73 research outputs found
Damage tolerance assessment by bend and shear tests of two multilayer composites: Glass fibre reinforced metal laminate and aluminium roll-bonded laminate
The damage tolerance of an aluminium roll-bonded laminate (ALH19) and a
glass fibre reinforced laminate (GLARE) (both based in Al 2024-T3) has been studied.
The composite laminates have been tested under 3-point bend and shear tests on the
interfaces to analyze their fracture behaviour. During the bend tests different fracture
mechanisms were activated for both laminates, which depend on the constituent
materials and their interfaces. The high intrinsic toughness of the pure Al 1050 layers
present in the aluminium roll-bonded laminate (ALH19), together with extrinsic
toughening mechanisms such as crack bridging and interface delamination were
responsible for the enhanced toughness of this composite laminate. On the other hand,
crack deflection by debonding between the glass fibres and the plastic resin in GLARE,
was the main extrinsic toughening mechanism present in this composite laminateFinancial support from CICYT (Project MAT2003-01172) is gratefully
acknowledged. C.M. Cepeda-Jiménez thanks the Spanish Ministry of Education and
Science for a Juan de la Cierva contract. Authors also thank Delft University of
Technology for providing the GLARE.Peer reviewe
Effect of thermal treatment on the interfacial shear toughness of an aluminium composite laminate
The microstructure and mechanical properties in the interface region of a
multilayer composite laminate based on Al-Zn (Al 7075) and Al-Cu (Al 2024) alloys
have been mainly characterized by EBSD and shear tests. It is shown that varying
solution heat treatments affect the microstructure of the constituent aluminium alloys in
the bonding region and, as a consequence, the interfacial mechanical properties. The
increase in the solution treatment time improves the interfacial toughness of the
multilayer aluminium laminate due to higher intrinsic toughness of the constituent
aluminium alloys.Financial support from CICYT (Project MAT2003-01172 and MAT2006-11202)
is gratefully acknowledged. C.M. Cepeda-Jiménez thanks the Spanish National
Research Council (CSIC) for a I3P contract. We also thank F.F. GonzĂĄlez-RodrĂguez
for assistance during hot rolling. Finally, an especial mention in memory of P.J.
GonzĂĄlez-Aparicio for his help and assistance with electron microscopy during all these
years is made.Peer reviewe
Evolution of the microstructure, texture and creep properties of the 7075 aluminium alloy during hot accumulative roll bonding
The 7075 Al alloy was severely deformed at 350 °C by a 3:1 thickness reduction per pass accumulative roll bonding (ARB) process up to six passes. It was found that discontinuous recrystallisation occurs during the inter-pass annealing stages from the third pass on, attributable to the increment of the mean particle size during processing. As a consequence, the mean crystallite size did not decrease, but remained approximately constant at 440 nm along the present ARB process and the mean boundary misorientation angle reached a maximum of 30° for the 3-passes sample. However, since nucleation of new grains takes place at the pre-existing grain boundaries, discontinuous recrystallisation results in slight changes in texture throughout the processing, being the orientations in the ARBed samples predominantly located along the typical rolling ÎČ-fibre. Uniaxial tests conducted at 300 °C and 350 °C revealed that the operating deformation mechanism in the processed alloy at such temperatures was grain boundary sliding; the optimum superplastic strain rate being 3Ă10â3â10â2 sâ1. Boundary misorientation and thermal stability are the two main factors that contribute to high elongations to failureFinancial support from the CICYT (Projects MAT2009-14452 and MAT2012-38962)Peer reviewe
All-sky search for long-duration gravitational wave transients with initial LIGO
We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4Ă10-5 and 9.4Ă10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society
All-sky search for long-duration gravitational wave transients with initial LIGO
We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; as a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4Ă10-5 and 9.4Ă10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves. © 2016 American Physical Society
Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background
The detection of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational waves. While general relativity allows for only two tensor gravitational-wave polarizations, general metric theories can additionally predict two vector and two scalar polarizations. The polarization of gravitational waves is encoded in the spectral shape of the stochastic gravitational-wave background, formed by the superposition of cosmological and individually unresolved astrophysical sources. Using data recorded by Advanced LIGO during its first observing run, we search for a stochastic background of generically polarized gravitational waves. We find no evidence for a background of any polarization, and place the first direct bounds on the contributions of vector and scalar polarizations to the stochastic background. Under log-uniform priors for the energy in each polarization, we limit the energy densities of tensor, vector, and scalar modes at 95% credibility to Ω0T<5.58Ă10-8, Ω0V<6.35Ă10-8, and Ω0S<1.08Ă10-7 at a reference frequency f0=25 Hz. © 2018 American Physical Society
Influence of the thermomechanical processing on the fracture mechanisms of high strength aluminium/pure aluminium multilayer laminate materials
The microstructure and mechanical properties, with emphasis in the impact
fracture toughness behaviour, of two multilayer laminate materials have been
investigated. The multilayer materials are constituted by alternated sheets of pure
aluminium (Al 1200 or Al 1050) and high strength Al 7075 alloy. Stacked layers of
these alloys have been successfully joined using two processing routes with different
total hot rolling strains. Both laminates have been tested at room temperature under
impact Charpy tests, 3-point bend tests and shear tests on the interfaces. Both laminates
exhibited more than eight times improvement in impact fracture toughness over the
monolithic Al 7075-T6. The toughness increase in the higher rolling strained laminate is
almost entirely due to crack blunting mechanism, while in the lower strained laminate,
crack deflection by delamination and crack renucleation processes were active.Financial support from CICYT (Project MAT2003-01172) is gratefully
acknowledged. C.M. Cepeda-Jiménez thanks the Spanish Ministry of Education and
Science for a Juan de la Cierva contract. We also thank L. del Real-AlarcĂłn for the
welding work, F.F. GonzĂĄlez-RodrĂguez for assistance during hot rolling and J. Chao-
Hermida for assistance with the Charpy impact test.Peer reviewe
Influence of the thermal treatment on the microstructure and hardness evolution of 7075 aluminium layers in a hot-rolled multilayer laminate composite
The microstructure and mechanical properties of the Al 7075 alloy present in a
hot roll-bonded laminate consisting of Al 7075/Al 2024 layers have been characterized
by high resolution electron backscattering diffraction (EBSD) analysis and Vickers
microhardness, respectively. The as-rolled deformation structure consisted in lamellar
bands aligned parallel to the rolling direction. It was found that a post-rolling tempering
at 175ÂșC/6 h, prior to the T6 treatment has a profound effect on the microstructure and
the mechanical properties of the Al 7075 alloy. This tempering reduces the driving
force for recrystallization during the usual solution treatment of 30 min that is part of
the T6 treatment. The performed procedures favour a more homogeneous precipitation
during the following age hardening step and the achievement of a noticeable increase in
Vickers microhardness.Financial support from CICYT (Projects MAT2003-01172 and MAT2006-
11202) is gratefully acknowledged. C.M. Cepeda-Jiménez thanks the Spanish National
Research Council (CSIC) for a I3P contract.Peer reviewe
Study of hot deformation of an Al-Cu-Mg alloy using processing maps and microstructural characterization
The forming behaviour of an AlâCuâMg alloy (Al 2024-T351) has been studied by processing maps and
microstructural characterization. Torsion tests were conducted in the range 278â467 âŠC, between 2.1 and
25.6 sâ1. Stressâstrain curves obtained from the experiment data were fitted using the Garofalo equation
to obtain the constitutive parameters, obtaining a stress exponent of 6.1 and an activation energy of
180 kJ/mol. Electron backscatter diffraction (EBSD) was employed to characterize the microtexture and
microstructure, before and after torsion testing, to evaluate the microstructural changes and instability
phenomena. A peak ductility of the Al 2024 alloy was found at about 400 âŠC at all strain rates considered.
According to the processing maps and microstructure observation, the optimum hot deformation
condition for the Al 2024 alloy is in the range 360â410 âŠC and 2.1â4.5 sâ1. Under these favourable conditions
a uniform and fine grain size is obtained by extended dynamic recovery (DRV), which leads to the
formation of subgrain boundaries that progressively transform at large strains into new high angle grain
boundariesFinancial support from CICYT (Project MAT2009-14452)Peer reviewe
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