2,243 research outputs found
TeV cosmic-ray proton and helium spectra in the myriad model
Recent measurements of cosmic ray proton and helium spectra show a hardening
above a few hundreds of GeV. This excess is hard to understand in the framework
of the conventional models of Galactic cosmic ray production and propagation.
We propose here to explain this anomaly by the presence of local sources
(myriad model). Cosmic ray propagation is described as a diffusion process
taking place inside a two-zone magnetic halo. We calculate the proton and
helium fluxes at the Earth between 50 GeV and 100 TeV. Improving over a similar
analysis, we consistently derive these fluxes by taking into account both local
and remote sources for which a unique injection rate is assumed. We find cosmic
ray propagation parameters compatible with B/C measurements and for which the
proton and helium spectra remarkably agree with the PAMELA and CREAM
measurements over four decades in energy.Comment: 5 pages, 3 figure
Transport parameters from AMS-02 F/Si data and fluorine source abundance
The AMS-02 collaboration recently released cosmic-ray F/Si data of
unprecedented accuracy. CR F is predominantly produced by fragmentation of
heavier progenitors, while Si is mostly accelerated at source. This ratio is
thus maximally sensitive to CR propagation. We study the compatibility of the
transport parameters derived from the F/Si ratio with those obtained from the
lighter Li/C, Be/C, and B/C ratios. We also inspect the CR source abundance of
F, one of the few elements with a high first ionisation potential but only
moderately volatile, and a potentially key element to study the acceleration
mechanism of CRs. We use the 1D diffusion model implemented in the USINE code
and perform analyses accounting for several systematic effects (energy
correlations in data, nuclear cross sections and solar modulation
uncertainties). We also take advantage of the EXFOR nuclear database to update
the F production cross sections for its most important progenitors (identified
to be 56Fe, 32S, 28Si, 27Al, 24Mg, 22Ne, and 20Ne). The transport parameters
obtained from AMS-02 F/Si data are compatible with those obtained from AMS-02
(Li,Be,B)/C data. The combined fit of all these ratios leads to a
, with adjustments of the B and F
production cross sections (the latter are based on very few nuclear data
points, and would strongly benefit from new measurements). The F/Si ratio is
compatible with a pure secondary origin of F, with a best-fit relative source
abundance 19F/28Si and an upper limit of . Unfortunately, this limit is not sufficient to test global
acceleration models of CR nuclei, for which values at the level of are required. Such levels could be attained with F/Si data of a few
percent accuracy at a few tens of TV, possibly within reach of the next
generation of CR experiments.Comment: 15 pages, 13 figures, 3 table (1 appendix). Submitted to A&
The rigidity dependence of galactic cosmic-ray fluxes and its connection with the diffusion coefficient
Thanks to tremendous experimental efforts, galactic cosmic-ray fluxes are being measured up to the unprecedented per cent precision level. The logarithmic slope of these fluxes is a crucial quantity that promises us information on the diffusion properties and the primary or secondary nature of the different species. However, these measured slopes are sometimes interpreted in the pure diffusive regime, guiding to misleading conclusions. In this paper, we have studied the propagation of galactic cosmic rays by computing the fluxes of species between H and Fe using the USINE code and considering all the relevant physical processes and an updated set of cross-section data. We show that the slope of the well-studied secondary-to-primary B/C ratio is distinctly different from the diffusion coefficient slope, by an offset of about 0.2 in the rigidity range in which the AMS-02 data reach their best precision (several tens of GV). Furthermore, we have demonstrated that none of the species from H to Fe follows the expectations of the pure-diffusive regime. We argue that these differences arise from propagation processes such as fragmentation, convection, and reacceleration, which cannot be neglected. On this basis, we also provide predictions for the spectral slope of elemental fluxes not yet analysed by the AMS collaboration
Antimatter signals of singlet scalar dark matter
We consider the singlet scalar model of dark matter and study the expected
antiproton and positron signals from dark matter annihilations. The regions of
the viable parameter space of the model that are excluded by present data are
determined, as well as those regions that will be probed by the forthcoming
experiment AMS-02. In all cases, different propagation models are investigated,
and the possible enhancement due to dark matter substructures is analyzed. We
find that the antiproton signal is more easily detectable than the positron one
over the whole parameter space. For a typical propagation model and without any
boost factor, AMS-02 will be able to probe --via antiprotons-- the singlet
model of dark matter up to masses of 600 GeV. Antiprotons constitute,
therefore, a promising signal to constraint or detect the singlet scalar model.Comment: 24 pages, 8 figures. v2: minor improvements. Accepted for publication
in JCA
Complementarity of Galactic radio and collider data in constraining WIMP dark matter models
In this work we confront dark matter models to constraints that may be
derived from radio synchrotron radiation from the Galaxy, taking into account
the astrophysical uncertainties and we compare these to bounds set by
accelerator and complementary indirect dark matter searches. Specifically we
apply our analysis to three popular particle physics models. First, a generic
effective operator approach, in which case we set bounds on the corresponding
mass scale, and then, two specific UV completions, the Z' and Higgs portals. We
show that for many candidates, the radio synchrotron limits are competitive
with the other searches, and could even give the strongest constraints (as of
today) with some reasonable assumptions regarding the astrophysical
uncertainties.Comment: 22 pages, 12 figure
B NMR study of pure and lightly carbon doped MgB superconductors
We report a B NMR line shape and spin-lattice relaxation rate
() study of pure and lightly carbon doped MgBC for
, 0.02, and 0.04, in the vortex state and in magnetic field of 23.5 kOe.
We show that while pure MgB exhibits the magnetic field distribution from
superposition of the normal and the Abrikosov state, slight replacement of
boron with carbon unveils the magnetic field distribution of the pure Abrikosov
state. This indicates a considerable increase of with carbon doping
with respect to pure MgB. The spin-lattice relaxation rate
demonstrates clearly the presence of a coherence peak right below in pure
MgB, followed by a typical BCS decrease on cooling. However, at
temperatures lower than K strong deviation from the BCS behavior is
observed, probably from residual contribution of the vortex dynamics. In the
carbon doped systems both the coherence peak and the BCS temperature dependence
of weaken, an effect attributed to the gradual shrinking of the
hole cylinders of the Fermi surface with electron doping.Comment: 8 pages, 6 figures, submitted to Phys. Rev.
Retention of Two-Band Superconductivity in Highly Carbon-Doped MgB2
Tunneling data on MgB_{1.8}C_{0.2} show a reduction in the energy gap of the
pi-bands by a factor of two from undoped MgB2 that is consistent with the Tc
reduction, but inconsistent with the expectations of the dirty limit.
Dirty-limit theory for undoped MgB2 predicts a single gap about three times
larger than measured and a reduced Tc comparable to that measured. Our
heavily-doped samples exhibit a uniform dispersion of C suggestive of
significantly enhanced scattering, and we conclude that the retention of
two-band superconductivity in these samples is caused by a selective
suppression of interband scattering.Comment: 4 pages, 4 figures; added one figure, added one reference, minor
changes to the text, manuscript accepted for publication as a Phys. Rev. B
Rapid Communicatio
R-parity preserving super-WIMP decays
We point out that when the decay of one electroweak scale super-WIMP state to
another occurs at second order in a super-weak coupling constant, this can
naturally lead to decay lifetimes that are much larger than the age of the
Universe, and create observable consequences for the indirect detection of dark
matter. We demonstrate this in a supersymmetric model with Dirac neutrinos,
where the right-handed scalar neutrinos are the lightest and next-to-lightest
supersymmetric partners. We show that this model produces a super-WIMP decay
rate scaling as m_nu^4/(weak scale)^3, and may significantly enhance the
fraction of energetic electrons and positrons over anti-protons in the decay
products. Such a signature is consistent with the observations recently
reported by the PAMELA experiment.Comment: 14 pages, v3 JHEP versio
A magnetization and B NMR study of MgAlB superconductors
We demonstrate for the first time the magnetic field distribution of the pure
vortex state in lightly doped MgAlB () powder
samples, by using B NMR in magnetic fields of 23.5 and 47 kOe. The
magnetic field distribution at T=5 K is Al-doping dependent, revealing a
considerable decrease of anisotropy in respect to pure MgB. This result
correlates nicely with magnetization measurements and is consistent with
-band hole driven superconductivity for MgB
The camera of the fifth H.E.S.S. telescope. Part I: System description
In July 2012, as the four ground-based gamma-ray telescopes of the H.E.S.S.
(High Energy Stereoscopic System) array reached their tenth year of operation
in Khomas Highlands, Namibia, a fifth telescope took its first data as part of
the system. This new Cherenkov detector, comprising a 614.5 m^2 reflector with
a highly pixelized camera in its focal plane, improves the sensitivity of the
current array by a factor two and extends its energy domain down to a few tens
of GeV.
The present part I of the paper gives a detailed description of the fifth
H.E.S.S. telescope's camera, presenting the details of both the hardware and
the software, emphasizing the main improvements as compared to previous
H.E.S.S. camera technology.Comment: 16 pages, 13 figures, accepted for publication in NIM
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