Klinischer Behandlungspfad Carotisstenose : Evaluation im Ländervergleich ; Poster

Poster Einleitung Im Rahmen effizienzsteigernder Maßnahmen sind klinische Behandlungspfade unter DRG- Bedingungen und im Rahmen der Qualitätssicherung wichtige Instrumente. Material und Methoden Aus der Analyse zweier erfahrungsbasierter klinischer Behandlungspfade in Frankfurt/D und Newcastle/GB wurde ein halbstandardisierter clinical pathway Carotisstenose entwickelt, der der heterogenen Befundkonstellation bei Aufnahme, den unterschiedlichen klinischen Stadien der Erkrankung und den individuellen Patientenbedürfnissen Rechnung trägt. Es wurden dazu zwei Gruppen mit je 25 konsekutiv in Frankfurt/D ( Gruppe FrankfurtI) und New Castle/GB ( Gruppe New Castle )operierten Patienten retrospektiv analysiert.Aus den retrospektiv erhobenen Daten wurde ein stadienbezogener und der Zuweisersituation gerecht werdender klinischer Behandlungspfad erstellt, der anhand von 20 konsekutiv operierten Patienten, davon 60 % im Stadium IV der Erkrankung, ( Gruppe FrankfurtII ) analysiert wurde. Ergebnisse In Frankfurt 1 wurde 21 mal eine Eversions-TEA und 4 mal eine TEA/ Patchplastik angewendet, 62 % der Patienten befanden sich im Stadium 1 der Erkrankung, ,65 % erhielten präoperativ eine i.a.DSA der supraaortalen Äste ,100% eine Duplexsonografie und eine CCT; postoperativ fielen insgesamt 12 Intensiv- Pflegetage an sowie eine Revision aufgrund einer Nachblutung. In der Gruppe New Castle befanden sich 68% der Patienten in einem klinischen Stadium 2,es wurde 25 mal offen thrombendarteriektomiert, davon 21 mal mit Direktnaht verschlossen und 4 mal mit Patchplastik, alle Patienten erhielten präoperativ eine CT- Angiografie und eine Duplexsonografie; postoperativ fiel 1 Intensivpflegetag an und eine Revision wegen Nachblutung. Die Morbiditäts-/ Mortalitätsrate betrug in beiden Gruppen 0%. Betriebswirtschaftlich wurden bei einer Liegedauer von durchschnittlich 10 Tagen in Frankfurt 1 tatsächliche Kosten von 2768.96€ pro Patient ermittelt, in New Castle,bei einer Liegedauer von durchschnittlich 5 Tagen und einer differenten Kostenstruktur von 2510.56 €. In der Gruppe Frankfurt 2 wurde 11mal eine TEA mit Patchplastik und 9 mal eine Eversions-TEA durchgeführt, alle Patienten erhielten präoperativ eine Duplexsonografie und eine CCT , postoperativ fielen insgesamt 6 Intensivtage an, es wurde nicht revidiert, die Morbiditäts-/Mortalitätsrate lag ebenfalls bei 0%. Durch Einführung eines klinischen Behandlungspfades wurde also die Liegedauer in Frankfurt um 40 % reduziert sowie die tatsächlichen Kosten auf 2384.41€ pro Fall und damit im Mittel um 14 % gemindert. Schlussfolgerung Unter DRG-Bedingungen trägt daher die Anwendung eines klinischen Behandlungspfades in der Carotischirurgie zu einer Verbesserung der Erlössituation ohne Qualitätseinbuße bei

Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption

Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies above 40 TeV, neutrinos are expected to be absorbed as they pass through the Earth. Experimentally, the cross section has been measured only at the relatively low energies (below 400 GeV) available at neutrino beams from accelerators \cite{Agashe:2014kda, Formaggio:2013kya}. Here we report the first measurement of neutrino absorption in the Earth, using a sample of 10,784 energetic upward-going neutrino-induced muons observed with the IceCube Neutrino Observatory. The flux of high-energy neutrinos transiting long paths through the Earth is attenuated compared to a reference sample that follows shorter trajectories through the Earth. Using a fit to the two-dimensional distribution of muon energy and zenith angle, we determine the cross section for neutrino energies between 6.3 TeV and 980 TeV, more than an order of magnitude higher in energy than previous measurements. The measured cross section is $1.30^{+0.21}_{-0.19}$ (stat.) $^{+0.39}_{-0.43}$ (syst.) times the prediction of the Standard Model \cite{CooperSarkar:2011pa}, consistent with the expectation for charged and neutral current interactions. We do not observe a dramatic increase in the cross section, expected in some speculative models, including those invoking new compact dimensions \cite{AlvarezMuniz:2002ga} or the production of leptoquarks \cite{Romero:2009vu}.Comment: Preprint version of Nature paper 10.1038/nature2445

Search for astrophysical sources of neutrinos using cascade events in IceCube

The IceCube neutrino observatory has established the existence of a flux of high-energy astrophysical neutrinos inconsistent with the expectation from atmospheric backgrounds at a significance greater than $5\sigma$. This flux has been observed in analyses of both track events from muon neutrino interactions and cascade events from interactions of all neutrino flavors. Searches for astrophysical neutrino sources have focused on track events due to the significantly better angular resolution of track reconstructions. To date, no such sources have been confirmed. Here we present the first search for astrophysical neutrino sources using cascades interacting in IceCube with deposited energies as small as 1 TeV. No significant clustering was observed in a selection of 263 cascades collected from May 2010 to May 2012. We show that compared to the classic approach using tracks, this statistically-independent search offers improved sensitivity to sources in the southern sky, especially if the emission is spatially extended or follows a soft energy spectrum. This enhancement is due to the low background from atmospheric neutrinos forming cascade events and the additional veto of atmospheric neutrinos at declinations $\lesssim-30^\circ$.Comment: 14 pages, 9 figures, 1 tabl

Search for astrophysical sources of neutrinos using cascade events in IceCube

The IceCube neutrino observatory has established the existence of a flux of high-energy astrophysical neutrinos inconsistent with the expectation from atmospheric backgrounds at a significance greater than $5\sigma$. This flux has been observed in analyses of both track events from muon neutrino interactions and cascade events from interactions of all neutrino flavors. Searches for astrophysical neutrino sources have focused on track events due to the significantly better angular resolution of track reconstructions. To date, no such sources have been confirmed. Here we present the first search for astrophysical neutrino sources using cascades interacting in IceCube with deposited energies as small as 1 TeV. No significant clustering was observed in a selection of 263 cascades collected from May 2010 to May 2012. We show that compared to the classic approach using tracks, this statistically-independent search offers improved sensitivity to sources in the southern sky, especially if the emission is spatially extended or follows a soft energy spectrum. This enhancement is due to the low background from atmospheric neutrinos forming cascade events and the additional veto of atmospheric neutrinos at declinations $\lesssim-30^\circ$.Comment: 14 pages, 9 figures, 1 tabl

Book Reviews

With the observation of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory, interest has risen in models of PeV-mass decaying dark matter particles to explain the observed flux. We present two dedicated experimental analyses to test this hypothesis. One analysis uses 6 years of IceCube data focusing on muon neutrino ‘track’ events from the Northern Hemisphere, while the second analysis uses 2 years of ‘cascade’ events from the full sky. Known background components and the hypothetical flux from unstable dark matter are fitted to the experimental data. Since no significant excess is observed in either analysis, lower limits on the lifetime of dark matter particles are derived: we obtain the strongest constraint to date, excluding lifetimes shorter than $10^{28}$ s at 90% CL for dark matter masses above 10 TeV

Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data

The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for their sources. We present constraints from seven years of IceCube Neutrino Observatory muon data on the neutrino flux coming from the Galactic plane. This flux is expected from cosmic-ray interactions with the interstellar medium or near localized sources. Two methods were developed to test for a spatially-extended flux from the entire plane, both maximum likelihood fits but with different signal and background modeling techniques. We consider three templates for Galactic neutrino emission based primarily on gamma-ray observations and models that cover a wide range of possibilities. Based on these templates and an unbroken $E^{-2.5}$ power-law energy spectrum, we set 90% confidence level upper limits constraining the possible Galactic contribution to the diffuse neutrino flux to be relatively small, less than 14% of the flux reported in Aartsen et al. (2015a) above 1 TeV. A stacking method is also used to test catalogs of known high energy Galactic gamma-ray sources.Comment: 14 pages, 4 figures, 4 tables, submitted to The Astrophysical Journa

Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atmospheric muons to a level which, for the first time, allows IceCube searching for point-like sources of neutrinos in the southern sky at energies between 100 GeV and several TeV in the muon neutrino charged current channel. No significant clustering of neutrinos above background expectation was observed in four years of data recorded with the completed IceCube detector. Upper limits on the neutrino flux for a number of spectral hypotheses are reported for a list of astrophysical objects in the southern hemisphere.Comment: 19 pages, 17 figures, 2 table