic 'heroic reading' of this relationship, I make the case for a 'subaltern reading,' arguing that Hegel presents in the figure of the bondsman a form of asymmetric recognition, in which the subject is bound to those conditions that hold it in disrespect. Finally, the third part aims at a reinterpretation of Hegel's thought from the perspective of disresprect in order to show that the other side of Hegel's theory of recognition forms a theory of symbolic vulnerability. Starting from this theory one can understand the paradoxical dynamic of disrespect that leads subjects to identify with the relations that subjugate them

Linking Covariant and Canonical General Relativity via Local Observers

Hamiltonian gravity, relying on arbitrary choices of "space," can obscure spacetime symmetries. We present an alternative, manifestly spacetime covariant formulation that nonetheless distinguishes between "spatial" and "temporal" variables. The key is viewing dynamical fields from the perspective of a field of observers -- a unit timelike vector field that also transforms under local Lorentz transformations. On one hand, all fields are spacetime fields, covariant under spacetime symmeties. On the other, when the observer field is normal to a spatial foliation, the fields automatically fall into Hamiltonian form, recovering the Ashtekar formulation. We argue this provides a bridge between Ashtekar variables and covariant phase space methods. We also outline a framework where the 'space of observers' is fundamental, and spacetime geometry itself may be observer-dependent.Comment: 8 pages; Essay written for the 2012 Gravity Research Foundation Awards for Essays on Gravitatio

PEPSI deep spectra. I. The Sun-as-a-star

As part of the first Potsdam Echelle Polarimetric and Spectroscopic Instrument (PEPSI) key-science project, we aim to provide well-exposed (viz. deep) high-resolution spectra of representative stellar targets. These spectra will be made available in form of (electronic) atlases. The first star in this series of papers is our Sun. It also acts as a system-performance cornerstone. The deep spectra in this paper are the results of combining up to 100 consecutive exposures per wavelength setting and are compared with other solar flux atlases. Our software for the optimal data extraction and reduction of PEPSI spectra is described and verified with the solar data. Three deep solar flux spectra with a spectral resolution of up to 270,000, a continuous wavelength coverage from 383 nm to 914 nm, and a photon signal to noise ratio (S/N) of between 2,000-8,000:1 depending on wavelength are presented. Additionally, a time-series of 996 high-cadence spectra in one cross disperser is used to search for intrinsic solar modulations. The wavelength calibration based on Th-Ar exposures and simultaneous Fabry-Perot combs enables an absolute wavelength solution within 10 m/s (rms) with respect to the HARPS laser-comb solar atlas and a relative rms of 1.2 m/s for one day. For science demonstration, we redetermined the disk-average solar Li abundance to 1.09+/-0.04 dex on the basis of 3D NLTE model atmospheres. We detected disk-averaged p-mode RV oscillations with a full amplitude of 47 cm/s at 5.5 min. Comparisons with two solar FTS atlases, as well as with the HARPS solar atlas, validate the PEPSI data product. Now, PEPSI/SDI solar-flux spectra are being taken with a sampling of one deep spectrum per day, and are supposed to continue a full magnetic cycle of the Sun.Comment: in press, 13 pages, 8 figures, data available from pepsi.aip.d

IGF-I receptor phosphorylation is impaired in cathepsin X-deficient prostate cancer cells

The cysteine-type peptidase cathepsin X is highly upregulated in several cancers and presumably promotes tumor invasion through bypassing cellular senescence. Here, we present first evidence that the underlying mechanism may involve the regulation of the insulin-like growth factor (IGF) system, a well-known activator of proliferating tumor cells. Cathepsin X deficiency leads to a reduced phosphorylation of the IGF-I receptor in response to IGF-I stimulation. In addition, downstream signaling through focal adhesion kinase was also affected. Taken together, our results indicate that cathepsin X is able to assist in IGF signaling, which may be an important progress toward understanding cathepsin X-dependent tumorigenesis