1,109 research outputs found
A Comparative Study of Coq and HOL
This paper illustrates the differences between the style of theory mechanisation of Coq and of HOL. This comparative study is based on the mechanisation of fragments of the theory of computation in these systems. Examples from these implementations are given to support some of the arguments discussed in this paper. The mechanisms for specifying definitions and for theorem proving are discussed separately, building in parallel two pictures of the different approaches of mechanisation given by these systems
Volume and surface propellant heating in an electrothermal radio-frequency plasma micro-thruster
The temporal evolution of neutral gas temperature over the first 5 min of operation for an electrothermal radio-frequency micro-thruster with nitrogen (N2) propellant was measured using rovibrational band matching of the second positive N2 system. Three distinct periods of gas heating were identified with time constants of Ï 1â=â8âĂâ10â»â” s, Ï 2â=â8âs, and Ï 3â=â100âs. The fast heating (Ï 1) is attributed to volumetric heating processes within the discharge driven by ion-neutral collisions. The slow heating (Ï 3) is from ion neutralization and vibrational de-excitation on the walls creating wall heating. The intermediate heating mechanism (Ï 2) is yet to be fully identified although some theories are suggested.This research was partially funded by the Australian
Space Research Program (APT project) and the Australian
Research Council Discovery Project (No. DP140100571)
Innovative small capacity gas driven ammonia-water absorption heat pump prototype for space heating and domestic hot water production
L'apport de lâinventaire des aires classĂ©es et protĂ©gĂ©es dans la connaissance de la diversitĂ© vĂ©gĂ©tale du Burkina Faso
Lâinventaire floristique du Burkina Faso est loin dâĂȘtre clos. Les rĂ©centes investigations floristiques ont permis de recenser un grand nombre dâespĂšces qui nâavaient jamais Ă©tĂ© mentionnĂ©es sur la liste floristique nationale. Une partie de ces espĂšces sont dâailleurs guinĂ©ocongolaises. Cet inventaire a concernĂ© les aires classĂ©es et protĂ©gĂ©es situĂ©es dans le secteur Sudsoudanien. Les richesses floristiques se retrouvent concentrĂ©es dans ces aires classĂ©es et protĂ©gĂ©es car ce sont des formations qui jouissent dâune relative bonne gestion par rapport aux autres aires non protĂ©gĂ©es qui ont Ă©tĂ© fortement dĂ©gradĂ©es par lâhomme. Lâobjectif de cette communication est de donner les informations issues de ces diffĂ©rentes investigations sur lâĂ©tat de connaissance de la diversitĂ© vĂ©gĂ©tale du Burkina Faso avec un accent particulier sur le mode de gestion et les utilisations de quelques espĂšces de la zone sud soudanienne
The POINT-AGAPE survey II: An Unrestricted Search for Microlensing Events towards M31
An automated search is carried out for microlensing events using a catalogue
of 44554 variable superpixel lightcurves derived from our three-year monitoring
program of M31. Each step of our candidate selection is objective and
reproducible by a computer. Our search is unrestricted, in the sense that it
has no explicit timescale cut. So, it must overcome the awkward problem of
distinguishing long-timescale microlensing events from long-period stellar
variables. The basis of the selection algorithm is the fitting of the
superpixel lightcurves to two different theoretical models, using variable star
and blended microlensing templates. Only if microlensing is preferred is an
event retained as a possible candidate. Further cuts are made with regard to
(i) sampling, (ii) goodness of fit of the peak to a Paczynski curve, (iii)
consistency of the microlensing hypothesis with the absence of a resolved
source, (iv) achromaticity, (v) position in the colour-magnitude diagram and
(vi) signal-to-noise ratio. Our results are reported in terms of first-level
candidates, which are the most trustworthy, and second-level candidates, which
are possible microlensing but have lower signal-to-noise and are more
questionable. The pipeline leaves just 3 first-level candidates, all of which
have very short full-width half-maximum timescale (<5 days) and 3 second-level
candidates, which have timescales of 31, 36 and 51 days respectively. We also
show 16 third-level lightcurves, as an illustration of the events that just
fail the threshold for designation as microlensing candidates. They are almost
certainly mainly variable stars. Two of the 3 first-level candidates correspond
to known events (PA 00-S3 and PA 00-S4) already reported by the POINT-AGAPE
project. The remaining first-level candidate is new.Comment: 22 pages, 18 figures, MNRAS, to appea
Energy Conservation Using Dynamic Voltage Frequency Scaling for Computational Cloud
Cloud computing is a new technology which supports resource sharing on a âPay as you goâ basis around the world. It provides various services such as SaaS, IaaS, and PaaS. Computation is a part of IaaS and the entire computational requests are to be served efficiently with optimal power utilization in the cloud. Recently, various algorithms are developed to reduce power consumption and even Dynamic Voltage and Frequency Scaling (DVFS) scheme is also used in this perspective. In this paper we have devised methodology which analyzes the behavior of the given cloud request and identifies the associated type of algorithm. Once the type of algorithm is identified, using their asymptotic notations, its time complexity is calculated. Using best fit strategy the appropriate host is identified and the incoming job is allocated to the victimized host. Using the measured time complexity the required clock frequency of the host is measured. According to that CPU frequency is scaled up or down using DVFS scheme, enabling energy to be saved up to 55% of total Watts consumption
First microlensing candidate towards M31 from the Nainital Microlensing Survey
We report our first microlensing candidate NMS-E1 towards M31 from the data
accumulated during the four years of Nainital Microlensing Survey. Cousin R and
I band observations of ~13'x13' field in the direction of M31 have been carried
out since 1998 and data is analysed using the pixel technique proposed by the
AGAPE collaboration. NMS-E1 lies in the disk of M31 at \alpha = 0:43:33.3 and
\delta = +41:06:44, about 15.5 arcmin to the South-East direction of the center
of M31. The degenerate Paczy\'{n}ski fit gives a half intensity duration of ~59
days. The photometric analysis of the candidate shows that it reached R~20.1
mag at the time of maximum brightness and the colour of the source star was
estimated to be (R-I)_0 ~ 1.1 mag. The microlensing candidate is blended by red
variable stars; consequently the light curves do not strictly follow the
characteristic Paczy\'{n}ski shape and achromatic nature. However its long
period monitoring and similar behaviour in R and I bands supports its
microlensing nature.Comment: no changes except typos corrected, to appear in A&
The Tactician (extended version): A Seamless, Interactive Tactic Learner and Prover for Coq
We present Tactician, a tactic learner and prover for the Coq Proof
Assistant. Tactician helps users make tactical proof decisions while they
retain control over the general proof strategy. To this end, Tactician learns
from previously written tactic scripts and gives users either suggestions about
the next tactic to be executed or altogether takes over the burden of proof
synthesis. Tactician's goal is to provide users with a seamless, interactive,
and intuitive experience together with robust and adaptive proof automation. In
this paper, we give an overview of Tactician from the user's point of view,
regarding both day-to-day usage and issues of package dependency management
while learning in the large. Finally, we give a peek into Tactician's
implementation as a Coq plugin and machine learning platform.Comment: 19 pages, 2 figures. This is an extended version of a paper published
in CICM-2020. For the project website, see https://coq-tactician.github.i
Cross-Over between universality classes in a magnetically disordered metallic wire
In this article we present numerical results of conduction in a disordered
quasi-1D wire in the possible presence of magnetic impurities. Our analysis
leads us to the study of universal properties in different conduction regimes
such as the localized and metallic ones. In particular, we analyse the
cross-over between universality classes occurring when the strength of magnetic
disorder is increased. For this purpose, we use a numerical Landauer approach,
and derive the scattering matrix of the wire from electron's Green's function.Comment: Final version, accepted for publication in New Journ. of Physics, 27
pages, 28 figures. Replaces the earlier shorter preprint arXiv:0910.427
A New Elimination Rule for the Calculus of Inductive Constructions
Published in the post-proceedings of TYPES but actually not presented orally to the conferenceInternational audienceIn Type Theory, definition by dependently-typed case analysis can be expressed by means of a set of equations â the semantic approach â or by an explicit pattern-matching construction â the syntactic approach. We aim at putting together the best of both approaches by extending the pattern-matching construction found in the Coq proof assistant in order to obtain the expressivity and flexibility of equation-based case analysis while remaining in a syntax-based setting, thus making dependently-typed programming more tractable in the Coq system. We provide a new rule that permits the omission of impossible cases, handles the propagation of inversion constraints, and allows to derive Streicher's K axiom. We show that subject reduction holds, and sketch a proof of relative consistency
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