Observation of Rayleigh-Lamb waves generated by the 2022 Hunga-Tonga volcanic eruption with the POLA detectors at Ny-Ålesund

The eruption of the Hunga-Tonga volcano in the South Pacific Ocean on January 15, 2022, at about 4:15 UTC, generated a violent explosion, which created atmospheric pressure disturbances in the form of Rayleigh-Lamb waves detected all over the globe. Here we discuss the observation of the Hunga-Tonga shock-wave performed at the Ny-Ålesund Research Station on the Spitsbergen island, by the detectors of the PolarquEEEst experiment and their ancillary sensors. Online pressure data as well as the results of dedicated offline analysis are presented and discussed in details. Results include wave arrival times, wave amplitude measurements and wave velocity calculation. We observed five passages of the shock wave with a significance larger than 3 [Formula: see text] and an amplitude up to 1 hPa. The average propagation velocity resulted to be (308 ± 0.6) m/s. Possible effects of the atmospheric pressure variation associated with the shock-wave multiple passages on the cosmic-ray rate at ground level are also investigated. We did not find any significant evidence of this effect.

Test of Electric Charge Conservation with Borexino

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single monoenergetic photon was obtained. This new bound, τ≥6.6×10^{28}  yr at 90% C.L., is 2 orders of magnitude better than the previous limit.

Lifetimes of (214)Po and (212)Po measured with Counting Test Facility at Gran Sasso National Laboratory

The decays of (214)Po into (210)Pb and of (212)Po into (208)Pb tagged by the previous decays from (214)Bi and (212)Bi have been studied inserting quartz vials inside the Counting Test Facility (CTF) at the underground laboratory in Gran Sasso (LNGS). We find that the mean lifetime of (214)Po is (236.00 ± 0.42(stat) ± 0.15(syst)) μs and that of (212)Po is (425.1 ± 0.9(stat) ± 1.2(syst)) ns. Our results are compatible with previous measurements, have a much better signal to background ratio, and reduce the overall uncertainties.

First evidence of pep solar neutrinos by direct detection in Borexino

We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We determined the rate of pep solar neutrino interactions in Borexino to be 3.1±0.6{stat}±0.3{syst}  counts/(day·100  ton). Assuming the pep neutrino flux predicted by the standard solar model, we obtained a constraint on the CNO solar neutrino interaction rate of <7.9  counts/(day·100  ton) (95% C.L.). The absence of the solar neutrino signal is disfavored at 99.97% C.L., while the absence of the pep signal is disfavored at 98% C.L. The necessary sensitivity was achieved by adopting data analysis techniques for the rejection of cosmogenic {11}C, the dominant background in the 1-2 MeV region. Assuming the Mikheyev-Smirnov-Wolfenstein large mixing angle solution to solar neutrino oscillations, these values correspond to solar neutrino fluxes of (1.6±0.3)×10{8}  cm{-2} s^{-1} and <7.7×10{8}  cm{-2} s{-1} (95% C.L.), respectively, in agreement with both the high and low metallicity standard solar models. These results represent the first direct evidence of the pep neutrino signal and the strongest constraint of the CNO solar neutrino flux to date.

Precision measurement of the (7)Be solar neutrino interaction rate in Borexino

The rate of neutrino-electron elastic scattering interactions from 862 keV (7)Be solar neutrinos in Borexino is determined to be 46.0±1.5(stat)(-1.6)(+1.5)(syst) counts/(day·100  ton). This corresponds to a ν(e)-equivalent (7)Be solar neutrino flux of (3.10±0.15)×10(9)  cm(-2) s(-1) and, under the assumption of ν(e) transition to other active neutrino flavours, yields an electron neutrino survival probability of 0.51±0.07 at 862 keV. The no flavor change hypothesis is ruled out at 5.0 σ. A global solar neutrino analysis with free fluxes determines Φ(pp)=6.06(-0.06)(+0.02)×10(10)  cm(-2) s(-1) and Φ(CNO)<1.3×10(9)  cm(-2) s(-1) (95% C.L.). These results significantly improve the precision with which the Mikheyev-Smirnov-Wolfenstein large mixing angle neutrino oscillation model is experimentally tested at low energy.

Direct measurement of the 7Be solar neutrino flux with 192 days of borexino data

We report the direct measurement of the 7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV 7Be neutrinos is 49+/-3stat+/-4syst counts/(day.100 ton). The hypothesis of no oscillation for 7Be solar neutrinos is inconsistent with our measurement at the 4sigma C.L. Our result is the first direct measurement of the survival probability for solar nu(e) in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of 7Be, pp, and CNO solar nu(e), and the limit on the effective neutrino magnetic moment using solar neutrinos.

The creatine transporter mediates the uptake of creatine by brain tissue, but not the uptake of two creatine-derived compounds

Hereditary creatine transporter deficiency causes brain damage, despite the brain having the enzymes to synthesize creatine. Such damage occurring despite an endogenous synthesis is not easily explained. This condition is incurable, because creatine may not be delivered to the brain without its transporter. Creatine-derived compounds that crossed the blood-brain barrier in a transporter-independent fashion would be useful in the therapy of hereditary creatine transporter deficiency, and possibly also in neuroprotection against brain anoxia or ischemia. We tested the double hypothesis that: (1) the creatine carrier is needed to make creatine cross the plasma membrane of brain cells and (2) creatine-derived molecules may cross this plasma membrane independently of the creatine carrier. In in vitro mouse hippocampal slices, incubation with creatine increased creatine and phosphocreatine content of the tissue. Inhibition of the creatine transporter with 3-guanidinopropionic acid (GPA) dose-dependently prevented this increase. Incubation with creatine benzyl ester (CrOBzl) or phosphocreatine-Mg-complex acetate (PCr-Mg-CPLX) increased tissue creatine content, not phosphocreatine. This increase was not prevented by GPA. Thus, the creatine transporter is required for creatine uptake through the plasma membrane. Since there is a strong indication that creatine in the brain is mainly synthesized by glial cells and transferred to neurons, this might explain why hereditary transporter deficiency is attended by severe brain damage despite the possibility of an endogenous synthesis. CrOBzl and PCr-Mg-CPLX cross the plasma membrane in a transporter-independent way, and might be useful in the therapy of hereditary creatine transporter deficiency. They may also prove useful in the therapy of brain anoxia or ischemia.

Intracerebroventricular administration of creatine protects against damage by global cerebral ischemia in rat

Although a large body of evidence shows that pretreatment of brain tissue with creatine protects against anoxic injury in vitro, only a couple of papers have investigated creatine protection in vivo, and they yielded conflicting results. We attempted to clarify how creatine may be protective in an in vivo model of global cerebral ischemia (GCI). We administered creatine either before of after GCI. We decided to administer it by intracerebroventricular infusion, to maximize its bioavailability to the brain. Our findings show that creatine is clearly protective in vivo when administered before ischemia. In that case, histological evaluation of damage was consistently improved in all regions examined, and neurological score was better in creatine-treated rats than in controls. When administered after ischemia, histology was improved in the hippocampus, while only a not significant trend toward improvement was observed in the cerebral cortex and in the caudo-putamen. Neurological score was not improved by creatine administration after GCI. Our findings show that creatine administration is protective in vivo. Such protection was clear in the case of pretreatment, and was present, to a lesser degree, when treatment was started after ischemia. Our results should encourage further research in the possible role of creatine therapy in neuroprotection.

Role of creatine and phosphocreatine in neuronal protection from anoxic and ischemic damage

Phosphocreatine can to some extent compensate for the lack of ATP synthesis that is caused in the brain by deprivation of oxygen or glucose. Treatment of in vitro rat hippocampal slices with creatine increases the neuronal store of phosphocreatine. In this way it increases the resistance of the tissue to anoxic or ischemic damage. In in vitro brain slices pretreatment with creatine delays anoxic depolarization (AD) and prevents the irreversible loss of evoked potentials that is caused by transient anoxia, although it seems so far not to be active against milder, not AD-mediated, damage. Although creatine crosses poorly the blood-brain barrier, its administration in vivo at high doses through the intracerebroventricular or the intraperitoneal way causes an increase of cerebral phosphocreatine that has been shown to be of therapeutic value in vitro. Accordingly, preliminary data show that creatine pretreatment decreases ischemic damage in vivo.

Microtubules, but not actin microfilaments, regulate vacuole motility and morphology in hyphae of Pisolithus tinctorius

While it is now recognised that transport within the endomembrane system may occur via membranous tubules, spatial regulation of this process is poorly understood. We have investigated the role of the cytoskeleton in regulating the motility and morphology of the motile vacuole system in hyphae of the fungus Pisolithus tinctorius by studying (1) the effects of anti-microtubule (oryzalin, nocodazole) and anti-actin drugs (cytochalasins, latrunculin) on vacuolar activity, monitored by fluorescence microscopy of living cells; and (2) the ultrastructural relationship of microtubules, actin microfilaments, and vacuoles in hyphae prepared by rapid-freezing and freeze-substitution. Anti-microtubule drugs reduced the tubular component of the vacuole system in a dose-dependent and reversible manner, the extent of which correlated strongly with the degree of disruption of the microtubule network (monitored by immunofluorescence microscopy). The highest doses of anti-microtubule drugs completely eliminated tubular vacuoles, and only spherical vacuoles were observed. In contrast, anti-actin drugs did not reduce the frequency of tubular vacuoles or the motility of these vacuoles, even though immunofluorescence microscopy confirmed perturbation of microfilament organisation. Electron microscopy showed that vacuoles were always accompanied by microtubules. Bundles of microtubules were found running in parallel along the length of tubular vacuoles and individual microtubules were often within one microtubule diameter of a vacuole membrane. Our results strongly support a role for microtubules, but not actin microfilaments, in the spatial regulation of vacuole motility and morphology in fungal hyphae.

The Golgi apparatus of the scaly green flagellate Scherffelia dubia: uncoupling of glycoprotein and polysaccharide synthesis during flagellar regeneration

The flagella of the green alga Scherffelia dubia are covered by scales which consist of acidic polysaccharides and glycoproteins. Experimental deflagellation results in the regeneration of flagella complete with scales. During flagellar regeneration, scales are newly synthesized in the Golgi apparatus, exocytosed and deposited on the growing flagella. Flagellar regeneration is dependent upon protein synthesis and N-glycosylation, as it is blocked by cycloheximide and partially inhibited by tunicamycin. Metabolic labeling with [35S]methionine/cysteine demonstrated that scale-associated proteins were not newly synthesized during flagellar regeneration, suggesting that the proteins deposited on regenerating flagella were drawn from a pool. Quantitative immunoelectron microscopy using a monospecific antibody directed against a scale-associated protein of 126 kDa (SAP126) revealed that the pool of SAP126 was primarily located at the plasma membrane, with minor labeling of the scale reticulum and trans-Golgi cisternae, both before deflagellation and during flagellar regeneration. Since SAP126 was sequestered during flagellar regeneration into secretory vesicles together with newly synthesized scales, it is concluded that the persistent presence of SAP126 in the trans-Golgi cisternae during scale biogenesis requires retrograde transport of the protein from the plasma membrane to the Golgi apparatus.