2,144 research outputs found
Differential Equation of Appell Polynomials Via the Factorization Method
Let {Pn(x)}∞n=0 be a sequence of polynomials of degree n. We define two sequences of differential operators Φn and Ψn satisfying the following properties:
By constructing these two operators for Appell polynomials, we determine their differential equations via the factorization method introduced by Infeld and Hull (Rev. Mod. Phys. 23 (1951) 21). The differential equations for both Bernoulli and Euler polynomials are given as special cases of the Appell polynomials
Boundaries of Universal Theories
Universal theories are a broad class of well-motivated microscopic dynamics
of the electroweak sector that go beyond the Standard Model description. The
long distance physics is described by electroweak parameters which correspond
to local operators in the Effective Field Theory. We show how unitarity and
analyticity constrain the space of parameters. In particular, the and
parameters are constrained to be positive and are necessarily the leading terms
in the low energy expansion. We assess the impact of unitarity on the
interpretation of Drell-Yan data. In passing, we uncover an unexpected Wilson
coefficient transcendental cancellation at the level.Comment: 15 pages, 3 figure
Asymptotics of Zeros of Relativistic Hermite Polynomials
The relativistic Hermite polynomial (RHP) is a class of orthogonal polynomials associated with varying weights. We study the asymptotics of the zeros of the RHP when both degree of polynomials and relativistic parameter approach infinity
On Quadrature Rules Associated with Appell Polynomials
A quadrature rule using Appell polynomials and generalizing both the Euler-MacLaurin quadrature formula and a similar quadrature rule, obtained in Bretti et al [15], which makes use of Euler (instead of Bernoulli) numbers and even (instead of odd) derivatives of the given function at the extrema of the considered interval, is derived. An expression of the remainder term and a numerical example are also enclosed
Quantifying the challenges of detecting unseen planetary companions with transit timing variations
Both ground and space-based transit observatories are poised to significantly
increase the number of known transiting planets and the number of precisely
measured transit times. The variation in a planet's transit times may be used
to infer the presence of additional planets. Deducing the masses and orbital
parameters of such planets from transit time variations (TTVs) alone is a rich
and increasingly relevant dynamical problem. In this work, we evaluate the
extent of the degeneracies in this process, systematically explore the
dependence of TTV signals on several parameters and provide phase space plots
that could aid observers in planning future observations. Our explorations are
focused on a likely-to-be prevalent situation: a known transiting short-period
Neptune or Jupiter-sized planet and a suspected external low-mass perturber on
a nearly-coplanar orbit. Through approximately 10^7 N-body simulations, we
demonstrate how TTV signal amplitudes may vary by orders of magnitude due to
slight variations in any one orbital parameter (0.001 AU in semimajor axis,
0.005 in eccentricity, or a few degrees in orbital angles), and quantify the
number of consecutive transit observations necessary in order to obtain a
reasonable opportunity to characterize the unseen planet (approximately greater
or equal to 50 observations). Planets in or near period commensurabilities of
the form p:q, where p < 21 and q < 4, produce distinct TTV signatures,
regardless of whether the planets are actually locked in a mean motion
resonance. We distinguish these systems from the secular systems in our
explorations. Additionally, we find that computing the autocorrelation function
of a TTV signal can provide a useful diagnostic for identifying possible orbits
for additional planets and suggest that this method could aid integration of
TTV signals in future studies of particular exosystems.Comment: 53 pages total, including 18 figures, 1 table, and 1 appendix.
Accepted for publication in ApJ. Better resolution plots will appear in
online journa
Exploring Stakeholder Value Models via Interactive Visualization
AbstractIn the design of complex systems, models can be used to predict a future system's performance as well as approximate stakeholder preferences on performance. This paper examines the problem of model truthfulness and the challenge of trusting models, with a focus on value models and how they are used to predict stakeholder preferences. A framework is proposed for the analysis of these issues (truthfulness and trust), which is used to discuss the relationship between models and decision outcomes. Interactive visualization is proposed as an efficient and effective method for increasing model truthfulness and model trust, and hence making better decisions. An interactive visualization tool is also presented, and an application of the tool to a complex decision case is discussed
Co-evolution and Nuclear Structure in the Dwarf Galaxy POX 52 Studied by Multi-wavelength Data From Radio to X-ray
The nearby dwarf galaxy POX 52 at hosts an active galactic
nucleus (AGN) with a black-hole (BH) mass of
and an Eddington ratio of 0.1-1. This object provides the rare
opportunity to study both AGN and host-galaxy properties in a low-mass highly
accreting system. To do so, we collected its multi-wavelength data from X-ray
to radio. First, we construct a spectral energy distribution, and by fitting it
with AGN and host-galaxy components, we constrain AGN-disk and dust-torus
components. Then, while considering the AGN-disk emission, we decompose optical
HST images. As a result, it is found that a classical bulge component is
probably present, and its mass () is consistent with an expected
value from a local relation. Lastly, we analyze new quasi-simultaneous X-ray
(0.2-30 keV) data obtained by NuSTAR and XMM-Newton. The X-ray spectrum can be
reproduced by multi-color blackbody, warm and hot coronae, and disk and torus
reflection components. Based on this, the spin is estimated to be , which could suggest that most of the current BH mass was
achieved by prolonged mass accretion. Given the presence of the bulge, POX 52
would have undergone a galaxy merger, while the -
relation and the inferred prolonged accretion could suggest that AGN feedback
occurred. Regarding the AGN structure, the spectral slope of the hot corona,
its relative strength to the bolometric emission, and the torus structure are
found to be consistent with Eddington-ratio dependencies found for nearby AGNs.Comment: 26 pages, 10 figures, 4 tables, accepted for publication in ApJ. The
data in Table 4 are available from
http://www.kusastro.kyoto-u.ac.jp/~kawamuro/arxiv/SEDplusComponents_u.tx
The Brave study: promoting active breaks in secondary school from students’ point of view
Background: According to the WHO recommendations, children and adolescents should perform at least 60 minutes per day of moderate to vigorous physical activity (PA). Active Breaks (ABs) interventions, short physical activity breaks of 5-
15 minutes during school hours, have been examined in primary school children as a potential strategy to counteract a sedentary lifestyle, with minimal disruption to school learning activities. The aim of the BRAVE STUDY is to investigate the
feasibility of ABs in a secondary school setting from the students’ point of view.
Methods: In December 2020, 10 students (age 12-13, 6 females and 4
males) attending the second and third grade of secondary schools located in Bologna province (Italy) were involved in a focus group (FG). The FG was conducted online because of COVID-19 and the answers transcribed for a later analysis. Students’ opinions were probed on the role of PA in school
and possible facilitators/barriers to implementation of ABs in the school.
Results: Students reported they wanted to be more active as a consequence of time spent in class sitting at a desk. Students also reported that an organized activity like ABs conducted in the classroom setting provides an excellent opportunity to
improve social relations with classmates. Students also highlighted the possible psycho-physical well-being benefits arising from PA. Among the potentially negative aspects reported, students underlined the possible confusion that would be created in classroom and the time subtracted from academic
learning activities. Conclusions: The FG represents an ideal mean to obtain in-depth
information on how people feel about a pending program or a change in their routine. The current FG reinforces positive outcomes from exposure to a PA program that can be intertwined with their daily classroom activities. ABs programs
can help to reconcile the needs of students that arise during the day with the PA objectives recommended by the WHO.
Key messages:
ABs can be a zero-cost intervention strategy to achieve
WHO recommendations and would create conditions for a
greater psycho-physical benefits in classrooms.
A qualitative approach, such as FGs, provides a mean to
collect information not obtainable with quantitative methods,
that could be useful to co-design interventions for children and adolescents
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