212 research outputs found
Efficient and secure digital signature algorithm (DSA)
The digital signature is used to ensure the integrity of messages as well as the authentication and non-repudiation of users. Today it has a very important role in information security. Digital signature is used in various fields such as e-commerce and e-voting, health, internet of things (IOT). Many digital signature schemes have been proposed, depending on the computational cost and security level. In this paper, we analyzed a recently proposed digital signature scheme based on the discrete logarithm problem (DLP). Our analysis shows that the scheme is not secure against the repeated random number attack to determine the secret keys of the signer. To overcome this problem, we propose a new improvement of the digital signature scheme
Oxinium femoral head damage generated by a metallic foreign body within the polyethylene cup following recurrent dislocation episodes
SummaryOxinium femoral heads are supposed to be more scratch-resistant thanks to their oxidized layer. However, damages to this thin layer can jeopardize implant's properties. Following revision total hip arthroplasty performed for recurrent posterior dislocations, the Oxinium femoral head initially implanted was observed to be dramatically damaged. A metallic foreign body from a trochanteric fixation wire was found within the polyethylene cup. Only few cases of damaged Oxinium femoral heads have been reported and all were related to either dislocation or reduction of THA. The aim of this report is to describe a non-reported mechanism of damaged Oxinium femoral head due to a broken trochanteric fixation wire device. Any broken metallic wire from a transtrochanteric approach should be carefully followed to detect migration within the polyethylene cup. If such a migration occurs, revision surgery should be rapidly scheduled
Improved Convergence Bounds For Operator Splitting Algorithms With Rare Extreme Errors
In this paper, we improve upon our previous work[24,22] and establish
convergence bounds on the objective function values of approximate
proximal-gradient descent (AxPGD), approximate accelerated proximal-gradient
descent (AxAPGD) and approximate proximal ADMM (AxWLM-ADMM) schemes. We
consider approximation errors that manifest rare extreme events and we
propagate their effects through iterations. We establish probabilistic
asymptotic and non-asymptotic convergence bounds as functions of the range
(upper/lower bounds) and variance of approximation errors. We use the derived
bound to assess AxPGD in a sparse model predictive control of a spacecraft
system and compare its accuracy with previously derived bounds
A Novel Approach for Enhancing Routing in Wireless Sensor Networks using ACO Algorithm
Wireless Sensors Network (WSN) is an emergent technology that aims to offer innovative capacities. In the last decade, the use of these networks increased in various fields like military, science, and health due to their fast and inexpressive deployment and installation. However, the limited sensor battery lifetime poses many technical challenges and affects essential services like routing. This issue is a hot topic of search, many researchers have proposed various routing protocols aimed at reducing the energy consumption in WSNs. The focus of this work is to investigate the effectiveness of integrating ACO algorithm with routing protocols in WSNs. Moreover, it presents a novel approach inspired by ant colony optimization (ACO) to be deployed as a new routing protocol that addresses key challenges in wireless sensor networks. The proposed protocol can significantly minimize nodes energy consumption, enhance the network lifetime, reduce latency, and expect performance in various scenarios
A Low-Power Hardware-Friendly Optimisation Algorithm With Absolute Numerical Stability and Convergence Guarantees
We propose Dual-Feedback Generalized Proximal Gradient Descent (DFGPGD) as a
new, hardware-friendly, operator splitting algorithm. We then establish
convergence guarantees under approximate computational errors and we derive
theoretical criteria for the numerical stability of DFGPGD based on absolute
stability of dynamical systems. We also propose a new generalized proximal ADMM
that can be used to instantiate most of existing proximal-based composite
optimization solvers. We implement DFGPGD and ADMM on FPGA ZCU106 board and
compare them in light of FPGA's timing as well as resource utilization and
power efficiency. We also perform a full-stack, application-to-hardware,
comparison between approximate versions of DFGPGD and ADMM based on dynamic
power/error rate trade-off, which is a new hardware-application combined
metric
The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at
We present a spectro-photometric study of a mass-complete sample of quiescent
galaxies at with
drawn from the
VANDELS survey, exploring the relationship between stellar mass, age and
star-formation history. Within our sample of 114 galaxies, we derive a
stellar-mass vs stellar-age relation with a slope of Gyr
per decade in stellar mass. When combined with recent literature results, we
find evidence that the slope of this relation remains consistent over the
redshift interval . The galaxies within the VANDELS quiescent display a
wide range of star-formation histories, with a mean star-formation timescale of
Gyr and a mean quenching timescale of Gyr. We also
find a large scatter in the quenching timescales of the VANDELS quiescent
galaxies, in agreement with previous evidence that galaxies at cease
star formation via multiple mechanisms. We then focus on the oldest galaxies in
our sample, finding that the number density of galaxies that quenched before with stellar masses is . Although
uncertain, this estimate is in good agreement with the latest observational
results at , tentatively suggesting that neither rejuvenation nor merger
events are playing a major role in the evolution of the oldest massive
quiescent galaxies within the redshift interval .Comment: Accepted for publication in MNRAS, 11 pages, 6 figure
The ultraviolet continuum slopes (β) of galaxies at z ≃ 8 − 16 from JWST and ground-based near-infrared imaging
The galaxy UV luminosity function at z≃11 from a suite of public JWST ERS, ERO and Cycle-1 programs
A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass, and age from z = 0.6 to z = 1.3
We study the relationships between stellar mass, size and age within the
quiescent population, using two mass-complete spectroscopic samples with
, taken from VANDELS at
, and LEGA-C at . Using robust D4000 values, we
demonstrate that the well-known 'downsizing' signature is already in place by
, with D4000 increasing by across a 1
dex mass interval for both VANDELS and LEGA-C. We then proceed to investigate
the evolution of the quiescent galaxy stellar mass-size relation from
to . We find the median size increases by a factor of
at , and
see tentative evidence for flattening of the relation, finding slopes of
and for VANDELS and LEGA-C
respectively. We finally split our sample into galaxies above and below our
fitted mass-size relations, to investigate how size and D4000 correlate.
For LEGA-C, we see a clear difference, with larger galaxies found to have
smaller D4000 at fixed stellar mass. Due to the faintness and smaller
numbers of the VANDELS sample, we cannot confirm whether a similar relation
exists at . We consider whether differences in stellar age or
metallicity are most likely to drive this size-D4000 relation, finding
that any metallicity differences are unlikely to fully explain the observed
offset, meaning smaller galaxies must be older than their larger counterparts.
We find the observed evolution in size, mass and D4000 across the
Gyr from to can be explained by a simple toy
model in which VANDELS galaxies evolve passively, whilst experiencing a series
of minor mergers.Comment: 14 pages, 9 figures, submitted to MNRA
A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass, and age from z = 0.6 to z = 1.3
We study the relationships between stellar mass, size, and age within the quiescent population, using two mass-complete spectroscopic samples with log10(M⊙/M⊙) > 10.3, taken from VANDELS at 1.0 < z < 1.3, and LEGA-C at 0.6 < z < 0.8. Using robust Dn4000 values, we demonstrate that the well-known 'downsizing' signature is already in place by z 1.1, with Dn4000 increasing by 0.1 across a 1 dex mass interval for both VANDELS and LEGA-C. We then proceed to investigate the evolution of the quiescent galaxy stellar mass-size relation from z -1.1 to z -0.7. We find the median size increases by a factor of 1.9 ± 0.1 at log10(M⊙/M⊙) = 10.5, and see tentative evidence for flattening of the relation, finding slopes of α = 0.72 ± 0.06 and α =\0.56\pm 0.04 for VANDELS and LEGA-C, respectively. We finally split our sample into galaxies above and below our fitted mass-size relations, to investigate how size and Dn4000 correlate. For LEGA-C, we see a clear difference, with larger galaxies found to have smaller Dn4000 at fixed stellar mass. Due to the faintness and smaller numbers of the VANDELS sample, we cannot confirm whether a similar relation exists at z -1.1. We consider whether differences in stellar age or metallicity are most likely to drive this size-Dn4000 relation, finding that any metallicity differences are unlikely to fully explain the observed offset, meaning smaller galaxies must be older than their larger counterparts. We find the observed evolution in size, mass, and Dn4000 across the -2 Gyr from z ∼1.1 to z ∼0.7 can be explained by a simple toy model in which VANDELS galaxies evolve passively whilst experiencing a series of minor mergers
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