16 research outputs found

    Neutralino spectrum in top-down models of UHECR

    Get PDF
    We calculate the cosmic ray spectrum of ultra high energy neutralinos that one should expect provided that the observed ultra high energy cosmic rays are produced by the decay of superheavy particles X, M_X>10^{12} GeV, in supersymmetric models. Our calculation uses an extended DGLAP formalism. Forthcoming cosmic ray observatories should be able to detect these neutralinos.Comment: 10 pages, revtex, 3 eps figures. Difference between the present work and Montecarlo simulations clarifie

    Gravitinos from Gravitational Collapse

    Get PDF
    We reanalyse the limits on the gravitino mass m3/2m_{3/2} in superlight gravitino scenarios derived from arguments on energy-loss during gravitational collapse. We conclude that the mass range 10−6eV≤m3/2≤2.3×10−5eV10^{-6}eV\leq m_{3/2}\leq2.3\times10^{-5}eV is excluded by SN1987A data. In terms of the scale of supersymmetry breaking Λ\Lambda, the range 70GeV≤Λ≤300GeV70GeV\leq\Lambda \leq 300GeV is not allowed.Comment: 6 pages, latex, no figures. Numerical typo correcte

    Gamma Rays from SN1987A due to Pseudoscalar Conversion

    Get PDF
    A light pseudoscalar coupled to two photons would be copiously emitted by the core of a supernova. Part of this flux would be converted to γ−\gamma-rays by the galactic magnetic field. Measurements on the SN1987A γ−\gamma-ray flux by the Gamma-Ray Spectrometer on the Solar Maximum Mission satellite already imply a bound on the coupling g<3×10−12g < 3 \times 10^{-12} GeV−1^{-1}. The improved generation of satellite-borne detectors, like EGRET or the project GLAST, could be able to detect a pseudoscalar-to-photon signal from a nearby supernova, for allowed values of gg.Comment: 8 pages, no figure

    On a Light Spinless Particle Coupled to Photons

    Full text link
    A pseudoscalar or scalar particle ϕ\phi that couples to two photons but not to leptons, quarks and nucleons would have effects in most of the experiments searching for axions, since these are based on the aγγa \gamma \gamma coupling. We examine the laboratory, astrophysical and cosmological constraints on ϕ\phi and study whether it may constitute a substantial part of the dark matter. We also generalize the ϕ\phi interactions to possess SU(2)×U(1)SU(2) \times U(1) gauge invariance, and analyze the phenomenological implications.Comment: LaTex, 20p., 6 figures. Changes in sections 4, 5 and figure 2, our bounds are now more stringent. To be published in Physical Review

    Nanocellulose/bioactive glass cryogels as scaffolds for bone regeneration

    Get PDF
    A major challenge exists in the preparation of scaffolds for bone regeneration, namely, achieving simultaneously bioactivity, biocompatibility, mechanical performance and simple manufacturing. Here, cellulose nanofibrils (CNF) are introduced for the preparation of scaffolds taking advantage of their biocompatibility and ability to form strong 3D porous networks from aqueous suspensions. CNF are made bioactive for bone formation through a simple and scalable strategy that achieves highly interconnected 3D networks. The resultant materials optimally combine morphological and mechanical features and facilitate hydroxyapatite formation while releasing essential ions for in vivo bone repair. The porosity and roughness of the scaffolds favor several cell functions while the ions act in the expression of genes associated with cell differentiation. Ion release is found critical to enhance the production of the bone morphogenetic protein 2 (BMP-2) from cells within the fractured area, thus accelerating the in vivo bone repair. Systemic biocompatibility indicates no negative effects on vital organs such as the liver and kidneys. The results pave the way towards a facile preparation of advanced, high performance CNF-based scaffolds for bone tissue engineering

    Free amino acid profile of Bubalus bubalis L. meat from the Campania region

    Get PDF
    ABSTRACT In this study, we determined the amount of carnosine and anserine in water buffalo meat without hanging treatment and the free amino acid profile by using amino acid analyser with post-column ninhydrin derivatization procedure. The main free amino acids present in samples were glutamic acid (>60 mg/100 g), followed by alanine, glycine, and arginine. Other protein amino acids were detected in minor amounts (less than 2 mg/100 g). Among the non-protein amine-containing compounds, taurine and urea were the most abundant. The analysis showed that 50% of the total free amino acids was represented by dipeptides carnosine (average ~130.3 mg/100 g) and anserine (average ~17.9 mg/100 g). Thus, this study for the first time reports the free amino acids profile of water buffalo meat and the content of carnosine and anserine, potentially involved in the darkening meat process and their ratio, that could be used to estimate the water buffalo meat portion in mixed meat products
    corecore