For several decades, the origin of ultra-high-energy cosmic rays (UHECRs) has been an unsolved question of high-energy astrophysics. One approach for solving this puzzle is to correlate UHECRs with ...high-energy neutrinos, since neutrinos are a direct probe of hadronic interactions of cosmic rays and are not deflected by magnetic fields. In this paper, we present three different approaches for correlating the arrival directions of neutrinos with the arrival directions of UHECRs. The neutrino data is provided by the IceCube Neutrino Observatory and ANTARES, while the UHECR data with energies above \(\sim\)50 EeV is provided by the Pierre Auger Observatory and the Telescope Array. All experiments provide increased statistics and improved reconstructions with respect to our previous results reported in 2015. The first analysis uses a high-statistics neutrino sample optimized for point-source searches to search for excesses of neutrinos clustering in the vicinity of UHECR directions. The second analysis searches for an excess of UHECRs in the direction of the highest-energy neutrinos. The third analysis searches for an excess of pairs of UHECRs and highest-energy neutrinos on different angular scales. None of the analyses has found a significant excess, and previously reported over-fluctuations are reduced in significance. Based on these results, we further constrain the neutrino flux spatially correlated with UHECRs.
This work presents a new search for magnetic monopoles using data taken with the ANTARES neutrino telescope over a period of 10 years (January 2008 to December 2017). Compared to previous ANTARES ...searches, this analysis uses a run-by-run simulation strategy, with a larger exposure as well as a new simulation of magnetic monopoles taking into account the Kasama, Yang and Goldhaber model for their interaction cross-section with matter. No signal compatible with the passage of relativistic magnetic monopoles is observed, and upper limits on the flux of magnetic monopoles with \(\beta\) = v/c \(\geq\) 0.55, are presented. For ultra-relativistic magnetic monopoles the flux limit is \(\sim\) 7$\times$$10^{-18}\( \)\rm cm^{-2} s^{-1} sr^{-1}$.
In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model. KM3NeT/ORCA is a neutrino ...detector optimised for measuring atmospheric neutrinos from a few GeV to around 100 GeV. In this paper, the sensitivity of the KM3NeT/ORCA detector to neutrino decay has been explored. A three-flavour neutrino oscillation scenario, where the third neutrino mass state \(\nu_3\) decays into an invisible state, e.g. a sterile neutrino, is considered. We find that KM3NeT/ORCA would be sensitive to invisible neutrino decays with \(1/\alpha_3=\tau_3/m_3 < 180\)~\(\mathrm{ps/eV}\) at \(90\%\) confidence level, assuming true normal ordering. Finally, the impact of neutrino decay on the precision of KM3NeT/ORCA measurements for \(\theta_{23}\), \(\Delta m^2_{31}\) and mass ordering have been studied. No significant effect of neutrino decay on the sensitivity to these measurements has been found.
To determine the role of genetic predisposition in the etiology of head and neck squamous cell carcinoma.
Retrospective study.
The outpatient clinics of the departments of otorhinolaryngology and ...maxillofacial surgery.
First-degree relatives of patients with new head and neck cancer, with first-degree relatives of the patients' spouses as controls.
Occurrence of cancer of the respiratory and upper digestive tract in relatives of patients with head and neck cancer and controls.
First-degree relatives (n = 617) of 105 patients with head and neck cancer had 31 cases of cancer of the respiratory and upper digestive tract vs 10 cases in the control group (n = 618) (relative risk, 3.5; P = .0002). This higher rate of cancer was even larger in siblings (16 vs 2, relative risk, 14.6; P = .0001).
Genetic predisposition is an important risk factor for squamous cell carcinoma of the head and neck.
In trauma patients a specific pattern of the hormone endocrine response to injury has been described. Conflicting data exist regarding the hormonal changes during sepsis. We studied the time course ...and variability of the hormonal and metabolic responses to severe sepsis in twelve medical patients.
Hormone levels were measured every 6 hours. Urinary nitrogen and 3-methylhistidine excretion were measured daily. Indirect calorimetry was used to calculate energy production rate (EPR).
None of the hormones measured showed a time course in individual patients. Growth hormone (1.69 +/- 0.17 ng/ml) and insulin (48 +/- 5 mU/L) values were within normal range. Cortisol value (474 +/- 44 nmol/L) was in the upper normal range. Insulin-like growth factor 1 level (12.5 +/- 5.7 nmol/L) was decreased. Nitrogen balance was negative and did not change during the study period. Neither oxygen consumption (VO2) (318 +/- 20 ml/min), carbon dioxide output (283 +/- 10 ml/min), EPR (2064 +/- 435 kcal/day), nor fuel utilization showed a time course. The variability during the study period compared with values on admission ranged from 20% (insulin-like growth factor 1) to 74% (growth hormone). The variability of calculated fuel utilization ranged from 35% (protein) to 180% (fat). The variability of VO2, carbon dioxide production, and EPR was for less, 8%.
A specific pattern in the endocrine and metabolic responses as observed in trauma patients does not occur in medical patients with severe sepsis. Hormones and calculated fuel utilization show large variations when compared with values on admission. VO2 and EPR vary for less. Nutritional needs in patients with sepsis, therefore, can be calculated on admission and need not be recalculated during the first week after admission.
In 28 diabetic patients and 62 control subjects spectral analysis of spontaneous beat-to-beat RR interval variations was performed. The spectral analysis focused on the dominant frequency of the ...mid-frequency band (0.04-0.12 Hz) or baro-oscillatory phenomenon (BOP). Compared with control subjects the dominant frequency of the BOP (BOP frequency) in the diabetic patients was lower (p less than 0.001), and the difference increased with age. The shift of the BOP frequency was positively correlated with the reduced variation in heart rate during deep breathing (r = 0.80, p less than 0.001) in the diabetic patients. These findings indicate that determination of the BOP frequency is a useful method for assessing cardiovascular autonomic function, supplementary to the known cardiovascular reflex tests. Measurement of the BOP frequency has the advantage that no active patient co-operation is required.
The KM3NeT research infrastructure is under construction in the Mediterranean Sea. KM3NeT will study atmospheric and astrophysical neutrinos with two multi-purpose neutrino detectors, ARCA and ORCA, ...primarily aimed at GeV-PeV neutrinos. Thanks to the multi-photomultiplier tube design of the digital optical modules, KM3NeT is capable of detecting the neutrino burst from a Galactic or near-Galactic core-collapse supernova. This potential is already exploitable with the first detection units deployed in the sea. This paper describes the real-time implementation of the supernova neutrino search, operating on the two KM3NeT detectors since the first months of 2019. A quasi-online astronomy analysis is introduced to study the time profile of the detected neutrinos for especially significant events. The mechanism of generation and distribution of alerts, as well as the integration into the SNEWS and SNEWS 2.0 global alert systems are described. The approach for the follow-up of external alerts with a search for a neutrino excess in the archival data is defined. Finally, an overview of the current detector capabilities and a report after the first two years of operation are given.
Searches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of new physics is ...being pushed by collider searches well beyond the TeV domain. This situation strongly motivates the exploration of DM masses much larger than a TeV. Secluded scenarios contain a natural way around the unitarity bound on the DM mass, via the early matter domination induced by the mediator of its interactions with the Standard Model. High-energy neutrinos constitute one of the very few direct accesses to energy scales above a few TeV. An indirect search for secluded DM signals has been performed with the ANTARES neutrino telescope using data from 2007 to 2015. Upper limits on the DM annihilation cross section for DM masses up to 6 PeV are presented and discussed.
The KM3NeT Collaboration is currently constructing a multi-site high-energy neutrino telescope in the Mediterranean Sea consisting of matrices of pressure-resistant glass spheres, each holding a set ...of 31 small-area photomultipliers. The main goals of the telescope are the observation of neutrino sources in the Universe and the measurement of the neutrino oscillation parameters with atmospheric neutrinos. Both extraterrestrial and atmospheric neutrinos are detected through the Cherenkov light induced in seawater by charged particles produced in neutrino interactions in the surrounding medium. A relative time synchronization between photomultipliers of the order of 1 ns is needed to guarantee the required angular resolution of the detector. Due to the large detector volumes to be instrumented by KM3NeT, a cost reduction of the different systems is a priority. To this end, the inexpensive Nanobeacon has been designed and developed by the KM3NeT Collaboration to be used for detector time-calibration studies. At present, more than 600 Nanobeacons have been already produced. The characterization of the optical pulse and the wavelength emission profile of the devices are critical for the time calibration. In this paper, the main features of the Nanobeacon design, production and operation, together with the main properties of the light pulse generated are described.
