[PDF] Top 20 Que papel para o psicólogo numa equipa de cuidados paliativos?
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Testing of almost all the hadronic interaction models by comparing calculated muon energy spectrum with data
... model energy spectra of the most energetic secondary charged mesons are ...partial energy spectra of the atmospheric vertical muons induced by primary cosmic particles with various fixed energies in terms ... See full document
10
Testing of the VENUS 4.12, DPMJET 2.55, QGSJET II-03 and SIBYLL 2.3 hadronic interaction models via help of the atmospheric vertical muon spectra
... of muon flux have been estimate as ...the muon partial energy spectrum in each individual shower have been cal- ...on energy of particles. Thus, we need also some expressions for the ... See full document
7
Constraints of hadronic interaction models from the cosmic muon observations
... interaction models. In the case of “soft” interaction the generation of secondary particles emitted at mostly small angles with respect to the projectile particle (the highest values of ... See full document
8
The hadronic interaction model Sibyll 2.3c and muon production in extensive air-showers
... the muon energy spectrum is again shown as a ratio with the energy spectrum in S ibyll ...two models where the extensions en- hancing the production of ρ 0 and baryon-pairs have ... See full document
16
First measurement of muon neutrino disappearance in NOvA
... neutrino interaction cross sec- tion and hadronization uncertainties are determined by altering each cross section and hadronization parameter by its predetermined uncertainties in the GENIE simula- tion, which ... See full document
17
Measurement of the cosmic ray spectrum and chemical composition in the 1015-1018 eV energy range
... "post-LHC" hadronic interaction models more widely used in the EAS simula- tion are: EPOS-LHC[6], QGSJetII-04[7] and ...from all of them is not reproducing all the experimental ... See full document
10
Extensive Air Showers and Cosmic Ray Physics above 1017 eV
... the energy is proportional to the total number of secondaries sampled at ground, while the composition is inferred either through a multi-component measurement, such as the electromagnetic and muonic components, ... See full document
38
Connecting accelerator experiments and cosmic ray showers
... Most of the Astronomy and Astrophysics is done using electromagnetic signals from radio to gamma rays. It gives precious informations on the various objects observed in the Universe and their history. In fact a part of ... See full document
9
Hadronic Interactions and Air Showers: Where Do We Stand?
... The model predictions are shown in Fig. 3 for p-p, π- air and p-air (as inelasticity = 1-elasticity) as a function of center of mass energy. Sibyll 2.3c has the largest elasticity which is probably related to the ... See full document
15
Open issues in hadronic interactions for air showers
... the models have larger differences for the multiplicity compared to the cross ...by all the models up to 1 TeV and even up to 13 TeV for EPOS LHC and QGSJETII-04 [60] and a difference appears between ... See full document
6
Measurements and tests of hadronic interactions at ultra-high energies with the Pierre Auger Observatory
... mass energy above those at- tained at the LHC are continuously happening in the upper layers of the Earth’s ...high energy cosmic rays (UHECR) collide with air nuclei, creating thousands of secondaries that ... See full document
7
Recent hadron production measurements performed by the NA61/SHINE collaboration
... experiment to study hadron production in hadron-nucleus and nucleus-nucleus collisions at the CERN Super Proton Synchrotron (SPS). Among its physics goals are precise hadron production measurements for improving ... See full document
8
Perspectives on the hadronic contribution to the muon g − 2
... energies, models like the extended Nambu–Jona-Lasinio model [48, 49] and/or the hidden local symmetry model [50, 51], which couples the lowest-lying vector resonance to the pseudoscalars, were ... See full document
8
LHC data and extensive air showers
... strain models used for air shower simulations. As shown in Fig. 6, these data help a lot to reduce the differences be- tween the models especially because they resolve an am- biguity on the phase ... See full document
5
Activation of Methanes by Doubly Charged Metal Dication Complexes in the Gas Phase
... was mass selected and directed by an ion guide into a Paul ion trap. The end caps of the latter were grounded and continuously cooled through direct contact with a liquid nitrogen reservoir. As a consequence, helium ... See full document
17
Measurement of the muon content in air showers at the Pierre Auger Observatory
... The muon content of extensive air showers produced by ultra-high energy cosmic rays is an observable sensitive to the composition of primary particles and to the properties of hadronic interactions ... See full document
25
Strategies For Improving Epistasis Detection And Replication
... genomic data with a focus on challenges to the ability to detect and replicate epistatic ...the interaction of genotypes to produce the resultant phenotype, may help explain the “missing heritability” of ... See full document
8
Summary of the main results of the KASCADE and KASCADE-Grande experiments
... eV with a statistical significance of 3.5σ [15] (see figure 5). The analysis was repeated on the basis of different hadronic interaction models [17]. Despite the fact, that the relative abundance of ... See full document
6
Forbidden Reflections in TeO 2in the Vicinity of the Te L 1A bsorption Edge
... reflection. Numerical calculations show that the latter tensor component is comparable to the first one, but the combination of several geometric factors leads to the fact that its contribution to the spectrum is ... See full document
18
Probing quantum decoherence with high-energy neutrinos
... Neutrinos provide a promising sector for observing the effects of quantum decoherence. Although atmo- spheric, solar and supernova neutrinos have been pre- viously studied in this context [3,4], high-energy ... See full document
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