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Coherent photoproduction of ρ⁰ vector mesons in ultra-peripheral Pb-Pb collisions at √sNN = 5.02 TeV
(2020)
Cross sections for the coherent photoproduction of ρ0 vector mesons in ultra-peripheral Pb-Pb collisions at sNN−−−√ = 5.02 TeV are reported. The measurements, which rely on the π+π− decay channel, are presented in three regions of rapidity covering the range |y| < 0.8. For each rapidity interval, cross sections are shown for different nuclear-breakup classes defined according to the presence of neutrons measured in the zero-degree calorimeters. The results are compared with predictions based on different models of nuclear shadowing. Finally, the observation of a coherently produced resonance-like structure with a mass around 1.7 GeV/c2 and a width of about 140 MeV/c2 is reported and compared with similar observations from other experiments.
Direct photon production at mid-rapidity in Pb–Pb collisions at √sNN=2.76 TeV was studied in the transverse momentum range 0.9<pT<14 GeV/c. Photons were detected with the highly segmented electromagnetic calorimeter PHOS and via conversions in the ALICE detector material with the e+e− pair reconstructed in the central tracking system. The results of the two methods were combined and direct photon spectra were measured for the 0–20%, 20–40%, and 40–80% centrality classes. For all three classes, agreement was found with perturbative QCD calculations for pT≳5 GeV/c. Direct photon spectra down to pT≈1 GeV/c could be extracted for the 20–40% and 0–20% centrality classes. The significance of the direct photon signal for 0.9<pT<2.1 GeV/c is 2.6σ for the 0–20% class. The spectrum in this pT range and centrality class can be described by an exponential with an inverse slope parameter of (297±12stat±41syst) MeV. State-of-the-art models for photon production in heavy-ion collisions agree with the data within uncertainties.
Hintergrund: Die chronische metabolischen Azidose (cmA) ist eine häufige Komplikation bei chronischer Niereninsuffizienz, deren Behandlung bei niereninsuffizienten Patienten mit Diabetes mellitus die Insulinresistenz verbessern kann. Um die aktuelle Therapiesituation der cmA im diabetologischen Umfeld abzubilden und mehr über die Zusammenarbeit von Diabetologen und Nephrologen zu erfahren, wurden diabetologisch tätige Haus- und Fachärzte zur cmA befragt.
Methoden An 5863 Ärzten mit diabetologischer Zusatzqualifikation wurde postalisch ein Fragebogen versandt. Alle 97 erhaltenen Antwortbögen wurden deskriptiv ausgewertet.
Ergebnisse Die meisten Teilnehmer sind Internisten mit diabetologischer Zusatzqualifikation (46 %) und behandeln im Median 50 (10; 112) Patienten mit Typ-1-Diabetes bzw. 210 (100; 450) Patienten mit Typ-2-Diabetes pro Quartal. Eine cmA wurde von 12 % der Teilnehmer in den letzten 12 Monaten bei median 4 (2; 6) Patienten mit Typ-1-Diabetes und 10 (3; 30) Patienten mit Typ-2-Diabetes beobachtet. Die cmA wird überwiegend durch Bestimmung des Serum-Bikarbonats (27; 28 %) und des Base Excess (19; 20 %) diagnostiziert. 38 (39 %) der Teilnehmer erhalten regelmäßig von Nephrologen die Empfehlung zur Behandlung der cmA. Sie wird von knapp 1 Drittel als relevant (29 %) und gut umsetzbar (27 %) betrachtet. Zur Behandlung der cmA wird vor allem orales Bikarbonat empfohlen (Bikarbonat: 39 %, Zitrat: 5 %, sonst: keine Angabe). Maßnahmen, die die Mehrheit der Diabetologen in der Verantwortung der Nephrologen sehen, sind ergänzende Diagnostik (87; 90 %) einschließlich Blutgasanalyse (59 %) sowie die Behandlung der cmA (62 %) und renalen Anämie (53 %). 34 % der Diabetologen gaben an, bisher noch keine cmA-Fälle in der Praxis behandelt zu haben. Die meisten Diabetologen überlassen die Behandlung und Überwachung der cmA dem Nephrologen (38 %). Dabei wird die Zusammenarbeit mit den Nephrologen als zufriedenstellend (81 %) bewertet. 38 % der Befragten haben in der täglichen Praxis beobachtet, dass die Einstellung der cmA auch die Insulinresistenz positiv beeinflusst. Eine CME-Fortbildung in der Diabetologie speziell zur cmA würden 76 (78 %) begrüßen.
Diskussion Bei der Behandlung der cmA wird die Kooperation zwischen Diabetologen und Nephrologen generell gut bewertet, wobei die Diagnose, Behandlung und Überwachung einer cmA in der Verantwortung des Nephrologen gesehen werden. Da die Behandlung der cmA die Insulinresistenz verringern kann, sollte der Stellenwert der cmA-Therapie im diabetologischen Umfeld nicht unterschätzt werden. Um die cmA-Behandlung bei diabetischer Nephropathie zu optimieren, wären CME-Fortbildungen zur cmA geeignet. Zudem könnten Schulungen im Rahmen einer interdisziplinären Kooperation mit Diätberatern die Umsetzbarkeit diätetischer Interventionen zur Behandlung der cmA verbessern.
An accurate measurement of the 140Ce(n,γ) energy-dependent cross-section was performed at the n_TOF facility at CERN. This cross-section is of great importance because it represents a bottleneck for the s-process nucleosynthesis and determines to a large extent the cerium abundance in stars. The measurement was motivated by the significant difference between the cerium abundance measured in globular clusters and the value predicted by theoretical stellar models. This discrepancy can be ascribed to an overestimation of the 140Ce capture cross-section due to a lack of accurate nuclear data. For this measurement, we used a sample of cerium oxide enriched in 140Ce to 99.4%. The experimental apparatus consisted of four deuterated benzene liquid scintillator detectors, which allowed us to overcome the difficulties present in the previous measurements, thanks to their very low neutron sensitivity. The accurate analysis of the p-wave resonances and the calculation of their average parameters are fundamental to improve the evaluation of the 140Ce Maxwellian-averaged cross-section.
Although the 12C(n,p)12B and 12C(n,d)11B reactions are of interest in several fields of basic and applied Nuclear Physics the present knowledge of these two cross-sections is far from being accurate and reliable, with both evaluations and data showing sizable discrepancies. As part of the challenging n_TOF program on (n,cp) nuclear reactions study, the energy differential cross-sections of the 12C(n,p)12B and 12C(n,d)11 B reactions have been measured at CERN from the reaction thresholds up to 30 MeV neutron energy. Both measurements have been recently performed at the long flight-path (185 m) experimental area of the n_TOF facility at CERN using a pure (99.95%) rigid graphite target and two silicon telescopes. In this paper an overview of the experiment is presented together with a few preliminary results.
Background: The photon strength functions (PSFs) and nuclear level density (NLD) are key ingredients for calculation of the photon interaction with nuclei, in particular the reaction cross sections. These cross sections are important especially in nuclear astrophysics and in the development of advanced nuclear technologies.
Purpose: The role of the scissors mode in the M1 PSF of (well-deformed) actinides was investigated by several experimental techniques. The analyses of different experiments result in significant differences, especially on the strength of the mode. The shape of the low-energy tail of the giant electric dipole resonance is uncertain as well. In particular, some works proposed a presence of the E1 pygmy resonance just above 7 MeV. Because of these inconsistencies additional information on PSFs in this region is of great interest.
Methods: The γ-ray spectra from neutron-capture reactions on the 234U, 236 U, and 238 U nuclei have been measured with the total absorption calorimeter of the n_TOF facility at CERN. The background-corrected sum-energy and multi-step-cascade spectra were extracted for several isolated s-wave resonances up to about 140 eV.
Results: The experimental spectra were compared to statistical model predictions coming from a large selection of models of photon strength functions and nuclear level density. No combination of PSF and NLD models from literature is able to globally describe our spectra. After extensive search we were able to find model combinations with modified generalized Lorentzian (MGLO) E1 PSF, which match the experimental spectra as well as the total radiative widths.
Conclusions: The constant temperature energy dependence is favored for a NLD. The tail of giant electric dipole resonance is well described by the MGLO model of the E1 PSF with no hint of pygmy resonance. The M1 PSF must contain a very strong, relatively wide, and likely double-resonance scissors mode. The mode is responsible for about a half of the total radiative width of neutron resonances and significantly affects the radiative cross section.
The spent fuel of current nuclear reactors contains fissile plutonium isotopes that can be combined with 238U to make mixed oxide (MOX) fuel. In this way the Pu from spent fuel is used in a new reactor cycle, contributing to the long-term sustainability of nuclear energy. The use of MOX fuels in thermal and fast reactors requires accurate capture and fission cross sections. For the particular case of 242Pu, the previous neutron capture cross section measurements were made in the 70's, providing an uncertainty of about 35% in the keV region. In this context, the Nuclear Energy Agency recommends in its “High Priority Request List” and its report WPEC-26 that the capture cross section of 242Pu should be measured with an accuracy of at least 7–12% in the neutron energy range between 500 eV and 500 keV. This work presents a brief description of the measurement performed at n_TOF-EAR1, the data reduction process and the first ToF capture measurement on this isotope in the last 40 years, providing preliminary individual resonance parameters beyond the current energy limits in the evaluations, as well as a preliminary set of average resonance parameters.
i-TED is an innovative detection system which exploits Compton imaging techniques to achieve a superior signal-to-background ratio in (n,γ) cross-section measurements using time-of-flight technique. This work presents the first experimental validation of the i-TED apparatus for high-resolution time-of-flight experiments and demonstrates for the first time the concept proposed for background rejection. To this aim both 197Au(n,γ) and 56Fe(n,γ) reactions were measured at CERN n\_TOF using an i-TED demonstrator based on only three position-sensitive detectors. Two \cds detectors were also used to benchmark the performance of i-TED. The i-TED prototype built for this study shows a factor of ∼3 higher detection sensitivity than state-of-the-art \cds detectors in the ∼10~keV neutron energy range of astrophysical interest. This paper explores also the perspectives of further enhancement in performance attainable with the final i-TED array consisting of twenty position-sensitive detectors and new analysis methodologies based on Machine-Learning techniques.
The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely (n,γ) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on total energy detectors will be presented to illustrate how, advances in instrumentation have led, over the years, to the assessment and discovery of many new aspects of s-process nucleosynthesis and to the progressive refinement of theoretical models of stellar evolution. A summary will be presented on current efforts to develop new detection concepts, such as the Total-Energy Detector with γ-ray imaging capability (i-TED). The latter is based on the simultaneous combination of Compton imaging with neutron time-of-flight (TOF) techniques, in order to achieve a superior level of sensitivity and selectivity in the measurement of stellar neutron capture rates.