cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Lepton flavor violation in $τ$ decays
Creators: name: Chen, Chuan-Hung
name: Geng, Chao-Qiang
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the lepton flavor violation (LFV) in tau decays in the framework of the supersymmetric seesaw mechanism with nonholomorphic terms for the lepton sector at a large $\tanβ$. In particular, we analyze two new decay modes $τ\to \ell f_0(980)$ and $τ\to \ell K^{+} K^{-}$ arising from the scalar boson exchanges contrast to $τ\to \ellη^{(\prime)}$ from the pseudoscalar ones. We find that the decay branching ratios of the two new modes could be not only as large as the current upper limits of $O(10^{-7})$, but also larger than those of $τ\to \ell η^{(\prime)}$. Experimental searches for the two modes are important for the LFV induced by the scalar-mediated mechanism. In addition, we show that the decay branching ratios of $τ\to \ell μ^{+} μ^{-}$ are related to those of $τ\to \ell η$ and $τ\to \ell f_0(980)$.
description: 11 pages, 3 figures, typos corrected, references added, version to fit journal
Rorippa indica Hiern 1825
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Rorippa
Rorippa indica

description: Sisymbrium indicum Linnaeus, Species Plantarum, ed. 2, 2: 917. 1763.
"Habitat in India orientali." RCN: 4803.
 Lectotype (Hara in J. Jap. Bot. 30: 194. 1955): Herb. Linn. No. 836.52 (LINN).
 Current name:  Rorippa indica  (L.) Hiern (Brassicaceae).
 Note: See notes by Jonsell (in Svensk Bot. Tidskr. 68: 386. 1974) who reached the same conclusion as Hara regarding the type.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 855, DOI: 10.5281/zenodo.291971
Levitating the noise performance of ultra-stable laser cavities assisted by a deep neural network: The non-intuitive role of the mirrors
Creators: name: Dickmann, J.
name: Shelling Neto, L.
name: Gaedtke, M.
name: Kroker, S.
Publisher: name: Washington, DC : Optica
Year: 2023
Subjects: subject: Laser mirrors
subject: Cutting edges
subject: Environmental influences
subject: High standards
subject: Laser frequency
subject: Measurand
subject: Noise performance
subject: Noise source
subject: Optical cavities
subject: Relative deviations
subject: Ultra-stable lasers
subject: Deep neural networks
subject: 530

description: The most precise measurand available to science is the frequency of ultra-stable lasers. With a relative deviation of 4 × 10−17 over a wide range of measuring times between one second and 100 seconds, the smallest effects in nature can thus be made measurable. To enable cutting-edge precision, the laser frequency is stabilized to an external optical cavity. This complex optical device must be manufactured to the highest standards and shielded from environmental influences. Given this assumption, the smallest internal sources of perturbation become dominant, namely the internal noise of the optical components. In this work, we present the optimization of all relevant noise sources from all components of the frequency-stabilized laser. We discuss the correlation between each individual noise source and the different parameters of the system and discover the significance of the mirrors. The optimized laser offers a design stability of 8 × 10−18 for an operation at room temperature for measuring times between one second and 100 seconds.
Childhood Memories of the Second World War
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: The contributor described her experience of the Second World War as a child. The contributor recalled going to an air raid shelter, which left her with claustrophobia, and seeing a "doodlebug" bomb flying overhead. The contributor's father joined the Air Force, and her mother joined the Air Raid Precautions nursing auxiliary. The contributor was raised by her grandparents during the war, and she did not live with her younger brother or see him during this time.The contributor's grandfather was a coal miner from Mexborough, South Yorkshire. Outside of the wartime, the contributor's father was an area manager at a commercial firm. He was stationed at a hospital in Iceland for a portion of the war, and the rest of his service was spent in Cologne, Germany. For a year after the war, the contributor's father was allocated to "cleaning up duty," at which time he worked as a dietician and cook. The contributor noted that her father was open about his stories of the Second World War, while her grandfather was not open about his experiences of the First World War. The contributor advised that she did not have a close relationship with her mother and did not hear much about her wartime experiences.This story was shared during an in-person interview at a Digital Collection Day. A transcription of the interview is attached to this record.
Dontostemon integrifolius Ledeb.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Dontostemon
Dontostemon integrifolius

description: Sisymbrium integrifolium Linnaeus, Species Plantarum 2: 660. 1753.
"Habitat in Sibiria." RCN: 4802.
 Lectotype (Ebel in Cafferty & Jarvis in Taxon 51: 536. 2002): Herb. Linn. No. 836.51 (LINN).
 Current name:  Dontostemon integrifolius  (L.) Ledeb. (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 855, DOI: 10.5281/zenodo.291971
Distributed Leadership-A 'Happily Ever After 'for the Post-Primary School?
Creators: name: Raftery, Marinella
Publisher: name: Student Teacher Educational Research (STER)
Year: 2019
Subjects: Education
Leadership
Post-Primary School

description: Marinella Raftery, graduate of the Master of Education in Mary Immacualte College, writes about her dissertation research Distributed Leadership-A ‘Happily Ever After ‘for the Post-Primary School?in volume 2 of the STER e-Journal, 2019.
Memories of the War - Kay Gostling
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: This story was shared during an in-person interview at a Digital Collection Day. A transcription of the interview is attached to this record.
Extracts from diaries of WJ Powell 1943-1945
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: This record relates to the wartime experience of W J Powell.
Additional file 1: of Dynamics of DNMT3A mutation and prognostic relevance in patients with primary myelodysplastic syndrome
Creators: name: Ming-En Lin
name: Hsin-An Hou
name: Tsai, Cheng-Hong
name: Shang-Ju Wu
name: Yuan-Yeh Kuo
name: Mei-Hsuan Tseng
name: Ming-Chih Liu
name: Liu, Chia-Wen
name: Wen-Chien Chou
name: Chien-Yuan Chen
name: Jih-Luh Tang
name: Yao, Ming
name: Chi-Cheng Li
name: Shang-Yi Huang
name: Bor-Sheng Ko
name: Szu-Chun Hsu
name: Chien-Ting Lin
name: Hwei-Fang Tien
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Hematology

description: Table S1. The mutation patterns in 37 MDS patients with DNMT3A mutations at diagnosis. Table S2. Cytogenetics between MDS patients with and without DNMT3A mutation. Figure S1. Kaplanâ Meier survival curves for overall survival among patients with DNMT3A mutations stratified by whether receiving allogeneic HSCT or not. Figure S2. Kaplan-Meier curves stratified by the status of DNMT3A mutations for overall survival among the 421 SF3B1-wild type MDS patients (A) and among the 48 SF3B1-mutated MDS patients (B). (DOC 242Â kb)
Testing Lorentz symmetry violation with an invariant minimum speed
Creators: name: Nassif, Cláudio
name: Faria, A. C. Amaro de
name: Santos, Rodrigo Francisco dos
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: This work presents an experimental test of Lorentz invariance violation in the infrared (IR) regime by means of an invariant minimum speed in the spacetime and its effects on the time when an atomic clock given by a certain radioactive single-atom (e.g.: isotope $Na^{25}$) is a thermometer for a ultracold gas like the dipolar gas $Na^{23}K^{40}$. So, according to a Deformed Special Relativity (DSR) so-called Symmetrical Special Relativity (SSR), where there emerges an invariant minimum speed $V$ in the subatomic world, one expects that the proper time of such a clock moving close to $V$ in thermal equilibrium with the ultracold gas is dilated with respect to the improper time given in lab, i.e., the proper time at ultracold systems elapses faster than the improper one for an observer in lab, thus leading to the so-called {\it proper time dilation} so that the atomic decay rate of a ultracold radioactive sample (e.g: $Na^{25}$) becomes larger than the decay rate of the same sample at room temperature. This means a suppression of the half-life time of a radioactive sample thermalized with a ultracold cloud of dipolar gas to be investigated by NASA in the Cold Atom Lab (CAL).
description: 11 pages, 4 figures. arXiv admin note: text overlap with arXiv:1510.00595, arXiv:1211.3612, arXiv:0805.1201
The stellar content of the COSMOS field as derived from morphological and SED based gtar/galaxy Separation
Creators: name: Robin, A. C.
name: Rich, R. M.
name: Aussel, H.
name: Capak, P.
name: Tasca, L. A. M.
name: Jahnke, K.
name: Kakazu, Y.
name: Kneib, J-P.
name: Koekemoer, A.
name: Leauthaud, A. C.
name: Lilly, S.
name: Mobasher, B.
name: Scoville, N.
name: Taniguchi, Y.
name: Thompson, D. J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the stellar content of the COSMOS two degree field, as derived from a rigorous star/galaxy separation approach developed for using stellar sources to define the point spread function variation map used in a study of weak galaxy lensing. The catalog obtained in one filter from the ACS (Advanced Camera for Survey on the Hubble Space Telescope) is cross-identified with ground based multi-wavelength catalogs. The classification is reliable to magnitude $F_{814W}=24$ and the sample is complete even fainter. We construct a color-magnitude diagram and color histograms and compare them with predictions of a standard model of population synthesis. We find features corresponding to the halo subdwarf main sequence turnoff, the thick disk, and the thin disk. This data set provides constraints on the thick disk and spheroid density laws and on the IMF at low mass. We find no evidence of a sharp spheroid edge out to this distance. We identify a blue population of white dwarfs with counts that agree with model predictions. We find a hint for a possible slight stellar overdensity at about 22-34 kpc but the data are not strong enough at present to claim detection of a stream feature in the halo (abridged).
description: 32 pages, 13 figures, accepted in APJ Suppl COSMOS special issue, replaced by larger figures. A full resolution figure preprint can be found at ftp://ftp.obs-besancon.fr/pub/outgoing/annie/star-cosmos.pdf
MOESM3 of Characterization of a novel sugar transporter involved in sugarcane bagasse degradation in Trichoderma reesei
Creators: name: Nogueira, Karoline
name: Paula, Renato De
name: Antoniêto, Amanda
name: Thaila Reis
name: Carraro, Cláudia
name: Alinne Silva
name: Almeida, Fausto
name: Carem Rechia
name: Goldman, Gustavo
name: Silva, Roberto
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Biotechnology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 3. Southern blot analyse to confirm deletion of Tr69957 in T. reesei. (A) Strategy used to confirm deletion of Tr69957 by Southern blot. The figure shows the promoter region (in green) and terminator (in purple) of the gene, with the substitution of the ORF by the pyrG selection marker. A specific DNA probe was created to bind the portion of the gene (in blue), confirming its presence in the analyzed genetic content. (B) Southern blot showing the parental fungus (QM6aΔtmus53Δpyr4) used as control and four deleted candidates that did not present detection of the gene portion equivalent to 3391 bp as in the parental and presented the region corresponding to 6698bp, confirming the deletion.
Sisymbrium irio Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Sisymbrium
Sisymbrium irio

description: Sisymbrium irio Linnaeus, Species Plantarum 2: 659. 1753.
"Habitat in Europae cultis." RCN: 4796.
 Lectotype (Jonsell & Jarvis in Nordic J. Bot. 22: 71. 2002): Löfling 496 , Herb. Linn. No. 836.35 (LINN).
 Current name:  Sisymbrium irio  L. (Brassicaceae).
 Note: Several authors from Franchetti (in Webbia 14: 194. 1958) onwards indicated unspecified material in LINN as type but failed to distinguish between several possible collections there. They are evidently not part of a single gathering so Art. 9.15 does not apply.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 855, DOI: 10.5281/zenodo.291971
Solutions of Coupled DGLAP Evolution Equations for Singlet and Gluon Structure Functions in leading order at low-x
Creators: name: Jamil, U.
name: Sarma, J. K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper, we solved the coupled Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) evolution equations for singlet and gluon structure functions in leading order (LO) at low-x assuming the Regge behaviour of quark and gluon structure functions at this limit, and t and x-evolutions of singlet and gluon structure functions are presented. We have compared our results of gluon structure function with global MRST 2004 and GRV 1998 gluon parameterizations and the results of deuteron structure function with New Muon Collaboration (NMC) data. We have shown that the solutions of coupled equations give accurate results for the structure functions and also the compatibility of Regge behaviour of quark and gluon structure functions with perturbative quantum chromodynamics (PQCD) at low-x.
description: 14 pages, 4 figures
Sisymbrium loeselii Linnaeus 1755
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Sisymbrium
Sisymbrium loeselii

description: Sisymbrium loeselii Linnaeus, Centuria I Plantarum: 18. 1755.
"Habitat in Borussia, Gedani, in montanis aequicolor." RCN: 4797.
 Lectotype (Jafri in Nasir & Ali, Fl. W. Pakistan 55: 251. 1973): Herb. Linn. No. 836.40 (LINN).
 Current name:  Sisymbrium loeselii  L. (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 855, DOI: 10.5281/zenodo.291971
A Potential Galaxy Threshing System in the Cosmos Field
Creators: name: Sasaki, S. S.
name: Taniguchi, Y.
name: Scoville, N.
name: Mobasher, B.
name: Aussel, H.
name: Sanders, D. B.
name: Koekemoer, A.
name: Ajiki, M.
name: Komiyama, Y.
name: Miyazaki, S.
name: Kaifu, N.
name: Karoji, H.
name: Okamura, S.
name: Arimoto, N.
name: Ohta, K.
name: Shioya, Y.
name: Murayama, T.
name: Nagao, T.
name: Koda, J.
name: Hainline, L.
name: Renzini, A.
name: Giavalisco, M.
name: LeFevre, O.
name: Impey, C.
name: Elvis, M.
name: Lilly, S.
name: Rich, M.
name: Schinnerer, E.
name: Sheth, K.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with $M_V \approx -21.6$ and a tidally disrupted satellite galaxy with $M_V \approx -17.7$ at a photometric redshift of $z \approx 0.08$. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are $3.7 \times 10^{12} \cal{M}_{\odot}$ and $3.1 \times 10^{9} \cal{M}_{\odot}$, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.
description: 17 pages, 7 figures, accepted for the COSMOS special issue of ApJS
Remarks on the Z' Drell-Yan cross section
Creators: name: Paz, Gil
name: Roy, Joydeep
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Many extension of the standard model contain an extra U(1)' gauge group with a heavy Z' gauge boson. Perhaps the most clear signal for such a Z' would be a resonance in the invariant mass spectrum of the lepton pairs to which it decays. In the absence of such a signal, experiments can set limits on the couplings of such a Z', using a standard formula from theory. We repeat its derivation and find that, unfortunately, the standard formula in the literature is a factor of 8 too small. We briefly explore the implication for existing experimental searches and encourage the high energy physics community to re-examine analyses that have used this formula.
description: 9 pages, 1 figure, two references added, journal version
title: ADCO, Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Cart. 23 (G 127), 310 folios, f. 00445
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2011
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00445, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Troisième cartulaire de Saint-Étienne de Dijon (XVIe), Archives départementales de la Côte-d'Or, Cart. 23 (G 127), 310 folios, f. 00445, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Coincya monensis Greuter & Burdet 1983
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Coincya
Coincya monensis

description: Sisymbrium monense Linnaeus, Species Plantarum 2: 658. 1753.
"Habitat in Mona, insula Angliae." RCN: 4787.
 Lectotype (Leadlay & Heywood in Bot. J. Linn. Soc. 102: 364. 1990): [icon] " Eruca Monensis laciniata, flore luteo majore" in Dillenius, Hort. Eltham. 1: 135, t. 111, f. 135. 1732.
 Current name:  Coincya monensis  (L.) Greuter & Burdet (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 855, DOI: 10.5281/zenodo.291971
Methods for compressible fluid simulation on GPUs using high-order finite differences
Creators: name: Pekkilä, Johannes
name: Väisälä, Miikka S.
name: Käpylä, Maarit J.
name: Käpylä, Petri J.
name: Anjum, Omer
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We focus on implementing and optimizing a sixth-order finite-difference solver for simulating compressible fluids on a GPU using third-order Runge-Kutta integration. Since graphics processing units perform well in data-parallel tasks, this makes them an attractive platform for fluid simulation. However, high-order stencil computation is memory-intensive with respect to both main memory and the caches of the GPU. We present two approaches for simulating compressible fluids using 55-point and 19-point stencils. We seek to reduce the requirements for memory bandwidth and cache size in our methods by using cache blocking and decomposing a latency-bound kernel into several bandwidth-bound kernels. Our fastest implementation is bandwidth-bound and integrates $343$ million grid points per second on a Tesla K40t GPU, achieving a $3.6 \times$ speedup over a comparable hydrodynamics solver benchmarked on two Intel Xeon E5-2690v3 processors. Our alternative GPU implementation is latency-bound and achieves the rate of $168$ million updates per second.
description: 14 pages, 7 figures
(Non)decoupling of the Higgs triplet effects
Creators: name: Chankowski, P. H.
name: Pokorski, S.
name: Wagner, J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the electroweak theory with an additional Higgs triplet at one loop using the hybrid renormalization scheme based on $α_{\rm EM}$, $G_F$ and $M_Z$ as input observables. We show that in this scheme loop corrections can be naturally split into the Standard Model part and corrections due to ``new physics''. The latter, however do not decouple in the limit of infinite triplet mass parameter, if the triplet trilinear coupling to SM Higgs doublets grows along with the the triplet mass. In electroweak observables computed at one loop this effect can be attributed to radiative generation in this limit of a nonvanishing vacuum expectation value of the triplet. We also point out that whenever tree level expressions for the electroweak observables depend on vacuum expectation values of scalar fields other than the Standard Model Higgs doublet, tadpole contribution to the ``oblique'' parameter $T$ should in principle be included. In the Appendix the origin of nondecoupling is discussed on the basis of symmetry principles in a simple scalar field theory.
description: 26 pages. An appendix explaining nondecoupling from symmetry point of view is included
Additional file 1: of High frequency of M. leprae DNA detection in asymptomatic household contacts
Creators: name: Gama, Rafael
name: Thalisson Gomides
name: Chaiana Gama
name: Suelen Moreira
name: Manta, Fernanda De Neves
name: Oliveira, Lorena De
name: Marçal, Pedro
name: Euzenir Sarno
name: Moraes, Milton
name: Garcia, Raúl
name: Fraga, Lucia De Oliveira
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Cancer
subject: 60506 Virology

description: Bank of data. Description of data: this file contains all raw data of the study. (PDF 219 kb)
Hybrid integration of solid-state quantum emitters on a silicon photonic chip
Creators: name: Kim, Je-Hyung
name: Aghaeimeibodi, Shahriar
name: Richardson, Christopher J. K.
name: Leavitt, Richard P.
name: Englund, Dirk
name: Waks, Edo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Scalable quantum photonic systems require efficient single photon sources coupled to integrated photonic devices. Solid-state quantum emitters can generate single photons with high efficiency, while silicon photonic circuits can manipulate them in an integrated device structure. Combining these two material platforms could, therefore, significantly increase the complexity of integrated quantum photonic devices. Here, we demonstrate hybrid integration of solid-state quantum emitters to a silicon photonic device. We develop a pick-and-place technique that can position epitaxially grown InAs/InP quantum dots emitting at telecom wavelengths on a silicon photonic chip deterministically with nanoscale precision. We employ an adiabatic tapering approach to transfer the emission from the quantum dots to the waveguide with high efficiency. We also incorporate an on-chip silicon-photonic beamsplitter to perform a Hanbury-Brown and Twiss measurement. Our approach could enable integration of pre-characterized III-V quantum photonic devices into large-scale photonic structures to enable complex devices composed of many emitters and photons.
description: 19 Pages in total, including 8 figures
Interacting Galaxies in Sparsely Populated Groups
Creators: name: Melnyk, Olga
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculated the median values of the following parameters for 87 groups of galaxies with three to eight components: the mean rms velocity of the galaxies in the group, S_v = 166 km/s; the harmonic mean radius, R_h = 29 kpc; and the mass-to-light ratio, M_vir/L = 33 Msun/Lsun. The M_vir/L ratio depends on the population of the system, while S_v does not depend on R_h. To ascertain the relationship between the activity of galaxies in groups and their morphological composition and the effect of the environment on the evolutionary processes in groups, we consider the fraction of galaxies with UV excess in the sample of interacting galaxies in groups (6%), single peculiar galaxies (8%), and isolated galaxies (4%) and their morphological composition. We also show that the number of active galaxies decreases with increasing population of the group of galaxies, while the frequency of occurrence of early-type (E/S0) galaxies increases.
Maize Grain Germination Is Accompanied by Acidification of the Environment
Creators: name: Wellmann, Konrad
name: Varnskühler, Jens
name: Leubner-Metzger, Gerhard
name: Mummenhoff, Klaus
Publisher: name: Universität Osnabrück
Year: 2023
Subjects: subject: Zea mays L.
subject: germination
subject: acidic pH
subject: H+-ATPase
subject: pericarp
subject: agriculture
subject: 580 - Pflanzen (Botanik)

description: Seed germination is a complex process involving several stages, starting with the imbibition of water and ending with the emergence of the radicle. In the current study, we address the observation of an unexpected pH shift during the imbibition of maize grains. We used direct pH measurements of soak water, the pH indicator methyl red, and anatomical analysis to shed light on the acidification associated with maize (Zea mays L.) germination, a largely overlooked phenomenon. Our work shows that acidification during imbibition of maize grains is a two-step process: (i) early, rapid acidification (pH values up to 4.4), in which protons stored in the (dead) pericarp/testa are mobilised and rapidly diffuse into the surrounding medium, and (ii) late, delayed acidification (pH values just below 6), starting hours after contact of grains with water, representing an active transport process caused by living cells of the seed. We discuss the physiological mechanisms and ecological relevance of environmental acidification during maize grain germination.
Models for jet power in elliptical galaxies: A case for rapidly spinning black holes
Creators: name: Nemmen, Rodrigo S.
name: Bower, Richard G.
name: Babul, Arif
name: Storchi-Bergmann, Thaisa
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The power of jets from black holes are expected to depend on both the spin of the black hole and the structure of the accretion disk in the region of the last stable orbit. We investigate these dependencies using two different physical models for the jet power: the classical Blandford-Znajek (BZ) model and a hybrid model developed by Meier. In the BZ case, the jets are powered by magnetic fields directly threading the spinning black hole while in the hybrid model, the jet energy is extracted from both the accretion disk as well as the black hole via magnetic fields anchored to the accretion flow inside and outside the hole's ergosphere. The hybrid model takes advantage of the strengths of both the Blandford-Payne and BZ mechanisms, while avoiding the more controversial features of the latter. We develop these models more fully to account for general relativistic effects and to focus on advection-dominated accretion flows (ADAF) for which the jet power is expected to be a significant fraction of the accreted rest mass energy. We apply the models to elliptical galaxies, in order to see if these models can explain the observed correlation between the Bondi accretion rates and the total jet powers. For typical values of the disk viscosity parameter alpha~0.04-0.3 and mass accretion rates consistent with ADAF model expectations, we find that the observed correlation requires j>0.9; i.e., it implies that the black holes are rapidly spinning. Our results suggest that the central black holes in the cores of clusters of galaxies must be rapidly rotating in order to drive jets powerful enough to heat the intracluster medium and quench cooling flows.
description: 12 pages, 4 figures, accepted for publication in MNRAS
Diplotaxis muralis
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Capparales
Brassicaceae
Diplotaxis
Diplotaxis muralis

description: Sisymbrium murale Linnaeus, Species Plantarum 2: 658. 1753.
"Habitat in Gallia, Sicilia." RCN: 4786.
 Lectotype (Jafri in Ali & Jafri, Fl. Libya 23: 37. 1977): Herb. Linn. No. 836.18 (LINN).
 Current name:  Diplotaxis muralis  (L.) DC. (Brassicaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 856, DOI: 10.5281/zenodo.291971
Additional file 1: of Pharmacists in general practice: a qualitative interview case study of stakeholdersâ experiences in a West London GP federation
Creators: name: Ryan, Kath
name: Nilesh Patel
name: Lau, Wing
name: Abu-Elmagd, Hamza
name: Stretch, Graham
name: Pinney, Helen
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Interview guides including indicative questions for pharmacists, general practitioners, managers, nurses, receptionists and patients. (DOCX 16Â kb)
Dipole model for double meson production in two-photon interactions at high energies
Creators: name: Goncalves, V. P.
name: Machado, M. V. T.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this work the double vector meson production in two-photon interactions at high energies is investigated considering saturation physics. We extend the color dipole picture for this process and study the energy and virtuality dependence of the forward differential cross section. Comparison with previous results is presented and the contribution of the different photon polarizations is estimated.
description: 20 pages, 8 figures, 1 table. Version to be published in European Physical Jornal C
TGF-β family ligands exhibit distinct signalling dynamics that are driven by receptor localisation.
Creators: name: Miller, Daniel SJ
name: Schmierer, Bernhard
name: Hill, Caroline S
Publisher: name: The Francis Crick Institute
Year: 2020
Subjects: Model organisms
Signalling & Oncogenes
Gene Expression
Genetics & Genomics
Developmental Biology
Cell Biology
Computational & Systems Biology

description: Growth factor-induced signal transduction pathways are tightly regulated at multiple points intracellularly, but how cells monitor levels of extracellular ligand and translate this information into appropriate downstream responses remains unclear. Understanding signalling dynamics is thus a key challenge in determining how cells respond to external cues. Here, we demonstrate that different TGF-β family ligands, namely Activin A and BMP4, signal with distinct dynamics, which differ profoundly from those of TGF-β itself. The signalling dynamics are driven by differences in the localisation and internalisation of receptors for each ligand, which in turn determine the capability of cells to monitor levels of extracellular ligand. Using mathematical modeling, we demonstrate that the distinct receptor behaviours and signalling dynamics observed may be primarily driven by differences in ligand-receptor affinity. Furthermore, our results provide a clear rationale for the different mechanisms of pathway regulation found in vivo for each of these growth factors.
Rorippa nasturtium
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Rorippa
Rorippa nasturtium

description: Sisymbrium nasturtium-aquaticum Linnaeus, Species Plantarum 2: 657. 1753.
"Habitat in Europa & America septentrionali ad fontes." RCN: 4777.
 Lectotype (Jonsell in Svensk Bot. Tidskr. 67: 293. 1973): Herb. Linn. No. 836.1 (LINN).
 Current name:  Rorippa nasturtium  -  aquaticum  (L.) Hayek (Brassicaceae).
 Note: Although Fawcett & Rendle (Fl. Jamaica 3: 237. 1914) indicated material in LINN as the type, they did not distinguish between sheets 836.1 and 836.2 (which are evidently not part of a single gathering so Arr. 9.15 does not apply).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part S), pp. 806-877 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 856, DOI: 10.5281/zenodo.291971
Spathius subtilis Chao. A 1977
Creators: name: Tang, Pu
name: Belokobylskij, Sergey
name: Chen, Xue-Xin
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Spathius
Spathius subtilis

description: Spathius subtilis Chao, 1977
(Fig. 43)
Spathius subtilis Chao, 1977: 216; Chen & Shi, 2004: 164; Yu et al., 2012.
Material examined. Female (holotype, IZCAS), Fujian Prov., Jianyang Guadun, 25.IX.1965, Chen Jiahua. China (ZJUH). 1 female, Yunnan Prov., Yingjiang Tongbiguan, 17. V.2009, Zeng Jie, No. 200904269; 1 female, Hainan Prov., Jianfengling Tianchi, 12–15.VII.2006, Weng Liqiong, No. 200803320.
Distribution. China (Fujian, Yunnan, Hainan).
description: Published as part of Tang, Pu, Belokobylskij, Sergey & Chen, Xue-Xin, 2015, Spathius Nees, 1818 (Hymenoptera: Braconidae, Doryctinae) from China with a key to species, pp. 1-132 in Zootaxa 3960 (1) on page 117, DOI: 10.11646/zootaxa.3960.1.1, http://zenodo.org/record/14951550
Star formation rates and stellar masses in z ~ 1 gamma ray burst hosts
Creators: name: Cerón, J. M. Castro
name: Michałowski, M. J.
name: Hjorth, J.
name: Watson, D.
name: Fynbo, J. P. U.
name: Gorosabel, J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyse 4.5, 8 and 24 um band Spitzer images of six gamma ray burst host galaxies at redshifts close to 1. We constrain their star formation rates (SFR) based on the entire available spectral energy distribution rather than the 24 um band only. Further, we estimate their stellar masses (M*) based on rest frame K band luminosities. Our sample spans a wide range of galaxy properties: derived SFRs range from less than 10 to a few hundred solar masses per year; values of M* range from 10^9 to 10^10 Mo with a median of 5.6 x 10^9 Mo. Comparing the specific star formation rate (PHI = SFR/M*) of our sample as a function of M* to other representative types of galaxies (distant red galaxies, Ly-alpha emitters, Lyman break galaxies, submillimeter galaxies and z ~ 2 galaxies from the Great Observatories Origins Deep Survey-North field), we find that gamma ray burst hosts are among those with the highest PHI.
description: 4 pages by emulateApJ, 1 table and 2 colour figures; published in ApJ Letters
Higgs Assisted Q-balls from Pseudo-Nambu-Goldstone Bosons
Creators: name: Bishara, Fady
name: Johnson, George
name: Lennon, Olivier
name: March-Russell, John
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Motivated by recent constructions of TeV-scale strongly-coupled dynamics, either associated with the Higgs sector itself as in pseudo-Nambu-Goldstone boson (pNGB) Higgs models or in theories of asymmetric dark matter, we show that stable solitonic Q- balls can be formed from light pion-like pNGB fields carrying a conserved global quantum number in the presence of the Higgs field. We focus on the case of thick-wall Q-balls, where solutions satisfying all constraints are shown to exist over a range of parameter values. In the limit that our approximations hold, the Q-balls are weakly bound and parametrically large, and the form of the interactions of the light physical Higgs with the Q-ball is determined by the breaking of scale symmetry.
description: 24 pages, 6 figures, 1 table
Injuries from the Battlefield
Creators: name: Project Team, Their Finest Hour
Publisher: name: University of Oxford
Year: 2024
Subjects: classificationCode: 430304
subject: British history
classificationCode: 430308
subject: European history (excl. British, classical Greek and Roman)
classificationCode: 430316
subject: International history

description: The contributor's father, Francis Edward Burnham, lost his leg during the Second World War. He was a quiet, strong man who never spoke about his experiences. The contributor had found photos of her father in the desert; however, she and her siblings could not piece his story together. The contributor noted that her father also had a "floppy ear" from being hit by a bullet, although the ear had been reshaped by a friend.The contributor explained that her father became a Sergeant and was ordered to serve in India. He sent a letter to his family after losing his leg, and the contributor highlighted that his tone was reminiscent of the phrase "stiff upper lip." The contributor's father became dangerously ill after losing his leg, as the wound had not closed properly, and more of his leg was removed. The contributor added that her father had received new boots just prior to losing his leg, and she recalled her father joking that it was a waste of a new pair of boots.The contributor commented that no male relatives spoke about their experiences of the Second World War. Her mother, Nelly Mary Burnham, did not speak about the war either. The contributor noted that her mother was supported by a few friends and that she would have been disapproving if the contributor's father had shared his stories of the war with his daughter when she was young. The contributor's father wrote his life story in a book, which was given to the church and subsequently lost. The contributor added that she was put in service to a clergyman at age 7, and she was raised with both discipline and kindness as a child.The contributor's mother had worked for the General Post Office (GPO) as a telephonist; however, the contributor was not aware of her mother's role during the Second World War. The contributor noted that the family did not have much information about who their relatives were and what their background was. The contributor mentioned that her mother may have been a member of the Women's Auxiliary Air Force (WAAFs); however, her mother was young and tried to escape home as she had struggled to cope. The military police found the contributor's mother and took her back. The contributor highlighted that she thinks her mother is an amazing person.
Evidence of a Bottom-heavy Initial Mass Function in Massive Early-type Galaxies from Near-infrared Metal Lines
Creators: name: Lagattuta, David J.
name: Mould, Jeremy R.
name: Forbes, Duncan A.
name: Monson, Andrew J.
name: Pastorello, Nicola
name: Persson, S. Eric
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present new evidence for a variable stellar initial mass function (IMF) in massive early-type galaxies, using high-resolution, near-infrared spectroscopy from the Folded-port InfraRed Echellette spectrograph (FIRE) on the Magellan Baade Telescope at Las Campanas Observatory. In this pilot study, we observe several gravity-sensitive metal lines between 1.1 $μ$m and 1.3 $μ$m in eight highly-luminous ($L \sim 10 L_*$) nearby galaxies. Thanks to the broad wavelength coverage of FIRE, we are also able to observe the Ca II triplet feature, which helps with our analysis. After measuring the equivalent widths (EWs) of these lines, we notice mild to moderate trends between EW and central velocity dispersion ($σ$), with some species (K I, Na I, Mn I) showing a positive EW-$σ$ correlation and others (Mg I, Ca II, Fe I) a negative one. To minimize the effects of metallicity, we measure the ratio $R$ = [EW(K I) / EW(Mg I)], finding a significant systematic increase in this ratio with respect to $σ$. We then probe for variations in the IMF by comparing the measured line ratios to the values expected in several IMF models. Overall, we find that low-mass galaxies ($σ\sim 100$ km s$^{-1}$) favor a Chabrier IMF, while high-mass galaxies ($σ\sim 350$ km s$^{-1}$) are better described with a steeper (dwarf-rich) IMF slope. While we note that our galaxy sample is small and may suffer from selection effects, these initial results are still promising. A larger sample of galaxies will therefore provide an even clearer picture of IMF trends in this regime.
description: 17 pages, 10 figures, 6 tables. Accepted for publication in ApJ
Skyrmions, Hadrons and isospin chemical potential
Creators: name: Loewe, M.
name: Mendizabal, S.
name: Rojas, J. C.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using the Hamiltonian formulation, in terms of collective variables, we explore the evolution of different skyrmionic parameters as function of the isospin chemical potential ($μ$), such as the energy density, the charge density, the isoscalar radius and the isoscalar magnetic radius. We found that the radii start to grow very fast for $μ\gtrsim 140$ MeV, suggesting the occurrence of a phase transition.
description: 10 pages, 5 figures
On the possibility of the implicit renormalization procedure for the Casimir energy
Creators: name: Dubikovsky, A. I.
name: Silaev, P. K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a procedure for the renormalization of Casimir energy, that is based on the implicit versions of standard steps of renormalization procedure --- regularization, subtraction and removing the regularization. The proposed procedure is based on the calculation of a set of convergent sums, which are related to the original divergent sum for the non-renormalized Casimir energy. Then one constructs a linear equations system, that connects this set of convergent sums with the renormalized Casimir energy, which is a solution to this equations system. This procedure slightly reduces the indeterminancy that arises in standard procedure when we choose the particular regularization and the explicit form of counterterm. The proposed procedure is more efficient from the computational point of view than the standard one. It can be applied not only for systems with the explicit transcendental equation for the spectrum, but also for systems with the spectrum that can be obtained only numerically.