154 research outputs found
Absolute resonance strengths in the 6,7Li(alpha,gamma)10,11B reactions
The absolute strengths of the Ea=1175keV resonance in the 6Li(a,g)10B
reaction and of the Ea=814 keV resonance in the 7Li(a,g)11B reaction have been
measured to =366+-38 meV and =300+-32 meV,
respectively, in good agreement with previous values.
These resonances can be used to measure the absolute acceptance of the recoil
separator ERNA to a precision of about 10%.Comment: 6 pages, 5 figures, to appear in European Physical Journal
Elliptic flow of charged particles in Pb-Pb collisions at 2.76 TeV
We report the first measurement of charged particle elliptic flow in Pb-Pb
collisions at 2.76 TeV with the ALICE detector at the CERN Large Hadron
Collider. The measurement is performed in the central pseudorapidity region
(||<0.8) and transverse momentum range 0.2< < 5.0 GeV/. The
elliptic flow signal v, measured using the 4-particle correlation method,
averaged over transverse momentum and pseudorapidity is 0.087 0.002
(stat) 0.004 (syst) in the 40-50% centrality class. The differential
elliptic flow v reaches a maximum of 0.2 near = 3
GeV/. Compared to RHIC Au-Au collisions at 200 GeV, the elliptic flow
increases by about 30%. Some hydrodynamic model predictions which include
viscous corrections are in agreement with the observed increase.Comment: 10 pages, 4 captioned figures, published version, figures at
http://aliceinfo.cern.ch/ArtSubmission/node/389
Evidence for an Excess of Soft Photons in Hadronic Decays of Z^0
Soft photons inside hadronic jets converted in front of the DELPHI main
tracker (TPC) in events of qqbar disintegrations of the Z^0 were studied in the
kinematic range 0.2 < E_gamma < 1 GeV and transverse momentum with respect to
the closest jet direction p_T < 80 MeV/c. A clear excess of photons in the
experimental data as compared to the Monte Carlo predictions is observed. This
excess (uncorrected for the photon detection efficiency) is (1.17 +/- 0.06 +/-
0.27) x 10^{-3} gamma/jet in the specified kinematic region, while the expected
level of the inner hadronic bremsstrahlung (which is not included in the Monte
Carlo) is (0.340 +/- 0.001 +/- 0.038) x 10^{-3} gamma/jet. The ratio of the
excess to the predicted bremsstrahlung rate is then (3.4 +/- 0.2 +/- 0.8),
which is similar in strength to the anomalous soft photon signal observed in
fixed target experiments with hadronic beams.Comment: 37 pages, 9 figures, Accepted by Eur. Phys. J.
The Galactic Chemical Evolution of phosphorus observed with IGRINS
Phosphorus (P) is considered to be one of the key elements for life, making
it an important element to look for in the abundance analysis of spectra of
stellar systems. Yet, there exists only a handful of spectroscopic studies to
estimate the P abundances and investigate its trend across a range of
metallicities. We have observed full HK band spectra at a spectral resolving
power of R=45,000 with IGRINS instrument. Abundances are determined using SME
in combination with 1D MARCS stellar atmosphere models. The investigated sample
of stars have reliable stellar parameters estimated using optical FIES spectra
(GILD; J\"onsson et al. in prep.). In order to determine the P abundances from
the 16482.92 Angstrom P line, we take special care of the CO() blend.
We determine the C, N, O abundances from atomic carbon and a range of
non-blended molecular lines (CO, CN, OH) which are aplenty in the H band region
of K giant stars, assuring an appropriate modelling of the blending
CO() line. We present [P/Fe] vs [Fe/H] trend for 38 K giant stars in
the metallicity range of -1.2 dex [Fe/H] 0.4 dex. We find that our
trend matches well with the compiled literature sample of prominently dwarf
stars and limited number of giant stars. Our trend is found to be higher by
0.05 - 0.1 dex compared to the theoretical chemical evolution trend in
Cescutti et al. 2012 resulting from core collapse supernova (type II) of
massive stars with the P yields from Kobayashi et al. (2006) arbitrarily
increased by a factor of 2.75. Thus the enhancement factor might need to be
0.05 - 0.1 dex higher to match our trend. We also find an empirically
determined primary behaviour for phosphorus. Furthermore, the phosphorus
abundance is found to be elevated by 0.6 - 0.9 dex in two metal poor
s-enriched stars compared to the theoretical chemical evolution trend.Comment: 13 pages, 9 figures, accepted for publication in Astronomy and
Astrophysic
Higher harmonic anisotropic flow measurements of charged particles in Pb-Pb collisions at 2.76 TeV
We report on the first measurement of the triangular , quadrangular
, and pentagonal charged particle flow in Pb-Pb collisions at 2.76
TeV measured with the ALICE detector at the CERN Large Hadron Collider. We show
that the triangular flow can be described in terms of the initial spatial
anisotropy and its fluctuations, which provides strong constraints on its
origin. In the most central events, where the elliptic flow and
have similar magnitude, a double peaked structure in the two-particle azimuthal
correlations is observed, which is often interpreted as a Mach cone response to
fast partons. We show that this structure can be naturally explained from the
measured anisotropic flow Fourier coefficients.Comment: 10 pages, 4 figures, published version, figures at
http://aliceinfo.cern.ch/ArtSubmission/node/387
Measurement of D+- and D0 production in deep inelastic scattering using a lifetime tag at HERA
The production of D-+/-- and D-0-mesons has been measured with the ZEUS detector at HERA using an integrated luminosity of 133.6 pb(-1). The measurements cover the kinematic range 5 < Q(2) < 1000 GeV2, 0.02 < y < 0.7, 1.5 < p(T)(D) < 15 GeV and |eta(D)| < 1.6. Combinatorial background to the D-meson signals is reduced by using the ZEUS microvertex detector to reconstruct displaced secondary vertices. Production cross sections are compared with the predictions of next-to-leading-order QCD, which is found to describe the data well. Measurements are extrapolated to the full kinematic phase space in order to obtain the open-charm contribution, F-2(c (c) over bar), to the proton structure function, F-2
Developmental trajectories of neuroanatomical alterations associated with the 16p11.2 Copy Number Variations
Practice patterns and 90-day treatment-related morbidity in early-stage cervical cancer
To evaluate the impact of the Laparoscopic Approach to Cervical Cancer (LACC) Trial on patterns of care and surgery-related morbidity in early-stage cervical cancer
The biological effects of diagnostic cardiac imaging on chronically exposed physicians: the importance of being non-ionizing
Ultrasounds and ionizing radiation are extensively used for diagnostic applications in the cardiology clinical practice. This paper reviewed the available information on occupational risk of the cardiologists who perform, every day, cardiac imaging procedures. At the moment, there are no consistent evidence that exposure to medical ultrasound is capable of inducing genetic effects, and representing a serious health hazard for clinical staff. In contrast, exposure to ionizing radiation may result in adverse health effect on clinical cardiologists. Although the current risk estimates are clouded by approximations and extrapolations, most data from cytogenetic studies have reported a detrimental effect on somatic DNA of professionally exposed personnel to chronic low doses of ionizing radiation. Since interventional cardiologists and electro-physiologists have the highest radiation exposure among health professionals, a major awareness is crucial for improving occupational protection. Furthermore, the use of a biological dosimeter could be a reliable tool for the risk quantification on an individual basis
The Radiation Issue in Cardiology: the time for action is now
The "radiation issue" is the need to consider possible deterministic effects (e.g., skin injuries) and long-term cancer risks due to ionizing radiation in the risk-benefit assessment of diagnostic or therapeutic testing. Although there are currently no data showing that high-dose medical studies have actually increased the incidence of cancer, the "linear-no threshold" model in radioprotection assumes that no safe dose exists; all doses add up in determining cancer risks; and the risk increases linearly with increasing radiation dose. The possibility of deterministic effects should also be considered when skin or lens doses may be over the threshold. Cardiologists have a special mission to avoid unjustified or non-optimized use of radiation, since they are responsible for 45% of the entire cumulative effective dose of 3.0 mSv (similar to the radiological risk of 150 chest x-rays) per head per year to the US population from all medical sources except radiotherapy. In addition, interventional cardiologists have an exposure per head per year two to three times higher than that of radiologists. The most active and experienced interventional cardiologists in high volume cath labs have an annual exposure equivalent to around 5 mSv per head and a professional lifetime attributable to excess cancer risk on the order of magnitude of 1 in 100. Cardiologists are the contemporary radiologists but sometimes imperfectly aware of the radiological dose of the examination they prescribe or practice, which can range from the equivalent of 1-60 mSv around a reference dose average of 10-15 mSv for a percutaneous coronary intervention, a cardiac radiofrequency ablation, a multi-detector coronary angiography, or a myocardial perfusion imaging scintigraphy. A good cardiologist cannot be afraid of life-saving radiation, but must be afraid of radiation unawareness and negligence
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