Varieties of Spiritual Sense: Cusanus and John Smith

This chapter offers a window into the theologies of Cusanus and the Cambridge Platonist John Smith (1618–52) by illuminating their contrasting appropriations of Origen’s concept of the spiritual senses. Both early modern Neoplatonists of sorts, they evince many common concerns even while a definitive link between them remains elusive. This traditional notion in mystical theology is essential to a proper account of Christian experience not adequately addressed by the scholasticism of their times. While both use the language of spiritual sensation throughout their extant works, their understandings thereof are markedly different. Each appropriated and reformulated the spiritual senses to meet their intellectual and religious contexts. Cusa attempted what has been called a synthesis of Aristotelian and Origenist aesthetics while Smith’s Reformed Neoplatonism led him to reject peripatetic philosophy outright. For Cusanus, spiritual sensation is a fundamentally apophatic process whereby we come to “see that we do not see” which points back to the sacramental practices and eschatological hope of the Catholic Church. For Smith, spiritual sensation is a direct and personal kataphatic process whereby we leave unfitting modes of perception behind in exchange for the divine intellect within us. For the Cardinal, ordinary sense perception, including contemplating images, is central. But this sacramental showing includes hiddenness within itself. For this reason spiritual sensation supplies a mediated “foretaste” of things only fully revealed in the eschatological future. Smith, on the other hand, allows little to no positive role for ordinary sense perception. Instead, he emphasizes that spiritual sensation is an intellectual matter more or less achievable in this life. Both sought to reform the Origenist tradition for their own situations sure that contemplation of the divine is more tasted than calculated

Horizontal Branch evolution, metallicity and sdB stars

Context. Abundance anomalies have been observed in field sdB stars and in nearly all Horizontal Branch (HB) stars of globular clusters with Teff > 11 000K whatever be the cluster metallicity. Aims. The aim is to determine the abundance variations to be expected in sdB stars and in HB stars of metallicities Z \geq 0.0001 and what observed abundances teach us about hydrodynamical processes competing with atomic diffusion. Methods. Complete stellar evolution models, including the effects of atomic diffusion and radiative acceleration, have been computed from the zero age main-sequence for metallicities of Z0 = 0.0001, 0.001, 0.004 and 0.02. On the HB the masses were selected to cover the Teff interval from 7000 to 37000K. Some 60 evolutionary HB models were calculated. The calculations of surface abundance anomalies during the horizontal branch depend on one parameter, the surface mixed mass. Results. For sdB stars with Teff 11 000K in all observed clusters, independent of metallicity, it was found that most observed abundance anomalies (even up to ~ x 200) were compatible, within error bars, with expected abundances. A mixed mass of ~1.E-7 M\odot was determined by comparison with observations. Conclusions. Observations of globular cluster HB stars with Teff > 11 000K and of sdB stars with Teff < 37 000K suggest that most observed abundance anomalies can be explained by element separation driven by radiative acceleration occuring at a mass fraction of ~1.E-7 M\odot. Mass loss or turbulence appear to limit the separation between 1.E-7 M\odot and the surface.Comment: Accepted for publication by A&

What part of Fides Quaerens don’t you Intellectum ? On the Persistent Philosophical Misunderstanding of Anselm’s Ontological Argument

A *very* rough draft of a paper on Anselm's "ontological argument" in which I argue that the argument in the Proslogion rests on a robust notion of having "that then which nothing greater can be thought" in one's mind

Microbiota, Oral Microbiome, and Pancreatic Cancer

Only 30% of patients diagnosed with pancreatic cancer survive one year post-diagnosis. Progress in understanding the causes of pancreatic cancer has been made, including solidifying the associations with obesity and diabetes, and a proportion of cases should be preventable through lifestyle modifications. Unfortunately, identifying reliable biomarkers of early pancreatic cancer has been extremely challenging, and no effective screening modality is currently available for this devastating form of cancer. Recent data suggest the microbiota may play a role in the disease process, but many questions remain. Future studies focusing on the human microbiome, both etiologically and as a marker of disease susceptibility, should shed light on how to better tackle prevention, early detection, and treatment of this highly fatal disease

Self-sustained oscillations in a Large Magneto-Optical Trap

We have observed self-sustained radial oscillations in a large magneto-optical trap (MOT), containing up to $10^{10}$ Rb$^{85}$ atoms. This instability is due to the competition between the confining force of the MOT and the repulsive interaction associated with multiple scattering of light inside the cold atomic cloud. A simple analytical model allows us to formulate a criterion for the instability threshold, in fair agreement with our observations. This criterion shows that large numbers of trapped atoms $N>10^9$ are required to observe this unstable behavior.Comment: submitted to Phys. Rev. Lett. 4 pages, 3 figure

The IDSA and the homogeneous sphere: Issues and possible improvements

In this paper, we are concerned with the study of the Isotropic Diffusion Source Approximation (IDSA) (Baxter et al., Phys. Rev. E 73, 046118, 2006) of radiative transfer. After having recalled well-known limits of the radiative transfer equation, we present the IDSA and adapt it to the case of the homogeneous sphere. We then show that for this example the IDSA suffers from severe numerical difficulties. We argue that these difficulties originate in the min-max switch coupling mechanism used in the IDSA. To overcome this problem we reformulate the IDSA to avoid the problematic coupling. This allows us to access the modeling error of the IDSA for the homogeneous sphere test case. The IDSA is shown to overestimate the streaming component, hence we propose a new version of the IDSA which is numerically shown to be more accurate than the old one. Analytical results and numerical tests are provided to support the accuracy of the new proposed approximation.Comment: 25 pages, 8 figures, accepted for publication in DCDS-

Instagram

Overview: Capturing pictures helps to preserve memories that will be saved forever, and looking at them allows someone to take a journey back in time to when any given picture was taken. In this day and age, smartphones such as Androids and iPhones help to make picture taking quick and easy. With the swipe of a finger and a tap on the screen, a picture can be taken and saved on a camera roll in mere seconds. But it doesn\u27t stop there, with the smartphone application (app) called Instagram, photography can be taken to the next level. Instagram is a website, and also a free app, compatible with most smartphones. It is a form of social media in which users create a profile, including their name and a small biography about themselves. It allows them to upload and post pictures or short fifteen-second videos of anything they please and include a caption that goes with it. Both gender and age play defining roles in how the user actually uses the app. When looking at gender, it is interesting to explore the differences between what men and women post and how often they post. It is suspected there are differences in their usage because of cultural context. In general, women like to share with others what is going on with their lives and men are usually more reserved. This could potentially explain why women post more often, so their followers know what they are experiencing. Age is also something that impacts usage. When looking at the younger generations compared to the older, there is a difference in what and how often they post as well, so it would be interesting to explore why in fact there is this inconsistency in posting rates. Different ages have different audiences, so this could play into why they post what they do. Maybe the younger generation posts more to look cool, and maybe the older generation does not post as much, because they are consumed with more important things, such as work or school. I want to illustrate a clear picture about why there is this split through asking questions about purpose of usage, why they post, and why they post what they post. In summary, I want to uncover what kind of identity they are forming for themselves based on their Instagram activity, and how what they post and like shows others who they are in the social media world