The Large Hadron Collider forward (LHCf) experiment is designed to use the LHC to verify the hadronic-interaction models used in cosmic-ray physics. Forward baryon production is one of the crucial ...points to understand the development of cosmic-ray showers. We report the neutron-energy spectra for LHC s=7 TeV proton–proton collisions with the pseudo-rapidity η ranging from 8.81 to 8.99, from 8.99 to 9.22, and from 10.76 to infinity. The measured energy spectra obtained from the two independent calorimeters of Arm1 and Arm2 show the same characteristic feature before unfolding the detector responses. We unfolded the measured spectra by using the multidimensional unfolding method based on Bayesian theory, and the unfolded spectra were compared with current hadronic-interaction models. The QGSJET II-03 model predicts a high neutron production rate at the highest pseudo-rapidity range similar to our results, and the DPMJET 3.04 model describes our results well at the lower pseudo-rapidity ranges. However, no model perfectly explains the experimental results over the entire pseudo-rapidity range. The experimental data indicate a more abundant neutron production rate relative to the photon production than any model predictions studied here.
Let X be a real Banach space. The rectangular constant
$\mu (X)$
and some generalisations of it,
$\mu _p(X)$
for
$p \geq 1$
, were introduced by Gastinel and Joly around half a century ago. In this ...paper we make precise some characterisations of inner product spaces by using
$\mu _p(X)$
, correcting some statements appearing in the literature, and extend to
$\mu _p(X)$
some characterisations of uniformly nonsquare spaces, known only for
$\mu (X)$
. We also give a characterisation of two-dimensional spaces with hexagonal norms. Finally, we indicate some new upper estimates concerning
$\mu (l_p)$
and
$\mu _p(l_p)$
.
The differential cross sections for inclusive neutral pions as a function of transverse and longitudinal momentum in the very forward-rapidity region have been measured at the LHC with the LHC ...forward detector in proton-proton collisions at sradical=2.76 and 7 TeV and in proton-lead collisions at nucleon-nucleon center-of-mass energies of super()sNNradical=5.02TeV. Such differential cross sections in proton-proton collisions are compatible with the hypotheses of limiting fragmentation and Feynman scaling. Comparing proton-proton with proton-lead collisions, we find a sizable suppression of the production of neutral pions in the differential cross sections after subtraction of ultraperipheral proton-lead collisions. This suppression corresponds to the nuclear modification factor value of about 0.1-0.3. The experimental measurements presented in this paper provide a benchmark for the hadronic interaction Monte Carlo simulation codes that are used for the simulation of cosmic ray air showers.
A
bstract
In this paper, we report the measurement of the energy flow, the cross section and the average inelasticity of forward neutrons (+ antineutrons) produced in
s
= 13 TeV proton-proton ...collisions. These quantities are obtained from the inclusive differential production cross section, measured using the LHCf Arm2 detector at the CERN Large Hadron Collider. The measurements are performed in six pseudorapidity regions: three of them (
η >
10
.
75, 8
.
99
< η <
9
.
21 and 8
.
80
< η <
8
.
99), albeit with smaller acceptance and larger uncertainties, were already published in a previous work, whereas the remaining three (10
.
06
< η <
10
.
75, 9
.
65
< η <
10
.
06 and 8
.
65
< η <
8
.
80) are presented here for the first time. The analysis was carried out using a data set acquired in June 2015 with a corresponding integrated luminosity of 0
.
194 nb
−
1
. Comparing the experimental measurements with the expectations of several hadronic interaction models used to simulate cosmic ray air showers, none of these generators resulted to have a satisfactory agreement in all the phase space selected for the analysis. The inclusive differential production cross section for
η >
10
.
75 is not reproduced by any model, whereas the results still indicate a significant but less serious deviation at lower pseudorapidities. Depending on the pseudorapidity region, the generators showing the best overall agreement with data are either SIBYLL 2.3 or EPOS-LHC. Furthermore, apart from the most forward region, the derived energy flow and cross section distributions are best reproduced by EPOS-LHC. Finally, even if none of the models describe the elasticity distribution in a satisfactory way, the extracted average inelasticity is consistent with the QGSJET II-04 value, while most of the other generators give values that lie just outside the experimental uncertainties.
A
bstract
The forward
η
mesons production has been observed by the Large Hadron Collider forward (LHCf) experiment in proton-proton collision at
$$ \sqrt{s} $$
s
= 13 TeV. This paper presents the ...measurement of the inclusive production rate of
η
in
p
T
<
1
.
1 GeV/c, expressed as a function of the Feynman-
x
variable. These results are compared with the predictions of several hadronic interaction models commonly used for the modelling of the air showers produced by ultra-high energy cosmic rays. This is both the first measurement of
η
mesons from LHCf and the first time a particle containing strange quarks has been observed in the forward region for high-energy collisions. These results will provide a powerful constraint on hadronic interaction models for the purpose of improving the understanding of the processes underlying the air showers produced in the Earth’s atmosphere by ultra-energetic cosmic rays.
In this paper, we report the production cross-section of forward photons in the pseudorapidity regions of η>10.94 and 8.99>η>8.81, measured by the LHCf experiment with proton–proton collisions at ...s=13TeV. The results from the analysis of 0.191nb−1 of data obtained in June 2015 are compared to the predictions of several hadronic interaction models that are used in air-shower simulations for ultra-high-energy cosmic rays. Although none of the models agree perfectly with the data, EPOS-LHC shows the best agreement with the experimental data among the models.
A
bstract
In this paper, we report the measurement relative to the production of forward neutrons in proton-proton collisions at
s
=
13
TeV obtained using the LHCf Arm2 detector at the Large Hadron ...Collider. The results for the inclusive differential production cross section are presented as a function of energy in three different pseudorapidity regions:
η
> 10.76, 8.99 <
η
< 9.22 and 8.81 <
η
< 8.99. The analysis was performed using a data set acquired in June 2015 that corresponds to an integrated luminosity of 0.194 nb
−1
. The measurements were compared with the predictions of several hadronic interaction models used to simulate air showers generated by Ultra High Energy Cosmic Rays. None of these generators showed good agreement with the data for all pseudorapidity intervals. For
η
> 10.76, no model is able to reproduce the observed peak structure at around 5 TeV and all models underestimate the total production cross section: among them, QGSJET II-04 shows the smallest deficit with respect to data for the whole energy range. For 8.99 <
η
< 9.22 and 8.81 <
η
< 8.99, the models having the best overall agreement with data are SIBYLL 2.3 and EPOS-LHC, respectively: in particular, in both regions SIBYLL 2.3 is able to reproduce the observed peak structure at around 1.5–2.5 TeV.
A
bstract
The forward
η
mesons production has been observed by the Large Hadron Collider forward (LHCf) experiment in proton-proton collision at
s
= 13 TeV. This paper presents the measurement of the ...inclusive production rate of
η
in
p
T
<
1
.
1 GeV/c, expressed as a function of the Feynman-
x
variable. These results are compared with the predictions of several hadronic interaction models commonly used for the modelling of the air showers produced by ultra-high energy cosmic rays. This is both the first measurement of
η
mesons from LHCf and the first time a particle containing strange quarks has been observed in the forward region for high-energy collisions. These results will provide a powerful constraint on hadronic interaction models for the purpose of improving the understanding of the processes underlying the air showers produced in the Earth’s atmosphere by ultra-energetic cosmic rays.
Abstract
The multi-TeV energy region of the cosmic-ray spectra has
been recently explored by direct detection experiments that used
calorimetric techniques to measure the energy of the cosmic
...particles. Interesting spectral features have been observed in both
all-electron and nuclei spectra. However, the interpretation of the
results is compromised by the disagreements between the data
obtained from the various experiments, that are not reconcilable
with the quoted experimental uncertainties. Understanding the
reason for the discrepancy among the measurements is of fundamental
importance in view of the forthcoming high-energy cosmic-ray
experiments planned for space, as well as for the correct
interpretation of the available results.
The purpose of this work is to investigate the possibility that a
systematic effect may derive from the non-proportionality of the
light response of inorganic crystals, typically used in high-energy
calorimetry due to their excellent energy-resolution performance.
The main reason for the non-proportionality of the crystals is that
scintillation light yield depends on ionisation density.
Experimental data obtained with ion beams were used to characterize
the light response of various scintillator materials. The obtained
luminous efficiencies were used as input of a Monte Carlo simulation
to perform a comparative study of the effect of the light-yield
non-proportionality on the detection of high-energy electromagnetic
and hadronic showers. The result of this study indicates that, if
the calorimeter response is calibrated by using the energy deposit
of minimum ionizing particles, the measured shower energy might be
affected by a significant systematic shift, at the level of few
percent, whose sign and magnitude depend specifically on the type of
scintillator material used.
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