cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Study of the direct $^{16}{\rm O}(p, γ)^{17}{\rm F}$ astrophysical capture reaction within a potential model approach
Creators: name: Tursunov, E. M.
name: Turakulov, S. A.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A potential model is applied for the analysis of the astrophysical direct nuclear capture process $^{16}$O(p,$γ)^{17}$F. The phase-equivalent potentials of the Woods-Saxon form for the p$-^{16}$O interaction are examined which reproduce the binding energies and the empirical values of ANC for the $^{17}$F(5/2$^+$) ground and $^{17}$F(1/2$^+$) ($E^*$=0.495 MeV) excited bound states from different sources. The best description of the experimental data for the astrophysical $S$ factor is obtained within the potential model which yields the ANC values of 1.043 fm$^{-1/2}$ and 75.484 fm$^{-1/2}$ for the $^{17}$F($5/2^{+}$) ground and $^{17}$F($1/2^{+}$) excited bound states, respectively. The zero-energy astrophysical factor $S(0)=9.321$ KeV b is obtained by using the asymptotic expansion method of D. Baye. The calculated reaction rates within the region up to 10$^{10}$ K are in good agreement with those from the R-matrix approach and the Bayesian model in both absolute values and temperature dependence.
description: 6 figures
Record-based transmuted unit omega distribution: different methods of estimation and applications
Creators: name: Pathak, Ashok Kumar
name: Arshad, Mohd.
name: Pandey, Alok Kumar
name: Ali, Alam
Publisher: name: arXiv
Year: 2024
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 60E05, 62F10, 62E15, 65C05, 33C05

description: Dombi et al. (2019) introduced a three parameter omega distribution and showed that its asymptotic distribution is the Weibull model. We propose a new record-based transmuted generalization of the unit omega distribution by considering Balakrishnan and He (2021) approach. We call it the RTUOMG distribution. We derive expressions for some statistical quantities, like, probability density function, distribution, hazard function, quantile function, moments, incomplete moments, inverted moments, moment generating function, Lorenz curve, and Bonferroni curve of the proposed distribution. The numerical values of various measures of central tendency and coefficient of skewness and kurtosis are also presented. Concepts of stochastic ordering and some results related to ordered statistics of the RTUOMG distribution are discussed. The parameters of the RTUOMG distribution are estimated using five distinct estimators. Additionally, the Monte Carlo simulations are performed to assess the performance of these estimators. Finally, two real data sets are analyzed to demonstrate the utility of the RTUOMG distribution.
description: 26 pages, 14 figures
Subproton-scale cascades in solar wind turbulence: driven hybrid-kinetic simulations
Creators: name: Cerri, S. S.
name: Califano, F.
name: Jenko, F.
name: Told, D.
name: Rincon, F.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: A long-lasting debate in space plasma physics concerns the nature of subproton-scale fluctuations in solar wind (SW) turbulence. Over the past decade, a series of theoretical and observational studies were presented in favor of either kinetic Alfvén wave (KAW) or whistler turbulence. Here, we investigate numerically the nature of the subproton-scale turbulent cascade for typical SW parameters by means of unprecedented high-resolution simulations of forced hybrid-kinetic turbulence in two real-space and three velocity-space dimensions. Our analysis suggests that small-scale turbulence in this model is dominated by KAWs at $β\gtrsim1$ and by magnetosonic/whistler fluctuations at lower $β$. The spectral properties of the turbulence appear to be in good agreement with theoretical predictions. A tentative interpretation of this result in terms of relative changes in the damping rates of the different waves is also presented. Overall, the results raise interesting new questions about the properties and variability of subproton-scale turbulence in the SW, including its possible dependence on the plasma $β$, and call for detailed and extensive parametric explorations of driven kinetic turbulence in three dimensions.
description: 6 pages, 4 figures, accepted for publication in The Astrophysical Journal Letters
Spilomicrus tinctipennis Cameron 1888
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Spilomicrus
Spilomicrus tinctipennis

description: Spilomicrus tinctipennis Cameron, 1888: 440, pl. 18, fig. 17.
Valid name
Idiotypa tinctipennis (Cameron, 1888).
Summary of types
Holotype ♀, BMNH number 9.747, by monotypy.
Primary type data
Bugaba/ Panama / Champion; B.C.A. Hymen. I./ Spilomicrus / tinctipennis/ Cam.; Type / H. T.; Spilomicrus / tinctipennis/ Cam./ B.C.A. ii 440.
Type locality
Panama, Bugaba.
Remarks
The description of this species was based on an unspecified number of females. One specimen was found which agreed with the description, except that it did not have a blunt, projecting, basal tooth on the hind femur; however, a piece of dirt was found on the base of the right hind femur which gave the appearance of a tooth (the base of the left femur was obscured). It is therefore considered that Cameron’s description is incorrect on this point, and should not prevent the specimen from being a type. It is most unlikely there would be another specimen with a piece of dirt on the base of the hind femur giving the appearance of a tooth, so it is considered that this was the only specimen Cameron saw and is therefore a holotype by monotypy. The holotype is mounted on a card and is dirty with the left wings crumpled. The piece of dirt which gave the appearance of a tooth on the femur has been removed, but the specimen is now clearly labelled so it can still be recognised.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 32, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Institute of Physics, Environmental Physics Group newsletter (16), Summer 1997
Creators: name: Brown, Sally
Publisher: name: Zenodo
Year: 1997
Subjects: subject: data and information
subject: Environmental Physics Group
subject: Institute of Physics
subject: https://id.loc.gov/authorities/subjects/sh85081263.html
subject: https://id.loc.gov/authorities/subjects/sh85040989.html
subject: https://id.loc.gov/authorities/subjects/sh85063458.html
subject: https://id.loc.gov/authorities/subjects/sh85101653.html
subject: https://id.loc.gov/authorities/subjects/sh85055077.html
subject: https://id.loc.gov/authorities/subjects/sh2018002590.html
subject: https://id.loc.gov/authorities/subjects/sh85040468.html
subject: https://id.loc.gov/authorities/subjects/sh85084334.html

description: This file contains the newsletters of the Environmental Physics Group at the Institute of Physics. The fundamental aim of the Group is to promote physics within the context of the environmental sciences. In achieving this aim we provide a forum for the discussion of physics as it applies to the environment and encourage the development and application of physical methods to environmental research. The Group also encourages the education and training of physicists in the environmental sciences through meetings and contacts with educationalists at all levels. Because of the broad nature of environmental physics the Group is involved in co-operative meetings with other professional organisations with interests in the environment. These newsletters are an archive of our activities since the formation of the Group. For more information about the Environmental Physics Group, see http://www.iop.org/activity/groups/subject/env/index.html
description: Previously curated at: http://cedadocs.ceda.ac.uk/837/ The publish date on this item was its original published date. Main files in this record: iop_epg_newsletter16_summer1997.pdf Item originally deposited with Centre for Environmental Data Analysis (CEDA) document repository by Dr Sally Brown. Transferred to CEDA document repository community on Zenodo on 2022-11-24
Anomalous capillary filling and wettability reversal in nanochannels
Creators: name: Gravelle, Simon
name: Ybert, Christophe
name: Bocquet, Lydéric
name: Joly, Laurent
Publisher: name: arXiv
Year: 2016
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: This work revisits capillary filling dynamics in the regime of nanometric to subnanometric channels. Using molecular dynamics simulations of water in carbon nanotubes, we show that for tube radii below one nanometer, both the filling velocity and the Jurin rise vary non-monotonically with the tube radius. Strikingly, with fixed chemical surface properties, this leads to confinement-induced reversal of the tube wettability from hydrophilic to hydrophobic for specific values of the radius. By comparing with a model liquid metal, we show that these effects are not specific to water. Using complementary data from slit channels, we then show that they can be described using the disjoin-ing pressure associated with the liquid structuring in confinement. This breakdown of the standard continuum framework is of main importance in the context of capillary effects in nanoporous media, with potential interests ranging from membrane selectivity to mechanical energy storage.
The low mass end of the neutral gas mass and velocity width functions of galaxies in $Λ$CDM
Creators: name: Yaryura, C. Y.
name: Helmi, A.
name: Abadi, M. G.
name: Starkenburg, E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use the high-resolution Aquarius cosmological dark matter simulations coupled to the semi-analytic model by Starkenburg et al. (2013) to study the HI content and velocity width properties of field galaxies at the low mass end in the context of $Λ$CDM. We compare our predictions to the observed ALFALFA survey HI mass and velocity width functions, and find very good agreement without fine-tuning, when considering central galaxies. Furthermore, the properties of the dark matter halos hosting galaxies, characterised by their peak velocity and circular velocity at 2 radial disk scalelengths overlap perfectly with the inferred values from observations. This suggests that our galaxies are placed in the right dark matter halos, and consequently at face value, we do not find any discrepancy with the predictions from the $Λ$CDM model. Our analysis indicates that previous tensions, apparent when using abundance matching models, arise because this technique cannot be straightforwardly applied for objects with masses $M_{vir} < 10^{10} M_{\odot}$.
description: Accepted for publication in MNRAS, 9 pages, 8 figures
Coupling renormalization flow in the strongly interacting regime of an asymptotically free quantum field theory in four dimensions
Creators: name: Berges, Jürgen
name: Gurau, Razvan
name: Keppler, Hannes
name: Preis, Thimo
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider a scalar quantum field theory with global $O(N)^3$ symmetry in four Euclidean dimensions and solve it numerically in closed form in the large-N limit. For imaginary tetrahedral coupling the theory is asymptotically free, with stable and real quantum effective action. We demonstrate the dynamical build-up of a strong interaction as the correlation length increases in a regime where the coupling renormalization flow remains well defined in the infrared. This is in contrast to perturbative results of asymptotically free theories, which predict that the coupling becomes ill-defined in the infrared, like in quantum chromodynamics. These properties make the model an important laboratory for the study of strong-coupling phenomena in quantum field theory from first principles.
description: 5+4 pages, 4+2 figures; published version
Danaea nodosa Sm.
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Marattiopsida
Marattiales
Marattiaceae
Danaea
Danaea nodosa

description: Acrostichum nodosum Linnaeus, Species Plantarum 2: 1070. 1753. "Habitat in Dominica." RCN: 7836. Basionym of: Asplenium nodosum (L.) L. (1763). Lectotype (Underwood in Bull. Torrey Bot. Club 29: 671. 1902): [icon] "Lingua Cervina nodosa major" in Plumier, Traité Foug. Amér.: 90, t. 108. 1705. Current name:  Danaea nodosa (L.) Sm. (Marattiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Mantara bifurcata Dodd 1920
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Mantara
Mantara bifurcata

description: Mantara bifurcata Dodd, 1920: 380.
Valid name
Aneuropria bifurcata (Dodd, 1920) comb. nov.
Summary of types
Holotype ♀, BMNH number 9.677, by original designation. Paratypes ♀, ♂.
Primary type data
1081.; Type; Madeira./ Wollaston./ 55.7; Mantara / bifurcata/ Dodd ♀; Holotype ♀ / Mantara / bifurcata Dodd / L.Huggert-81.
Type locality
Madeira.
Remarks
This species was described from two females and a male, referred to in the original description as a “type” and “cotypes”. Three specimens matching the description were found, one of the females has Dodd’s identification label, and this is considered to be the holotype by original designation. The holotype is mounted on a card, with the left antenna mounted separately. Mantara bifurcata is actually a species of Aneuropria Kieffer, 1905. Since Mantara bifurcata is the type species of Mantara, this means Mantara Dodd, 1920 is a junior synonym of Aneuropria Kieffer, 1905 syn. nov. Aneuropria bifurcata comb. nov. is clearly a different species (in head shape, antennal proportions and the lack of notauli) from the widespread European A. foersteri Kieffer, 1910, which is also found in Madeira.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 38, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Comparison of magneto-optical properties of various excitonic complexes in CdTe and CdSe self-assembled quantum dots
Creators: name: Kobak, J.
name: Smoleński, T.
name: Goryca, M.
name: Rousset, J. -G.
name: Pacuski, W.
name: Bogucki, A.
name: Oreszczuk, K.
name: Kossacki, P.
name: Nawrocki, M.
name: Golnik, A.
name: Płachta, J.
name: Wojnar, P.
name: Kruse, C.
name: Hommel, D.
name: Potemski, M.
name: Kazimierczuk, T.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present a comparative study of two self-assembled quantum dot (QD) systems based on II-VI compounds: CdTe/ZnTe and CdSe/ZnSe. Using magneto-optical techniques we investigated a large population of individual QDs. The systematic photoluminescence studies of emission lines related to the recombination of neutral exciton X, biexciton XX, and singly charged excitons (X$^+$, X$^-$) allowed us to determine average parameters describing CdTe QDs (CdSe QDs): X-XX transition energy difference 12 meV (24 meV); fine-structure splitting $δ_{1}=$0.14 meV ($δ_{1}=$0.47 meV); $g$-factor $g=$2.12 ($g=$1.71); diamagnetic shift $γ=$2.5 $μ$eV$/$T$^{2}$ ($γ=$1.3 $μ$eV$/$T$^{2}$). We find also statistically significant correlations between various parameters describing internal structure of excitonic complexes.
description: 6 pages, 1 table, 4 figures
Schizaea pectinata Sw.
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Schizaeales
Schizaeaceae
Schizaea
Schizaea pectinata

description: Acrostichum pectinatum Linnaeus, Species Plantarum 2: 1068. 1753. "Habitat in Aethiopia." RCN: 7771. Lectotype (Schelpe & Anthony in Leistner, Fl. Southern Africa, Pteridophyta: 51. 1986): Herb. Linn. No. 1245.2 (LINN). Current name:  Schizaea pectinata (L.) Sw. (Schizaeaceae). Note: Verdcourt (in Beentje, Fl. Trop. E. Africa, Schizaeaceae: 2. 2000) rejected the type choice of Schelpe & Anthony because they incorrectly referred to 1245.2 (LINN) as the holotype, and designated a Morison plate in its place. However, under Art. 9.8, their type statement is correctable to lectotype, and their choice has priority.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Impact of atrial fibrillation in onco-hematological patients in Europe: a targeted literature review
Creators: name: Barrigón, Fernando Escalante
name: Bas, Cristina
name: Tang, Boxiong
name: Yang, Keri
name: Pomares, Elisenda
name: García, Alejandra
name: Bahar, Nasim
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: Atrial fibrillation (AF) is a common complication in cancer patients, and the increased risk associated with certain therapies poses a major challenge. The objective was to determine the clinical and economic burden of AF in onco-hematological patients in Europe. A targeted literature review was completed for observational, retrospective and case studies, and reviews on AF in onco-hematology published between January 2010 and 2022 in PubMed, Science Direct, Medes and IBECS. The search was based on epidemiology, cost, health-related quality of life (HRQoL), disease burden and management, and patient journey. Thirty-one studies fulfilled eligibility criteria. Annual incidence of AF during treatment varies up to 25%, and increased with first-generation Bruton tyrosine kinase inhibitors (BTKi). Risk factors include age ≥65, prior AF or hypertension, hyperlipidemia and ibrutinib use. Complications are managed with anticoagulants and/or antiarrhythmics, and regular monitoring. When AF is no longer controllable, dose reduction or discontinuation is recommended. No data on costs, HRQoL and patient journey were identified. There is scarce and heterogeneous information on AF in onco-hematology in Europe. Available evidence reports a higher risk of AF associated with first-generation BTKi. Further studies are needed to understand the burden of AF in these patients.
Acidopria spinosiceps Dodd 1920
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Acidopria
Acidopria spinosiceps

description: Acidopria spinosiceps Dodd, 1920: 380.
Valid name
Trichopria spinosiceps (Dodd, 1920) comb. nov.
Summary of types
Holotype ♀, BMNH number 9.692, by original designation. Paratype ♀.
Primary type data
Type; Kuching/ J.H.; P.Cameron Coll./ 1914-110; Brachyaulax / erythrocerus/ Cam. Type Borneo; Acidopria / spinosiceps/ Dodd ♀ type.
Type locality
Malaysia, Borneo, Sarawak, Kuching.
Remarks
This species was described from two females referred to as “type” and “cotype”. Two specimens were found corresponding to the description, one of which had Dodd’s type label and is regarded as the holotype by original designation. The holotype is mounted on a card and has parts of five legs missing. This species was placed by Dodd in Acidopria Kieffer, 1913 (now a junior synonym of Basalys) because of the spines on the head; however, it is a species of Trichopria. It differs from those species of Basalys with spinose heads in having the spines behind the ocellar triangle rather than in front of it. A non-type male was found which agrees closely with the females and it shows that this species belongs to the group of Trichopria with whorled hairs on the male antenna.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 38, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Institute of Physics, Environmental Physics Group newsletter (17), 1998
Creators: name: Brown, Sally
Publisher: name: Zenodo
Year: 1998
Subjects: subject: data and information
subject: Environmental Physics Group
subject: Institute of Physics
subject: https://id.loc.gov/authorities/subjects/sh85081263.html
subject: https://id.loc.gov/authorities/subjects/sh85040989.html
subject: https://id.loc.gov/authorities/subjects/sh85063458.html
subject: https://id.loc.gov/authorities/subjects/sh85101653.html
subject: https://id.loc.gov/authorities/subjects/sh85055077.html
subject: https://id.loc.gov/authorities/subjects/sh2018002590.html
subject: https://id.loc.gov/authorities/subjects/sh85040468.html
subject: https://id.loc.gov/authorities/subjects/sh85084334.html

description: This file contains the newsletters of the Environmental Physics Group at the Institute of Physics. The fundamental aim of the Group is to promote physics within the context of the environmental sciences. In achieving this aim we provide a forum for the discussion of physics as it applies to the environment and encourage the development and application of physical methods to environmental research. The Group also encourages the education and training of physicists in the environmental sciences through meetings and contacts with educationalists at all levels. Because of the broad nature of environmental physics the Group is involved in co-operative meetings with other professional organisations with interests in the environment. These newsletters are an archive of our activities since the formation of the Group. For more information about the Environmental Physics Group, see http://www.iop.org/activity/groups/subject/env/index.html
description: Previously curated at: http://cedadocs.ceda.ac.uk/838/ The publish date on this item was its original published date. Main files in this record: iop_epg_newsletter17_1998.pdf Item originally deposited with Centre for Environmental Data Analysis (CEDA) document repository by Dr Sally Brown. Transferred to CEDA document repository community on Zenodo on 2022-11-24
Asplenium platyneuron var. platyneuron Britton & al. var. platyneuron
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Aspleniaceae
Asplenium
Asplenium platyneuron
Asplenium platyneuron (l.) britton & al. var. platyneuron

description: Acrostichum platyneuron Linnaeus, Species Plantarum 2: 1069. 1753. "Habitat in Virginia." RCN: 7782. Lectotype (Fernald in Rhodora 37: 383. 1935): Clayton 14 (BM-000062962). Current name:  Asplenium platyneuron (L.) Britton & al. var.  platyneuron (Aspleniaceae). Note: Specific epithet spelled “platyneuros” in the protologue.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Investigation of the Radial Profile of Galactic Magnetic Fields using Rotation Measure of Background Quasars
Creators: name: Burman, Shivam
name: Sharma, Paras
name: Malik, Sunil
name: Singh, Suprit
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Probing magnetic fields in high-redshift galactic systems is crucial to investigate galactic dynamics and evolution. Utilizing the rotation measure of the background quasars, we have developed a radial profile of the magnetic field in a typical high-$z$ galaxy. We have compiled a catalog of 59 confirmed quasar sightlines, having one intervening Mg \rom{2} absorber in the redshift range $0.372\leq z_{\text{abs}} \leq 0.8$. The presence of the foreground galaxy is ensured by comparing the photometric and spectroscopic redshifts within $3 σ_{z-\text{photo}}$ and visual checks. These quasar line-of-sights (LoS) pass through various impact parameters (D) up to $160$ kpc, covering the circumgalactic medium of a typical Milky-Way type galaxy. Utilizing the residual rotation measure (RRM) of these sightlines, we estimated the excess in RRM dispersion, $σ_{\text{ex}}^{\text{RRM}}$. We found $σ_{\text{ex}}^{\text{RRM}}$ decreases with increasing D. We translated $σ_{\text{ex}}^{\text{RRM}}$ to average LoS magnetic field strength, $\langle B_{\|}\rangle$ by considering a typical electron column density. Consequently, the decreasing trend is sustained in the magnetic field. In particular for sightlines with $\text{D} \leq 50$ kpc and $\text{D} > 50$ kpc, $\langle B_{\|}\rangle$ is found to be $2.39 \pm 0.7 \ μ$G and $1.67 \pm 0.38 \ μ$G, respectively. This suggests a clear indication of varying magnetic field from the disk to the circumgalactic medium. This work provides a methodology that, when applied to ongoing and future radio polarisation surveys such as LOFAR and SKA, promises to significantly enhance our understanding of magnetic field mapping in galactic systems.
description: Published in JCAP
Institute of Physics, Environmental Physics Group newsletter (18), Summer 1998
Creators: name: Brown, Sally
Publisher: name: Zenodo
Year: 1998
Subjects: subject: data and information
subject: Environmental Physics Group
subject: Institute of Physics
subject: https://id.loc.gov/authorities/subjects/sh85081263.html
subject: https://id.loc.gov/authorities/subjects/sh85040989.html
subject: https://id.loc.gov/authorities/subjects/sh85063458.html
subject: https://id.loc.gov/authorities/subjects/sh85101653.html
subject: https://id.loc.gov/authorities/subjects/sh85055077.html
subject: https://id.loc.gov/authorities/subjects/sh2018002590.html
subject: https://id.loc.gov/authorities/subjects/sh85040468.html
subject: https://id.loc.gov/authorities/subjects/sh85084334.html

description: This file contains the newsletters of the Environmental Physics Group at the Institute of Physics. The fundamental aim of the Group is to promote physics within the context of the environmental sciences. In achieving this aim we provide a forum for the discussion of physics as it applies to the environment and encourage the development and application of physical methods to environmental research. The Group also encourages the education and training of physicists in the environmental sciences through meetings and contacts with educationalists at all levels. Because of the broad nature of environmental physics the Group is involved in co-operative meetings with other professional organisations with interests in the environment. These newsletters are an archive of our activities since the formation of the Group. For more information about the Environmental Physics Group, see http://www.iop.org/activity/groups/subject/env/index.html
description: Previously curated at: http://cedadocs.ceda.ac.uk/839/ The publish date on this item was its original published date. Main files in this record: iop_epg_newsletter18_summer1998.pdf Item originally deposited with Centre for Environmental Data Analysis (CEDA) document repository by Dr Sally Brown. Transferred to CEDA document repository community on Zenodo on 2022-11-24
Paramesius longior Dodd 1920
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Paramesius
Paramesius longior

description: Paramesius longior Dodd, 1920: 378.
Valid name
Paramesius longior Dodd, 1920.
Summary of types
Holotype ♀, BMNH number 9.663, by original designation. Paratype ♂.
Primary type data
Type; Hewitt/ Kuching; J2; P.Cameron Coll./ 1914-110; Brachyaulax / rufipes Cam. ♀ / Type Borneo; Paramesius ♀ / longior Dodd.
Type locality
Malaysia, Borneo, Sarawak, Kuching.
Remarks
This species was described from a specimen of each sex which had been labelled with the manuscript name “ Brachyaulax rufipes ” by Cameron. One female and four males were found labelled “ B. rufipes ” in Cameron’s hand. Of these two of the males were mounted together; these could not have been seen by Dodd as he only mentioned one male. A third male is labelled as a type but is not, as the antennae are the wrong colour. The female and remaining male are the types. The female is labelled “type” and the male “cotype”, following Dodd’s published, designation so the female is the holotype by original designation. The holotype is mounted on a card, and has its wings torn and partly missing.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 37, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Discs in misaligned binary systems
Creators: name: Rawiraswattana, Krisada
name: Hubber, David A.
name: Goodwin, Simon P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We perform SPH simulations to study precession and changes in alignment between the circumprimary disc and the binary orbit in misaligned binary systems. We find that the precession process can be described by the rigid-disc approximation, where the disc is considered as a rigid body interacting with the binary companion only gravitationally. Precession also causes change in alignment between the rotational axis of the disc and the spin axis of the primary star. This type of alignment is of great important for explaining the origin of spin-orbit misaligned planetary systems. However, we find that the rigid-disc approximation fails to describe changes in alignment between the disc and the binary orbit. This is because the alignment process is a consequence of interactions that involve the fluidity of the disc, such as the tidal interaction and the encounter interaction. Furthermore, simulation results show that there are not only alignment processes, which bring the components towards alignment, but also anti-alignment processes, which tend to misalign the components. The alignment process dominates in systems with misalignment angle near 90 degrees, while the anti-alignment process dominates in systems with the misalignment angle near 0 or 180 degrees. This means that highly misaligned systems will become more aligned but slightly misaligned systems will become more misaligned.
description: 15 pages, 16 figures, 1 table, accepted for publication in MNRAS
Marginaria polypodioides var. polypodioides Tidestr. var. polypodioides
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Polypodiaceae
Marginaria
Marginaria polypodioides
Marginaria polypodioides (l.) tidestr. var. polypodioides

description: Acrostichum polypodioides Linnaeus, Species Plantarum 2: 1068. 1753. "Habitat in Virginia, Jamaica." RCN: 7775. Lectotype (Verdcourt in Beentje, Fl. Trop. E. Africa, Polypodiaceae: . 31. 2001): [icon] "Filix Polypodium dicta minima, Jamaicensis, foliis aversa parte, ferrugineo pulvere Asplenii ritu, circumquaque respersis" in Plukenet, Phytographia: t. 289, f. 1. 1694; Almag. Bot.: 153. 1696. - Typotype: Herb. Sloane 129: 29 (BM-SL). Current name:  Marginaria polypodioides (L.) Tidestr. var.  polypodioides (Polypodiaceae). Note: Weather by (in Contr. Gray Herb. 124: 28. 1939), followed by later authors, treated material in Plukenet’s herbarium as the type but this was not seen by Linnaeus and is not original material for the name.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Global sensitivity analysis with 2d hydraulic codes: applied protocol and practical tool
Creators: name: Abily, M
name: Bertrand, N
name: Delestre, O
name: Gourbesville, P
name: Richet, Y
name: Duluc, C. -M
Publisher: name: arXiv
Year: 2016
Subjects: subject: Computational Engineering, Finance, and Science (cs.CE)
subject: FOS: Computer and information sciences

description: Global Sensitivity Analysis (GSA) methods are useful tools to rank input parameters uncertainties regarding their impact on result variability. In practice, such type of approach is still at an exploratory level for studies relying on 2D Shallow Water Equations (SWE) codes as GSA requires specific tools and deals with important computational capacity. The aim of this paper is to provide both a protocol and a tool to carry out a GSA for 2D hydraulic modelling applications. A coupled tool between Prom{é}th{é}e (a parametric computation environment) and FullSWOF 2D (a code relying on 2D SWE) has been set up: Prom{é}th{é}e-FullSWOF 2D (P-FS). The main steps of our protocol are: i) to identify the 2D hydraulic code input parameters of interest and to assign them a probability density function, ii) to propagate uncertainties within the model, and iii) to rank the effects of each input parameter on the output of interest. For our study case, simulations of a river flood event were run with uncertainties introduced through three parameters using P-FS tool. Tests were performed on regular computational mesh, spatially discretizing an urban area, using up to 17.9 million of computational points. P-FS tool has been installed on a cluster for computation. Method and P-FS tool successfully allow the computation of Sobol indices maps. Keywords Uncertainty, flood hazard modelling, global sensitivity analysis, 2D shallow water equation, Sobol index. Analyse globale de sensibilit{é} en mod{é}lisation hydrauliqu{è} a surface libre 2D : application d'un protocole et d{é}veloppement d'outils op{é}rationnels -- Les m{é}thodes d'analyse de sensibilit{é} permettent de contr{ô}ler la robustesse des r{é}sultats de mod{é}lisation ainsi que d'identifier le degr{é} d'influence des param etres d' entr{é}e sur le r{é}sultat en sortie d'un mod ele. Le processus complet constitue une analyse globale de sensibilit{é} (GSA). Ce type d'approche pr{é}sente un grand int{é}r{ê}t pour analyser les incer-titudes de r{é}sultats de mod{é}lisation , mais est toujours a un stade exploratoire dans les etudes appliqu{é}es mettant en jeu des codes bas{é}s sur la r{é}solution bidimensionnelle des equations de Saint-Venant. En effet, l' impl{é}mentation d'une GSA est d{é}licate car elle
Institute of Physics, Environmental Physics Group newsletter (20), April 2000
Creators: name: Brown, Sally
Publisher: name: Zenodo
Year: 2000
Subjects: subject: data and information
subject: Environmental Physics Group
subject: Institute of Physics
subject: https://id.loc.gov/authorities/subjects/sh85081263.html
subject: https://id.loc.gov/authorities/subjects/sh85040989.html
subject: https://id.loc.gov/authorities/subjects/sh85063458.html
subject: https://id.loc.gov/authorities/subjects/sh85101653.html
subject: https://id.loc.gov/authorities/subjects/sh85055077.html
subject: https://id.loc.gov/authorities/subjects/sh2018002590.html
subject: https://id.loc.gov/authorities/subjects/sh85040468.html
subject: https://id.loc.gov/authorities/subjects/sh85084334.html

description: This file contains the newsletters of the Environmental Physics Group at the Institute of Physics. The fundamental aim of the Group is to promote physics within the context of the environmental sciences. In achieving this aim we provide a forum for the discussion of physics as it applies to the environment and encourage the development and application of physical methods to environmental research. The Group also encourages the education and training of physicists in the environmental sciences through meetings and contacts with educationalists at all levels. Because of the broad nature of environmental physics the Group is involved in co-operative meetings with other professional organisations with interests in the environment. These newsletters are an archive of our activities since the formation of the Group. For more information about the Environmental Physics Group, see http://www.iop.org/activity/groups/subject/env/index.html
description: Previously curated at: http://cedadocs.ceda.ac.uk/841/ The publish date on this item was its original published date. Main files in this record: iop_epg_newsletter20_april2000.pdf Item originally deposited with Centre for Environmental Data Analysis (CEDA) document repository by Dr Sally Brown. Transferred to CEDA document repository community on Zenodo on 2022-11-24
Galesus muscidorum Dodd 1920
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Galesus
Galesus muscidorum

description: Galesus muscidorum Dodd, 1920: 381.
Valid name
Coptera muscidorum (Dodd, 1920).
Summary of types
Holotype ♀, BMNH number 9.654, by original designation.
Primary type data
Type/ H. T.; Reared/ from pupa found/ in palpalis/ breeding ground/ similar holes can/ often be found in/ palpalis pupae/ G.D.H.Carpenter/ Uganda / Aug 10.1910.; Galesus / muscidorum/ Dodd ♀.
Type locality
Uganda.
Remarks
The holotype is micropinned, with the left antenna missing beyond a8 and mounted with a fly puparium, presumably the host. The generic placement established by Masner (1965) is confirmed here.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 39, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Asplenium adiantum-nigrum Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Aspleniaceae
Asplenium
Asplenium adiantum-Nigrum

description: Acrostichum pulchrum Linnaeus, Species Plantarum 2: 1072. 1753. "Habitat Monspelii, inque Harcynia." RCN: 7794. Type not designated. Original material: Herb. Burser XX: 12 (UPS); Herb. Linn. No. 1245.20 (LINN). Current name:  Asplenium adiantum-nigrum L. (Aspleniaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile
Creators: name: Barura, Chams Gharib Ali
name: Kobayashi, Hajime
name: Mukohyama, Shinji
name: Oshita, Naritaka
name: Takahashi, Kazufumi
name: Yingcharoenrat, Vicharit
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study static tidal Love numbers (TLNs) of a static and spherically symmetric black hole for odd-parity metric perturbations. We describe black hole perturbations using the effective field theory (EFT), formulated on an arbitrary background with a timelike scalar profile in the context of scalar-tensor theories. In particular, we obtain a static solution for the generalized Regge-Wheeler equation order by order in a modified-gravity parameter and extract the TLNs uniquely by analytic continuation of the multipole index $\ell$ to non-integer values. For a stealth Schwarzschild black hole, the TLNs are vanishing as in the case of Schwarzschild solution in general relativity. We also study the case of Hayward black hole as an example of non-stealth background, where we find that the TLNs are non-zero (or there is a logarithmic running). This result suggests that our EFT allows for non-vanishing TLNs and can in principle leave a detectable imprint on gravitational waves from inspiralling binary systems, which opens a new window for testing gravity in the strong-field regime.
description: 40 pages. Matches JCAP version
Aneurhynchus indicus Dodd 1920
Creators: name: Notton, David G.
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diapriidae
Aneurhynchus
Aneurhynchus indicus

description: Aneurhynchus indicus Dodd, 1920: 382.
Valid name
Aneurhynchus indicus Dodd, 1920.
Summary of types
Holotype ♀, BMNH number 9.634, by original designation.
Primary type data
Type; Kangra Valley/ 4,500 ft. / Apr. 1899 / Dudgeon.; Punjab./ G.C.Dudgeon./ 1903-37.; Aneurhynchus / indicus Dodd ♀.
Type locality
India, Punjab Province, Kangra Valley.
Remarks
This species was described from a single female. The holotype is mounted on a card and is entire.
description: Published as part of Notton, David G., 2014, A catalogue of the types of Diapriinae (Hymenoptera, Diapriidae) at the Natural History Museum, London, pp. 1-123 in European Journal of Taxonomy 75 on page 39, DOI: 10.5852/ejt.2014.75, http://zenodo.org/record/3862773
Thermal Conductivity of Chirality-Sorted Carbon Nanotube Networks
Creators: name: Lian, Feifei
name: Llinas, Juan P.
name: Li, Zuanyi
name: Estrada, David
name: Pop, Eric
Publisher: name: arXiv
Year: 2016
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The thermal properties of single-walled carbon nanotubes (SWNTs) are of significant interest, yet their dependence on SWNT chirality has been, until now, not explored experimentally. Here we used electrical heating and infrared thermal imaging to simultaneously study thermal and electrical transport in chirality-sorted SWNT networks. We examined solution processed 90% semiconducting, 90% metallic, purified unsorted (66% semiconducting), and as-grown HiPco SWNT films. The thermal conductivities of these films range from 80 to 370 W/m/K but are not controlled by chirality, instead being dependent on the morphology (i.e. mass and junction density, quasi-alignment) of the networks. The upper range of the thermal conductivities measured is comparable to that of the best metals (Cu and Ag) but with over an order of magnitude lower mass density. This study reveals important factors controlling the thermal properties of light-weight chirality-sorted SWNT films, for potential thermal and thermoelectric applications.
Institute of Physics, Environmental Physics Group newsletter (21), October 2000
Creators: name: Brown, Sally
Publisher: name: Zenodo
Year: 2000
Subjects: subject: data and information
subject: Environmental Physics Group
subject: Institute of Physics
subject: https://id.loc.gov/authorities/subjects/sh85081263.html
subject: https://id.loc.gov/authorities/subjects/sh85040989.html
subject: https://id.loc.gov/authorities/subjects/sh85063458.html
subject: https://id.loc.gov/authorities/subjects/sh85101653.html
subject: https://id.loc.gov/authorities/subjects/sh85055077.html
subject: https://id.loc.gov/authorities/subjects/sh2018002590.html
subject: https://id.loc.gov/authorities/subjects/sh85040468.html
subject: https://id.loc.gov/authorities/subjects/sh85084334.html

description: This file contains the newsletters of the Environmental Physics Group at the Institute of Physics. The fundamental aim of the Group is to promote physics within the context of the environmental sciences. In achieving this aim we provide a forum for the discussion of physics as it applies to the environment and encourage the development and application of physical methods to environmental research. The Group also encourages the education and training of physicists in the environmental sciences through meetings and contacts with educationalists at all levels. Because of the broad nature of environmental physics the Group is involved in co-operative meetings with other professional organisations with interests in the environment. These newsletters are an archive of our activities since the formation of the Group. For more information about the Environmental Physics Group, see http://www.iop.org/activity/groups/subject/env/index.html
description: Previously curated at: http://cedadocs.ceda.ac.uk/842/ The publish date on this item was its original published date. Main files in this record: iop_epg_newsletter21_oct2000.pdf Item originally deposited with Centre for Environmental Data Analysis (CEDA) document repository by Dr Sally Brown. Transferred to CEDA document repository community on Zenodo on 2022-11-24
Microsorum punctatum Copel.
Creators: name: Jarvis, Charlie
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Polypodiopsida
Polypodiales
Polypodiaceae
Microsorum
Microsorum punctatum

description: Acrostichum punctatum Linnaeus, Species Plantarum, ed. 2, 2: 1524. 1763. "Habitat in China. J. Fothergill." RCN: 7769. Type not designated. Original material: none traced. Current name:  Microsorum punctatum (L.) Copel. (Polypodiaceae). Note: Many authors since Schelpe & Anthony (in Leistner, Fl. Southern Africa, Pteridophyta: 163. 1986) have noted the absence of original material in LINN, and the name appears to need a neotype.
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part A), pp. 252-342 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 260, DOI: 10.5281/zenodo.291971
Spectroscopy and Dynamics of a Two-Dimensional Electron Gas on top of Ultrathin Helium Films on Cu(111)
Creators: name: Armbrust, Nico
name: Güdde, Jens
name: Höfer, Ulrich
name: Kossler, Sarah
name: Feulner, Peter
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Electrons in image-potential states on the surface of bulk helium represent a unique model system of a two-dimensional electron gas. Here, we investigate their properties in the extreme case of reduced film thickness: a monolayer of helium physisorbed on a single-crystalline (111)-oriented Cu surface. For this purpose we have utilized a customized setup for time-resolved two-photon photoemission (2PPE) at very low temperatures under ultra-high vacuum conditions. We demonstrate that the highly polarizable metal substrate increases the binding energy of the first (n = 1) image-potential state by more than two orders of magnitude as compared to the surface of liquid helium. An electron in this state is still strongly decoupled from the metal surface due to the large negative electron affinity of helium and we find that even one monolayer of helium increases its lifetime by one order of magnitude compared to the bare Cu(111) surface.
description: 4 pages, 3 figures