Density Distribution of a Bose-Einstein Condensate of Photons in a Dye-Filled Microcavity

The achievement of Bose-Einstein condensation of photons (phBEC) in a dye-filled microcavity has led to a renewed interest in the density distribution of the ideal Bose gas in a two-dimensional harmonic oscillator. We present measurements of the radial profile of photons inside the microcavity below and above the critical point for phBEC with a good signal-to-noise ratio. We obtain a good agreement with theoretical profiles obtained using exact summation of eigenstates.Comment: 5 pages, 4 figure

Density Distribution of a Bose-Einstein Condensate of Photons in a Dye-Filled Microcavity

The achievement of Bose-Einstein condensation of photons (phBEC) in a dye-filled microcavity has led to a renewed interest in the density distribution of the ideal Bose gas in a two-dimensional harmonic oscillator. We present measurements of the radial profile of photons inside the microcavity below and above the critical point for phBEC with a good signal-to-noise ratio. We obtain a good agreement with theoretical profiles obtained using exact summation of eigenstates.Comment: 5 pages, 4 figure

Surface structure of thin asymmetric PS-b-PMMA diblock copolymers investigated by atomic force microscopy

Asymmetric poly(styrene-b-methyl methacrylate) (PS-b-PMMA) diblock copolymers of molecular weight M-n = 29,700g mol(-1) (M-PS = 9300 g mol(-1) M-PMMA = 20,100 g mol(-1), PD = 1.15, chi(PS) = 0.323, chi(PMMA) = 0.677) and M-n = 63,900 g mol(-1) (M-PS = 50,500 g mol(-1), M-PMMA = 13,400 g mol(-1), PD = 1.18, chi(PS) = 0.790, chi(PMMA) = 0.210) were prepared via reversible addition-fragmentation chain transfer (RAFT) polymerization. Atomic force microscopy (AFM) was used to investigate the surface structure of thin films, prepared by spin-coating the diblock copolymers on a silicon substrate. We show that the nanostructure of the diblock copolymer depends on the molecular weight and volume fraction of the diblock copolymers. We observed a perpendicular lamellar structure for the high molar mass sample and a hexagonal-packed cylindrical patterning for the lower molar mass one. Small-angle X-ray scattering investigation of these samples without annealing did not reveal any ordered structure. Annealing of PS-b-PMMA samples at 160 degrees C for 24 h led to a change in surface structure

Utilisation de la mesure thermique du flux de sève pour l'évaluation de la transpiration d'un palmier dattier

International audienceL'amélioration de la gestion de l'eau en système oasien constitue l'un des principaux défis pour la préservation de son agrosystème. Des approches complémentaires doivent être mises en oeuvre pour y contribuer par la prise en compte du comportement des agriculteurs mais aussi par la compréhension du système biophysique. En particulier, la quantification des différents termes du bilan hydrique, et notamment celui de la transpiration du palmier dattier, a été relativement peu étudiée jusqu'à présent. Le terme de consommation hydrique du palmier est un indicateur indispensable en regard des contraintes de gestion de l'eau et du bilan hydrique global. Cette problématique a été abordée au sein de l'oasis de Fatnassa Nord à Kébili (33°,8 N ; 8°,7 E) dans un contexte caractérisé à la fois par de faibles fréquences de tour d'eau et une salinité plutôt élevée. L'agrosystème bi-étagée palmier/fourrage du système oasien de cette région nécessite de bien cerner la composante palmier de la strate fourrage. Une technique de mesure thermique du flux de sève a donc été mise en oeuvre pour évaluer la transpiration spécifique du palmier dattier au sein d'une parcelle dont les termes du bilan hydriques sont bien mesurés en continu. L'avantage de cette méthode est qu'elle permet aussi une mesure continue et qu'elle intègre, grâce au suivi simultané de quatre arbres, une certaine hétérogénéité du système palmier à la fois due au système radiculaire et au développement de la canopée, tous deux liés au stipe, voie unique de passage de la sève entre ces deux compartiments de l'arbre. Dans cet article, les principaux résultats des mesures réalisées depuis plus d'un an sont analysés et présentent une bonne cohérence avec la dynamique nycthémérale de la nappe superficielle donnée par un suivi piézométrique fin. Les flux de transpiration cumulés sur la journée ont varié globalement de 0.5 à 3,5 mm/j avec une moyenne de l'ordre de 2 mm/jour reflétant une consommation hydrique modeste en regard de la demande climatique. Les valeurs montrent également que ces flux journaliers, malgré leur variation inter-arbres importantes, varient en lien étroit avec le cycle des apports d'eau par irrigation. Le palmier étant malgré sa résistance aux conditions climatiques, dont en particulier une demande forte, une espèce qui régule ses pertes par régulation stomatique

Ethical difficulties in clinical practice : experiences of European doctors

Background: Ethics support services are growing in Europe to help doctors in dealing with ethical difficulties. Currently, insufficient attention has been focused on the experiences of doctors who have faced ethical difficulties in these countries to provide an evidence base for the development of these services. Methods: A survey instrument was adapted to explore the types of ethical dilemma faced by European doctors, how they ranked the difficulty of these dilemmas, their satisfaction with the resolution of a recent ethically difficult case and the types of help they would consider useful. The questionnaire was translated and given to general internists in Norway, Switzerland, Italy and the UK. Results: Survey respondents (n = 656, response rate 43%) ranged in age from 28 to 82 years, and averaged 25 years in practice. Only a minority (17.6%) reported having access to ethics consultation in individual cases. The ethical difficulties most often reported as being encountered were uncertain or impaired decisionmaking capacity (94.8%), disagreement among caregivers (81.2%) and limitation of treatment at the end of life (79.3%). The frequency of most ethical difficulties varied among countries, as did the type of issue considered most difficult. The types of help most often identified as potentially useful were professional reassurance about the decision being correct (47.5%), someone capable of providing specific advice (41.1%), help in weighing outcomes (36%) and clarification of the issues (35.9%). Few of the types of help expected to be useful varied among countries. Conclusion: Cultural differences may indeed influence how doctors perceive ethical difficulties. The type of help needed, however, did not vary markedly. The general structure of ethics support services would not have to be radically altered to suit cultural variations among the surveyed countries

No planet for HD 166435

The G0V star HD166435 has been observed by the fiber-fed spectrograph ELODIE as one of the targets in the large extra-solar planet survey that we are conducting at the Observatory of Haute-Provence. We detected coherent, low-amplitude, radial-velocity variations with a period of 3.7987days, suggesting a possible close-in planetary companion. Subsequently, we initiated a series of high-precision photometric observations to search for possible planetary transits and an additional series of CaII H and K observations to measure the level of surface magnetic activity and to look for possible rotational modulation. Surprisingly, we found the star to be photometrically variable and magnetically active. A detailed study of the phase stability of the radial-velocity signal revealed that the radial-velocity variability remains coherent only for durations of about 30days. Analysis of the time variation of the spectroscopic line profiles using line bisectors revealed a correlation between radial velocity and line-bisector orientation. All of these observations, along with a one-quarter cycle phase shift between the photometric and the radial-velocity variationss, are well explained by the presence of dark photospheric spots on HD166435. We conclude that the radial-velocity variations are not due to gravitational interaction with an orbiting planet but, instead, originate from line-profile changes stemming from star spots on the surface of the star. The quasi-coherence of the radial-velocity signal over more than two years, which allowed a fair fit with a binary model, makes the stability of this star unusual among other active stars. It suggests a stable magnetic field orientation where spots are always generated at about the same location on the surface of the star.Comment: 9 pages, 8 figures, Accepted for publication in A&