Fresnel laws at curved dielectric interfaces of microresonators

We discuss curvature corrections to Fresnel's laws for the reflection and transmission of light at a non-planar refractive-index boundary. The reflection coefficients are obtained from the resonances of a dielectric disk within a sequential-reflection model. The Goos-H\"anchen effect for curved light fronts at a planar interface can be adapted to provide a qualitative and quantitative extension of the ray model which explains the observed deviations from Fresnel's laws.Comment: submitted to Phys. Rev.

Pentacene islands grown on ultra-thin SiO2

Ultra-thin oxide (UTO) films were grown on Si(111) in ultrahigh vacuum at room temperature and characterized by scanning tunneling microscopy. The ultra-thin oxide films were then used as substrates for room temperature growth of pentacene. The apparent height of the first layer is 1.57 +/- 0.05 nm, indicating standing up pentacene grains in the thin-film phase were formed. Pentacene is molecularly resolved in the second and subsequent molecular layers. The measured in-plane unit cell for the pentacene (001) plane (ab plane) is a=0.76+/-0.01 nm, b=0.59+/-0.01 nm, and gamma=87.5+/-0.4 degrees. The films are unperturbed by the UTO's short-range spatial variation in tunneling probability, and reduce its corresponding effective roughness and correlation exponent with increasing thickness. The pentacene surface morphology follows that of the UTO substrate, preserving step structure, the long range surface rms roughness of ~0.1 nm, and the structural correlation exponent of ~1.Comment: 15 pages, 4 figure

Differential sensitivity of murine leukemia virus to APOBEC3-mediated inhibition is governed by virion exclusion

While members of the APOBEC3 family of human intrinsic resistance factors are able to restrict the replication of Vif-deflcient forms of human immunodeficiency virus type 1 (HIV-1), they are unable to block replication of wild-type HIV-1 due to the action of Vif, which induces their degradation. In contrast, HIV-1 Vif is unable to block inhibition mediated by APOBEC3 proteins expressed by several heterologous species, including mice. Here, we have asked whether the simple retrovirus murine leukemia virus (MLV) is sensitive to restriction by the cognate murine or heterologous, human APOBEC3 proteins. We demonstrate that MLV is highly sensitive to inhibition by human APOBEC3G and APOBEC3B but resistant to inhibition by murine APOBEC3 or by other human APOBEC3 proteins, including APOBEC3F. This sensitivity fully correlates with the ability of these proteins to be packaged into MLV virion particles: i.e., human APOBEC3G and APOBEC3B are packaged while murine APOBEC3 and human APOBEC3F are excluded. Moreover, this packaging in turn correlates with the differential ability of these APOBEC3 proteins to bind MLV Gag. Together, these data suggest that MLV Gag has evolved to avoid binding, and hence virion packaging, of the cognate murine APOBEC3 protein but that MLV infectivity is still restricted by certain heterologous APOBEC3 proteins that retain this ability. Moreover, these results suggest that APOBEC3 proteins may help prevent the zoonotic infection of humans by simple retroviruses and provide a mechanism for how simple retroviruses can avoid inhibition by APOBEC3 family members

Genetic Modification of Human Peripheral Blood Lymphocytes with a Transdominant Negative Form of Rev: Safety and Toxicity

Overview summary Expression of Rev M10, a transdominant mutant form of the Rev gene, in T cell lines confers resistance to HIV in vitro. Isertion of this Rev M10 gene into PBL appears to be nontoxic and well-tolerated by SCID mice. These results demonstrate that genetic modification of T cells by an antiviral gene can be performed safely and without overt toxicity. This finding encourages the development of therapeutic strategies to genetically protect T cells to prolong their survival in HIV-infected individuals.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/63234/1/hum.1995.6.8-997.pd

Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adopting the GW event's 3D localization, to less than 2×1051-2×1054 erg. © 2017 American Physical Society

NEOTROPICAL XENARTHRANS: a data set of occurrence of xenarthran species in the Neotropics

Xenarthrans – anteaters, sloths, and armadillos – have essential functions for ecosystem maintenance, such as insect control and nutrient cycling, playing key roles as ecosystem engineers. Because of habitat loss and fragmentation, hunting pressure, and conflicts with 24 domestic dogs, these species have been threatened locally, regionally, or even across their full distribution ranges. The Neotropics harbor 21 species of armadillos, ten anteaters, and six sloths. Our dataset includes the families Chlamyphoridae (13), Dasypodidae (7), Myrmecophagidae (3), Bradypodidae (4), and Megalonychidae (2). We have no occurrence data on Dasypus pilosus (Dasypodidae). Regarding Cyclopedidae, until recently, only one species was recognized, but new genetic studies have revealed that the group is represented by seven species. In this data-paper, we compiled a total of 42,528 records of 31 species, represented by occurrence and quantitative data, totaling 24,847 unique georeferenced records. The geographic range is from the south of the USA, Mexico, and Caribbean countries at the northern portion of the Neotropics, to its austral distribution in Argentina, Paraguay, Chile, and Uruguay. Regarding anteaters, Myrmecophaga tridactyla has the most records (n=5,941), and Cyclopes sp. has the fewest (n=240). The armadillo species with the most data is Dasypus novemcinctus (n=11,588), and the least recorded for Calyptophractus retusus (n=33). With regards to sloth species, Bradypus variegatus has the most records (n=962), and Bradypus pygmaeus has the fewest (n=12). Our main objective with Neotropical Xenarthrans is to make occurrence and quantitative data available to facilitate more ecological research, particularly if we integrate the xenarthran data with other datasets of Neotropical Series which will become available very soon (i.e. Neotropical Carnivores, Neotropical Invasive Mammals, and Neotropical Hunters and Dogs). Therefore, studies on trophic cascades, hunting pressure, habitat loss, fragmentation effects, species invasion, and climate change effects will be possible with the Neotropical Xenarthrans dataset

First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the case of known pulsars a fully coherent search, based on matched filtering, which uses the position and rotational parameters obtained from electromagnetic observations, can be carried out. Matched filtering maximizes the signal-to-noise (SNR) ratio, but a large sensitivity loss is expected in case of even a very small mismatch between the assumed and the true signal parameters. For this reason, narrow-band analysis methods have been developed, allowing a fully coherent search for gravitational waves from known pulsars over a fraction of a hertz and several spin-down values. In this paper we describe a narrow-band search of 11 pulsars using data from Advanced LIGO's first observing run. Although we have found several initial outliers, further studies show no significant evidence for the presence of a gravitational wave signal. Finally, we have placed upper limits on the signal strain amplitude lower than the spin-down limit for 5 of the 11 targets over the bands searched; in the case of J1813-1749 the spin-down limit has been beaten for the first time. For an additional 3 targets, the median upper limit across the search bands is below the spin-down limit. This is the most sensitive narrow-band search for continuous gravitational waves carried out so far. © 2017 American Physical Society