8,359 research outputs found
Computation of the Marcum Q-function
Methods and an algorithm for computing the generalized Marcum function
() and the complementary function () are described.
These functions appear in problems of different technical and scientific areas
such as, for example, radar detection and communications, statistics and
probability theory, where they are called the non-central chi-square or the non
central gamma cumulative distribution functions.
The algorithm for computing the Marcum functions combines different methods
of evaluation in different regions: series expansions, integral
representations, asymptotic expansions, and use of three-term homogeneous
recurrence relations. A relative accuracy close to can be obtained
in the parameter region ,
, while for larger parameters the accuracy decreases (close to
for and close to for ).Comment: Accepted for publication in ACM Trans. Math. Soft
Asymptotic approximations to the nodes and weights of Gauss-Hermite and Gauss-Laguerre quadratures
Asymptotic approximations to the zeros of Hermite and Laguerre polynomials
are given, together with methods for obtaining the coefficients in the
expansions. These approximations can be used as a standalone method of
computation of Gaussian quadratures for high enough degrees, with Gaussian
weights computed from asymptotic approximations for the orthogonal polynomials.
We provide numerical evidence showing that for degrees greater than the
asymptotic methods are enough for a double precision accuracy computation
(- digits) of the nodes and weights of the Gauss--Hermite and
Gauss--Laguerre quadratures.Comment: Submitted to Studies in Applied Mathematic
Conical: an extended module for computing a numerically satisfactory pair of solutions of the differential equation for conical functions
Conical functions appear in a large number of applications in physics and
engineering. In this paper we describe an extension of our module CONICAL for
the computation of conical functions. Specifically, the module includes now a
routine for computing the function , a
real-valued numerically satisfactory companion of the function for . In this way, a natural basis for solving
Dirichlet problems bounded by conical domains is provided.Comment: To appear in Computer Physics Communication
Ranking efficient DMUs using cooperative game theory
The problem of ranking Decision Making Units (DMUs) in Data Envelopment Analysis (DEA) has been widely studied in the literature. Some of the proposed approaches use cooperative game theory as a tool to perform the ranking. In this paper, we use the Shapley value of two different cooperative games in which the players are the efficient DMUs and the characteristic function represents the increase in the discriminant power of DEA contributed by each efficient DMU. The idea is that if the efficient DMUs are not included in the modified reference sample then the efficiency score of some inefficient DMUs would be higher. The characteristic function represents, therefore, the change in the efficiency scores of the inefficient DMUs that occurs when a given coalition of efficient units is dropped from the sample. Alternatively, the characteristic function of the cooperative game can be defined as the change in the efficiency scores of the inefficient DMUs that occurs when a given coalition of efficient DMUs are the only efficient DMUs that are included in the sample. Since the two cooperative games proposed are dual games, their corresponding Shapley value coincide and thus lead to the same ranking. The more an ef- ficient DMU impacts the shape of the efficient frontier, the higher the increase in the efficiency scores of the inefficient DMUs its removal brings about and, hence, the higher its contribution to the overall discriminant power of the method. The proposed approach is illustrated on a number of datasets from the literature and compared with existing methods
Jets as diagnostics of the circumstellar medium and the explosion energetics of supernovae: the case of Cas A
We present hydrodynamical models for the Cassiopeia A (Cas A) supernova
remnant and its observed jet / counter-jet system. We include the evolution of
the progenitor's circumstellar medium, which is shaped by a slow red supergiant
wind that is followed by a fast Wolf-Rayet (WR) wind.
The main parameters of the simulations are the duration of the WR phase and
the jet energy. We find that the jet is destroyed if the WR phase is
sufficiently long and a massive circumstellar shell has formed. We therefore
conclude that the WR phase must have been short (a few thousand yr), if present
at all. Since the actual jet length of Cas A is not known we derive a lower
limit for the jet energy, which is ~10^{48} erg. We discuss the implications
for the progenitor of Cas A and the nature of its explosion.Comment: 9 pages, 5 figures, ApJ accepted. Version with high resolution
figures available at http://www.phys.uu.nl/~schure/CasA_jet.pd
La transgresión cenomanense en el sector septentrional de la "Serranía de Cuenca" (provincias de Cuenca y Guadalajara, Cordillera Ibérica)
[ES] Los materiales del Albense-Cenomanense que afloran al N. de la Serrania
de Cuenca se encuentran delimitados entre dos discordancias,
una previa al depósito de las arenas en Facies Utrillas y otra de edad
Cenomanense superior. Estos materiales forman una sucesión con
diez tramos litológicos diferentes, entre 10s que se indentifican, bastante
reducidos de potencia, alguna de las unidades litoestratigráficas
recientemente definidas en la Cordillera Ibérica.
Estos tramos pueden agruparse en tres unidades litoestratigraficas
con rango de Formación: Arenas de Utrillas, Dolomias y margas (sin
denominación formal) y Calizas dolomiticas de Nuévalos-Dolomias
Tableadas de Villa de ves. Desde el punto de vista evolutivo, estos
materiales forman una transgresión compleja, con cinco secuencias
deposicionales separadas por discontinuidades. Por ultimo, se define
la existencia de un elemento paleogeografico en la región de
Peñalen-Taravilla, un escalón que delimita la extensión hacia el N.
de la unidad secuencia deposicional basal.[EN] The Albian-Cenomanian material outcropping in the Northern part
of the Serrania de Cuenca are bounded by angular unconformities.
The one at the base was prior to the ({Facies Utrillas)) (sandstones)
deposition, and the unconformity which constitutes the upper boundary
is considered to be Upper Cenomanian.
Ten lithological units form the entire succession, being identified
from among them some of the recently defined stratigraphical Units
of the Iberian Ranges, although thicknesses are always very reduced.
Th beds can be brouped into three lithoestratigraphical Formations,
named: Utrillas Sandstones, Dolomites and marls (unformal
denomination) and Dolomitic limestones of ~uévalos-Laminated dolomites
of Villa de Ves. From the evolutionary point of view, the succession represents a complex transgression with several impulses,
specifically, five stratigraphical cycles, separates by unconformities
(non-depositional unconformities) are distinguished. Finally, it is defined
the existence of a paleogeographical feature in the Peíialen-
Taravilla region, a step that conditioned the extension towards the
North of the basal cycle.Peer reviewe
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