The 10 most recently published documents
We summarize previous work on b̅b̅ud four-quark systems in the Born-Oppenheimer approximation and discuss first steps towards an extension to the theoretically more challenging bb̅ud̅ system. Strategies to identify a possibly existing bb̅ud̅ bound state are discussed and first numerical results are presented.
An important experimental program on Nuclear Astrophysics is being carried out at the n_TOF since several years, in order to address the still open issues in stellar and primordial nucleosynthesis. Several neutron capture reactions relevant to s-process nucleosynthesis have been measured so far, some of which on important branching point radioisotopes. Furthermore, the construction of a second experimental area has recently opened the way to challenging measurements of (n, charged particle) reactions on isotopes of short half-life. The Nuclear Astrophysics program of the n_TOF Collaboration is here described, with emphasis on recent results relevant for stellar nucleosynthesis, stellar neutron sources and primordial nucleosynthesis.
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.
Who should hold bail-inable debt and how can regulators police holding restrictions effectively?
(2023)
This paper analyses the demand-side prerequisites for the efficient application of the bail-in tool in bank resolution, scrutinises whether the European bank crisis management and deposit insurance (CMDI) framework is apt to establish them, and proposes amendments to remedy identified shortcomings.
The first applications of the new European CMDI framework, particularly in Italy, have shown that a bail-in of debt holders is especially problematic if they are households or other types of retail investors. Such debt holders may be unable to bear losses, and the social implications of bailing them in may create incentives for decision makers to refrain from involving them in bank resolution. In turn, however, if investors can expect resolution authorities (RAs) to behave inconsistently over time and bail-out bank capital and debt holders despite earlier vows to involve them in bank rescues, the pricing and monitoring incentives that the crisis management framework seeks to invigorate would vanish. As a result, market discipline would be suboptimal and moral hazard would persist. Therefore, the policy objectives of the CMDI framework will only be achieved if critical bail-in capital is not held by retail investors without sufficient loss-bearing capacity. Currently, neither the CMDI framework nor capital market regulation suffice to assure that this precondition is met. Therefore, some amendments are necessary. In particular, debt instruments that are most likely to absorb losses in resolution should have a high minimum denomination and banks should not be allowed to self-place such securities.
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.
Ein persistierender Ductus arteriosus (PDA) stellt bei Frühgeborenen mit <1500g Geburtsgewicht einen relevanten Faktor für eine Erhöhung der Morbidität und Mortalität dar. Aufgrund fehlender Evidenz konnte bisher keine allgemeine Therapieempfehlung nach frustranem medikamentösem Verschlussversuch erarbeitet werden, sowohl eine Ligatur im Rahmen eines operativen Eingriffs, als auch eine Katheterintervention sind möglich. In der vorliegenden Arbeit wurde retrospektiv die Auswirkung dieser verschiedenen Therapiemethoden auf die Morbidität und Mortalität bei Frühgeborenen <1500g Geburtsgewicht mit hämodynamisch signifikantem persistierendem Ductus arteriosus untersucht. Insbesondere wurde geprüft, ob eine Katheterintervention das Risiko einer Bronchopulmonalen Dysplasie (BPD) oder des Versterbens der Kinder, sowie andere häufige Folgeerkrankungen des Frühgeborenen erhöht. Analysiert wurden dafür alle 469 stationär behandelten Kinder des Schwerpunktes Neonatologie, die zwischen dem 01.01.2013 und dem 31.12.2019 in der Uniklinik Frankfurt am Main mit einem Geburtsgewicht von <1500g geboren oder innerhalb der ersten 13 Lebenstage aus einem anderen Krankenhaus übernommen wurden. Diese wurden in 4 Gruppen eingeteilt: Kinder ohne hämodynamisch signifikanten PDA (n=341), Kinder die erfolgreich medikamentös therapiert wurden (n=92), solche, die eine Ligatur erhielten (n=16) und zuletzt solche, die interventionell behandelt wurden (n=12). Die Daten der medikamentös behandelten Kinder wurden in dieser Untersuchung nicht berücksichtigt. Es wurden sowohl verschiedene Geburtsparameter um eine Vergleichbarkeit der Gruppen zu untersuchen, als auch relevante Parameter des Outcomes ausgewertet. Es zeigte sich, dass Kinder ohne PDA zum Zeitpunkt der Geburt ein höheres Gestationsalter hatten als solche mit PDA und daraus resultierend eine geringere Intensivmedizinische Betreuung und geringere Morbidität aufwiesen. Im Vergleich der Interventionskinder mit einer Matched-pair Gruppe aus 24 Kindern der Kontrollgruppe ohne PDA (± 8 Schwangerschaftstage bei Geburt und ± 410 g Geburtsgewicht) konnten keine Unterschiede in Mortalität oder Morbidität festgestellt werden. Kinder nach Intervention zeigten kein signifikant schlechteres Outcome (Bronchopulmonale Dysplasie, Intraventrikuläre Hämorrhagie, operativ versorgte nekrotisierende Enterokolitis, therapiebedürftige Retinopathia praematurorum, Periventrikuläre Leukomalazie) im Vergleich zu Kindern nach Ligatur. Eine schwere Bronchopulmonale Dysplasie trat mit einem Relativen Risiko von 2,25 seltener auf. Diese Ergebnisse lassen den Schluss zu, dass die Interventionelle Therapie des hsPDA ein ähnlich gutes Outcome im Vergleich zur Ligatur aufweist und sogar einen Vorteil für die Kinder bringt. Aufgrund der geringen Fallzahlen muss die Relevanz diese Ergebnisse kritisch hinterfragt werden. Eine mögliche randomisierte kontrollierte Studie könnte diese bestätigen.
The Cosmological Lithium Problem refers to the large discrepancy between the abundance of primordial 7Li predicted by the standard theory of Big Bang Nucleosynthesis and the value inferred from the so-called “Spite plateau” in halo stars. A possible explanation for this longstanding puzzle in Nuclear Astrophysics is related to the incorrect estimation of the destruction rate of 7Be, which is responsible for the production of 95% of primordial Lithium. While charged-particle induced reactions have mostly been ruled out, data on the 7Be(n,α) and 7Be(n,p) reactions are scarce or completely missing, so that a large uncertainty still affects the abundance of 7Li predicted by the standard theory of Big Bang Nucleosynthesis. Both reactions have been measured at the n_TOF facility at CERN, providing for the first time data in a wide neutron energy range.
The 33S(n,α)30Si cross section measurement, using 10B(n,α) as reference, at the n_TOF Experimental Area 2 (EAR2) facility at CERN is presented. Data from 0.01 eV to 100 keV are provided and, for the first time, the cross section is measured in the range from 0.01 eV to 10 keV. These data may be used for a future evaluation of the cross section because present evaluations exhibit large discrepancies. The 33S(n,α)30Si reaction is of interest in medical physics because of its possible use as a cooperative target to boron in Neutron Capture Therapy (NCT).
High precision measurement of the radiative capture cross section of 238U at the n_TOF CERN facility
(2017)
The importance of improving the accuracy on the capture cross-section of 238U has been addressed by the Nuclear Energy Agency, since its uncertainty significantly affects the uncertainties of key design parameters for both fast and thermal nuclear reactors. Within the 7th framework programme ANDES of the European Commission three different measurements have been carried out with the aim of providing the 238U(n,γ) cross-section with an accuracy which varies from 1 to 5%, depending on the energy range. Hereby the final results of the measurement performed at the n_TOF CERN facility in a wide energy range from 1 eV to 700 keV will be presented.
New results are presented of the 234U neutron-induced fission cross section, obtained with high accuracy in the resonance region by means of two methods using the 235U(n,f) as reference. The recent evaluation of the 235U(n,f) obtained with SAMMY by L. C. Leal et al. (these Proceedings), based on previous n_TOF data [1], has been used to calculate the 234U(n,f) cross section through the 234U/235U ratio, being here compared with the results obtained by using the n_TOF neutron flux.
