cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Contribution of Long Wavelength Gravitational Waves to the CMB Anisotropy
Creators: name: White, Martin
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an in depth discussion of the production of gravitational waves from an inflationary phase that could have occurred in the early universe, giving derivations for the resulting spectrum and energy density. We also consider the large-scale anisotropy in the cosmic microwave background radiation coming from these waves. Assuming that the observed quadrupole anisotropy comes mostly from gravitational waves (consistent with the predictions of a flat spectrum of scalar density perturbations and the measured dipole anisotropy) we describe in detail how to derive a value for the scale of inflation of $(1.5-5)\times 10^{16}$GeV, which is at a particularly interesting scale for particle physics. This upper limit corresponds to a 95\% confidence level upper limit on the scale of inflation assuming only that the quadrupole anisotropy from gravitational waves is not cancelled by another source. Direct detection of gravitational waves produced by inflation near this scale will have to wait for the next generation of detectors.
description: (LaTeX 16 pages), 2 figures not included, YCTP-P16-92
Photovoltages and hot electrons in plasmonic nanogaps
Creators: name: Natelson, Douglas
name: Evans, Charlotte I.
name: Zolotavin, Pavlo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In metal nanostructures under illumination, multiple different processes can drive current flow, and in an open- circuit configuration some of these processes lead to the production of open-circuit photovoltages. Structures that have plasmonic resonances at the illumination wavelength can have enhanced photovoltage response, due to both increased interactions with the incident radiation field, and processes made possible through the dynamics of the plasmon excitations themselves. Here we review photovoltage response driven by thermoelectric effects in continuous metal nanowires and photovoltage response driven by hot electron production and tunneling. We discuss the prospects for enhancing and quantifying hot electron generation and response via the combination of local plasmonic resonances and propagating surface plasmon polaritons.
description: 9 pages, 6 figures, Proceedings for SPIE OPTO, 2018 (Photonics West)
Average Effective Potential for the Conformal Factor
Creators: name: Floreanini, R.
name: Percacci, R.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In a four dimensional theory of gravity with lagrangian quadratic in curvature and torsion, we compute the effective action for metrics of the form $g_{μν}=ρ^2δ_{μν}$, with $ρ$ constant. Using standard field-theoretic methods we find that one loop quantum effects produce a nontrivial effective potential for $ρ$. We explain this unexpected result by showing how our regularization procedure differs from the one that is usually adopted in Quantum Gravity. Using the method of the average effective potential, we compute the scale dependence of the v.e.v. of the conformal factor.
description: 8 pages, plain TEX, SISSA 71/93-EP
Slow proton production in semi-inclusive deep inelastic scattering and the pion cloud in the nucleon
Creators: name: Szczurek, A.
name: Bosveld, G. D.
name: Dieperink, A. E. L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The semi-inclusive cross section for producing slow protons in charged current deep inelastic (anti-) neutrino scattering on protons and neutrons is calculated as a function of the Bjorken $x$ and the proton momentum. The standard hadronization models based upon the colour neutralization mechanism appear to underestimate the rate of slow proton production on hydrogen. The presence of the virtual mesons (pions) in the nucleon leads to an additional mechanism for proton production, referred to as spectator process. It is found that at low proton momenta both mechanisms compete, whereas the spectator mechanism dominates at very small momenta, while the color neutralization mechanism dominates at momenta larger than 1-2 \, GeV$/c$. The results of the calculations are compared with the CERN bubble chamber (BEBC) data. The spectator model predicts a sharp increase of the semi-inclusive cross section at small $x$ due to the sea quarks in virtual mesons.
description: LaTeX, 19 pages, 10 figures
“O brave new world” CRISPR Mediated Gene Editing in Somatic and Germ Line Contexts for Therapeutics and Enhancement of the Human Species – an Ethical and Legal Discussion.
Creators: name: Farrell, Cathal B.
Publisher: name: Royal College of Surgeons in Ireland
Year: 2019
Subjects: Uncategorized

description: Gene editing has been a topic of controversy since the late 1970’s, however as of 2015 the topic of gene editing and its potential applications has shot to the forefront of biomedical, ethical and legal debate. CRISPR is a new molecular technology, which is essentially a molecular scissors capable of cutting a single gene, or multiple genes out of the genome of any species. Scientists have further manipulated CRISPR so that after it has excised a gene, or genes, it can then insert a gene of choice, into the excised area. The ramifications of CRISPR mediated gene editing technology are huge in the cellular therapeutics arena (somatic), and in the preventative medicine landscape (germ line). CRISPR mediated gene editing requires us to reflect on how as a society we view genetically driven diseases, and disabilities. Furthermore, there are calls from scientists for clarification on the legal and regulatory landscape of gene editing, in all its platforms, within their jurisdiction. In this piece, I examine the ethical and legal implications of CRISPR mediated gene editing in somatic and germ line contexts, using the British Medical Associations Eclectic Method.
Squarks Below the Z
Creators: name: Clavelli, L.
name: Coulter, P. W.
name: Fenyi, B.
name: Hester, C.
name: Povinec, Peter
name: Yuan, Kajia
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the possibility that the difference between the measurements of $α_3(M_Z)$ from the hadronic branching ratio of the $Z^0$ and the world average of other measurements is due to the decay of the $Z^0$ into quark, anti-squark, and gluino. Consequences for supersymmetry breaking models are discussed.
description: 9 pages, 4 figures not included
Accurate nucleon electromagnetic form factors from dispersively improved chiral effective field theory
Creators: name: Alarcón, J. M.
name: Weiss, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We present a theoretical parametrization of the nucleon electromagnetic form factors (FFs) based on a combination of chiral effective field theory and dispersion analysis. The isovector spectral functions on the two-pion cut are computed using elastic unitarity, chiral pion-nucleon amplitudes, and timelike pion FF data. Higher-mass isovector and isoscalar t-channel states are described by effective poles, whose strength is fixed by sum rules (charges, radii). Excellent agreement with the spacelike proton and neutron FF data is achieved up to Q^2 \sim 1 GeV^2. Our parametrization provides proper analyticity and theoretical uncertainty estimates and can be used for low-Q^2 FF studies and proton radius extraction.
description: 5 pages, 3 figures, 2 tables
Chicago Face Database
Creators: name: Stolier, Ryan
Publisher: name: figshare
Year: 2018
Subjects: subject: 170113 Social and Community Psychology
subject: FOS: Psychology

description: This is a public stimulus database reference:
The Chicago Face Database: "The Chicago Face Database was developed at the University of Chicago by Debbie S. Ma, Joshua Correll, and Bernd Wittenbrink. The CFD is intended for use in scientific research. It provides high-resolution, standardized photographs of male and female faces of varying ethnicity between the ages of 17-65. Extensive norming data are available for each individual model. These data include both physical attributes (e.g., face size) as well as subjective ratings by independent judges (e.g., attractiveness). Detailed information about the construction of the database and the available norming data can be found in Ma, Correll, & Wittenbrink (2015)."
http://faculty.chicagobooth.edu/bernd.wittenbrink/cfd/index.html
Entropy balancing for causal effects in discrete choice analysis: The Blue Planet II effect
Creators: name: Hynes, Stephen
name: Ankamah-Yeboah, Isaac
name: O'Neill, Stephen
name: Simpson, Katherine
name: Xuan, Bui Bich
name: Armstrong, Claire
Publisher: name: Zenodo
Year: 2021
Subjects: entropy balancing; willingness to pay; discrete choice model; marine ecosystem services; nature documentaries

description: In this study the discrete choice experiment approach was employed in a survey of the Scottish general public to analyse how respondents make trade-offs between blue growth potential and marine ecosystem service delivery associated with the Mingulay cold water reef complex. Results indicate a higher willingness to pay for management options associated with the highest possible levels of marine litter control followed by the highest possible levels of fish health. Using entropy balancing, a multivariate reweighting method to produce balanced samples in observational studies, we also test the impact that having watched the BBC Blue Planet II documentary series may have had on individuals’ willingness to support marine conservation activity. Whether or not respondents had seen the BBC Blue Planet II series was found to have a significant impact on people’s preferences. Despite this, the willingness to pay (WTP) does not differ between the two groups suggesting that such documentaries may impact preferences but not the final action of WTP. It is argued that the entropy weighting approach can be a useful tool in discrete choice modelling when the researcher is concerned with estimating differences in preferences between a group of interest and a comparison group.
Electromagnetic transition form factors of baryons in a relativistic Faddeev approach
Creators: name: Alkofer, Reinhard
name: Fischer, Christian S.
name: Sanchis-Alepuz, Helios
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The covariant Faddeev approach which describes baryons as relativistic three-quark bound states and is based on the Dyson-Schwinger and Bethe-Salpeter equations of QCD is briefly reviewed. All elements, including especially the baryons' three-body-wave-functions, the quark propagators and the dressed quark-photon vertex, are calculated from a well-established approximation for the quark-gluon interaction. Selected previous results of this approach for the spectrum and elastic electromagnetic form factors of ground-state baryons and resonances are reported. The main focus of this talk is a presentation and discussion of results from a recent investigation of the electromagnetic transition form factors between ground-state octet and decuplet baryons as well as the octet-only $Σ^0$ to $Λ$ transition.
description: 10 pages, 6 figures; to be published in the EPJ Web of Conferences (proceedings of the conference EXA17)
Additional file 1 of Modulation of chemoimmunotherapy efficacy in non-small cell lung cancer by sex and histology: a real-world, patient-level analysis
Creators: name: Tuminello, Stephanie
name: Alpert, Naomi
name: Veluswamy, Rajwanth R.
name: Kumar, Arvind
name: Gomez, Jorge E.
name: Flores, Raja
name: Taioli, Emanuela
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Supplemental Fig. 1. Patient Selection. Supplemental Table 1. Drug agents classified as immunotherapy according to the NCDB.
Low-energy theorem for a composite particle in mean scalar and vector fields
Creators: name: Birse, Michael C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: For a relativistic particle moving in the presence of mean scalar and vector fields, the energy at second order in the scalar field is shown to contain two contributions in general. One is a momentum-dependent repulsive interaction satisfying a low-energy theorem pointed out by Wallace, Gross and Tjon. The other does not vanish at zero-momentum and involves a ``polarisability" of the particle by the scalar field. The first of these contributions is independent of the details of the structure of the particle and the couplings of its constituents to the external fields. The appearance of such a piece in the central nucleon-nucleus potential thus would support the existence of strong scalar fields in nuclei, without requiring the use of a Dirac equation for the nucleon.
description: 8 pages, REVTeX
Carrier recovery for coherent optical communication systems
Creators: name: JIGNESH DHRUVAKUMAR JOKHAKAR
Publisher: name: Monash University
Year: 2018
Subjects: subject: 100506 Optical Fibre Communications
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: 90609 Signal Processing

description: Carrier recovery and synchronization are the base foundation for data extraction in any coherent communication system. Although explored for decades now, the most appropriate carrier recovery technique changes with application and requirements. While some implementation scenarios require less complex hardware, some may require lower latency and less computation. Some scenarios intend to use low-precision components to reduce the cost, while some relax the cost-constraints to boost the throughput. Considering these different requirements, this thesis explores different approaches to carrier recovery namely: digital signal processing, optoelectronic processing and all-optical processing. The improvements in performance or implementation constraints demonstrated by the proposed techniques over the conventional methods suggest their beneficial usage in future.
Charged Boson Stars and Vacuum Instabilities
Creators: name: Jetzer, P.
name: Liljenberg, P.
name: Skagerstam, B. -S.
Publisher: name: arXiv
Year: 1993
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider charged boson stars and study their effect on the structure of the vacuum. For very compact particle like ``stars", with constituent mass $m_{*}$ close to the Planck mass $m_{Pl}$, i.e. $m_{*}^{2} = {\cal O} (αm_{Pl}^{2})$, we argue that there is a limiting total electric charge $Z_c$, which, primarily, is due to the formation of a pion condensate ($Z_{c} \simeq 0.5α^{-1}e$, where $α$ is the fine structure constant and $e$ is the electric charge of the positron). If the charge of the ``star" is larger than $Z_c$ we find numerical evidence for a complete screening indicating a limiting charge for a very compact object. There is also a less efficient competing charge screening mechanism due to spontaneous electron-positron pair creation in which case $Z_{c} \simeq α^{-1}e$. Astrophysical and cosmological abundances of charged compact boson stars are briefly discussed in terms of dark matter.
description: latex,29p,9 figs not included can be sent by fax on request,ITP 92-24,ZU-TH-38/92
"LS_cHW:cHbox.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{HW} and c_{Hbox}
description: No data abstract available.
Upper limits on the presence of central massive black holes in two ultra-compact dwarf galaxies in Centaurus A
Creators: name: Voggel, Karina T.
name: Seth, Anil C.
name: Neumayer, Nadine
name: Mieske, Steffen
name: Chilingarian, Igor
name: Ahn, Christopher
name: Baumgardt, Holger
name: Hilker, Michael
name: Nguyen, Dieu D.
name: Romanowsky, Aaron J.
name: Walsh, Jonelle L.
name: Brok, Mark den
name: Strader, Jay
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The recent discovery of massive black holes (BHs) in the centers of high-mass ultra compact dwarf galaxies (UCDs) suggests that at least some are the stripped nuclear star clusters of dwarf galaxies. We present the first study that investigates whether such massive BHs, and therefore stripped nuclei, also exist in low-mass ($M<10^{7}M_{\odot}$) UCDs. We constrain the BH masses of two UCDs located in Centaurus A (UCD320 and UCD330) using Jeans modeling of the resolved stellar kinematics from adaptive optics VLT/SINFONI data. No massive BHs are found in either UCD. We find a $3\,σ$ upper limit on the central BH mass in UCD\,330 of $M_{\bullet}<1.0\times10^{5}M_{\odot}$, which corresponds to 1.7\% of the total mass. This excludes a high mass fraction BH and would only allow a low-mass BHs similar to those claimed to be detected in Local Group GCs. For UCD320, poorer data quality results in a less constraining $3\,σ$ upper limit of $M_{\bullet}<1\times10^{6}M_{\odot}$, which is equal to 37.7\% of the total mass. The dynamical $M/L$ of UCD320 and UCD330 are not inflated compared to predictions from stellar population models. The non-detection of BHs in these low-mass UCDs is consistent with the idea that elevated dynamical $M/L$s do indicate the presence of a substantial BH. Despite not detecting massive BHs, these systems could still be stripped nuclei. The strong rotation ($v/σ$ of 0.3 to 0.4) in both UCDs and the two-component light profile in UCD330 support the idea that these UCDs may be stripped nuclei of low-mass galaxies where the BH occupation fraction is not yet known.
description: Accepted for publication in ApJ, 21 pages, 10 Figures
Additional file 2 of The incidence, risk factors and maternal and foetal outcomes of uterine rupture during different birth policy periods: an observational study in China
Creators: name: Zhou, Yangwen
name: Mu, Yi
name: Chen, Peiran
name: Xie, Yanxia
name: Zhu, Jun
name: Liang, Juan
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 2. Changes over different birth policy periods in age, parity and previous caesarean section distributions of women in 438 hospitals, China.
Autonomous Renormalization of the One-Loop Effective Potential and a 2 Tev Higgs in SU(2)xU(1)
Creators: name: Ibanez-Meier, R.
name: Stevenson, P. M.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Branchina et al and Consoli have recently shown that the one-loop effective potential (1LEP) of massless lambda-phi**4 theory can be renormalized in two distinct ways. One of these is the conventional renormalization of Coleman and Weinberg. The other requires an infinite wavefunction renormalization, and is very similar to the "autonomous" renormalization of the Gaussian effective potential. We apply the "autonomous" renormalization to the 1LEP of the SU(2)x U(1) electroweak theory with zero bare Higgs mass. The predicted physical Higgs mass is 1.9 TeV.
description: 10 pages, LaTeX, (Revision includes additional discussion) DOE-ER-05096-52
title: ADCO, Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Cart. 169 (11 H 63), f. 0004r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2011
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0004r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux dit Cartularium Vetus (milieu XIIIe siècle) et Notices du XIIe siècle, Archives départementales de la Côte-d'Or, Cart. 169 (11 H 63), f. 0004r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
The chemical composition of NGC5824, a globular cluster without iron spread but with an extreme Mg-Al anticorrelation
Creators: name: Mucciarelli, A.
name: Lapenna, E.
name: Ferraro, F. R.
name: Lanzoni, B.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: NGC5824 is a massive Galactic globular cluster suspected to have an intrinsic spread in its iron content, according to the strength of the calcium triplet lines. We present chemical abundances of 117 cluster giant stars using high-resolution spectra acquired with the multi-object spectrograph FLAMES. The metallicity distribution of 87 red giant branch stars is peaked at [Fe/H]=-2.11+-0.01 dex, while that derived from 30 asymptotic giant branch stars is peaked at [Fe/H]=-2.20+-0.01 dex. Both the distributions are compatible with a null spread, pointing out that this cluster did not retain the ejecta of supernovae. The small iron abundance offset between the two groups of stars is similar to those already observed among red and asymptotic giant branch stars in other clusters. The lack of intrinsic iron spread rules out the possibility that NGC5824 is the remnant of a disrupted dwarf galaxy, as previously suggested. We also find evidence of the chemical anomalies usually observed in globular clusters, namely the Na-O and the Mg-Al anticorrelations. In particular, NGC5824 exhibits a huge range of [Mg/Fe] abundance, observed only in a few metal-poor and/or massive clusters. We conclude that NGC5824 is a normal globular cluster, without spread in [Fe/H] but with an unusually large spread in [Mg/Fe], possibly due to an efficient self-enrichment driven by massive asymptotic giant branch stars.
description: accepted for publication in ApJ. 31 pages, 9 figures, 4 tables
Effective Group Structure in the Interacting Boson Model
Creators: name: Whelan, N. D.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Spectrum generating algebras are used in various fields of physics as models to determine quantum structure, including energy levels and transition strengths. The advantage of such models is that their group structure allows an extensive understanding of the system being studied. In addition they possess a simple classical limit, at least for bosonic systems. In this paper we discuss an algebraic model of nuclear structure, the Interacting Boson Model (IBM), and show that in one limit its group structure is particularly simple. For zero angular momentum there is an effective lower dimensional group structure which describes the system both classically and quantum mechanically.
description: To appear in Nuc. Phys. A. Written in RevTeX. One not-very-important figure available by snail mail
Supplemental material
Creators: name: Muhammad, Ammar
name: Coopmans, Eva
name: Gatto, Federico
name: Franck, Sanne
name: Janssen, Joseph
name: Lely, Aart Jan Van Der
name: Hofland, Leo
name: Neggers, Sebastian
Publisher: name: figshare
Year: 2018
Subjects: Medicine

description: Supplemental material article: Pasireotide responsiveness in acromegaly is mainly driven by somatostatin receptor subtype 2 expression.
"LS_cHl3:cHq3.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{Hl3} and c_{Hq3}
description: No data abstract available.
Gravitational Waves and $γ$-Ray Bursts
Creators: name: Kochanek, Christopher S.
name: Piran, Tsvi
Publisher: name: arXiv
Year: 1993
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Coalescing binaries in distant galaxies are one of the most promising sources of gravitational waves detectable by the LIGO project.$^{[1-5]}$ They are also a copious source of neutrinos,$^{[1]}$ however these neutrino pulses are far too weak to be detected on earth. Several years ago Eichler \etal$\,$$^{[6]}$ suggested that they are also sources of $γ$-ray bursts (GRBs). Recently it was found$^{[7]}$ that GRBs are likely to be cosmological in origin, and coalescing binary systems$^{[6,8-11]}$ are probably the most promising cosmological sources. The current estimates of the burst and LIGO rates from a cosmologically distributed population are based on the systems observed in our galaxy.$^{[12-14]}$ These estimates are based on only three binarys so there are large statistical uncertainties in the coalescence rate. If we accept the cosmological/coalescing binary hypothesis for GRBs, then we get a more accurate estimate of the rate at which binaries coalesce and hence of the predicted LIGO signal. The association between GRBs and binaries can significantly improve the performance of LIGO. The detection of gravitational radiation from a GRB source not only confirms the coalescing binary model, but it will also provide information on the geometry and energy generation mechanism of the burst.
description: 6 pages, tex, 1 figure not included, can be obtained by request from tsvi@cfata4.harvard.Edu CFA-3637
"LS_cHW:FT0.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{HW} and f_{T0}
description: No data abstract available.
"LS_cHW:FS0.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{HW} and f_{S0}
description: No data abstract available.
Supplemental material Muhammad et al.pdf
Creators: name: Muhammad, Ammar
name: Coopmans, Eva
name: Gatto, Federico
name: Franck, Sanne
name: Janssen, Joseph
name: Lely, Aart Jan Van Der
name: Hofland, Leo
name: Neggers, Sebastian
Publisher: name: figshare
Year: 2018
Subjects: Medicine

description: Supplemental material article: Pasireotide responsiveness in acromegaly is mainly driven by somatostatin receptor subtype 2 expression.
The Sensitivity of Ligo to a Stochastic Background, and its Dependance on the Detector Orientations
Creators: name: Flanagan, Eanna
Publisher: name: arXiv
Year: 1993
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We analyze the sensitivity of a network of interferometer gravitational-wave detectors to the gravitational-wave stochastic background, and derive the dependence of this sensitivity on the orientations of the detector arms. We build on and extend the recent work of Christensen, but our conclusion for the optimal choice of orientations of a pair of detectors differs from his. For a pair of detectors (such as LIGO) that subtends an angle at the center of the earth of $\,\alt 70^\circ$, we find that the optimal configuration is for each detector to have its arms make an angle of $45^\circ$ (modulo $90^\circ$) with the arc of the great circle that joins them. For detectors that are farther separated, each detector should instead have one arm aligned with this arc. We also describe in detail the optimal data-analysis algorithm for searching for the stochastic background with a detector network, which is implicit in earlier work of Michelson. The LIGO pair of detectors will be separated by $\sim 3000 \, {\rm km}$. The minimum detectable stochastic energy-density for these detectors with their currently planned orientations is $\sim 3\%$ greater than what it would be if the orientations were optimal.
description: 56 pages, 10 figures, Caltech preprint GRP-347, submitted to Phys Rev D, uses revtex macros
"LS_cHW:cHWB.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{HW} and c_{HWB}
description: No data abstract available.
Broadband loop gap resonator for nitrogen vacancy centers in diamond
Creators: name: Eisenach, Erik
name: Barry, John
name: Rojas, Roberto
name: Pham, Linh M.
name: Englund, Dirk R.
name: Braje, Danielle
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: We present an S-band tunable loop gap resonator (LGR) providing strong, homogeneous, and directionally uniform broadband microwave (MW) drive for nitrogen-vacancy (NV) ensembles. With 42 dBm of input power, the composite device provides drive field amplitudes approaching 5 G over a circular area $\gtrsim\!50$ mm$^2$ or cylindrical volume $\gtrsim\!250$ mm$^3$. The wide 80 MHz device bandwidth allows driving all eight NV Zeeman resonances for bias magnetic fields below 20 G. For pulsed applications the device realizes percent-scale microwave drive inhomogeneity; we measure a fractional root-mean-square inhomogeneity $σ_\text{rms}\!=\! 1.6\%$ and a peak-to-peak variation $σ_\text{pp}\!=\! 3\%$ over a circular area of 11 mm$^2$, and $σ_\text{rms} \!=\! 3.2\%$ and $σ_\text{pp}\! =\! 10.5\%$ over a larger 32 mm$^2$ circular area. We demonstrate incident MW power coupling to the LGR using multiple methodologies: a PCB-fabricated exciter antenna for deployed compact bulk sensors and an inductive coupling coil suitable for microscope-style imaging. The inductive coupling coil allows for approximately $2π$ steradian combined optical access above and below the device, ideal for envisioned and existing NV imaging and bulk sensing applications.
description: 8 pages, 8 figures
Are There Oscillations in the Baryon/Meson Ratio?
Creators: name: Cudell, Jean-Rene
name: Dienes, Keith R.
Publisher: name: arXiv
Year: 1992
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: All available data indicate a surplus of baryon states over meson states for energies greater than about 1.5 GeV. Since hadron-scale string theory suggests that their numbers should become equal with increasing energy, it has recently been proposed that there must exist exotic mesons with masses just above 1.7 GeV in order to fill the deficit. We demonstrate that a string-like picture is actually consistent with the present numbers of baryon and meson states, and in fact predicts regular oscillations in their ratio. This suggests a different role for new hadronic states.
description: 14 pages (RevTeX), McGill/92-07
Additional file 2: of microRNA-690 regulates induced pluripotent stem cells (iPSCs) differentiation into insulin-producing cells by targeting Sox9
Creators: name: Xu, Yang
name: Huang, Yan
name: Guo, Yibing
name: Xiong, Yicheng
name: Zhu, Shajun
name: Xu, Liancheng
name: Lu, Jingjing
name: Li, Xiaohong
name: Wan, Jian
name: Lu, Yuhua
name: Wang, Zhiwei
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Figure S2. Quantitative RT-PCR for the expression levels of 13 candidate miRNAs. U6 was used as the internal control for mRNA. Error bars show the SD (nâ =â 3). (PDF 565 kb)
Saisonnalité et contre-saisonnalité pour une alimentation durable
Creators: name: Régnier, Faustine
name: Caillavet, France
name: Badji, Ikpidi
name: Régnier, Faustine
name: Caillavet, France
name: Badji, Ikpidi
Publisher: name: Unknown
Year: 2019
Subjects: Food Consumption/Nutrition/Food Safety

description: Dans un contexte d’inégalités croissantes et de souci marqué des décideurs publics, des acteurs économiques et des consommateurs pour l’environnement, l’adoption de pratiques alimentaires plus respectueuses de l’environnement constitue un défi écologique, économique et social. Un levier en particulier, encore peu exploré, s’offre aux consommateurs pour limiter l’empreinte environnementale des choix alimentaires : le recours aux aliments de saison, qui limitent les importations lointaines et la production locale hors-saison, toutes deux coûteuses en énergie. Mais on connait mal les variations saisonnières de nos consommations. Observe-t-on un réel affranchissement des saisons, ou suivons-nous encore les rythmes alimentaires saisonniers ? De même, s’abstraire des contraintes saisonnières était autrefois le privilège des riches : alors, qu’en est-il aujourd’hui ? Qui veut « manger de saison » ? Dans quelle mesure, enfin, le recours aux aliments de saison peut-il constituer le levier d’une alimentation plus durable ?
"LS_cHbox:FS0.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{Hbox} and f_{S0}
description: No data abstract available.
Conservation of the Ca2+-permeability through the voltage sensor domain of mammalian CatSper subunit
Creators: name: Arima, Hiroki
name: Tsutsui, Hidekazu
name: Okamura, Yasushi
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Computational Biology

description: Cation channel of Spermatozoa (CatSper) is one of the voltage-gated ion channels consisting of voltage sensor domains (VSDs) and pore-gate domains. CatSper is exclusively expressed in spermatozoa and indispensable for Ca2+ influx into cytosol. Recently, we have reported that the VSD of ascidian CatSper induces Ca2+-permeable pathways in heterologous expression systems. However, it is not known whether ion permeability through the VSD of CatSper is conserved in mammals. In the present study, electrophysiology and fluorometry in Xenopus oocytes revealed that Ca2+-permeable paths are also formed by expressing the VSD of murine CatSper. We also examined the permeability to monovalent cations other than Na+ in the VSD of ascidian CatSper.
The energy dependence of the $πN$ amplitude and the three-nucleon interaction
Creators: name: Saito, T-Y
name: Afnan, I. R.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: By calculating the contribution of the $π-π$ three-body force to the three-nucleon binding energy in terms of the $πN$ amplitude using perturbation theory, we are able to determine the importance of the energy dependence and the contribution of the different partial waves of the $πN$ amplitude to the three-nucleon force. A separable representation of the non-pole $πN$ amplitude allows us to write the three-nucleon force in terms of the amplitude for $NN\rightarrow NN^*$, propagation of the $NNN^*$ system, and the amplitude for $NN^*\rightarrow NN$, with $N^*$ being the $πN$ quasi-particle amplitude in a given state. The division of the $πN$ amplitude into a pole and non-pole gives a procedure for the determination of the $πNN$ form factor within the model. The total contribution of the three-body force to the binding energy of the triton for the separable approximation to the Paris nucleon-nucleon potential (PEST) is found to be very small mainly as a result of the energy dependence of the $πN$ amplitude, the cancellation between the $S$- and $P$-wave $πN$ amplitudes, and the soft $πNN$ form factor.
description: RevTex file, 36 pages, 10 figures available from authors: phira@flinders.edu.au
Enhanced EEG/ECG Measurements with IntraCavi: Leveraging All 12 Cranial Nerves for Non-Invasive Neurostimulation and Data Acquisition
Creators: name: Dzikowski, Ryszard
Publisher: name: Zenodo
Year: 2025
Subjects: subject: intracavi
subject: EEG, ECG,
subject: Neurostimulation
subject: Cranial Nerves
subject: Brain-Computer Interfaces
subject: Brain-Computer Interfaces/standards
subject: Brain-Computer Interfaces/ethics
subject: Brain-Computer Interface
subject: Cognitive Augmentation
subject: Non-Invasive Neuromodulation
subject: AI-Enhanced Neurotechnology
subject: AI
subject: Hybrid Intelligence
subject: Human-AI Synergy
subject: Neuroplasticity
subject: Neurotechnology
subject: TENS
subject: PoNS
subject: NeuroChat
subject: Biomedical Engineering
subject: FOS: Medical engineering
subject: Biomedical Engineering/classification
subject: Biomedical Engineering/instrumentation

description: This study explores IntraCavi, a groundbreaking non-invasive neurostimulation device that utilizes all 12 cranial nerves for enhanced EEG and ECG measurements. Building on technologies like PoNS, TENS, and NeuroChat, IntraCavi introduces a bidirectional interface for real-time brain-computer communication. The device enables cognitive enhancement, stress regulation, and neuroplasticity optimization while offering applications in medical diagnostics and human-AI synergy. This research outlines its methodology, technical implementation, and transformative potential in cognitive science and neural augmentation.
Fast and accurate quantum Monte Carlo for molecular crystals
Creators: name: Zen, Andrea
name: Brandenburg, Jan Gerit
name: Klimeš, Jiří
name: Tkatchenko, Alexandre
name: Alfè, Dario
name: Michaelides, Angelos
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Computational Physics (physics.comp-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Computer simulation plays a central role in modern day materials science. The utility of a given computational approach depends largely on the balance it provides between accuracy and computational cost. Molecular crystals are a class of materials of great technological importance which are challenging for even the most sophisticated \emph{ab initio} electronic structure theories to accurately describe. This is partly because they are held together by a balance of weak intermolecular forces but also because the primitive cells of molecular crystals are often substantially larger than those of atomic solids. Here, we demonstrate that diffusion quantum Monte Carlo (DMC) delivers sub-chemical accuracy for a diverse set of molecular crystals at a surprisingly moderate computational cost. As such, we anticipate that DMC can play an important role in understanding and predicting the properties of a large number of molecular crystals, including those built from relatively large molecules which are far beyond reach of other high accuracy methods.
"LS_cW:cHW.root" of "Study of same-sign W boson scattering and anomalous couplings in events with one tau lepton from pp collisions at $\sqrt{s} $ = 13 TeV"
Creators: name: CMS Collaboration
Publisher: name: HEPData
Year: 2024

description: Original ROOT file containing the TCanvas cc2 for c_{W} and c_{HW}
description: No data abstract available.
Sector models - A toolkit for teaching general relativity: III. Spacetime geodesics
Creators: name: Kraus, Ute
name: Zahn, Corvin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics Education (physics.ed-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Sector models permit a model-based approach to the general theory of relativity. The approach has its focus on the geometric concepts and uses no more than elementary mathematics. This contribution shows how to construct the paths of light and free particles on a spacetime sector model. Radial paths close to a black hole are used by way of example. We outline two workshops on gravitational redshift and on vertical free fall, respectively, that we teach for undergraduate students. The contribution also describes a simplified calculation of the spacetime sector model that students can carry out on their own, if they are familiar with the Minkowski metric. The teaching materials presented in this paper are available online for teaching purposes at http://www.spacetimetravel.org . ----- Sektormodelle ermöglichen einen modellbasierten Zugang zur Allgemeinen Relativitätstheorie, der auf das Verständnis der geometrischen Konzepte abzielt und in seinen mathematischen Anforderungen nicht über Schulmathematik hinausgeht. Dieser Beitrag zeigt, wie die Bahnen von Licht und freien Teilchen auf einem raumzeitlichen Sektormodell konstruiert werden können. Als Beispiel dienen radiale Bahnen in der Nähe eines Schwarzen Lochs. Wir beschreiben zwei Workshops zu den Themen gravitative Rotverschiebung sowie radialer freier Fall, die wir in dieser Form mit Bachelorstudierenden durchführen. Der Beitrag beschreibt auch eine vereinfachte Berechnung des verwendeten raumzeitlichen Sektormodells, die von Teilnehmer/innen selbstständig durchgeführt werden kann, falls sie mit der Minkowskimetrik vertraut sind. Die vorgestellten Materialien stehen online unter http://www.tempolimit-lichtgeschwindigkeit.de für den Unterricht zur Verfügung.
description: bilingual: English version 15 pages, 12 figures, German version 16 pages, 12 figures
Additional file 3: of A Glycine soja group S2 bZIP transcription factor GsbZIP67 conferred bicarbonate alkaline tolerance in Medicago sativa
Creators: name: Wu, Shengyang
name: Zhu, Pinghui
name: Jia, Bowei
name: Yang, Junkai
name: Shen, Yang
name: Cai, Xiaoxi
name: Sun, Xiaoli
name: Zhu, Yanming
name: Sun, Mingzhe
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Table S1. Primers used in this study. (DOCX 16Â kb)
A New Test of Copper and Zinc Abundances in Late-Type Stars Using Ultraviolet Cu II and Zn II Lines
Creators: name: Roederer, Ian U.
name: Barklem, Paul S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present new abundances derived from Cu I, Cu II, Zn I, and Zn II lines in six warm (5766 < Teff < 6427 K), metal-poor (-2.50 < [Fe/H] < -0.95) dwarf and subgiant (3.64 < log g < 4.44) stars. These abundances are derived from archival high-resolution ultraviolet spectra from the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope and ground-based optical spectra from several observatories. Ionized Cu and Zn are the majority species, and abundances derived from Cu II and Zn II lines should be largely insensitive to departures from local thermodynamic equilibrium (LTE). We find good agreement between the [Zn/H] ratios derived separately from Zn I and Zn II lines, suggesting that departures from LTE are, at most, minimal (< 0.1 dex). We find that the [Cu/H] ratios derived from Cu II lines are 0.36 +/- 0.06 dex larger than those derived from Cu I lines in the most metal-poor stars ([Fe/H] < -1.8), suggesting that LTE underestimates the Cu abundance derived from Cu I lines. The deviations decrease in more metal-rich stars. Our results validate previous theoretical non-LTE calculations for both Cu and Zn, supporting earlier conclusions that the enhancement of [Zn/Fe] in metal-poor stars is legitimate, and the deficiency of [Cu/Fe] in metal-poor stars may not be as large as previously thought.
description: Accepted for publication in the Astrophysical Journal (15 pages, 5 figures, 8 tables)
Deformed Hartree-Fock Calculation of Proton-Rich Nuclei
Creators: name: Tajima, N.
name: Onishi, N.
name: Takahara, S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We perform Hartree-Fock+BCS calculations for even-even nuclei with 2 <= Z <= 82 and N ranging from outside the proton drip line to the experimental frontier on the neutron-rich side. The ground state solutions are obtained for 737 nuclei, together with shape-coexistence solutions for 480 nuclei. Our method features the Cartesian-mesh representation of single-particle wavefunctions, which is advantageous in treating nucleon skins and exotic shapes. The results are compared with those of the finite-range droplet model of Moller et al. as well as the experimental values.
description: 7 pages Latex, 5 postscript figures appended as uufile