Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ~100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is ${16.0}_{-0.6}^{+0.7}$ (${21.3}_{-0.8}^{+1.1}$) cm−2 for muon neutrinos (muon antineutrinos), with an error range of ±5° around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of −2. The fluence limit for neutrino energies less than 100 MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6 × 107 cm−2 for anti-electron neutrinos under the assumption of a Fermi–Dirac spectrum with average energy of 20 MeV

Quantifying the impact of baryon-CDM perturbations on halo clustering and baryon fraction

International audienceBaryons and cold dark matter (CDM) did not comove prior to recombination. This leads to differences in the local baryon and CDM densities, the so-called baryon-CDM isocurvature perturbations δ_bc. These perturbations are usually neglected in the analysis of Large-Scale Structure data but taking them into account might become important in the era of high precision cosmology. Using gravity-only 2-fluid simulations we assess the impact of such perturbations on the dark matter halos distribution. In particular, we focus on the baryon fraction in halos as a function of mass and large-scale δbc, which also allows us to study details of the nontrivial numerical setup required for such simulations. We further measure the cross-power spectrum between the halo field and δbc over a wide range of mass. This cross-correlation is nonzero and negative which shows that halo formation is impacted by δbc. We measure the associated bias parameter bδbc and compare it to recent results, finding good agreement. Finally we quantify the impact of such perturbations on the halo-halo power spectrum and show that this effect can be degenerate with the one of massive neutrinos for surveys like DESI

A New Approach to Upper Eyelid Reconstruction

Background: Reconstruction of large defects of the upper eyelid is challenging because of its complex anatomy and specialized function. The aim of this work is to develop a single-stage reconstruction procedure based on a new approach. The technique consists of the advancement of an orbicularis oculi myocutaneous flap designed within the blepharoplasty skin excision pattern. Methods: After the tumor’s excision is completed with clear margins, the borders of the flap are incised down to the submuscular plane inside the classical pattern of upper eyelid blepharoplasty. Two myocutaneous triangles are excised on both sides of the flap to allow its advancement to cover the defect. When it is necessary to repair the posterior lamella, we harvest a mucochondral graft. Results: From 2012 to 2015, we performed upper eyelid reconstruction with this technique on six patients. The flap survived in all the patients, without total or partial necrosis. No patient required surgical revision. The results were aesthetically satisfying, and no tumor recurrence was noted. Conclusions: Our new approach to upper eyelid reconstruction maximizes the cosmetic outcome respecting the principles of radicality. This flap is better suited for lesions involving the median or paramedian eyelid border from the marginal zone up to the palpebral crease. The approach we propose is safe and versatile, and it ensures either a functional or a good aesthetic reconstruction. Level of Evidence IV: This journal requires that authors assign a level of evidence to each article. For a full description of these Evidence-Based Medicine ratings, please refer to the Table of Contents or the online Instructions to Authors www.springer.com/00266

Organization of Bio-Molecules in Bulk and Over the Nano-Substrate: Perspective to the Molecular Dynamics Simulations

The properties of bio-molecules are explicitly influenced by their organization in bulk and vicinity of substrate. Organization of bio-molecules can be of various kinds such as folded, unfolded, helix, swollen, globule, and so forth. These organizations of bio-molecule also depend on the local surrounding environmental conditions like temperature, solvency, adsorption, and encapsulation. Variation in environmental conditions helps to manipulate and control the organizations for the desired applications. Adsorption and encapsulation of bio-molecule over substrate have many applications in the area of drug delivery, design and development of bio-sensors, advance bio-separation process, etc. Molecular dynamics simulation is a very powerful tool to investigate the molecular structures, synthesis process and optimum properties, etc. A large number of efficient force field parameters and molecular dynamics simulators are available for large-scale simulation