984 research outputs found
The secretary problem with items arriving according to a random permutation avoiding a pattern of length three
In the classical secretary problem, ranked items arrive one by one, and
each item's rank relative to its predecessors is noted. The observer must
select or reject each item as it arrives, with the object of selecting the item
of highest rank. For , let
denote the strategy whereby the observer rejects the first items, and
then selects the first later-arriving item whose rank is higher than that of
any of the first items (if such an item exists). If the ranked items
arrive in a uniformly random order, it is well-known that the limiting optimal
probability of success is , which occurs if . It has
been shown that when the ranked items arrive according to certain non-uniform
distributions on the set of permutations, serves as a lower bound for
the optimal probability. There is a fundamental reason for this phenomenon. We
consider certain distributions for which that reason does not apply. We begin
by noting a cooked-up class of distributions for which
yields the lowest possible probability of success -- namely , for all
. We then consider the uniform distribution over all permutations avoiding a
particular pattern of length three. In the case of the pattern 231 or 132, for
any choice of , the strategy yields the very same
probability of success; namely , which gives a limiting
probability of . For the pattern 213, the optimal strategy is obtained
for , also yielding a limiting probability of . For the
pattern 123, the optimal strategy is obtained for , yielding a limiting
probability of . For the other two patterns, 312 and 321, an optimal
strategy will yield a limiting probability of at least
Modeling the Behavior of Novice Young Drivers Using Data from In- Vehicle Data Recorders
Novice young drivers suffer from increased crash risk that translates into over-representation in road injuries. A better understanding of the driving behavior of novice young drivers and of their determinants is needed to tackle this problem. To this extent, this study analyzes the behavior of novice young drivers within a Graduated Driver Licensing (GDL) program. Data on driving behavior of novice drivers and their parents is collected using in-vehicle data recorders, which calculate compound risk indices as measures of the risk taking behavior of the various drivers. Data is used to estimate a negative binomial model to identify the major factors that affect the driving behavior of the young drivers. Estimation results suggest that the risk taking behavior of young drivers is influenced by that of their parents and decreases with higher levels of supervised driving and stricter monitoring by the parents
Obtaining research biopsies during pediatric colonoscopy: Safety and adverse events
AIM: To investigate the safety profile of acquiring additional intestinal biopsies for research purposes in children undergoing a medically indicated colonoscopy. METHODS: A retrospective review of 122 pediatric patients who underwent colonoscopy over a 9 mo time period was completed. 38/122 participants consented to a research study in which 4 additional biopsies were obtained, in addition to routine biopsies. The outcomes after colonoscopy were measured in the research participants, and compared to 84 control participants who did not consent for the study. Groups were compared with regard to number of biopsies obtained, underlying diagnosis, and both serious and minor adverse outcomes. Data was collected including: age, gender, race, indication, diagnosis, number of biopsies obtained per case and post procedure adverse events. Medical records were reviewed and a questionnaire was completed by each of the ten gastroenterologists who performed procedures during the study. Physicians were asked about individual patient outcomes to ensure that all adverse events, such as perforation, excessive bleeding, infection, and minor gastrointestinal outcomes, were captured and included. RESULTS: The research group had more biopsies obtained (mean = 13.58 +/- 4.21) compared to controls (mean = 9.33 +/- 4.40),
Volatility of Linear and Nonlinear Time Series
Previous studies indicate that nonlinear properties of Gaussian time series
with long-range correlations, , can be detected and quantified by studying
the correlations in the magnitude series , i.e., the ``volatility''.
However, the origin for this empirical observation still remains unclear, and
the exact relation between the correlations in and the correlations in
is still unknown. Here we find analytical relations between the scaling
exponent of linear series and its magnitude series . Moreover, we
find that nonlinear time series exhibit stronger (or the same) correlations in
the magnitude time series compared to linear time series with the same
two-point correlations. Based on these results we propose a simple model that
generates multifractal time series by explicitly inserting long range
correlations in the magnitude series; the nonlinear multifractal time series is
generated by multiplying a long-range correlated time series (that represents
the magnitude series) with uncorrelated time series [that represents the sign
series ]. Our results of magnitude series correlations may help to
identify linear and nonlinear processes in experimental records.Comment: 7 pages, 5 figure
Mass growth and mergers: direct observations of the luminosity function of LRG satellite galaxies out to z=0.7 from SDSS and BOSS images
We present a statistical study of the luminosity functions of galaxies
surrounding luminous red galaxies (LRGs) at average redshifts =0.34 and
=0.65. The luminosity functions are derived by extracting source photometry
around more than 40,000 LRGs and subtracting foreground and background
contamination using randomly selected control fields. We show that at both
studied redshifts the average luminosity functions of the LRGs and their
satellite galaxies are poorly fitted by a Schechter function due to a
luminosity gap between the centrals and their most luminous satellites. We
utilize a two-component fit of a Schechter function plus a log-normal
distribution to demonstrate that LRGs are typically brighter than their most
luminous satellite by roughly 1.3 magnitudes. This luminosity gap implies that
interactions within LRG environments are typically restricted to minor mergers
with mass ratios of 1:4 or lower. The luminosity functions further imply that
roughly 35% of the mass in the environment is locked in the LRG itself,
supporting the idea that mass growth through major mergers within the
environment is unlikely. Lastly, we show that the luminosity gap may be at
least partially explained by the selection of LRGs as the gap can be reproduced
by sparsely sampling a Schechter function. In that case LRGs may represent only
a small fraction of central galaxies in similar mass halos.Comment: ApJ accepted versio
Searching for a Gravitational Heating Signature in Nearby Luminous Ellipticals
We present a new deep optical study of a luminosity limited sample of nearby
elliptical galaxies, attempting to observe the effects of gravitational
interactions on the ISM of these objects. This study is motivated by recent
observations of M86, a nearby elliptical galaxy that shows possible evidence
for gas heating through a recent gravitational interaction. The complete sample
includes luminous ellipticals in clusters, groups and the field. For each of
the galaxies we objectively derive a tidal parameter which measures the
deviation of the stellar body from a smooth, relaxed model and find that 73% of
them show tidal disturbance signatures in their stellar bodies. This is the
first time that such an analysis is done on a statistically complete sample and
it confirms that elliptical galaxies continue to grow and evolve through
gravitational interactions even in the local Universe. Our study of ellipticals
in a wide range of interaction stages, along with available ISM data will
attempt to shed light on this possibly alternative mechanism for maintaining
the observed ISM temperatures of elliptical galaxies.Comment: To appear in proceedings of The Monster's Fiery Breath: Feedback in
Galaxies, Groups, and Clusters (AIP conference series
Light-Heavy Symmetry: Geometric Mass Hierarchy for Three Families
The Universal Seesaw pattern coupled with a LightHeavy
symmetry principle leads to the Diophantine equation , where and distinct. Its unique non-trivial
solution gives rise to the geometric mass hierarchy ,
, for fermion families. This is realized in
a model where the hybrid (yet UpDown symmetric) quark mass
relations play a
crucial role in expressing the CKM mixings in terms of simple mass ratios,
notably .Comment: 12 pages, no figures, Revtex fil
Rhizomatic affective spaces and the therapeutic potential of music in prison: a qualitative meta-synthesis
Research literature supports that music programmes in prisons can have a therapeutic effect in prisoners’ lives that could promote personal development and assist the process towards desistance. The authors use a meta-synthetic approach to examine 12 qualitative articles published worldwide to explore the therapeutic potential of such programmes. The findings suggest that music programmes in prison are perceived by participating prisoners as a liberating process which encourages participation and allows for non-coercive personal development. The therapeutic potential of music programmes is located in the combination of the benefits emanating from the effect and practice of music and the creation of mental, spatial and temporal zones of free expression and those that derive from the egalitarian and non-authoritative approach employed by the facilitators. These findings are discussed along with aspects involved in the provision of offender treatment as well as factors that affect treatment response and engagement
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