Effect of a Tibetan herbal mixture on microvascular endothelial function, heart rate variability and biomarkers of inflammation, clotting and coagulation

In this 6-week prospective, randomized, placebo-controlled and double-blind study, we investigated the effects of a natural herbal remedy based on a recipe from Tibet (Padma® 28), on microvascular endothelial function, heart rate variability and biomarkers of inflammation, clotting and coagulation in 80 coronary artery disease (CAD) patients (age 66 ± 8 years) on guideline-based medication for secondary prevention. We found no significant effects of Padma 28 and conclude that the addition of Padma 28 to guideline-based secondary prevention treatment of CAD did not lead to significant effects on important surrogate markers in elderly male CAD patients.

Dispersion relation for hadronic light-by-light scattering: theoretical foundations

In this paper we make a further step towards a dispersive description of the hadronic light-by-light (HLbL) tensor, which should ultimately lead to a data-driven evaluation of its contribution to (g − 2) μ . We first provide a Lorentz decomposition of the HLbL tensor performed according to the general recipe by Bardeen, Tung, and Tarrach, generalizing and extending our previous approach, which was constructed in terms of a basis of helicity amplitudes. Such a tensor decomposition has several advantages: the role of gauge invariance and crossing symmetry becomes fully transparent; the scalar coefficient functions are free of kinematic singularities and zeros, and thus fulfill a Mandelstam double-dispersive representation; and the explicit relation for the HLbL contribution to (g − 2) μ in terms of the coefficient functions simplifies substantially. We demonstrate explicitly that the dispersive approach defines both the pion-pole and the pion-loop contribution unambiguously and in a model-independent way. The pion loop, dispersively defined as pion-box topology, is proven to coincide exactly with the one-loop scalar QED amplitude, multiplied by the appropriate pion vector form factors.

Explication as a Method of Conceptual Re-engineering

Taking Carnap’s classic exposition as a starting point, this paper develops a pragmatic account of the method of explication, defends it against a range of challenges and proposes a detailed recipe for the practice of explicating. It is then argued that confusions are involved in characterizing explications as definitions, and in advocating precising definitions as an alternative to explications. Explication is better characterized as conceptual re-engineering for theoretical purposes, in contrast to conceptual re-engineering for other purposes and improving exactness for purely practical reasons. Finally, three limitations which call for further development of the method of explication are discussed.

Room for Experiment: The Countess of Arundel’s "Site of Medication"

The so-called Dutch Pranketing Room of Alethea Talbot, Countess of Arundel, at Tart Hall was a site of domestic experiments, courtly splendour and global ambition. Lady Arundel, the probable author of a famous recipe book, would have used Tart Hall for cooking and experiments as well as for impressive dinner parties, and she would have used large amounts of sugar to create intricate imitations of meat and vegetables to astonish, entertain and delight her guests. Linking household practice with global trade as well as artistic creation, Lady Arundel’s banquets are situated not only between a national tradition of cooking, as it appears in Markham’s manuals, and the new possibilities the arising global trade provided, but also played with a mismatch between taste and sight. This mediating role could be compared to that played by the artists the Countess employed. Within this context it is worth noting that a series of paintings displayed in the building’s gallery showed still lifes, markets, and a cook. The inventory of Tart Hall gives an insight into the world of the widely travelled collector and patron of Van Dyck and Rubens, but raises also a number of questions. In my talk I would like to explore the Countess’ Pranketing Room as a site of mediation between alimentary and painterly experiments, considering the use of recipes, experience, invention and transformation

CHEOPS Performance for Exomoons: The Detectability of Exomoons by Using Optimal Decision Algorithm

Many attempts have already been made to detect exomoons around transiting exoplanets, but the first confirmed discovery is still pending. The experiences that have been gathered so far allow us to better optimize future space telescopes for this challenge already during the development phase. In this paper we focus on the forthcoming CHaraterising ExOPlanet Satellite (CHEOPS), describing an optimized decision algorithm with step-by-step evaluation, and calculating the number of required transits for an exomoon detection for various planet moon configurations that can be observable by CHEOPS. We explore the most efficient way for such an observation to minimize the cost in observing time. Our study is based on PTV observations (photocentric transit timing variation) in simulated CHEOPS data, but the recipe does not depend on the actual detection method, and it can be substituted with, e.g., the photodynamical method for later applications. Using the current state-of-the-art level simulation of CHEOPS data we analyzed transit observation sets for different star planet moon configurations and performed a bootstrap analysis to determine their detection statistics. We have found that the detection limit is around an Earth-sized moon. In the case of favorable spatial configurations, systems with at least a large moon and a Neptune-sized planet, an 80% detection chance requires at least 5-6 transit observations on average. There is also a nonzero chance in the case of smaller moons, but the detection statistics deteriorate rapidly, while the necessary transit measurements increase quickly. After the CoRoT and Kepler spacecrafts, CHEOPS will be the next dedicated space telescope that will observe exoplanetary transits and characterize systems with known Doppler-planets. Although it has a smaller aperture than Kepler (the ratio of the mirror diameters is about 1/3) and is mounted with a CCD that is similar to Kepler's, it will observe brighter stars and operate with larger sampling rate; therefore, the detection limit for an exomoon can be the same as or better, which will make CHEOPS a competitive instruments in the quest for exomoons.