Quantum gravity phenomenology at the dawn of the multi-messenger era—A review

The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review, prepared within the COST Action CA18108 “Quantum gravity phenomenology in the multi-messenger approach”, is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers.publishedVersio

Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review

The exploration of the universe has recently entered a new era thanks to the multi-messenger paradigm, characterized by a continuous increase in the quantity and quality of experimental data that is obtained by the detection of the various cosmic messengers (photons, neutrinos, cosmic rays and gravitational waves) from numerous origins. They give us information about their sources in the universe and the properties of the intergalactic medium. Moreover, multi-messenger astronomy opens up the possibility to search for phenomenological signatures of quantum gravity. On the one hand, the most energetic events allow us to test our physical theories at energy regimes which are not directly accessible in accelerators; on the other hand, tiny effects in the propagation of very high energy particles could be amplified by cosmological distances. After decades of merely theoretical investigations, the possibility of obtaining phenomenological indications of Planck-scale effects is a revolutionary step in the quest for a quantum theory of gravity, but it requires cooperation between different communities of physicists (both theoretical and experimental). This review is aimed at promoting this cooperation by giving a state-of-the art account of the interdisciplinary expertise that is needed in the effective search of quantum gravity footprints in the production, propagation and detection of cosmic messengers

Euclid: I. Overview of the Euclid mission

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients,dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015–2025 programme of theEuropean Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy,over about 14 000 deg² of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structureformation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range ofscience. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processingsteps, and data products. We also highlight the main science objectives and expected performance

1106 Twins with uncertain significant mutations, slightly different cardiomyopathies and different oucmes

Abstract Dilated cardiomyopathy (DCM) is defined as left ventricle (LV) dilatation and dysfunction in the absence of abnormal loading conditions or coronary artery disease enough to cause global systolic impairment. It is the leading cause of heart failure and sudden cardiac death, and even in the early stages of life 5,7/1.000.000 children are diagnosed each year. Lately, genetic screening has revealed that 30-50% of the cases have a familial origin, with a high genetic heterogeneity. We present the case of a 4-month-old boy (case A) referred to our Hospital with high suspicion of dilated cardiomyopathy. He had a twin brother, pregnancy went without complications, pre-birth ultrasound and blood tests were completely normal and a caesarean birth was planned at 37 weeks of pregnancy. He also has an older sibling with no medical history. Our patient was the first to be born and was admitted to the neonatal-ICU due to tachypnea, labored breathing and desaturation. In the physical exam a 5cm hepatomegaly was detected and on the X-Ray a cardiomegaly and enlarged mediastinum were confirmed. ECG showed no electrical abnormalities besides vague repolarization changes. A TTE was done, showing remarkable left cavities enlargement with severe left ventricle dysfunction and moderate mitral regurgitation, comprising the right filling and therefore the right cardiac output. These findings were confirmed by MRI, not detecting enhancement patterns compatible with myocarditis. A genetic test was performed in the index case detecting the presence of a mutation in the desmin gene (Des C.568 + 10c) and the myosin heavy chain 7 gene (Myh7p - glu883Ala) both associated either with dilated and noncompaction cardyomiopathies. Due to the elevated chances of a familiar-DCM his twin brother was admitted to study (case B), with no symptoms or clinical signs besides an isolated bronchitis episode. The clinical examination and EKG were normal, detecting in the TTE a slightly dilated left ventricle with non-compactation morphology in the LV lateral wall, but no left ventricle dysfunction. Also, a TTE was performed in their father with similar findings: mild LV dilatation with minor systolic disfunction and uncertain non-compactation morphology in the LVl apex. Abnormalities of specific genes are now known to be responsible for different types of congenital heart diseases with important implications in genetic counseling. We want to emphasize the different manifestation of a single mutation on different members of a family, even in this two twin-brothers that, under the same probable conditions during preganancy, had slightly different cardyomyopathies but very different severity, and probable mid to long term prognosis. Abstract 1106 Figure.</jats:p

Anthocyanins enhance yeast’s adsorption of Ochratoxin A during the alcoholic fermentation

Ochratoxin A (OTA) is a mycotoxin that can be present in food products and beverages such as wine, in which the European Union has regulated its maximum concentration. Since yeasts can adsorb OTA during the alcoholic fermentation (AF), we have analyzed whether anthocyanins influence the reduction of OTA in wine during AF carried out by two Saccharomyces cerevisiae strains. Laboratory experiments were conducted with one white must and two red musts that were obtained by adding to the white must two different concentrations of anthocyanins extract. Musts were supplemented with OTA and tested at two pHs. A reduction of OTA was observed in all wines, being higher in red wines. These data point that a chemical bond between anthocyanins and OTA is probably responsible for enhanced adsorption of OTA by yeast. On the other hand, the removal of OTA between the two inoculated yeast strains was different. This result cannot be only attributed to differences in the yeasts’ cell wall composition, because differences were not detected in white wines

Antibacterial Properties of hLf1-11 Peptide onto Titanium Surfaces: A Comparison Study Between Silanization and Surface Initiated Polymerization

Dental implant failure can be associated with infections that develop into peri-implantitis. In order to reduce biofilm formation, several strategies focusing on the use of antimicrobial peptides (AMPs) have been studied. To covalently immobilize these molecules onto metallic substrates, several techniques have been developed, including silanization and polymer brush prepared by surface-initiated atom transfer radical polymerization (ATRP), with varied peptide binding yield and antibacterial performance. The aim of the present study was to compare the efficiency of these methods to immobilize the lactoferrin-derived hLf1-11 antibacterial peptide onto titanium, and evaluate their antibacterial activity in vitro. Smooth titanium samples were coated with hLf1-11 peptide under three different conditions: silanization with 3-aminopropyltriethoxysilane (APTES), and polymer brush based coatings with two different silanes. Peptide presence was determined by X-ray photoelectron spectroscopy, and the mechanical stability of the coatings was studied under ultrasonication. The LDH assays confirmed that HFFs viability and proliferation were no affected by the treatments. The in vitro antibacterial properties of the modified surfaces were tested with two oral strains (Streptococcus sanguinis and Lactobacillus salivarius) showing an outstanding reduction. A higher decrease in bacterial attachment was noticed when samples were modified by ATRP methods compared to silanization. This effect is likely due to the capacity to immobilize more peptide on the surfaces using polymer brushes and the nonfouling nature of polymer PDMA segment.Peer Reviewe