Institution
International School for Advanced Studies
Education•Trieste, Friuli-Venezia Giulia, Italy•
About: International School for Advanced Studies is a education organization based out in Trieste, Friuli-Venezia Giulia, Italy. It is known for research contribution in the topics: Galaxy & Dark matter. The organization has 3751 authors who have published 13433 publications receiving 588454 citations. The organization is also known as: SISSA & Scuola Internazionale Superiore di Studi Avanzati.
Papers published on a yearly basis
Papers
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TL;DR: In this article, an inclusive search for a new-physics signature of lepton-jet resonances has been performed by the ATLAS experiment, where first and second generation leptoquarks were sought in events with two electrons (muons) and two or more jets.
Abstract: An inclusive search for a new-physics signature of lepton-jet resonances has been performed by the ATLAS experiment. Scalar leptoquarks, pair-produced in pp collisions at √s = 13 TeV at the large hadron collider, have been considered. An integrated luminosity of 3.2 fb−1, corresponding to the full 2015 dataset was used. First (second) generation leptoquarks were sought in events with two electrons (muons) and two or more jets. The observed event yield in each channel is consistent with Standard Model background expectations. The observed (expected) lower limits on the leptoquark mass at 95% confidence level are 1100 and 1050 GeV (1160 and 1040 GeV) for first and second generation leptoquarks, respectively, assuming a branching ratio into a charged lepton and a quark of 100%. Upper limits on the aforementioned branching ratio are also given as a function of leptoquark mass. Compared with the results of earlier ATLAS searches, the sensitivity is increased for leptoquark masses above 860 GeV, and the observed exclusion limits confirm and extend the published results.
130 citations
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TL;DR: Observations support the idea that word-meaning associations rely on systematic relations between the physical properties of speech sounds and their ref-erents.
Abstract: Historically, the link between the sounds and meanings of words has been reported as being arbitrary (de Saussure, 1959). Some observations, however, support the idea that word-meaning associations rely on systematic relations between the physical properties of speech sounds and their ref-erents (Brown, 1958; Ohala, 1994; Sapir, 1929).In pioneering studies, Edward Sapir (e.g., Sapir, 1929) invented pairs of pseudowords, such as
130 citations
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TL;DR: The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic owing to the paucity of relevant observations needed to test existing models as discussed by the authors.
Abstract: The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic owing to the paucity of relevant observations needed to test existing models. The Planck all-sky maps of linearly polarized emission from dust at 353 GHz provide the required combination of imaging and statistics to study the correlation between the structures of the Galactic magnetic field and of interstellar matter over the whole sky, both in the diffuse ISM and in molecular clouds. The data reveal that structures, or ridges, in the intensity map have counterparts in the Stokes Q and/or U maps. We focus our study on structures at intermediate and high Galactic latitudes, which cover two orders of magnitude in column density, from 1020 to 1022 cm-2. We measure the magnetic field orientation on the plane ofthe sky from the polarization data, and present an algorithm to estimate the orientation of the ridges from the dust intensity map. We use analytical models to account for projection effects. Comparing polarization angles on and off the structures, we estimate the mean ratio between the strengths of the turbulent and mean components of the magnetic field to be between 0.6 and 1.0, with a preferred value of 0.8. We find that the ridges are usually aligned with the magnetic field measured on the structures. This statistical trend becomes more striking for increasing polarization fraction and decreasing column density. There is no alignment for the highest column density ridges. We interpret the increase in alignment with polarization fraction as a consequence of projection effects. We present maps to show that the decrease in alignment for high column density is not due to a loss of correlation between the distribution of matter and the geometry of the magnetic field. In molecular complexes, we also observe structures perpendicular to the magnetic field, which, statistically, cannot be accounted for by projection effects. This first statistical study of the relative orientation between the matter structures and the magnetic field in the ISM points out that, at the angular scales probed by Planck, the field geometry projected on the plane of the sky is correlated with the distribution of matter. In the diffuse ISM, the structures of matter are usually aligned with the magnetic field, while perpendicular structures appear in molecular clouds. We discuss our results in the context of models and MHD simulations, which attempt to describe the respective roles of turbulence, magnetic field, and self-gravity in the formation of structures in the magnetized ISM.
130 citations
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TL;DR: The diverse intracellular signaling pathways used by CGRP and NGF show that the sensitization of P2X3 receptor function persists if the action of only one of these migraine mediators is blocked, implying that inhibiting a migraine attack might be most efficient by a combinatorial approach.
Abstract: Migraine headache originates from the stimulation of nerve terminals of trigeminal ganglion neurons that innervate meninges. Characteristic features of migraine pain are not only its delayed onset but also its persistent duration. Current theories propose that endogenous substances released during a migraine attack (the neuropeptide calcitonin gene-related peptide [CGRP] and the neurotrophin nerve growth factor [NGF]) sensitize trigeminal neurons to transmit nociceptive signals to the brainstem, though the mechanisms remain poorly understood. Recent studies indicate that acute, long-lasting sensitization of trigeminal nociceptive neurons occurs via distinct processes involving enhanced expression and function of adenosine triphosphate (ATP)-gated P2X3 receptors known to play a role in chronic pain. In particular, on cultured trigeminal neurons, CGRP (via protein kinase A-dependent signaling) induces a slowly developing upregulation of the ionic currents mediated by P2X3 receptors by enhancing receptor trafficking to the neuronal membrane and activating their gene transcription. Such upregulated receptors acquire the ability to respond repeatedly to extracellular ATP, thus enabling long-lasting signaling of painful stimuli. In contrast, NGF induces rapid, reversible upregulation of P2X3 receptor function via protein kinase C phosphorylation, an effect counteracted by anti-NGF antibodies. The diverse intracellular signaling pathways used by CGRP and NGF show that the sensitization of P2X3 receptor function persists if the action of only one of these migraine mediators is blocked. These findings imply that inhibiting a migraine attack might be most efficient by a combinatorial approach. The different time domains of P2X3 receptor modulation by NGF and CGRP suggest that the therapeutic efficacy of novel antimigraine drugs depends on the time of administration.
130 citations
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TL;DR: In this paper, the authors studied a class of nonlinear Schrodinger equations with dimension n = 1, 2, 3 and showed that there exists a solution with one multi-bump component having bumps located near the vertices of a regular polytope, where the other component has one negative peak.
Abstract: This paper is devoted to study a class of systems of nonlinear Schrodinger equations: $$\left\{\begin{array}{rcl} -\Delta u+u-u^{3}=\epsilon v, \\ -\Delta v+v-v^{3}=\epsilon u, \end{array}\right.$$
in $$\mathbb{R}^{n}$$
with dimension n = 1,2,3. Our main result states that if $$\mathcal{P}$$
denotes a regular polytope centered at the origin of $$\mathbb{R}^{n}$$
such that its side is greater than the radius, then there exists a solution with one multi-bump component having bumps located near the vertices of $$\xi\mathcal{P}$$
, where $${\xi\sim \log(1/\varepsilon)}$$
, while the other component has one negative peak.
130 citations
Authors
Showing all 3802 results
Name | H-index | Papers | Citations |
---|---|---|---|
Sabino Matarrese | 155 | 775 | 123278 |
G. de Zotti | 154 | 718 | 121249 |
J. González-Nuevo | 144 | 500 | 108318 |
Matt J. Jarvis | 144 | 1064 | 85559 |
Carlo Baccigalupi | 137 | 518 | 104722 |
L. Toffolatti | 136 | 376 | 95529 |
Michele Parrinello | 133 | 637 | 94674 |
Marzio Nessi | 129 | 1046 | 78641 |
Luigi Danese | 128 | 394 | 92073 |
Lidia Smirnova | 127 | 944 | 75865 |
Michele Pinamonti | 126 | 846 | 69328 |
David M. Alexander | 125 | 652 | 60686 |
Davide Maino | 124 | 410 | 88117 |
Dipak Munshi | 124 | 365 | 84322 |
Peter Onyisi | 114 | 694 | 60392 |