2,468 research outputs found
Child’s play at war memorials: insights from a social media debate
Each year, thousands of children visit memorials and other heritage sites during family or school trips, yet heritage scholars possess little understanding of their experiences. Despite its absence from the scholarly literature, children’s exploratory play at war memorials recurs frequently in the popular media. Extensive social media interest suggests that public sentiment, often emotional and vividly expressed, deserves study as a potential influence on children’s experiences at these and other dark heritage sites. This paper provides new insights of behavioral expectations for children at memorials, based on content analysis of 150 comments on a viral social media post picturing children playing on the Vietnam Women’s Memorial in Washington, DC. Conducting a stance analysis of comments, we considered commenters’ behavioral expectations, meanings they ascribed to memorials, and rationales for their intensely worded positions. Commenters shared several values: that memorials represented soldiers’ sacrifice, veterans’ service, general places for respect or to do what is right, or artistic value. Yet despite these shared rationales, many commenters expressed polarized opinions of children’s play at memorials. Commenters also referenced memorials and battlefields worldwide. This study provides greater understanding of the cultural context of children’s visits to memorials and other sites of painful heritage
Classical and Quantum Equations of Motion for a BTZ Black String in AdS Space
We investigate gravitational collapse of a -dimensional BTZ black
string in AdS space in the context of both classical and quantum mechanics.
This is done by first deriving the conserved mass per unit length of the
cylindrically symmetric domain wall, which is taken as the classical
Hamiltonian of the black string. In the quantum mechanical context, we take
primary interest in the behavior of the collapse near the horizon and near the
origin (classical singularity) from the point of view of an infalling observer.
In the absence of radiation, quantum effects near the horizon do not change the
classical conclusions for an infalling observer, meaning that the horizon is
not an obstacle for him/her. The most interesting quantum mechanical effect
comes in when investigating near the origin. First, quantum effects are able to
remove the classical singularity at the origin, since the wave function is
non-singular at the origin. Second, the Schr\"odinger equation describing the
behavior near the origin displays non-local effects, which depend on the energy
density of the domain wall. This is manifest in that derivatives of the
wavefunction at one point are related to the value of the wavefunction at some
other distant point.Comment: 9 pages, 1 figure. Minor Clarification and corrections. Accepted for
Publication in JHE
Two binary stars gravitational waves - homotopy perturbation method
Homotopy perturbation is one of the newest methods for numerical analysis of
deferential equations. We have used for solving wave equation around a black
hole. Our conclusions have this method far reaching consequences for comparison
of theoritical physics and experimental physics.Comment: The manuscript considers the important problem of solve equation wave
around a black hole. We have solved that by using Homotopy perturbation
methods. Homotopy perturbation is one of the newest methods for numerical
analysis of deferential equations. Our conclusions have far reaching
consequences for comparison of theoritical physics and experimental physic
Enhancing photoluminescence yields in lead halide perovskites by photon recycling and light out-coupling
In lead halide perovskite solar cells, there is at least one recycling event of electron-hole pair to photon to electron-hole pair at open circuit under solar illumination. This can lead to a significant reduction in the external photoluminescence yield from the internal yield. Here we show that, for an internal yield of 70%, we measure external yields as low as 15% in planar films, where light out-coupling is inefficient, but observe values as high as 57% in films on textured substrates that enhance out-coupling. We analyse in detail how externally measured rate constants and photoluminescence efficiencies relate to internal recombination processes under photon recycling. For this, we study the photo-excited carrier dynamics and use a rate equation to relate radiative and non-radiative recombination events to measured photoluminescence efficiencies. We conclude that the use of textured active layers has the ability to improve power conversion efficiencies for both LEDs and solar cells.We acknowledge financial support from the Engineering and Physical Sciences Research Council of the U.K. (EPSRC). J.M.R. and M.T. thank the Winton Programme for the Physics of Sustainability (University of Cambridge). L.M.P.-O. thanks the Cambridge Home European Scheme for financial support. L.M.P.-O. and J.P.H.R. also thank the Nano Doctoral Training Center (NanoDTC) of the EPSRC for financial support. M.A.-J. thanks Nyak Technology Limited for a PhD scholarship. F.D. acknowledges funding from a Herchel Smith Research Fellowship
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The LSST DESC data challenge 1: Generation and analysis of synthetic images for next-generation surveys
Data Challenge 1 (DC1) is the first synthetic data set produced by the Rubin Observatory Legacy Survey of Space and Time (LSST) Dark Energy Science Collaboration (DESC). DC1 is designed to develop and validate data reduction and analysis and to study the impact of systematic effects that will affect the LSST data set. DC1 is comprised of r-band observations of 40 deg2 to 10 yr LSST depth. We present each stage of the simulation and analysis process: (a) generation, by synthesizing sources from cosmological N-body simulations in individual sensor-visit images with different observing conditions; (b) reduction using a development version of the LSST Science Pipelines; and (c) matching to the input cosmological catalogue for validation and testing. We verify that testable LSST requirements pass within the fidelity of DC1. We establish a selection procedure that produces a sufficiently clean extragalactic sample for clustering analyses and we discuss residual sample contamination, including contributions from inefficiency in star-galaxy separation and imperfect deblending. We compute the galaxy power spectrum on the simulated field and conclude that: (i) survey properties have an impact of 50 per cent of the statistical uncertainty for the scales and models used in DC1; (ii) a selection to eliminate artefacts in the catalogues is necessary to avoid biases in the measured clustering; and (iii) the presence of bright objects has a significant impact (2-6) in the estimated power spectra at small scales (> 1200), highlighting the impact of blending in studies at small angular scales in LSST
Understanding the dynamics of Toll-like Receptor 5 response to flagellin and its regulation by estradiol
© 2017 The Author(s). Toll-like receptors (TLRs) are major players of the innate immune system. Once activated, they trigger a signalling cascade that leads to NF-ΰ B translocation from the cytoplasm to the nucleus. Single cell analysis shows that NF-ΰ B signalling dynamics are a critical determinant of transcriptional regulation. Moreover, the outcome of innate immune response is also affected by the cross-talk between TLRs and estrogen signalling. Here, we characterized the dynamics of TLR5 signalling, responsible for the recognition of flagellated bacteria, and those changes induced by estradiol in its signalling at the single cell level. TLR5 activation in MCF7 cells induced a single and sustained NF-k B translocation into the nucleus that resulted in high NF-k B transcription activity. The overall magnitude of NF-k B transcription activity was not influenced by the duration of the stimulus. No significant changes are observed in the dynamics of NF-k B translocation to the nucleus when MCF7 cells are incubated with estradiol. However, estradiol significantly decreased NF-k B transcriptional activity while increasing TLR5-mediated AP-1 transcription. The effect of estradiol on transcriptional activity was dependent on the estrogen receptor activated. This fine tuning seems to occur mainly in the nucleus at the transcription level rather than affecting the translocation of the NF-k B transcription factor
Quasi-Normal Modes of Stars and Black Holes
Perturbations of stars and black holes have been one of the main topics of
relativistic astrophysics for the last few decades. They are of particular
importance today, because of their relevance to gravitational wave astronomy.
In this review we present the theory of quasi-normal modes of compact objects
from both the mathematical and astrophysical points of view. The discussion
includes perturbations of black holes (Schwarzschild, Reissner-Nordstr\"om,
Kerr and Kerr-Newman) and relativistic stars (non-rotating and
slowly-rotating). The properties of the various families of quasi-normal modes
are described, and numerical techniques for calculating quasi-normal modes
reviewed. The successes, as well as the limits, of perturbation theory are
presented, and its role in the emerging era of numerical relativity and
supercomputers is discussed.Comment: 74 pages, 7 figures, Review article for "Living Reviews in
Relativity
X-ray spectropolarimetric measurements of the Kerr metric
It is thought that the spacetime geometry around black hole candidates is
described by the Kerr solution, but an observational confirmation is still
missing. Today, the continuum-fitting method and the analysis of the iron
K line cannot unambiguously test the Kerr paradigm because of the
degeneracy among the parameters of the system, in the sense that it is
impossible with current X-ray data to distinguish a Kerr black hole from a
non-Kerr object with different values of the model parameters. In this paper,
we study the possibility of testing the Kerr nature of black hole candidates
with X-ray spectropolarimetric measurements. Within our simplified model that
does not include the effect of returning radiation, we find that it is
impossible to test the Kerr metric and the problem is still the strong
correlation between the spin and possible deviations from the Kerr geometry.
Moreover, the correlation is very similar to that of other two techniques,
which makes the combination of different measurements not very helpful.
Nevertheless, our results cannot be taken as conclusive and, in order to arrive
at a final answer, the effect of returning radiation should be properly taken
into account.Comment: 12 pages, 8 figures. v2: refereed versio
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