90 research outputs found
P-D Effects on the Reliability of Oil Offshore Jacket Platforms in Mexico
Given the important economic consequences of an oil platform failure, all the aspects of its structural behavior and safety issues need to be carefully considered. In particular, P-D effects on the deck legs of marine offshore jacket platforms may be relevant when the deck height and the vertical load are significant. In this paper, the impact of the moment amplification, due to lenderness of the deck legs, on the platform safety is examined and appraised from he viewpoint of the structural reliability. The formulation is applied to a typical tall deck marine platform under the environmental loading at the Bay of Campeche, Mexico, and its reliability index is calculated with and without the P-D effect. The results presented herein may be sed to improve the current practice in the design and assessment of offshore marine platforms in Mexico and to update the current version of the code
Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory
We present the results of dark matter (DM) searches in a sample of 31 dwarf
irregular (dIrr) galaxies within the field of view of the HAWC Observatory.
dIrr galaxies are DM dominated objects, which astrophysical gamma-ray emission
is estimated to be negligible with respect to the secondary gamma-ray flux
expected by annihilation or decay of Weakly Interacting Massive Particles
(WIMPs). While we do not see any statistically significant DM signal in dIrr
galaxies, we present the exclusion limits () for annihilation
cross-section and decay lifetime for WIMP candidates with masses between
and . Exclusion limits from dIrr galaxies are relevant and
complementary to benchmark dwarf Spheroidal (dSph) galaxies. In fact, dIrr
galaxies are targets kinematically different from benchmark dSph, preserving
the footprints of different evolution histories. We compare the limits from
dIrr galaxies to those from ultrafaint and classical dSph galaxies previously
observed with HAWC. We find that the contraints are comparable to the limits
from classical dSph galaxies and orders of magnitude weaker than
the ultrafaint dSph limits.Comment: 22 pages, 11 figures, 3 table
Limits on the Diffuse Gamma-Ray Background above 10 TeV with HAWC
The high-energy Diffuse Gamma-Ray Background (DGRB) is expected to be
produced by unresolved isotropically distributed astrophysical objects,
potentially including dark matter annihilation or decay emissions in galactic
or extragalactic structures. The DGRB has only been observed below 1 TeV; above
this energy, upper limits have been reported. Observations or stringent limits
on the DGRB above this energy could have significant multi-messenger
implications, such as constraining the origin of TeV-PeV astrophysical
neutrinos detected by IceCube. The High Altitude Water Cherenkov (HAWC)
Observatory, located in central Mexico at 4100 m above sea level, is sensitive
to gamma rays from a few hundred GeV to several hundred TeV and continuously
observes a wide field-of-view (2 sr). With its high-energy reach and large area
coverage, HAWC is well-suited to notably improve searches for the DGRB at TeV
energies. In this work, strict cuts have been applied to the HAWC dataset to
better isolate gamma-ray air showers from background hadronic showers. The
sensitivity to the DGRB was then verified using 535 days of Crab data and Monte
Carlo simulations, leading to new limits above 10 TeV on the DGRB as well as
prospective implications for multi-messenger studies.Comment: 8 pages, 3 figure
Search for Decaying Dark Matter in the Virgo Cluster of Galaxies with HAWC
The decay or annihilation of dark matter particles may produce a steady flux
of very-high-energy gamma rays detectable above the diffuse background. Nearby
clusters of galaxies provide excellent targets to search for the signatures of
particle dark matter interactions. In particular, the Virgo cluster spans
several degrees across the sky and can be efficiently probed with a wide
field-of-view instrument. The High Altitude Water Cherenkov (HAWC) observatory,
due to its wide field of view and sensitivity to gamma rays at an energy scale
of 300 GeV--100 TeV is well-suited for this search. Using 2141 days of data, we
search for gamma-ray emission from the Virgo cluster, assuming well-motivated
dark matter sub-structure models. Our results provide some of the strongest
constraints on the decay lifetime of dark matter for masses above 10 TeV.Comment: 7 pages, 3 figures. Submitted to PR
HAWC Study of Very-High-Energy -ray Spectrum of HAWC J1844-034
Recently, the region surrounding eHWC J1842-035 has been studied extensively
by gamma-ray observatories due to its extended emission reaching up to a few
hundred TeV and potential as a hadronic accelerator. In this work, we use 1,910
days of cumulative data from the High Altitude Water Cherenkov (HAWC)
observatory to carry out a dedicated systematic source search of the eHWC
J1842-035 region. During the search we have found three sources in the region,
namely, HAWC J1844-034, HAWC J1843-032, and HAWC J1846-025. We have identified
HAWC J1844-034 as the extended source that emits photons with energies up to
175 TeV. We compute the spectrum for HAWC J1844-034 and by comparing with the
observational results from other experiments, we have identified HESS
J1843-033, LHAASO J1843-0338, and TASG J1844-038 as very-high-energy gamma-ray
sources with a matching origin. Also, we present and use the multi-wavelength
data to fit the hadronic and leptonic particle spectra. We have identified four
pulsar candidates in the nearby region from which PSR J1844-0346 is found to be
the most likely candidate due to its proximity to HAWC J1844-034 and the
computed energy budget. We have also found SNR G28.6-0.1 as a potential
counterpart source of HAWC J1844-034 for which both leptonic and hadronic
scenarios are feasible.Comment: 13 pages, 9 figures, published in Ap
Validation of standardized data formats and tools for ground-level particle-based gamma-ray observatories
Ground-based gamma-ray astronomy is still a rather young field of research,with strong historical connections to particle physics. This is why mostobservations are conducted by experiments with proprietary data and analysissoftware, as it is usual in the particle physics field. However in recentyears, this paradigm has been slowly shifting towards the development and useof open-source data formats and tools, driven by upcoming observatories such asthe Cherenkov Telescope Array (CTA). In this context, a community-driven,shared data format (the gamma-astro-data-format or GADF) and analysis toolssuch as Gammapy and ctools have been developed. So far these efforts have beenled by the IACT community, leaving out other types of ground-based gamma-rayinstruments.We aim to show that the data from ground particle arrays, such asthe High-Altitude Water Cherenkov (HAWC) observatory, is also compatible withthe GADF and can thus be fully analysed using the related tools, in this caseGammapy. We reproduce several published HAWC results using Gammapy and dataproducts compliant with GADF standard. We also illustrate the capabilities ofthe shared format and tools by producing a joint fit of the Crab spectrumincluding data from six different gamma-ray experiments. We find excellentagreement with the reference results, a powerful check of both the publishedresults and the tools involved. The data from particle detector arrays such asthe HAWC observatory can be adapted to the GADF and thus analysed with Gammapy.A common data format and shared analysis tools allow multi-instrument jointanalysis and effective data sharing. Given the complementary nature of pointingand wide-field instruments, this synergy will be distinctly beneficial for thejoint scientific exploitation of future observatories such as the SouthernWide-field Gamma-ray Observatory and CTA.<br
High Altitude characterization of the Hunga Pressure Wave with Cosmic Rays by the HAWC Observatory
High-energy cosmic rays that hit the Earth can be used to study large-scale
atmospheric perturbations. After a first interaction in the upper parts of the
atmosphere, cosmic rays produce a shower of particles that sample the
atmosphere down to the detector level. The HAWC (High-Altitude Water Cherenkov)
cosmic-ray observatory in Central Mexico at 4,100 m elevation detects air
shower particles continuously with 300 water Cherenkov detectors with an active
area of 12,500 m. On January 15th, 2022, HAWC detected the passage of the
pressure wave created by the explosion of the Hunga volcano in the Tonga
islands, 9,000 km away, as an anomaly in the measured rate of shower particles.
The HAWC measurements are used to characterize the shape of four pressure wave
passages, determine the propagation speed of each one, and correlate the
variations of the shower particle rates with the barometric pressure changes,
extracting a barometric parameter. The profile of the shower particle rate and
atmospheric pressure variations for the first transit of the pressure wave at
HAWC is compared to the pressure measurements at Tonga island, near the
volcanic explosion. This work opens the possibility of using large particle
cosmic-ray air shower detectors to trace large atmospheric transient waves.Comment: Contact about this analysis: A. Sandoval ([email protected]),
A. Lara ([email protected]) & H. Le\'on Vargas
([email protected]
HAWC and Fermi-LAT Detection of Extended Emission from the Unidentified Source 2HWC J2006+341
The discovery of the TeV point source 2HWC J2006+341 was reported in the
second HAWC gamma-ray catalog. We present a follow-up study of this source
here. The TeV emission is best described by an extended source with a soft
spectrum. At GeV energies, an extended source is significantly detected in
Fermi-LAT data. The matching locations, sizes and spectra suggest that both
gamma-ray detections correspond to the same source. Different scenarios for the
origin of the emission are considered and we rule out an association to the
pulsar PSR J2004+3429 due to extreme energetics required, if located at a
distance of 10.8 kpc.Comment: 12 pages, 2 figures. To appear in ApJ
Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC
We present the first catalog of gamma-ray sources emitting above 56 and 100
TeV with data from the High Altitude Water Cherenkov (HAWC) Observatory, a wide
field-of-view observatory capable of detecting gamma rays up to a few hundred
TeV. Nine sources are observed above 56 TeV, all of which are likely Galactic
in origin. Three sources continue emitting past 100 TeV, making this the
highest-energy gamma-ray source catalog to date. We report the integral flux of
each of these objects. We also report spectra for three highest-energy sources
and discuss the possibility that they are PeVatrons.Comment: Accepted by Physical Review Letter
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