Potential of Core-Collapse Supernova Neutrino Detection at JUNO

JUNO is an underground neutrino observatory under construction in Jiangmen, China. It uses 20kton liquid scintillator as target, which enables it to detect supernova burst neutrinos of a large statistics for the next galactic core-collapse supernova (CCSN) and also pre-supernova neutrinos from the nearby CCSN progenitors. All flavors of supernova burst neutrinos can be detected by JUNO via several interaction channels, including inverse beta decay, elastic scattering on electron and proton, interactions on C12 nuclei, etc. This retains the possibility for JUNO to reconstruct the energy spectra of supernova burst neutrinos of all flavors. The real time monitoring systems based on FPGA and DAQ are under development in JUNO, which allow prompt alert and trigger-less data acquisition of CCSN events. The alert performances of both monitoring systems have been thoroughly studied using simulations. Moreover, once a CCSN is tagged, the system can give fast characterizations, such as directionality and light curve

Detection of the Diffuse Supernova Neutrino Background with JUNO

As an underground multi-purpose neutrino detector with 20 kton liquid scintillator, Jiangmen Underground Neutrino Observatory (JUNO) is competitive with and complementary to the water-Cherenkov detectors on the search for the diffuse supernova neutrino background (DSNB). Typical supernova models predict 2-4 events per year within the optimal observation window in the JUNO detector. The dominant background is from the neutral-current (NC) interaction of atmospheric neutrinos with 12C nuclei, which surpasses the DSNB by more than one order of magnitude. We evaluated the systematic uncertainty of NC background from the spread of a variety of data-driven models and further developed a method to determine NC background within 15\% with {\it{in}} {\it{situ}} measurements after ten years of running. Besides, the NC-like backgrounds can be effectively suppressed by the intrinsic pulse-shape discrimination (PSD) capabilities of liquid scintillators. In this talk, I will present in detail the improvements on NC background uncertainty evaluation, PSD discriminator development, and finally, the potential of DSNB sensitivity in JUNO

Real-time Monitoring for the Next Core-Collapse Supernova in JUNO

Core-collapse supernova (CCSN) is one of the most energetic astrophysical events in the Universe. The early and prompt detection of neutrinos before (pre-SN) and during the SN burst is a unique opportunity to realize the multi-messenger observation of the CCSN events. In this work, we describe the monitoring concept and present the sensitivity of the system to the pre-SN and SN neutrinos at the Jiangmen Underground Neutrino Observatory (JUNO), which is a 20 kton liquid scintillator detector under construction in South China. The real-time monitoring system is designed with both the prompt monitors on the electronic board and online monitors at the data acquisition stage, in order to ensure both the alert speed and alert coverage of progenitor stars. By assuming a false alert rate of 1 per year, this monitoring system can be sensitive to the pre-SN neutrinos up to the distance of about 1.6 (0.9) kpc and SN neutrinos up to about 370 (360) kpc for a progenitor mass of 30$M_{\odot}$ for the case of normal (inverted) mass ordering. The pointing ability of the CCSN is evaluated by using the accumulated event anisotropy of the inverse beta decay interactions from pre-SN or SN neutrinos, which, along with the early alert, can play important roles for the followup multi-messenger observations of the next Galactic or nearby extragalactic CCSN.Comment: 24 pages, 9 figure

Use of food-grade proteases to recover umami protein\u2013peptide mixtures from rice middlings

The effects of enzymatic hydrolysis induced by food-grade exo- plus endo-proteases (i.e. Umamizyme and Flavourzyme) on the sensory characteristics and functional properties of rice middlings were investigated. Enzymatic hydrolysis was confirmed by sodium dodecylsulfate polyacrylamide gel electrophoresis (SDS-PAGE), by monitoring the rate of hydrolysis with the Coefficient of Protein Degradation (CPD). The presence of medium-low size polypeptides at the end point of 24. h was detected, resulting from 24.84 \ub1 1.28 % and 67.04 \ub1 0.55 % hydrolysis for Flavourzyme and Umamyzyme, respectively. Sensory and functional properties, including emulsifying and foaming properties, were evaluated on hydrolysates obtained after 24. h incubation. The sensory analysis described the umami taste as the most intense attribute for all the products and good emulsifying and foaming properties were observed, mainly in Umamizyme hydrolysates. Then the hydrolysis procedure here described could be convenient to provide ingredients characterized by a good taste profile and by functional properties useful for industrial food processing, storage and consumption

Italy: Health system review

The Health Systems in Transition (HiT) series consists of country-based reviews that provide a detailed description of a health system and of reform and policy initiatives in progress or under development in a specific country. Each review is produced by country experts in collaboration with the Observatory’s staff. In order to facilitate comparisons between countries, reviews are based on a template prepared by the European Observatory, which is revised periodically. The template provides detailed guidelines and specific questions, definitions and examples needed to compile a report

Italy: Health System Review

This analysis of the Italian health system reviews recent developments in organization and governance, health financing, health care provision, health reforms and health system performance. Italy has a regionalized National Health Service (SSN) that provides universal coverage largely free of charge at the point of delivery, though certain services and goods require a co-payment. Life expectancy in Italy is historically among the highest in the EU. However, regional differences in health indicators are marked, as well as in per capita spending, distribution of health professionals and in the quality of health services. Overall, Italy's health spending per capita is lower than the EU average and is among the lowest in western European countries. Private spending has increased in recent years, although this trend was halted in 2020 during the coronavirus disease 2019 (COVID-19) pandemic. A key focus of health policies in recent decades was to promote a shift away from unnecessary inpatient care, with a considerable reduction of acute hospital beds and stagnating overall growth in health personnel. However, this was not counterbalanced by a sufficient strengthening of community services in order to cope with the ageing population's needs and related chronic conditions burden. This had important repercussions during the COVID-19 emergency, as the health system felt the impact of previous reductions in hospital beds and capacity and underinvestment in community-based care. Reorganizing hospital and community care will require a strong alignment between central and regional authorities. The COVID-19 crisis also highlighted several issues pre-dating the pandemic that need to be addressed to improve the sustainability and resilience of the SSN. The main outstanding challenges for the health system are linked to addressing historic underinvestment in the health workforce, modernizing outdated infrastructure and equipment, and enhancing information infrastructure. Italy's National Recovery and Resilience Plan, underwritten by the Next Generation EU budget to assist with economic recovery from the COVID-19 pandemic, contains specific health sector priorities, such as strengthening the country's primary and community care, boosting capital investment and funding the digitalization of the health care system

Solar neutrino detection in a large volume double-phase liquid argon experiment

International audiencePrecision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution. Given the expected neutrino fluxes and known detection reactions, such measurements require detectors capable of collecting neutrino-electron scattering data in exposures on the order of 1 ktonne-yr, with good energy resolution and extremely low background. Two-phase liquid argon time projection chambers (LAr TPCs) are under development for direct Dark Matter WIMP searches, which possess very large sensitive mass, high scintillation light yield, good energy resolution, and good spatial resolution in all three cartesian directions. While enabling Dark Matter searches with sensitivity extending to the ``neutrino floor'' (given by the rate of nuclear recoil events from solar neutrino coherent scattering), such detectors could also enable precision measurements of solar neutrino fluxes using the neutrino-electron elastic scattering events

Solar neutrino detection in a large volume double-phase liquid argon experiment

International audiencePrecision measurements of solar neutrinos emitted by specific nuclear reaction chains in the Sun are of great interest for developing an improved understanding of star formation and evolution. Given the expected neutrino fluxes and known detection reactions, such measurements require detectors capable of collecting neutrino-electron scattering data in exposures on the order of 1 ktonne-yr, with good energy resolution and extremely low background. Two-phase liquid argon time projection chambers (LAr TPCs) are under development for direct Dark Matter WIMP searches, which possess very large sensitive mass, high scintillation light yield, good energy resolution, and good spatial resolution in all three cartesian directions. While enabling Dark Matter searches with sensitivity extending to the ``neutrino floor'' (given by the rate of nuclear recoil events from solar neutrino coherent scattering), such detectors could also enable precision measurements of solar neutrino fluxes using the neutrino-electron elastic scattering events